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temperature defn
Temperature is a measure of heat. It is measured by a thermometer in degrees Celsius (Centigrade) or Fahrenheit.
Celsius Scale
: 0°C = melting point of ice; 100°C = boiling point of pure water at normal pressure. Used
internationally, in aviation and science
Fahrenheit Scale:
32°F = melting point; 212°F = boiling point. Used in a few English-speaking countries
Absolute Zero:
The minimum temperature attainable for all substances. Value = −273.15°C = 0K.
temp conversion formulae 3
F = (9C/5) + 32
C = 5/9 × (F − 32)
K = C + 273
F = C what value
Special value — same on both scales:
–40°C = –40°F
instruments for measuring temp
Dry Bulb Thermometer
wet bulb thermometer
Maximum thermometer
minimum thermometer
thermograph
temp vs heat
Temperature measures how hot or cold something is. Heat is the energy that flows from one thing to another because of a temperature difference.
Temperature
It tells you the average kinetic energy of the molecules: how fast, on average, they are moving.
It does not depend on how much substance you have.
It is measured in °C, °F or K, with a thermometer.
2. Heat
It is energy in transit. Heat always flows from the hotter body to the colder one.
It depends on the amount of substance as well as its temperature.
It is measured in joules (or calories
3. Example: the bath and the cup
A cup of boiling water at 100°C and a bath of water at 40°C.
The cup has the higher temperature.
The bath holds far more heat, because it has many more molecules, each carrying energy.
The bath could warm a whole room. The cup could barely warm a bowl.
dry bulb thermometer
Standard mercury thermometer measuring ambient air
temperature.
wet bulb thermometer
Standard mercury thermometer measuring ambient air
temperature.
Maximum Thermnometer
Like a Doctor's thermometer — records maximum
temperature attained. Has a constriction to prevent mercury
from falling back.
Minimum
Thermometer
Uses Alcohol instead of mercury (alcohol doesn't freeze). Has
a dumbbell-shaped iron index. When temperature falls,
alcohol drags index back; index stays at minimum psn
Thermograph
Gives a continuous record of temperature. Uses bimetallic
strips in Upper Air measurements
stevenson screen
surface temp is recorded at a height of 4ft (1.25m) above ground in shade , inside a stevenson screen - a louvred whitepainted wooden box that protects instruments from radiation while allowing free air circulation
types of temp
surface temp
ambient temp
virtual temp
surface temp
Temperature recorded at 4 ft (1.25 m) above ground in shade (inside Stevenson's Screen).
ambient temp
temp of surroundings
Virtual temperature
In a thermodynamic process, the temperature at which dry air parcel would have the same
pressure and density as a moist parcel of air. VT allows use of dry air equation of state for moist
air also. VT is always higher than actual temperature.
heat & temp defn
Heat is energy transferred because of a temperature difference. Internal energy is energy stored in the substance.
temp is the avg KE of all molecules and atoms of substance
**Heat is energy transferred because of a temperature difference; internal energy is energy stored in a substance. Temperature alone does not tell us the total internal energy of a quantity of material. Keep these three ideas separate when explaining atmospheric heating.
Specific Heat
Specific Heat is the heat required to raise the temperature of unit mass of a substance by 1°C
land vs sea specific heat
Aviation Implication: Because land has a much lower specific heat than water ( 0.2 vs 1.0 ), land
heats and cools much faster than the sea. This drives sea breezes, land breezes, and monsoon circulation.
Latent heat defn
Latent Heat is defined as the "amount of heat absorbed or released during change of phase from/to
solid/liquid/vapour".
• Absorbed during: solid → liquid, liquid → vapour
• Released during: vapour → liquid (condensation), liquid → solid (freezing)
Latent heat is "hidden" — it does not change temp , only phase
evaporation vs condensation
Key Point: Evaporation = heat absorbed from surroundings = cooling effect. Condensation = heat
released = warming effect. This is why clouds release heat (Latent Heat Release = LHR) — critical for
thunderstorm development!
Methods for Heat Transfer
Heat is transferred by Conduction, Convection, Radiation, and other methods. In the atmosphere,
Radiation plays the most significant role
conduction
Physical transfer by molecular contact
Important very close to the ground. Heats
lowest air layer in contact with warm surface.
Convection
Convection is the transfer of heat and thermal energy through the movement of a fluid (a liquid or gas)
Free Convection = intense solar heating.
Forced Convection = topography. Air lifts to
higher levels and transfers heat.
Radiaation
Every body radiates at its temperature
Medium neither affected nor required. Solar
radiation heats earth directly.
Advection
Horizontal motion of the atmosphere
transferring heat.
Transfers heat horizontally by winds (e.g.,
warm/cold advection
Turbulence
Irregular eddy motion of the atmosphere causes redistribution of heat
important in the lowest atmospheric layers
Latent heat release
Latent heat absorbed by evaporation is released by condensation or freezing.
released in atmosphere — major heat
source for cloud systems and thunderstorms.
Insolation
is the total amount of radiation received over a particular area
Insolation depends on the obliquity (angle) of sun's rays:
Maximum when sun is overhead (vertical rays cover less area → more energy per unit area)
Least at sunrise and sunset (oblique rays spread over large area)
Maximum insolation in the Tropics (between Tropic of Cancer and Tropic of Capricorn)
Least at the Poles
Laws of Radiation ; what is Black Body?
