The Sky Sourcebook
1. Sky Content
2. Sky Levels
3. Weather
4. Altitude Sickness
5. Tornados
6. Aerial Cities
7. Aerial Races
8. Aerial Classes
9. Aerial Bestiary
10. Flight
11. Air Combat
12. Air Vehicles
13. Organizations
14. The Celestialscape
15. Air Elemental Magic
16. Aerial Powers
The sky realms are a mysterious place. Cloud cities come and go with the
drifting of the winds, while mysterious winged
creatures migrate vast distances in a single week. Some “terrain features” are
permanent (such as persistent rainstorms or
clouds that orbit in a fixed pattern), while others are completely unpredictable
(such as cloud cities that move entirely at the
whims of the wind).
1. Sky Content |
The sky (or celestial dome) is everything that lies above the surface of the Earth, including the atmosphere and outer space. During daylight, the sky appears to be blue because air scatters blue sunlight more than it scatters red. At night, the sky appears to be a mostly dark surface or region scattered with stars. During the day, the Sun can be seen in the sky unless obscured by clouds. In the night sky (and to some extent during the day) the moon, planets and stars are visible in the sky. Some of the natural phenomena seen in the sky are clouds, rainbows, and aurora. Lightning and precipitation can also be seen in the sky during storms. Birds, insects, aircraft, and kites are often considered to fly in the sky. Due to human activities, smog during the day and light pollution during the night are often seen above large cities. Individual water droplets exposed to white light will create a set of collared rings. If a cloud is thick enough, scattering from multiple water droplets will wash out the set of collared rings and create a washed-out white colour. The sky can turn a multitude of colours such as red, orange, purple and yellow (especially near sunset or sunrise) when the light must pass through a much longer path (or optical depth) through the atmosphere. Because red light also scatters if there is enough air between the source and the observer, these longer wavelengths of light will also scatter significantly, making parts of the sky change colour during a sunset. As the amount of atmosphere nears infinity, the scattered light appears whiter and whiter. At higher altitudes, the sky tends toward darker colours since scattering is reduced due to lower air density; an extreme example is the moon, where there is no atmosphere and no scattering, making the sky on the moon black even when the sun is visible. The atmosphere of Earth is the layer of gases surrounding the planet Earth that
is retained by Earth's gravity. The atmosphere protects life on Earth by
absorbing ultraviolet solar radiation, warming the surface through heat
retention (greenhouse effect), and reducing temperature extremes between day and
night (the diurnal temperature variation). The average temperature of the atmosphere at Earth's surface is 14 °C or 15 °C
depending on the reference.
The average atmospheric pressure at sea level is defined by the International
Standard Atmosphere as 101325 pascals (760.00 Torr; 14.6959 psi; 760.00 mmHg).
This is sometimes referred to as a unit of standard atmospheres (atm). Total
atmospheric mass is 5.1480×1018 kg (1.135×1019 lb), about 2.5% less than
would be inferred from the average sea level pressure and Earth's area of
51007.2 megahectares, this portion being displaced by Earth's mountainous
terrain. Atmospheric pressure is the total weight of the air above unit area at
the point where the pressure is measured. Thus air pressure varies with location
and weather.
If the entire mass of the atmosphere had a uniform density from sea level, it
would terminate abruptly at an altitude of 8.50 kms. It actually
decreases exponentially with altitude, dropping by half every 5.6 kms
or by a factor of 1/e every 7.64 kms, the average scale height of the
atmosphere below 70 kms. However, the atmosphere is more
accurately modelled with a customized equation for each layer that takes
gradients of temperature, molecular composition, solar radiation and gravity
into account. Even above the Kármán line, significant atmospheric effects such as auroras still occur. Meteors begin to glow in this region though the larger ones may not burn up until they penetrate more deeply. The various layers of Earth's ionosphere, important to HF radio propagation, begin below 100 kms and extend beyond 500 kms. By comparison, the International Space Station and Space Shuttle typically orbit at 350–400 kms, within the F-layer of the ionosphere where they encounter enough atmospheric drag to require reboosts every few months. Depending on solar activity, satellites can experience noticeable atmospheric drag at altitudes as high as 700–800 kms. The division of the atmosphere into layers mostly by reference to temperature is
discussed above. Temperature decreases with altitude starting at sea level, but
variations in this trend begin above 11 kms, where the temperature stabilizes
through a large vertical distance through the rest of the troposphere. In the
stratosphere, starting above about 20 km, the temperature increases with height,
due to heating within the ozone layer caused by capture of significant
ultraviolet radiation from the Sun by the dioxygen and ozone gas in this region.
Still another region of increasing temperature with altitude occurs at very high
altitudes, in the aptly-named thermosphere above 90 kms. The density of air at sea level is about 1.2 kg/m3 (1.2 g/L). Density is not measured directly but is calculated from measurements of temperature, pressure and humidity using the equation of state for air (a form of the ideal gas law). Atmospheric density decreases as the altitude increases. This variation can be approximately modelled using the barometric formula. More sophisticated models are used to predict orbital decay of satellites. The average mass of the atmosphere is about 5 quadrillion (5×1015) tonnes or 1/1,200,000 the mass of Earth. According to the American National Centre for Atmospheric Research, "The total mean mass of the atmosphere is 5.1480×1018 kg with an annual range due to water vapour of 1.2 or 1.5×1015 kg depending on whether surface pressure or water vapour data are used; somewhat smaller than the previous estimate. The mean mass of water vapour is estimated as 1.27×1016 kg and the dry air mass as 5.1352 ±0.0003×1018 kg. Solar radiation (or sunlight) is the energy Earth receives from the Sun. Earth also emits radiation back into space, but at longer wavelengths that we cannot see. Part of the incoming and emitted radiation is absorbed or reflected by the atmosphere. |
2. Sky Levels |
In general, air pressure and density decrease with altitude in the atmosphere.
However, temperature has a more complicated profile with altitude, and may
remain relatively constant or even increase with altitude in some regions (see
the temperature section, below). Because the general pattern of the
temperature/altitude profile is constant and recognizable through means such as
balloon soundings, the temperature behaviour provides a useful metric to
distinguish between atmospheric layers. In this way, Earth's atmosphere can be
divided (called atmospheric stratification) into five main layers. Excluding the
exosphere, Earth has four primary layers, which are the troposphere,
stratosphere, mesosphere, and thermosphere. From highest to lowest, the five
main layers are: |
Exosphere |
The exosphere is the outermost layer of Earth's atmosphere (i.e. the upper limit
of the atmosphere). It extends from the exobase, which is located at the top of
the thermosphere at an altitude of about 700 kms above sea level, to about 10,000
kms. The exosphere merges with the emptiness of outer
space, where there is no atmosphere. This layer is mainly composed of extremely low densities of hydrogen, helium and several heavier molecules including nitrogen, oxygen and carbon dioxide closer to the exobase. The atoms and molecules are so far apart that they can travel hundreds of kilometres without colliding with one another. Thus, the exosphere no longer behaves like a gas, and the particles constantly escape into space. These free-moving particles follow ballistic trajectories and may migrate in and out of the magnetosphere or the solar wind. The exosphere is located too far above Earth for any meteorological phenomena to be possible. However, the aurora borealis and aurora australis sometimes occur in the lower part of the exosphere, where they overlap into the thermosphere. The exosphere contains most of the satellites orbiting Earth. The most common molecules within Earth's exosphere are those of the lightest atmospheric gasses. Hydrogen is present throughout the exosphere, with some helium, carbon dioxide, and atomic oxygen near its base. Because it can be difficult to define the boundary between the exosphere and outer space, the exosphere may be considered a part of interplanetary or outer space. The lower boundary of the exosphere is called the exobase. It is also called exopause and 'critical altitude' as this is the altitude where barometric conditions no longer apply. Atmospheric temperature becomes nearly a constant above this altitude. On Earth, the altitude of the exobase ranges from about 500 to 1,000 kilometres depending on solar activity. The fluctuation in the height of the exobase is important because this provides atmospheric drag on satellites, eventually causing them to fall from orbit if no action is taken to maintain the orbit. In principle, the exosphere covers distances where particles are still gravitationally bound to Earth, i.e. particles still have ballistic orbits that will take them back towards Earth. The upper boundary of the exosphere can be defined as the distance at which the influence of solar radiation pressure on atomic hydrogen exceeds that of Earth's gravitational pull. This happens at half the distance to the Moon (the average distance between Earth and the Moon is 384,400 kilometres. The exosphere, observable from space as the geocorona, is seen to extend to at least 10,000 kilometres from Earth's surface. The exosphere is a transitional zone between Earth's atmosphere and space. Very high up, the Earth's atmosphere becomes very thin. The region where atoms and molecules escape into space is referred to as the exosphere. The exosphere is on top of the thermosphere. |
Thermosphere |
The thermosphere is the second-highest layer of Earth's atmosphere. It extends
from the mesopause (which separates it from the mesosphere) at an altitude of
about 80 kms up to the thermopause at an altitude range of
500–1000 kms. The height of the thermopause
varies considerably due to changes in solar activity. Because the thermopause
lies at the lower boundary of the exosphere, it is also referred to as the
exobase. The lower part of the thermosphere, from 80 to 550 kilometres above Earth's surface, contains the ionosphere.
This atmospheric layer undergoes a gradual increase in temperature with height.
Unlike the stratosphere, wherein a temperature inversion is due to the
absorption of radiation by ozone, the inversion in the thermosphere occurs due
to the extremely low density of its molecules. The temperature of this layer can
rise as high as 1500 °C , though the gas molecules are so far apart
that its temperature in the usual sense is not very meaningful. The air is so
rarefied that an individual molecule (of oxygen, for example) travels an average
of 1 kilometre between collisions with other molecules.
Even though the thermosphere has a very high proportion of molecules with
immense amounts of energy, the thermosphere would not feel hot to a human in
direct contact, because the low density in the thermosphere would not be able to
conduct a significant amount of energy to or from the skin. In other words, a
person would not feel warm because of the thermosphere's extremely low pressure. This layer is completely cloudless and free of water vapour. However non-hydrometeorological phenomena such as the aurora borealis and aurora australis are occasionally seen in the thermosphere. The International Space Station orbits in this layer, between 320 and 380 kms. The thermosphere is the layer of the Earth's atmosphere directly above the mesosphere and directly below the exosphere. Within this layer, ultraviolet radiation causes photoionization/ photodissociation of molecules present. Thermospheric temperatures increase with altitude due to absorption of highly energetic solar radiation. Temperatures are highly dependent on solar activity, and can rise to 2,000 °C. Radiation causes the atmosphere particles in this layer to become electrically charged (see ionosphere), enabling radio waves to bounce off and be received beyond the horizon. In the exosphere, beginning at 500 to 1,000 kilometres above the Earth's surface, the atmosphere turns into space. The highly diluted gas in this layer can reach 2,500 °C during the day. Even though the temperature is so high, one would not feel warm in the thermosphere, because it is so near vacuum that there is not enough contact with the few atoms of gas to transfer much heat. A normal thermometer would be significantly below 0 °C, because the energy lost by thermal radiation would exceed the energy acquired from the atmospheric gas by direct contact. In the anacoustic zone above 160 kilometres, the density is so low that molecular interactions are too infrequent to permit the transmission of sound. The dynamics of the thermosphere are dominated by atmospheric tides, which are driven by the very significant diurnal heating. Atmospheric waves dissipate above this level because of collisions between the neutral gas and the ionospheric plasma. The International Space Station orbits within the middle of the thermosphere, between 330 and 435 kilometres (decaying by 2 kms per month and raised by periodic reboosts), whereas the Gravity Field and Steady-State Ocean Circulation Explorer satellite at 260 kilometres utilized winglets and an innovative ion engine to maintain a stable orientation and orbit. It is convenient to separate the atmospheric regions according to the two temperature minima at about 12 kms altitude (the tropopause) and at about 85 kms (the mesopause). The thermosphere (or the upper atmosphere) is the height region above 85 kms, while the region between the tropospause and the mesopause is the middle atmosphere (stratosphere and mesosphere) where absorption of solar UV radiation generates the temperature maximum near 45 kms altitude and causes the ozone layer. Turbulence causes the air within the lower atmospheric regions below the turbopause at about 110 kms to be a mixture of gases that does not change its composition. Its mean molecular weight is 29 g/mol with molecular oxygen (O2) and nitrogen (N2) as the two dominant constituents. Above the turbopause, however, diffusive separation of the various constituents is significant, so that each constituent follows its own barometric height structure with a scale height inversely proportional to its molecular weight. The lighter constituents atomic oxygen (O), helium (He), and hydrogen (H) successively dominate above about 200 kms altitude and vary with geographic location, time, and solar activity. The ratio N2/O which is a measure of the electron density at the ionospheric F region is highly affected by these variations. The solar X-ray and extreme ultraviolet radiation (XUV) at wavelengths < 170 nm is almost completely absorbed within the thermosphere. This radiation causes the various ionospheric layers as well as a temperature increase at these heights. While the solar visible light (380 to 780 nm) is nearly constant with a variability of not more than about 0.1% of the solar constant, the solar XUV radiation is highly variable in time and space. For instance, X-ray bursts associated with solar flares can dramatically increase their intensity over preflare levels by many orders of magnitude over a time span of tens of minutes. In the extreme ultraviolet, the Lyman α line at 121.6 nm represents an important source of ionization and dissociation at ionospheric D layer heights. During quiet periods of solar activity, it alone contains more energy than the rest of the XUV spectrum. Quasi-periodic changes of the order of 100% and more with period of 27 days and 11 years belong to the prominent variations of solar XUV radiation. However, irregular fluctuations over all time scales are present all the time. During low solar activity, about one half of the total energy input into the thermosphere is thought to be solar XUV radiation. Evidently, that solar XUV energy input occurs only during daytime conditions, maximizing at the equator during equinox. A second source of energy input into the thermosphere is solar wind energy which is transferred to the magnetosphere by mechanisms that are not completely understood. One possible way to transfer energy is via a hydrodynamic dynamo process. Solar wind particles penetrate into the polar regions of the magnetosphere where the geomagnetic field lines are essentially vertically directed. An electric field is generated, directed from dawn to dusk. Along the last closed geomagnetic field lines with their footpoints within the auroral zones, field aligned electric currents can flow into the ionospheric dynamo region where they are closed by electric Pedersen and Hall currents. Ohmic losses of the Pedersen currents heat the lower thermosphere (see e.g., Magnetospheric electric convection field). In addition, penetration of high energetic particles from the magnetosphere into the auroral regions enhance drastically the electric conductivity, further increasing the electric currents and thus Joule heating. During quiet magnetospheric activity, the magnetosphere contributes perhaps by a quarter to the energy budget of the thermosphere. This is about 250 K of the exospheric temperature. During very large activity, however, this heat input can increase substantially, by a factor of four or more. That solar wind input occurs mainly in the auroral regions during the day as well as during the night. Heating, predominately by tidal waves, occurs mainly at lower and middle latitudes. The variability of this heating depends in general on the meteorological conditions within troposphere and middle atmosphere, and may not exceed about 50%.In contrast to solar XUV radiation, magnetospheric disturbances, indicated on the ground by geomagnetic variations, show an unpredictable impulsive character, from short periodic disturbances of the order of hours to long standing giant storms of several day's duration. The reaction of the thermosphere to a large magnetospheric storm is called thermospheric storm. In addition, due to the impulsive form of the disturbance, higher order terms are generated which, however, possess short decay times and thus quickly disappear. The sum of these modes determines the "travel time" of the disturbance to the lower latitudes, and thus the response time of the thermosphere with respect to the magnetospheric disturbance. Important for the development of an ionospheric storm is the increase of the ratio N2/O during a thermospheric storm at middle and higher latitude. An increase of N2 increases the loss process of the ionospheric plasma and causes therefore a decrease of the electron density within the ionospheric F-layer (negative ionospheric storm). The mesosphere is the third highest layer of Earth's atmosphere, occupying the region above the stratosphere and below the thermosphere. It extends from the stratopause at an altitude of about 50 kms to the mesopause at 80–85 kms above sea level. Temperatures drop with increasing altitude to the mesopause that marks the top of this middle layer of the atmosphere. It is the coldest place on Earth and has an average temperature around −85 °C. Just below the mesopause, the air is so cold that even the very scarce water vapour at this altitude can be sublimated into polar-mesospheric noctilucent clouds. These are the highest clouds in the atmosphere and may be visible to the naked eye if sunlight reflects off them about an hour or two after sunset or a similar length of time before sunrise. They are most readily visible when the Sun is around 4 to 16 degrees below the horizon. A type of lightning referred to as either sprites or ELVES, occasionally form far above tropospheric thunderclouds. The mesosphere is also the layer where most meteors burn up upon atmospheric entrance. It is too high above Earth to be accessible to aircraft and balloons, and too low to permit orbital spacecraft. The mesosphere is mainly accessed by sounding rockets. The Earth's thermosphere also includes the region of the atmosphere called the ionosphere. The ionosphere is a region of the atmosphere that is filled with charged particles. The high temperatures in the thermosphere can cause molecules to ionize. This is why an ionosphere and thermosphere can overlap. Scientists call the ionosphere an extension of the thermosphere. So technically, the ionosphere is not another atmospheric layer. The ionosphere represents less than 0.1% of the total mass of the Earth's atmosphere. Even though it is such a small part, it is extremely important. The upper atmosphere is ionized by solar radiation. That means the Sun's energy is so strong at this level, that it breaks apart molecules. So there ends up being electrons floating around and molecules which have lost or gained electrons. When the Sun is active, more and more ionization happens. Different regions of the ionosphere make long distance radio communication possible by reflecting the radio waves back to Earth. It is also home to auroras. Temperatures in the ionosphere just keep getting hotter as you go up. The ionosphere is broken down into the D, E and F regions. The breakdown is based on what wavelength of solar radiation is absorbed in that region most frequently. The D region is the lowest in altitude, though it absorbs the most energetic radiation, hard x-rays. The D region doesn't have a definite starting and stopping point, but includes the ionization that occurs below about 90kms. The E region peaks at about 105kms. It absorbs soft x-rays. The F region starts around 105kms and has a maximum around 600kms. It is the highest of all of the regions. Extreme ultra-violet radiation (EUV) is absorbed there. On a more practical note, the D and E regions reflect AM radio waves back to Earth. Radio waves with shorter lengths are reflected by the F region. Visible light, television and FM wavelengths are all too short to be reflected by the ionosphere. So your t.v. stations are made possible by satellite transmissions. Invisible layers of ions and electrons are found in the Earth's atmosphere. We call this region of atmosphere the ionosphere. The main source of these layers is the Sun's ultraviolet light which ionizes atoms and molecules in the Earth's upper atmosphere. During this process, electrons are knocked free from molecules or particles in the atmosphere. Flares and other big events on the Sun produce increased ultraviolet, x-ray and gamma-ray photons that arrive at the Earth just 8 minutes later (other particles from the Sun may arrive days later) and dramatically increase the ionization that happens in the atmosphere. So, the more active the Sun, the thicker the ionosphere. |
Mesosphere |
The mesosphere is
the layer of the Earth's atmosphere that is directly above the stratopause and
directly below the mesopause. In the mesosphere temperature decreases as the
altitude increases. The upper boundary of the mesosphere is the mesopause, which
can be the coldest naturally occurring place on Earth with temperatures below
−143 °C. The exact upper and lower boundaries of the mesosphere
vary with latitude and with season, but the lower boundary of the mesosphere is
usually located at heights of about 50 kilometres above the
Earth's surface and the mesopause is usually at heights near 100 kilometres, except at middle and high latitudes in summer where it descends to heights
of about 85 kilometres. This is also
around the same altitude as the turbopause, below which different chemical
species are well mixed due to turbulent eddies. Above this level the atmosphere
becomes non-uniform; the scale heights of different chemical species differ by
their molecular masses.