Objects emit thermal radiation. An ideal blackbody absorbs all incident radiation; real objects
need not behave as perfect blackbodies.
Stefan boltzmanns law
The total amount of energy radiated by a black body is
proportional to the fourth power of its absolute
temperature.
wiens law
the wavelength of the most intense radiation is inversely proportional to the absolute temperature
plancks law
describes distribution of radiated energy with absolute temp
memory aid stefan and wien ?
Stefan = T to the FOURTH (Total energy)
Wien = Wavelength INVERSELY proportional to T (hot = short wave, cold = long wave)
"Hot Sun = Short Wave; Cold Earth = Long Wave" — this is central to the greenhouse effect!
The temperature of the surface of the sun is about
6000 degree celcius
type of solar radiation
Complete solar radiation (including visible, UV, and IR) is responsible for all the heat the earth receives from
the sun as short wave radiation

terrestrial radiation
The earth radiates at its own temperature and loses heat. These are called Terrestrial Radiation. They are
Long Wave Infra-Red (IR) radiation and are invisible.
The earth receives heat as short-wave radiation from the sun and loses heat as long-wave radiation
Nocturnal Radiation
At night, the short-wave radiation from the sun is absent. Only the earth radiates and loses heat. The
radiation emitted by the earth at night is called Nocturnal Radiation.
nocturnal radiation Aviation Significance:
Nocturnal radiation causes surface cooling at night → ground fog formation,
radiation fog, frost → hazardous for takeoff/landing!
solar radiation absorbed by earth surface
51%
solar rdn absorbed by water vapor , dust , ozone
16%
solar radiation absorbed by clouds
3%
total absorbed solar rdn
70%
solar rdn back scattered by air
6%
reflected back by clouds
20%
reflected back by earths surface
4%
total reflected/backscattered rdn
30%
albedo defn
reflected rdn or incident rdn
The 30% of solar radiation reflected back to space by the earth and clouds is the reflecting power of earth,
called Albedo.
In clear weather, about 5/6 of the solar radiation reaches earth surface → about 1/6 (≈17%) is reflected.
Earth surface reflects about 10% in clear conditions.
Snow surface reflects about 80% of incident energy (very high albedo).
sea vs land diurnal variation of temp
Sea vs Land: The sea surface temperature shows a variation of less than 1°C from day to night. Over
land, diurnal variation may average as much as 20°C .
Near the coast, the diurnal variation near the coast may be as large as inland, but with a wind off the sea it
will be small. Sea breezes have a pronounced cooling effect
why diurnal variation small over the sea
Higher specific heat of water (5× that of land)
larger mixing depth - surface water mixes with deeper layers
Evaporation from sea surface moderates temperature changes
4. Diurnal variation is maximum when wind is calm; with strong winds, surface air mixes with air above and
heat spreads through the friction layers (upto 1km above)
Minimum
Temperature what time of day
½ to 1 hour after
sunrise/dawn
Nocturnal cooling continues slightly past sunrise until incoming
solar radiation exceeds outgoing terrestrial radiation. Takes 2–3
hours for heat to transfer from screen level (1.25m)
maximum tempwhen during day
Early afternoon (2–3
hours after noon)
Highest insolation at noon, but 2–3 hours needed for heat to
transfer to screen level. Surface is highest at noon; screen level
maximum occurs 2–3 hours later.
Effect of Clouds on Surface Temperature
Can cut off a fair proportion of solar radiation during the day → reduces daytime heating
A thick layer of stratus cloud can block radiation and reduces a major part going back to space
A thick lower cloud also blocks most of the outgoing terrestrial radiation at night
why cloudy nights are hotter
thelower the cloud the more effectively it reduced the cooling
day with clouds vs night with clouds
reduced insolation → less daytime heating diurnal variation is small
clouds act as blanket - trap outgoing IR
night temp stays higher
Temperature conversion: °F from °C
Temperature conversion: °C from °F
C = 5(F−32)/9
Temperature conversion: K from °C
K = C + 273
Special crossover temperature
-40c = -40 f
Absolute zero
-2731.15c = 0k
Freezing point of water
0c = 32F = 273 k
boiling point of water
100 c = 212 F= 373K
Surface temp measurement height(stevenson screen)
4ft 1.25m
Minimum temperature timing
½ to 1 hr after sunrise
Maximum temp timing
2-3 hrs after noon (early afternoon)
Ocean diurnal Temp variation
< 1 degree celcius
Land diurnal temp variation
upto 20 degree celcius
Specific Heat of water
1 highest
specificheat of ice
0.5
Specific heat of soil / land
0.2
Solar radiation IR component
46
solar radiation Visible component
45%
solar radiation UV component
9%
Solar radiation absorbed by earths surface
51%
Solar radiation Absorbed by water vapour, dust, ozone
16%
solar radiation absorbed by clouds
3%
Total absorbed Solar radiation
70%
Back Scattered by Air
6 %
Reflected by clouds
20%
Reflected by earths surface
4%
Total reflected albedo of earth
30%
clear day radiation reaching the earth
5/6 83%
Snow surface albedo
80%
sun surface temp
6000 degree celcius
Friction layer depth (wind mixing)
upto 1 km above
convection covers more than
70% of earth (water covered )