Within the mesosphere, temperature decreases with increasing height. This is due
to decreasing solar heating and increasing cooling by CO2 radiative emission.
The top of the mesosphere, called the mesopause, is the coldest part of Earth's
atmosphere. Temperatures in the upper mesosphere fall as low as −100 °C, varying according to latitude and season.
The main dynamic features in this region are strong zonal (East-West) winds,
atmospheric tides, internal atmospheric gravity waves (commonly called "gravity
waves") and planetary waves. Most of these tides and waves are excited in the
troposphere and lower stratosphere, and propagate upward to the mesosphere. In
the mesosphere, gravity-wave amplitudes can become so large that the waves
become unstable and dissipate. This dissipation deposits momentum into the
mesosphere and largely drives global circulation. Noctilucent clouds are located in the mesosphere. The upper mesosphere is also
the region of the ionosphere known as the D layer. The D layer is only present
during the day, when some ionization occurs with nitric oxide being ionized by
Lyman series-alpha hydrogen radiation. The ionization is so weak that when night
falls, and the source of ionization is removed, the free electron and ion form
back into a neutral molecule. The mesosphere is also known as the "Ignorosphere"
because it is poorly studied compared to the stratosphere (which can be
accessed with high-altitude balloons) and the thermosphere (in which
satellites can orbit). A 5 km deep sodium layer is located between 80–105 kms. Made
of unbound, non-ionized atoms of sodium, the sodium layer radiates weakly to
contribute to the airglow. Millions of meteors enter the atmosphere, an average
of 40 tons per year.
The mesosphere lies above the maximum altitude for aircraft and nearly all
balloons, and below the minimum altitude for orbital spacecraft. Above the 53
km balloon altitude record, the mesosphere has only been accessed through the
use of sounding rockets. As a result, it is the most poorly understood part of
the atmosphere. The presence of red sprites and blue jets (electrical discharges
or lightning within the lower mesosphere), noctilucent clouds and density shears
within the poorly understood layer are of current scientific interest. In the Earth's mesosphere, the air is relatively mixed together and the
temperature decreases with altitude. The atmosphere reaches its coldest
temperature of around -90°C in the mesosphere. This is also the layer in which a
lot of meteors burn up while entering the Earth's atmosphere. |
Stratosphere |
The stratosphere is the second-lowest layer of Earth's atmosphere. It lies above
the troposphere and is separated from it by the tropopause. This layer extends
from the top of the troposphere at roughly 12 kms above
Earth's surface to the stratopause at an altitude of about 50 to 55 kms.
The atmospheric pressure at the top of the stratosphere is roughly 1/1000 the
pressure at sea level. It contains the ozone layer, which is the part of Earth's
atmosphere that contains relatively high concentrations of that gas. The
stratosphere defines a layer in which temperatures rise with increasing
altitude. This rise in temperature is caused by the absorption of ultraviolet
radiation (UV) radiation from the Sun by the ozone layer, which restricts
turbulence and mixing. Although the temperature may be −60 °C at the
tropopause, the top of the stratosphere is much warmer, and may be near 0
°C.
The stratospheric temperature profile creates very stable atmospheric
conditions, so the stratosphere lacks the weather-producing air turbulence that
is so prevalent in the troposphere. Consequently, the stratosphere is almost
completely free of clouds and other forms of weather. However, polar
stratospheric or nacreous clouds are occasionally seen in the lower part of this
layer of the atmosphere where the air is coldest. This is the highest layer that
can be accessed by jet-powered aircraft. The stratosphere is the second major layer of Earth's atmosphere, just above the troposphere, and below the mesosphere. It is stratified in temperature, with warmer layers higher up and cooler layers farther down. This is in contrast to the troposphere near the Earth's surface, which is cooler higher up and warmer farther down. The border of the troposphere and stratosphere, the tropopause, is marked by where this inversion begins, which in terms of atmospheric thermodynamics is the equilibrium level. At moderate latitudes the stratosphere is situated between about 10–13 kms and 50 kms altitude above the surface, while at the poles it starts at about 8 kms altitude, and near the equator it may start at altitudes as high as 18 kms. Within this layer, temperature increases as altitude increases (see temperature inversion); the top of the stratosphere has a temperature of about −3°Cs, just slightly below the freezing point of water.s The stratosphere is layered in temperature because ozone (O3) here absorbs high energy ultraviolet (UVB and UVC) radiation from the Sun and is broken down into the allotropes of atomic oxygen (O1) and common molecular oxygen (O2). The mid stratosphere has less UV light passing through it; O and O2 are able to combine, and this is where the majority of natural ozone is produced. It is when these two forms of oxygen recombine to form ozone that they release the heat found in the stratosphere. The lower stratosphere receives very low amounts of UVC; thus atomic oxygen is not found here and ozone is not formed (with heat as the byproduct). This vertical stratification, with warmer layers above and cooler layers below, makes the stratosphere dynamically stable: there is no regular convection and associated turbulence in this part of the atmosphere. The top of the stratosphere is called the stratopause, above which the temperature decreases with height. Methane (CH4), while not a direct cause of ozone destruction in the stratosphere, does lead to the formation of compounds that destroy ozone. Monatomic oxygen (O) in the upper stratosphere reacts with methane (CH4) to form a hydroxyl radical (OH·). This hydroxyl radical is then able to interact with non-soluble compounds like chlorofluorocarbons, and UV light breaks off chlorine radicals (Cl·). These chlorine radicals break off an oxygen atom from the ozone molecule, creating an oxygen molecule (O2) and a hypochloryl radical (ClO·). The hypochloryl radical then reacts with an atomic oxygen creating another oxygen molecule and another chlorine radical, thereby preventing the reaction of monatomic oxygen with O2 to create natural ozone. Commercial airliners typically cruise at altitudes of 9–12 kms (30,000–39,000 ft)
in temperate latitudes (in the lower reaches of the stratosphere). This
optimizes fuel burn, mostly due to the low temperatures encountered near the
tropopause and low air density, reducing parasitic drag on the airframe. (Stated
another way, it allows the airliner to fly faster for the same amount of drag.)
It also allows them to stay above hard weather (extreme turbulence). Because the temperature in the tropopause and lower stratosphere remains constant (or slightly decreases) with increasing altitude, very little convective turbulence occurs at these altitudes. Though most turbulence at this altitude is caused by variations in the jet stream and other local wind shears, areas of significant convective activity (thunderstorms) in the troposphere below may produce convective overshoot. Although a few gliders have achieved great altitudes in the powerful thermals in thunderstorms, this is dangerous. Most high altitude flights by gliders use lee waves from mountain ranges and were used to set the current record of 15,447 mtrs. The stratosphere is a region of intense interactions among radiative, dynamical, and chemical processes, in which the horizontal mixing of gaseous components proceeds much more rapidly than in vertical mixing. An interesting feature of stratospheric circulation is the quasi-biennial oscillation (QBO) in the tropical latitudes, which is driven by gravity waves that are convectively generated in the troposphere. The QBO induces a secondary circulation that is important for the global stratospheric transport of tracers, such as ozone or water vapour. Also, some bird species have been reported to fly at the lower levels of the stratosphere. About 90% of the ozone in the Earth's atmosphere is found in the region called the stratosphere. This is the atmospheric layer between 16 and 48 kilometres above the Earth's surface. Ozone forms a kind of layer in the stratosphere, where it is more concentrated than anywhere else. Ozone and oxygen molecules in the stratosphere absorb ultraviolet light from the Sun, providing a shield that prevents this radiation from passing to the Earth's surface. While both oxygen and ozone together absorb 95 to 99.9% of the Sun's ultraviolet radiation, only ozone effectively absorbs the most energetic ultraviolet light, known as UV-C and UV-B. This ultraviolet light can cause biological damage like skin cancer, tissue damage to eyes and plant tissue damage. The protective role of the ozone layer in the upper atmosphere is so vital that scientists believe life on land probably would not have evolved - and could not exist today - without it. The ozone layer would be quite good at its job of protecting Earth from too much ultraviolet radiation - that is, it would if humans did not contribute to the process. It's now known that ozone is destroyed in the stratosphere and that some human-released chemicals such as CFC’s are speeding up the breakdown of ozone, so that there are "holes" now in our protective shield. While the stratospheric ozone issue is a serious one, in many ways it can be thought of as an environmental success story. Scientists detected the developing problem, and collected the evidence that convinced governments around the world to take action. Although the elimination of ozone-depleting chemicals from the atmosphere will take decades yet, we have made a strong and positive beginning. For the first time in our species' history, we have tackled a global environmental issue on a global scale. Many jet aircrafts fly in the stratosphere because it is very stable. Also, the ozone layer absorbs harmful rays from the Sun. |
Troposphere |
The troposphere is the lowest layer of Earth's atmosphere. It extends from
Earth's surface to an average height of about 12 kms, although this altitude
actually varies from about 9 kms at the poles to 17 kms at
the equator, with some variation due to weather. The troposphere is bounded
above by the tropopause, a boundary marked in most places by a temperature
inversion (i.e. a layer of relatively warm air above a colder one), and in
others by a zone which is isothermal with height. Although variations do
occur, the temperature usually declines with increasing altitude in the
troposphere because the troposphere is mostly heated through energy transfer
from the surface. Thus, the lowest part of the troposphere (i.e. Earth's
surface) is typically the warmest section of the troposphere. This promotes
vertical mixing. The troposphere contains roughly 80% of the mass of
Earth's atmosphere. The troposphere is denser than all its overlying
atmospheric layers because a larger atmospheric weight sits on top of the
troposphere and causes it to be most severely compressed. Fifty percent of the
total mass of the atmosphere is located in the lower 5.6 kms of the
troposphere. It is primarily composed of nitrogen (78%) and oxygen (21%) with
only small concentrations of other trace gases.
Nearly all atmospheric water vapour or moisture is found in the troposphere, so
it is the layer where most of Earth's weather takes place. It has basically all
the weather-associated cloud genus types generated by active wind circulation,
although very tall cumulonimbus thunder clouds can penetrate the tropopause from
below and rise into the lower part of the stratosphere. Most conventional
aviation activity takes place in the troposphere, and it is the only layer that
can be accessed by propeller-driven aircraft. The troposphere is the lowest portion of Earth's atmosphere. It contains
approximately 75% of the atmosphere's mass and 99% of its water vapour and
aerosols. The average depth of the troposphere is approximately 17 kms
in the middle latitudes. It is deeper in the tropics, up to 20 kms, and
shallower near the polar regions, approximately 7 kms in winter. The
lowest part of the troposphere, where friction with the Earth's surface
influences air flow, is the planetary boundary layer. This layer is typically a
few hundred meters to 2 kms deep depending on the landform and time of day. The
border between the troposphere and stratosphere, called the tropopause, is a
temperature inversion. The chemical composition of the troposphere is essentially uniform, with the notable exception of water vapour. The source of water vapour is at the surface through the processes of evaporation and transpiration. Furthermore, the temperature of the troposphere decreases with height, and saturation vapour pressure decreases strongly as temperature drops, so the amount of water vapour that can exist in the atmosphere decreases strongly with height. Thus the proportion of water vapour is normally greatest near the surface and decreases with height. Since temperature in principle also depends on altitude, one needs a second equation to determine the pressure as a function of height. The temperature of the troposphere generally decreases as altitude increases. The rate at which the temperature decreases, -dT/dz, is called the environmental lapse rate (ELR). The ELR is nothing more than the difference in temperature between the surface and the tropopause divided by the height. The reason for this temperature difference is that most absorption of the sun's energy occurs at the ground which then heats the lower levels of the atmosphere, and the radiation of heat occurs at the top of the atmosphere cooling the earth, this process maintaining the overall heat balance of the earth. As parcels of air in the atmosphere rise and fall, they also undergo changes in temperature for reasons described below. The rate of change of the temperature in the parcel may be less than or more than the ELR. When a parcel of air rises, it expands, because the pressure is lower at higher altitudes. As the air parcel expands, it pushes on the air around it, doing work; but generally it does not gain heat in exchange from its environment, because its thermal conductivity is low (such a process is called adiabatic). Since the parcel does work and gains no heat, it loses energy, and so its temperature decreases. (The reverse, of course, will be true for a sinking parcel of air.). Measuring the temperature change with height through the troposphere and the stratosphere identifies the location of the tropopause. In the troposphere, temperature decreases with altitude. In the stratosphere, however, the temperature remains constant for a while and then increases with altitude. The region of the atmosphere where the lapse rate changes from positive (in the troposphere) to negative (in the stratosphere), is defined as the tropopause. Thus, the tropopause is an inversion layer, and there is little mixing between the two layers of the atmosphere. |
Other Layers |
Within the five principal layers that are largely determined by temperature,
several secondary layers may be distinguished by other properties: The ozone layer is contained within the stratosphere. In this layer ozone concentrations are about 2 to 8 parts per million, which is much higher than in the lower atmosphere but still very small compared to the main components of the atmosphere. It is mainly located in the lower portion of the stratosphere from about 15–35 kms, though the thickness varies seasonally and geographically. About 90% of the ozone in Earth's atmosphere is contained in the stratosphere. The ionosphere is a region of the atmosphere that is ionized by solar radiation. It is responsible for auroras. During daytime hours, it stretches from 50 to 1,000 kms and includes the mesosphere, thermosphere, and parts of the exosphere. However, ionization in the mesosphere largely ceases during the night, so auroras are normally seen only in the thermosphere and lower exosphere. The ionosphere forms the inner edge of the magnetosphere. It has practical importance because it influences, for example, radio propagation on Earth. The homosphere and heterosphere are defined by whether the atmospheric gases are well mixed. The surface-based homosphere includes the troposphere, stratosphere, mesosphere, and the lowest part of the thermosphere, where the chemical composition of the atmosphere does not depend on molecular weight because the gases are mixed by turbulence. This relatively homogeneous layer ends at the turbopause found at about 100 kms, which places it about 20 kms above the mesopause. Above this altitude lies the heterosphere, which includes the exosphere and most of the thermosphere. Here, the chemical composition varies with altitude. This is because the distance that particles can move without colliding with one another is large compared with the size of motions that cause mixing. This allows the gases to stratify by molecular weight, with the heavier ones, such as oxygen and nitrogen, present only near the bottom of the heterosphere. The upper part of the heterosphere is composed almost completely of hydrogen, the lightest element. The planetary boundary layer is the part of the troposphere that is closest to Earth's surface and is directly affected by it, mainly through turbulent diffusion. During the day the planetary boundary layer usually is well-mixed, whereas at night it becomes stably stratified with weak or intermittent mixing. The depth of the planetary boundary layer ranges from as little as about 100 metres on clear, calm nights to 3000 metres or more during the afternoon in dry regions. |
3. Weather | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Another challenge of travelling outdoors is surviving the elements.
Only extreme temperatures and heavy precipitation need
produce game mechanic effects. Precipitation most often causes problems with
visibility. Extreme temperatures may cause minor damage to
the characters.
Weather is the state of the atmosphere as measured on a scale of hot or cold, wet or dry, calm or storm, clear or cloudy. Most weather phenomena occur in the troposphere, just below the stratosphere. Weather refers to day-to-day temperature and precipitation activity whereas climate is the term for the average atmospheric conditions over longer periods of time. Weather occurs due to density (temperature and moisture) differences between one place and another. These differences can occur due to the sun angle at any particular spot which varies by latitude from the tropics. The strong temperature contrast between polar and tropical air gives rise to the jet stream. Weather systems in the mid-latitudes such as extratropical cyclones are caused by instabilities of the jet stream flow. Because the Earth's axis is tilted relative to its orbital plane sunlight is incident at different angles at different times of the year. On Earth's surface temperatures usually range 40 °C (100 °F to −40 °F) annually. Surface temperature differences in turn cause pressure differences. Higher altitudes are cooler than lower altitudes due to differences in compressional heating. The atmosphere is a chaotic system, so small changes to one part of the system can grow to have large effects on the system as a whole. There are several good indicators of climatic changes. Birds and insects fly lower to the ground than normal in heavy, moisture-laden air. Such flight indicates that rain is likely. Most insect activity increases before a storm, but bee activity increases before fair weather. Clouds come in a variety of shapes and patterns. A general knowledge of clouds and the atmospheric conditions they indicate can help you predict the weather. Slow moving or imperceptible winds and heavy, humid air often indicate a low-pressure front. Such a front promises bad weather that will probably linger for several days. You can smell and hear this front. The sluggish, humid air makes wilderness odours more pronounced than during high-pressure conditions. In addition, sounds are sharper and carry farther in low-pressure than high-pressure conditions. Smoke rising in a thin vertical column indicates fair weather. Low rising or flattened out smoke indicates stormy weather. You can determine wind direction by dropping a few leaves or grass or by watching the treetops. Once you determine the wind direction, you can predict the type of weather that is imminent. Rapidly shifting winds indicate an unsettled atmosphere and a likely change in the weather.
Rain is liquid precipitation as opposed to non-liquid kinds of precipitation such as snow, hail and sleet. Rain requires the presence of a thick layer of the atmosphere to have temperatures above the melting point of water near and above the Earth's surface. On Earth it is the condensation of atmospheric water vapour into drops of water heavy enough to fall often making it to the surface. Moisture moving along three-dimensional zones of temperature and moisture contrasts known as weather fronts is the major method of rain production. If enough moisture and upward motion is present, precipitation falls from convective clouds (those with strong upward vertical motion) such as cumulonimbus (thunderstorms) which can organize into narrow rainbands. In mountainous areas heavy precipitation is possible where upslope flow is maximized within windward sides of the terrain at elevation which forces moist air to condense and fall out as rainfall along the sides of mountains. On the leeward side of mountains desert climates can exist due to the dry air caused by downslope flow which causes heating and drying of the air mass. The movement of the monsoon trough or intertropical convergence zone brings rainy seasons to savannah climes. Rain is the primary source of freshwater for most areas of the world providing suitable conditions for diverse ecosystems.
A character caught out in the open during a hailstorm may suffer damage from
being pelted by the rocklike clumps of ice, but a well-prepared or
well-armoured character can often avoid any difficulties. A character who is
wearing splint A
lightning storm presents no special hazard to characters who take simple
precautions. However, the word “simple” in this context is an expression of
complexity and not necessarily a measure of difficulty. For instance, it may
not be at all easy for a character to find somewhere to hole up during a
lightning storm if he’s in the middle of a flat, featureless plain that
extends for hundreds of metres, or kilometres, in every direction.
The most important precaution to take against being struck by
lightning in the outdoors is to get rid of, and get away from, any
metal armour, weapons, and equipment. If time permits, it is a
good idea to scatter individual pieces of metal (the parts of a suit
of armour, for instance) over an area at least several yards in diametre
to minimize the possibility of lightning hitting the armour and
gear. Heaping everything up in a pile for easier access later is
asking for trouble, especially if the top of the pile is higher than
any surrounding terrain.
Second, if solid cover is not available, get as low as possible,
either by dropping flat on the ground or lying in a ditch or depression.
Lightning is not immediately absorbed into the ground after
it hits; the electrical force may travel some distance (up to several
hundred metres, if the stroke is very powerful) along the ground
before dissipating, and along its route it will seek out gullies, ruts,
and other such low spots. Thus, someone lying in a ditch is not
entirely safe, but this course of action is still better than presenting Standing beneath a thick cover of trees of equal height is perhaps the best precaution one can take against lightning in the outdoors when no better cover is available. Of course, if an enclosed structure is within running distance, that is the place to head for. If lightning hits the structure, the electrical charge will ground itself through the roof and walls. A structure with an earthen floor is the safest of all, since the ground provides additional insulation against any electricity that may leak through the structure. The chance of a character being struck by lightning is a very small one, even considering the possibility of normal foolish behaviour, such as standing out in the open while wearing a suit of plate mail. In contrast, abnormal foolish behaviour is rushing to the only tall tree in sight, climbing to the top, and thrusting your sword toward the heavens. The suggestions that follow do not take abnormal behaviour into account; the Dungeon Master is free to arbitrate such occurrences, and it is strongly recommended that if a character voluntarily and knowingly engages in such behaviour, he be given exactly what he appears to want the jolt to end all jolts. |
4. Altitude Sickness |
To people unfamiliar with altitude
and its effects on the human body a trip from sea level to 3048 metres
(10,000 feet) may seem like no big deal. Many people can make this change
without feeling ill effects or may have only minor symptoms. However
others acclimatize more slowly and may become extremely ill. This may include:
headaches, nausea, loss of appetite, heavy fatigue and vomiting. None are life
threatening, neither are they serious. However the person experiencing
them is probably not having a good time. Moreover the patient must be
monitored closely to insure that dehydration does not develop. In any case, the first rule is: don't go
any higher until the symptoms reduce. This is followed closely by the
second rule: if the symptoms continue to get worse or don't improve
within 48 hours, go down. More severe forms are High Altitude
Pulmonary Edema (characterized
by the following: loss of muscle control resulting in difficulty
maintaining balance, coughing, crackling or gurgling sounds while
breathing, difficulty breathing and cyanosis; leading to respiratory and
cardiac arrest) and High Altitude Cerebral Edema
(characterized by the following: severe
headache, ataxia, hallucinations and seizures; leading to
unconsciousness and death. If someone experiences signs and symptoms of
either of these, they must be taken to a lower elevation without delay or
they will die. For every 500 metres above sea level reduce the normal abilities of STR, DEX, CON and MR by 1. Over 1000 metres and the negative effects of cold must also be added. |
Hypothermia |
Hypothermia is the lowering of the
body temperature at a rate faster than the body can produce heat. Causes
of hypothermia may be general exposure or the sudden wetting of the body
by falling into a lake or spraying with fuel or other liquids. The initial symptom is shivering. This
shivering may progress to the point that it is uncontrollable and
interferes with an individual's ability to care for himself. This begins
when the body's core (rectal) temperature falls to about 35.5C.
When the core temperature reaches 32C, sluggish
thinking, irrational reasoning, and a false feeling of warmth may occur.
Core temperatures of 30C and below result in muscle
rigidity, unconsciousness, and barely detectable signs of life. If the
victim's core temperature falls below 25C, death is almost
certain. To treat hypothermia, rewarm the entire body.
If there are means available, rewarm the person by first immersing the
trunk area only in warm water of 37.7 to 43.3C.
Rewarming the total body in a warm water bath should be done only in a hospital environment because of the increased risk of cardiac arrest and rewarming shock. One of the quickest ways to get heat to the inner core is to give warm water enemas. Such an action, however, may not be possible in a survival situation. Another method is to wrap the victim in a warmed sleeping bag with another person who is already warm; both should be naked. The individual placed in the sleeping bag with victim could also become a hypothermia victim if left in the bag too long. If the person is conscious, give him hot, sweetened fluids. One of the best sources of calories is honey or dextrose; if unavailable, use sugar, cocoa, or a similar soluble sweetener. Do not force an unconscious person to drink. There are two dangers in treating hypothermia; rewarming too rapidly and after drop. Rewarming too rapidly can cause the victim to have circulatory problems, resulting in heart failure. After drop is the sharp body core temperature drop that occurs when taking the victim from the warm water. Its probable muse is the return of previously stagnant limb blood to the core (inner torso) area as recirculation occurs. Concentrating on warming the core area and stimulating peripheral circulation will lessen the effects of after drop. Immersing the torso in a warm bath, if possible, is the best treatment. |
Frostbite |
Exposure to severe
cold can seriously injure characters. If a character spends time exposed to
the cold without adequate protection (warm clothing or some kind of magic),
he runs the risk of frostbite. For every half hour of exposure, the
character suffers 1 point of damage to all affected areas. No armour protects against this damage. The
gamemaster may increase the damage for exceptionally harsh conditions
such as snowstorms or being buried beneath an avalanche. If the character
remains in the cold long enough, he will eventually fall unconscious and
freeze to death.
When a character susceptible to frostbite suffers cold damage,
the first points of that damage are applied to any vulnerable extremities
for the purpose of determining whether frostbite occurs.
If more than one body part is vulnerable and the damage cannot
be distributed evenly among the parts, apply the “leftover” damage
to the body part(s) named first, making the distribution as even as possible.
Frostbitten ears will cause discomfort and distraction; the victim takes a - 1
penalty on all initiative rolls, and any opponent’s chance to surprise him is
increased by 1 in 6. Severely frostbitten ears are numb; the victim suffers no
noticeable discomfort, and the penalties given above no longer apply - but if
the victim does not treat or receive treatment for the frostbite within two
turns after it becomes severe, his ear(s) will be permanently damaged.
Frostbitten feet are a great hindrance to mobility and manoeuvrability for a
character on foot; he moves at one-half normal speed and takes a -2
penalty to armour class in any situation that requires dodging ability or abrupt
changes of position (such as defending himself in combat). Severely frostbitten
feet are no longer painful, and because of this the character can once again
move on foot at normal speed, but the penalty to armour class still applies. A
victim who is riding or being carried or is otherwise elevated so that his feet
are not touching the ground does not suffer either of the above penalties, but
is still in danger of serious injury from the frostbite. If the victim does not
receive treatment for severely frostbitten feet within one turn after the onset
of that condition, his feet will be permanently damaged.
A character with frostbitten hands has a -6 penalty to hit with
any thrown or fired missile weapon, and is -4 to hit with a melee weapon. If his hands become severely frostbitten, the penalty to hit with a melee weapon lessens to -2, but the -6 penalty for missile weapons still applies. |
Other Dangers |
Exposed skin can become sunburned
even when the air temperature is below freezing. The sun's rays reflect at
all angles from snow, ice, and water, hitting sensitive areas of skin;
lips, nostrils, and eyelids. Exposure to the sun results in sunburn more
quickly at high altitudes than at low altitudes. Apply sunburn cream or
lip salve to your face when in the sun. The reflection of the sun's
ultraviolet rays off a snow-covered area causes this condition. The
symptoms of snow blindness are a sensation of grit in the eyes, pain in
and over the eyes that increases with eyeball movement, red and teary
eyes, and a headache that intensifies with continued exposure to light.
Prolonged exposure to these rays can result in permanent eye damage.
A human needs to drink at least one quart of water each day, assuming he doesn’t get involved in any strenuous activity. Others require less or more water, proportionate to their size. For each day that a character does not get sufficient water, he takes a -1 penalty to all STR, DEX and CON tests from dehydration (no armour provides protection). Additionally, he receives a penalty to his recovery equal to the number of days he has gone without adequate water. This damage may be added to any damage inflicted by heat exposure. If a character becomes exhausted when the effective
temperature for that character is high enough to require a Clothing that becomes water-soaked will not be damaged as
such, but if it is porous and becomes waterlogged by prolonged
exposure to moisture it will lose some of its insulating quality until
it is taken off and dried out. The wetness and loss of insulating
ability may result in an alteration of the personal temperature for
the character wearing the clothes: Someone decked out in wet
clothing when the environment is at an effective temperature of |
5. Tornadoes | |||
A tornado is a
vortex of air rising into a cloud. In their early and mature stages all
thunderstorms are characterized by rising air called updrafts. These
updrafts supply the warm, humid air that fuels thunderstorms. But in some
cases the column of rising air becomes a vortex, a funnel cloud or tornado.
In a few cases the vortex becomes a strong tornado with wind whirling around
at speeds close to 480kph. Often a tornado is located on the edge of the
updraft, next to air that's coming down from the thunderstorm with falling
rain or hail. This is why a burst of heavy rain or hail sometimes announces
a tornado's arrival.
Air rising from the ground in the tornado vortex creates low air pressure near the ground which air rushes inward to fill. Such inflow winds can be damaging. In other words a house or auto doesn't have to be hit directly by the tornado to be damaged. The centre of the tornado's vortex is a low-pressure area. As air rushes into the vortex its pressure lowers, which cools the air. Cooling condenses water vapour in the air into the tornado's familiar funnel-shaped cloud. As the swirling winds pick up dust, dirt, and debris from the ground, the funnel turns even darker. Twisters that pick up little dirt can retain their white, cloud coloration. Some tornadoes have taken on a red hue by picking up red dirt. Although the air is rising in a tornado the funnel itself grows from the cloud toward the ground as the tornado is forming. The term funnel cloud' refers to a tornado-like vortex that doesn't reach the ground. When a funnel cloud touches the ground, it becomes a tornado. Often, however, apparent funnel clouds are already tornadoes. But the part nearest the ground is still invisible because cloud hasn't formed there and little dirt is being picked up. The lesson: Don't think you're safe near or under a funnel cloud. Experts once thought tornado winds exceeded 800kph. But research in recent years including detailed analysis of movies and video tapes shows that winds rarely exceed 400kph and most tornadoes have winds of less than 112 mph. Tornadoes are also relatively small. An average tornado will be 400 to 150mtrs wide and travel 6 to 8 kilometres on the ground lasting only a few minutes. A mile wide tornado is an extremely large one and tornadoes this big are rare. Many tornadoes are small, less than 30 metres wide, and last only a few minutes. A few monster tornadoes are a mile or more wide and can last for an hour or more. As the parent thunderstorm travels along tornadoes can come down from the cloud, run along the ground and lift back up to be followed by other tornadoes. Generally tornadoes move along the ground at around 32 to 76kph but some race along faster than 112kph. Often the most destructive tornadoes have smaller vortices, known as suction vortices rotating around the main vortex. These show up in some photos and leave distinctive, looped patterns in fields of corn or other crops knocked over by the winds. |
|||
Wind Damage Scale | |||
Forecasters and researchers use a wind damage scale created by T. Theodore Fujita to classify tornadoes and sometimes the damage done by other wind storms. The F for Fujita scale uses numbers from 0 through 5. The ratings are based on the amount and type of wind damage. The scale had been calculated through F-12, which is Mach 1 the speed of sound (750 mph), but tornado wind speeds are not expected to reach these speeds. F-0 and F-1 tornadoes are considered weak, F-2 and F-3 are strong and F-4 and F-5 are violent. F-6 or higher rated tornadoes aren't thought to exist. The damage they would do would be inconceivable. The ratings are: | |||
F-0 | Gale tornado (64-116kph): Some damage to chimneys; breaks branches off trees; pushes over shallow-rooted trees; damages sign boards. | ||
F-1 | Moderate tornado (117 to 180kph): The lower limit is the beginning of hurricane wind speed; peels surface off roofs; mobile homes pushed off foundations or overturned; moving autos pushed off the roads; attached garages may be destroyed. | ||
F-2 | Significant tornado (181 to 251kph): Considerable damage. Roofs torn off frame houses; mobile homes demolished; boxcars pushed over; large trees snapped or uprooted; light object missiles generated. | ||
F-3 | Severe tornado (252 to 330kph): Roof and some walls torn off well-constructed houses; trains overturned; most trees in forest uprooted. | ||
F-4 | Devastating tornado (331 to 416kph): Well-constructed houses levelled; structures with weak foundations blown off some distance; cars thrown and large missiles generated. | ||
F-5 | Incredible tornado (417-509kph): Strong frame houses lifted off foundations and carried considerable distances to disintegrate; automobile sized missiles fly through the air in excess of 100 metres; trees debarked; steel-reinforced concrete structures badly damaged. | ||
F-6 | Inconceivable tornado (510-606kph): These winds are very unlikely. The small area of damage they might produce would probably not be recognizable along with the mess produced by F-4 and F-5 wind that would surround the F-6 winds. Missiles, such as cars and refrigerators would do serious secondary damage that could not be directly identified as F-6 damage. If this level is ever achieved, evidence for it might only be found in some manner of ground swirl pattern, for it may never be identifiable through engineering studies. | ||
Further classifying tornadoes by path length, width | |||
The original wind damage scale developed by T. Theodore Fujita, which bares his name, had two additional sections added to further categorize tornadoes by the lengths and widths of their damage paths. Both ratings were the products of researcher Allen Pearson, director of the National Weather Service's National Severe Storms Forecast Centre, in 1971. The P - for Pearson scale was accepted for use by NSSFC in 1973, creating the Fujita-Pearson Scale, or FPP Scale, which is still mentioned in some literature. In practice, the Pearson Scales are not as widely used today; | |||
Scale | Fujita Wind Speed | Pearson Path Length | Pearson Path Width |
- | 0-64 kph | less than 0.5 kms | less than 5.4 metres |
0 | 65-115 kph | 0.6-1.5 kms | 5.5-6.5 metres |
1 | 116-179 kph | 1.6-4.9 kms | 7-49.5 metres |
2 | 180-251 kph | 5-16 kms | 50-67.5 metres |
3 | 252-329 kph | 17-50 kms | 68-509.5 metres |
4 | 330-416 kph | 51-159 kms | 510 metres -1 km |
5 | 417-508 kph | 160-504 kms | 1.6-5 kms |
Waterspouts: Tornadoes over water | |||
Typically waterspouts are described as tornadoes over water. But scientific work over the last 30 or so years has led to a more complicated picture. Waterspouts and all the different kinds of tornadoes have a similar basic structure with air moving upward. At the ground or ocean surface, winds are rushing faster and faster as they swirl into the vortex and then upward. Often with both tornadoes and waterspouts, the vortex is seen coming down from the cloud but not obviously touching the ground or ocean. Such vortices that don't seem to touch the ground are called funnels or funnel clouds. We begin to see the vortex when its lower air pressure cools the air enough to condense water vapour in the air into tiny water droplets. Cool air brought down by the rain cuts off the supply of warm, humid air that's feeding into the waterspout to keep it going. | |||
Other types | |||
Dust
devils are swirls that go upward to fizzle out in clear air; they aren't
attached to clouds. While they are most commonly found on deserts and form
when air at the ground becomes much hotter than the air above. The lighter,
hot air begins rising and takes on a whirling motion that carries dust and
sand upward. Top wind speeds seem to be around 96kph.
Hurricanes - called typhoons or tropical cyclones in some parts of the world - form over all of the world's tropical oceans except the South Atlantic and the South-eastern Pacific. In all parts of the world, a tropical storm has 63 kph to 117 kph winds. When the winds reach at least 118kph the storm becomes a hurricane, typhoon or tropical cyclone, depending on its location. Technically, a cyclone is any kind of circular wind storm. But now, it is only used to describe a strong tropical storm found off of the coast of India. Hurricanes and Typhoons are the same thing, but in different places. On the coast of Florida it is called hurricane. In the Philipines, it is called typhoon. Hurricanes occur in the Atlantic and typhoons, in the Pacific. Basically, hurricanes and typhoons form over water and are huge, while tornados form over land and are much smaller in size. A tornado is a violent windstorm characterised by a twisting, funnel-shaped cloud. In the United States, twister is used as a a colloquial term for tornado. |
6. Aerial Cities |
Click on the above link for information on the following sky and cloud
cities; Aerie |
7. Aerial Races | |
Aerial races include all species which can fly and inhabit the sky. | |
01-06 | Aarakocra |
07-12 | Atomie |
13-18 | Avariel |
19-24 | Enduk |
25-30 | Fey'ri |
31-36 | Grig |
37-42 | Harpy |
43-48 | Immaculate |
49-54 | Kenku |
55-60 | Nephilim |
61-66 | Pegataur |
67-72 | Pixie |
73-78 | Raptoran |
79-88 | Sky People |
89-94 | Sprite |
95-00 | Swanmay |
8. Aerial Classes | |
Elemental, Air | Reborn as sentient air. |
Elemental, Smoke | A modern day variation of the air elemental. |
Sky Knight | Protecting the skies from dangerous invaders |
9. Aerial Bestiary | ||||
A guide to real and mythological animals which inhabit the sky. | ||||
Type (real) | Size (metres) | HPs | AC | Speed (MR) |
Bat | 1 | 2 | 8 | 96 |
Chicken, Turkey | 1/2 | 5 | 9 | 14 |
Condor | 1 | 27 | 7 | 88 |
Cockatoo, Parrot | 1/2 | 3 | 9 | 24 |
Dove, Pigeon | 1/2 | 2 | 8 | 80 |
Duck, Goose, Ibis | 1/2 | 6 | 9 | 70 |
Eagle | 1 | 11 | 6 | 32 |
Falcon | 1 | 9 | 5 | 90 |
Hawk | 1 | 8 | 6 | 192 |
Owl | 1 | 8 | 5 | 64 |
Raven | 1/2 | 2 | 7 | 31 |
Swan | 1 | 10 | 7 | 135 |
Vulture | 1 | 9 | 6 | 35 |
Type (fantasy) | Size (metres) | HPs | AC | Speed (MR) |
Amphisbaena | 1 | 48 | 3 | 100 |
Chimera | 3 | 72 | 6 | 100 |
Dinosaur Dimorphodon | 1 | 18 | 6 | 30kph |
Dinosaur Pterandon | 8 | 80 | 7 | 350kph |
Dinosaur Quetzalcoatlus | 12 | 121 | 5 | 50kph |
Dinosaur Rhamphorhynchus | 1 | 8 | 7 | 30kph |
Dinosaur Pterodactyl | 8 | 80 | 7 | 350 |
Dragon Amethyst | 26-54 | 350-600 | 1 | 330 |
Dragon Black | 26-54 | 350-600 | 1 | 330 |
Dragon Blue | 26-54 | 350-600 | 1 | 330 |
Dragon Brass | 26-54 | 350-600 | 1 | 330 |
Dragon Bronze | 26-54 | 350-600 | 1 | 330 |
Dragon Copper | 26-54 | 350-600 | 1 | 330 |
Dragon Crystal | 26-54 | 350-600 | 1 | 330 |
Dragon Dragonet | 26-54 | 350-600 | 1 | 330 |
Dragon Emerald | 26-54 | 350-600 | 1 | 330 |
Dragon Gold | 26-54 | 350-600 | 1 | 330 |
Dragon Green | 26-54 | 350-600 | 1 | 330 |
Dragon Red | 26-54 | 350-600 | 1 | 330 |
Dragon Sapphire | 26-54 | 350-600 | 1 | 330 |
Dragon Silver | 26-54 | 350-600 | 1 | 330 |
Dragon Topaz | 26-54 | 350-600 | 1 | 330 |
Dragon White | 26-54 | 350-600 | 1 | 330 |
Elemental Air | 1-30 | 120 | 2 | 90 |
Elemental Smog | 1-30 | 120 | 2 | 90 |
Giant Bat | 5 | 48 | 7 | 100 |
Giant Bee | 1 | 25 | 5 | 30 |
Giant Dragonfly | 1 | 21 | 3 | 50 |
Giant Eagle | 6 | 32 | 7 | 340 |
Giant Moth | 1 | 41 | 1 | 40 |
Giant Owl | 6 | 32 | 6 | 150 |
Giant Vulture | 2 | 18 | 7 | 200 |
Giant Wasp | 1 | 32 | 4 | 30 |
Gremlin | 1 | 32 | 4 | 40 |
Griffin | 3 | 56 | 3 | 350 |
Hippogriff | 3 | 27 | 5 | 370 |
Manticore | 5 | 30 | 4 | 250 |
Pegasus | 2 | 32 | 6 | 350 |
Roc | 4 | 144 | 4 | 60 |
Sphinx | 3 | 80 | 0 | 70 |
Wyvern | 11 | 64 | 3 | 250 |
10. Flight | ||||||||||||||||||||||||||||||||||||||||
Basic flight consists
of turning, level flight, climbing, diving, and (usually) maintaining a
minimum forward speed. Because a flying creature's ability to change
direction is limited, and because flight takes place in three dimensions, you
must know a creature's manoeuvrability rating, forward speed, direction of
travel, and altitude to handle flaying correctly. Forward Speed: Forward speed is the number of squares a flying creature
traverses during the course of its movement for the round. Some flight
manoeuvres
(such as turning in place) use up flying movement but don't contribute to
forward speed. Many flyers must maintain a minimum forward speed each round. If
they fail to do so, they stall (see Minimum Forward Speed). Minimum forward Speed: If a flying creature fails to maintain its minimum forward
speed, it must land at the end of its movement. If it is too high above the
ground to land, it stalls.
A creature in a stall falls straight down, descending 45 metres in the first
round of falling. If this distance brings it to the ground, it takes falling
damage. If the fall doesn't bring the creature to the ground, it must spend its
next turn recovering from the stall. It must succeed on a DEX save to
recover. Otherwise it falls another 90 metres. If it hits the ground, it takes
falling damage. Otherwise, it has another chance to recover on its next turn.
Keep track of minimum forward speed by the turn, not by the move.
As noted earlier, only moving from square to square counts toward minimum
forward speed. Movement spent turning in place doesn't count.
In some cases, a creature may spend part of its turn on the ground (or perhaps
on a flying mount or flying device). If the creature uses a move or standard
action on the ground, it need maintain only half its minimum forward speed once
it takes to the air. If a flying creature moves along the ground and then takes
to the air as part of the same move action, it must maintain all of its minimum
forward speed to avoid stalling. Turn in Place: A creature can use some of its speed to turn in place. (This represents the creature slowing down and banking hard to make a tight turn.) The extra movement spent turning does not count toward minimum forward speed; a creature that turns too sharply at low speeds stalls. Maximum Turn: This is how much the creature can turn in any one space. No matter
how much movement the creature spends on turning, it can't change direction more
than this in a single square. Down Angle: The down angle is the maximum angle at which the creature can dive
through the air. A creature with a down angle of 45º must move ahead at least
1.5 metres for every 1.5 metres it climbs. Between Down and Up: An average, poor, or clumsy flier must fly level for a
minimum distance after descending and before climbing (but it can turn). Any
flier can begin descending after a climb without an intervening distance of
level flight. Stalling and Freefalling: Stalling represents the failure of a flying creature's wings (or other motive agent) to keep the creature aloft. A stalling creature falls, but it wings provide considerable drag and tend to slow the creature's fall. As noted earlier, a creature falls 45 metres during the first round spent stalling, and it falls 90 metres each round thereafter. Wingless flyers that stall still have some residual lift and fall more slowly than non-flyers. A flying creature that cannot maintain its minimum forward speed because it has been rendered unconscious, has become paralyzed, has become magically held, or becomes unable to move for some other reason stalls at the beginning of its first turn after the debilitating effect occurs. A stalling creature can take no actions, except to recover from the stall. It loses its Dexterity bonus to Armour Class (if any) while stalling. A stalling creature falls more or less straight down, but it also tumbles and spins erratically. Melee or ranged attacks made against a stalling creature have a 20% miss chance. A nonflyer (or flyer falling through the air) freefalls rather than stalls. A creature in freefall drops 150 metres the first round and 300 metres each round thereafter. While in freefall, a creature can attempt a single action each round. It must make a Dexterity or Strength check to avoid dropping any item it tries to use. Spellcasting is possible, but doing so requires a Concentration check. Deliberately Freefalling: A flying creature can simply stop flying and allow itself to drop like a stone. Exiting a freefall requires a full-round action (during which the creature falls 150 or 300 metres). Fast Freefalls: A creature with a fly speed can propel itself downward as a move action, adding up to twice its flying speed to the distance it freefalls. Catching: As a full-round action, a flyer can catch a freefalling creature or object, or a stalling creature, provided that the falling creature or object is at least one size category smaller than the creature attempting the catch. To make the catch, the creature must make a successful melee touch attack to grab the falling creature or object (a creature can voluntarily forego any Dexterity bonus to AC if desired). If the grab succeeds, the catching creature must make a DEX save to keep flying. If the save fails by 4 or less, the catcher drops the falling creature or object. If the save fails by 5 or more, the catcher drops the falling creature or object and stalls if it has a minimum forward speed. If the catcher does not have a minimum forward speed, it falls D4 x3 metres. Obstacles and Collisions: Because flying creatures cannot always change direction when they wish to, they must take great care to avoid blundering into obstacles or into other creatures. To turn and avoid an obstacle at its own altitude, a flying creature must be able to turn in place. If it cannot turn in place, it needs at least 1.5 metres of space between it and the obstacle if it wishes to turn to avoid a collision (because in an aerial turn you move into the square ahead of you and then turn left or right 45° ). It cannot move diagonally past a corner in the air or on the ground, so any turn you make must carry you past an obstacle's corner before you can fly past it. If turning to avoid an obstacle isn't possible, it may be possible to climb over or dive under the obstacle. A creature with maximum up or down angle of 45° needs at least 1.5 metres of clear space between it and an obstacle for every 1.5 metres it must climb or dive to get over or under the obstacle (you can't move past a corner on a diagonal, even when climbing or diving). A creature with a maximum up or down angle of 60° needs at least 1.5 metres of clear space between it and an obstacle for every 3 metres it must climb or dive to get over or under the obstacle. Flying past another creature works much like flying past an obstacle except that you can move on a diagonal to get past a creature. This makes it slightly easier to pass by without colliding. If you fly into an obstacle and you cannot land there, you must make a DEX save to avoid damage. If you fail the save, you and the object you strike take damage as though an object of your weight fell a distance equal to half your flying speed before you hit. (If it isn't clear what your speed before the collision was, use your flying speed during your previous turn.) Your flying movement stops when you strike, forcing you to stall (even if you don't have a minimum forward speed) and fall straight down. If you're still conscious after the collision, you can make DEX check to catch yourself and keep from falling. You can freely pass through your allies' spaces in the air just as you can on the ground. If you fly into a creature that is not your ally, you effectively attempt to overrun it. You can execute a bull rush against the creature instead, if you wish. An overrun or bull rush normally requires a standard action. If you accidentally enter an enemy's space you must make a DEX save; if you fail, you stall (even if you don't have a minimum forward speed). If you succeed, you can continue with your accidental bull rush or overrun, but you suffer a -4 penalty to all the opposed checks you make to resolve the bull rush or overrun. As with an overrun attack, the creature can decide not to block your movement, though this might cause the creature to stall (see the section on overruns). If so, you simply move through its space (even if you decide to bull rush the creature). You cannot stop in another creature's square, however, and if your speed isn't sufficient to carry you through the other creature's space, you must attempt an overrun or bull rush. If the creature is too small to overrun, you must try to bull rush it instead if you can't pass through its space. If the creature is too big to overrun, you strike it just as if it were an obstacle, and you and the creature take nonlethal damage. Both you and the creature you strike make DEX saves to avoid damage, but the creature you strike gets a +4 bonus for each size category it is bigger than you. You stall just as if you struck an obstacle. The creature you strike stalls if it fails its DEX save. If you are at least three size categories smaller than the creature whose space you are entering (or if you are Tiny, Diminutive, or Fine size) you can enter the creature's space without colliding, bull rushing, or overrunning, but entering the creature's space provokes an attack of opportunity. Likewise, if you are at least three size categories smaller than the creature whose space you are entering, you also can enter the creature's space without colliding, bull rushing, or overrunning, but entering the creature's space provokes an attack of opportunity. Actions while Flying: Most actions work exactly the same way in the air as they do on the ground; exceptions are noted here. A creature with a minimum forward speed usually cannot use full-round actions in the air unless those actions allow it to move forward at least at its minimum speed. Flying spellcasters can cast their spells without too much difficulty; however, aerial spellcasters often encounter some problems other spellcasters do not. The rules for flanking apply in the air. It is possible, however, to flank a flying creature from the top and bottom. Aerial combat takes place in three dimensions, and each flying creature occupies a roughly cubical space and can reach above and below itself. An aerial bull rush requires the attacker to ram a foe, which can prove risky for both the attacker and the defender. Flying creatures can use the charge action. A flying charge must be in straight line and most cover at least 3 metres (2 squares). A flyer can charge while diving, but not while gaining more than 1.5 metres altitude. High Wind Speeds: Flying in high winds adds penalties on your Fly checks as noted below. "Halted" means that creatures of that size or smaller must succeed on a DEX Fly check to move at all so long as the wind persists. "Pushed back" means that creatures of that size or smaller must make a DEX Fly check or be blown back 2D6 × 3 metres and take 2D6 points of nonlethal damage. This check must be made every round the creature remains airborne. A creature that is blown away must still make a DEX Fly check to move due to also being checked.
|
11. Air Combat |
Air to air combat
can be broken down into essentially two elements; combat which occurs
without the opponents seeing each other and the more direct Dogfighting. As explained here each aircraft has; an Armour Class (AC) rating, an Acceleration/Deceleration Factor (A/DF); Hit Points (HPs); a manoeuvre rating (MR); and the vehicle's Speed. Aircraft move just like ground vehicles, but fixed-wing aircraft (airplanes and jets but not helicopters or craft capable of Vertical Take-Off and Landing) can never go below one quarter of their Top Speed while flying or they stall and automatically lose D4 metres of altitude at the end of their movement.
Should an aircraft hit the ground while moving forward,
it suffers damage normally for its current speed (D6 per A pilot can try to save his aircraft—even if it is wrecked—by making a crash landing. This is a Piloting roll at -4. If he makes it, halve the damage for the landing. If the roll is failed, the craft takes damage as usual.
Aerial Initiative Unlike in standard combat, in air combat the direction
in which a flying creature points is often extremely important.
Aerial Manoeuvres: Pop-Up (0): Helicopters, VTOLs, and other aircraft capable of hovering can hide behind cover, rise, attack, and then descend again—usually before the stunned enemy can react. This manoeuvre simply allows the pilot to ascend above an obstacle and then descend again in the same move, so that he’s only vulnerable to opponents with Hold actions. It takes a Piloting roll to ascend and fire in time to descend again. If failed, the craft simply stays at its firing altitude or fails to fire—pilot’s choice. Power Dive (0): A pilot can enter a controlled power dive by making a Piloting roll. If failed, he loses control. If successful, he may descend up to 24 metres per round. Sharp turn (-1): You may use expert handling to make more turns in a round, or sharper turns, than your plane could normally make. Determine how many extra turns you wish to make that round. If you wish to make an especially sharp turn (i.e., make 2-45 degree turns in a space instead of only 1) each additional 45 degree turn in the space counts as an extra turn for this purpose. Thus, a ship that can normally make 2 turns per round that instead wants to make 3 turns all in the same space would count as making 3 extra turns for this purpose (1 extra turn, +2 for making two additional turns in the same space). If this check is made successfully, the plane turns as desired. Climb (0): By turning a ship up, the pilot can ascend quicker than normal, adding the ship’s normally-horizontal movement to the distance climbed. Just as when diving, standing creatures must pass a DEX save or fall prone. Climbing is similar to diving, except only half of the horizontal movement sacrificed is added to the distance climbed. Failing the pilot check causes the ship to stall and go into freefall (described under conditions below). Defensive Piloting (-1): You take evasive action, granting your vehicle an extra +1 dodge bonus to AC. Offensive Piloting (-1): You manoeuvre your vehicle in such a way as to aid your gunners. Any attack roll made by a creature aboard your vehicle against a target not aboard your vehicle gains a +1 bonus to their Thac0 roll. Ram (0): When two planes enter the same space at the same altitude
band, there is a chance they will crash into each other. Other times,
the pilot of a plane may deliberately crash into a building or creature
in an attempt to destroy it. When a plane crashes into another plane,
creature, or object, they are performing a ramming manoeuvre. If both ship
pilots want to ram each other, the ram happens automatically. If both pilots
don’t wish to ram each other, the ram does not happen. When one party wants
to ram and the other doesn’t, the pilot attempting to initiate the ram makes
an attack roll against their intended target.
There are three ways one ship may ram another: Called Shot (-2): When firing weapons at a ship, it is possible to make a Called Shot, firing not just at a location, but at an individual Hardpoint/Deck. This becomes an especially useful tactic when targeting a vehicle’s engine, sails, or attempting to blow a hole in their cargo bay to aid in boarding. Any damage dealt with a called shot is still subtracted from the location’s total HP (up to the total addition that Hardpoint or Deck made to the location’s total HP), but is also tracked separately as well. When a Hardpoint/Deck is reduced to 0 hp, it is destroyed and anything within that Deck or Hardpoint suffers all excess damage. Flat-Hatting (-2): This is a dangerous manoeuvre, but it can save a pilot’s life. Flat-hatting is flying at high speed at barely above ground level. It requires a Piloting roll every round to avoid the various obstacles, including the Earth itself. Unless your opponent is also flat-hatting, you gain a minimum concealment of –2 and other aircraft must make a Notice roll each round to pick out your position. Perch (-1): Most air combat takes place on generally the same level as the pilots jockey so one does not get the height advantage. By using this manoeuvre and getting a raise on an opposed Piloting roll, a pilot can get that height advantage on his opponent. This gives the pilot a +2 bonus to attack rolls. Unlike Tail (below), the pilot must get a raise on his Piloting roll each round to maintain the advantage. Tail (0): The pilot must move into a square adjacent to another plane and then makes an opposed Piloting roll with the other pilot. If the initiating pilot can get a raise, they are considered tailing the other plane. The tailing plane moves with the other plane and gains a +2 bonus to attack rolls. It is impossible for a slower plane to tail a faster plane for more than one round. Shake a Tail (0): A pilot that is being tailed can attempt to lose his pursuer. This is a simple opposed Piloting roll, only the tailing plane gets a +2 bonus. If successful, the plane takes its movement, leaving the tail behind. With a raise, the pilot can choose to reverse positions, and tail his old pursuer. If the tailed plane has a lower stall speed that his pursuer, the pilot gains the difference as a bonus to his Piloting roll. Rolling: Sometimes, when a pilot attempts a sharp turn unsuccessfully, they can cause their plane to roll in the air. When a vehicle begins to roll, every creature aboard must pass a DEX save to secure themselves, or slide off the end of the vehicle, falling to the ground below. If a target is tethered to the vehicle they fall prone if they fail this check, but otherwise do not slide off. When a vehicle begins to roll, the pilot has one round to attempt to correct the vehicle with a piloting check. If they fail (or if they are unable to make this check), then the next round the vehicle turns completely upside down; all targets still aboard the vehicle must pass another DEX save to hold on tightly, or be dropped to the ground below. At this point, the pilot must pass a piloting check to correct the vehicle. If they fail or are unable to make this check, the vehicle stalls.
Uncontrolled
Aircraft Random Damage Table
Emergency Landings
|
12. Air Vehicles | ||||||
Air vehicles are
crafts which are able to fly by being supported by the air, or in general,
the atmosphere of a planet. An aircraft counters the force of gravity by
using either static lift or by using the dynamic lift of an airfoil, or in a
few cases the downward thrust from jet engines. Balloons and Airships use
buoyancy to float in the air in much the same way that ships float on the
water. Airplanes or aeroplanes are technically called fixed-wing aircraft
and may either use propellers or jets to fly. Helicopters, also known as
rotorcraft or rotary-wing aircraft use a spinning rotor with aerofoil
section blades (a rotary wing) to provide lift.
For more information on Skyships and how they function, see here. |
||||||
Airships | ||||||
Type | Size (metres) | HPs | AC | A/DF | MR | Speed |
Airship, Large | 24 | 150 | 5 | 1 | 3 | 130 |
Airship, Medium | 12 | 100 | 5 | 1 | 3 | 110 |
Airship, Small | 6 | 50 | 5 | 1 | 3 | 90 |
Balloon | 30 | 30 (basket) | 6 | 1 | 3 | 35 |
Glider | 9 | 50 | 6 | 0 | 2 | 0 |
Helicopters | ||||||
Type | Size (metres) | HPs | AC | A/DF | MR | Speed |
Autogyro | 4.5 | 50 | 6 | 1 | 2 | 100 |
Cargo | 15 | 500 | 2 | 2 | 3 | 150 |
Corporate, 6 seater | 15 | 300 | 3 | 2 | 3 | 210 |
Small, 2 seater | 11 | 200 | 4 | 2 | 3 | 285 |
Planes (Prop) | ||||||
Type | Size (metres) | HPs | AC | A/DF | MR | Speed |
Four Prop Cargo | 50 | 500 | 5 | 4 | 1 | 500 |
Sea Plane | 19 | 350 | 5 | 2 | 2 | 390 |
Single Prop Plane | 12 | 300 | 5 | 2 | 2 | 280 |
Twin Prop Cessna | 12 | 300 | 5 | 3 | 2 | 320 |
Twin Prop Transport | 23 | 500 | 5 | 4 | 1 | 450 |
Planes (Jet) | ||||||
Type | Size (metres) | HPs | AC | A/DF | MR | Speed |
Lear Jet | 13 | 600 | 4 | 5 | 2 | 877 |
Passenger Jet, Jumbo | 70 | 1000 | 4 | 7 | 1 | 920 |
Passenger Jet, Medium | 50 | 850 | 4 | 6 | 1 | 811 |
Passenger Jet, Small | 31 | 600 | 4 | 5 | 2 | 547 |
Scramjet | 40 | 1000 | 4 | 8 | 2 | M12 |
Space Shuttle | 37 | 2000 | 2 | 7 | 1 | M20 |
Planes (Military) | ||||||
Type | Size (metres) | HPs | AC | A/DF | MR | Speed |
Combat Helicopter | 18 | 400 | 2 | 3 | 3 | 340 |
Four Prop Bomber Plane | 43 | 600 | 4 | 4 | 1 | 500 |
Jet Fighter | 19 | 800 | 2 | 8 | 2 | M2 |
Twin Jet Bomber | 21 | 1000 | 2 | 7 | 1 | M1 |
Ancient Fantasy | ||||||
Type | Size (metres) | HPs | AC | A/DF | MR | Speed |
Flying Broom | 1 | 10 | 10 | 3 | 5 | 160 |
Flying Carpet | 1-2 | 10 | 10 | 2 | 2 | 100 |
Skyship, Flying Fortress | 200 | 1500 | 0 | 1 | 1 | 75 |
Skyship, Skimmer | 5 | 45 | 5 | 3 | 4 | 300 |
Skyship, Transport Civilian Large | 40 | 600 | 4 | 1 | 1 | 100 |
Skyship, Transport Civilian Standard | 20 | 450 | 4 | 1 | 1 | 100 |
Skyship, Transport, Military | 20 | 450 | 4 | 1 | 2 | 250 |
Skyship, Warship, Escort | 35 | 550 | 3 | 1 | 1 | 350 |
Skyship, Warship, Destroyer | 55 | 750 | 2 | 1 | 1 | 250 |
Skyship, Warship, Dreadnaught | 80 | 950 | 1 | 1 | 1 | 150 |
13. Organizations |
Aerotech The Skyreavers |
14. The Celestialscape |
Beyond the physical dimension of earth exists other surrounding dimensions which have an influence on it. One of those is the Elementalverse, an offshoot of Eighth Space. Within this dimension is the subdimension of Air or Celestialscape, an infinite universe consisting of differing combined gases with varying visibility. It cannot be visited by conventional means requiring either the use of magic or dimension shifting powers or technology. |
15. Air Elemental Magic |
Air is a wild and mercurial element, flowing like quicksilver in a dance that many perceive, but few understand. The power of air is that of motion, from the tiniest manipulation to the greatest translocation. Air embodies all manner of weather, from the gentle breeze to the raging storm. In addition, Air is the medium of voice and speech, and the wind may carry a mage's words far from his lips to where they are most needed. Air is lively and unpredictable, as quick to change as the weather. |
16. Aerial Powers |
Aerialkinesis |
Beyond Heroes | Index |