Temperature Flashcards
How does temperature ‘drive the weather machine’?
Temperature and heating differences are important in weather processes. Unequal heating within the atmosphere ‘drives the weather machine’ by setting up pressure gradients that give us our winds and frontal systems. The developments of clouds, showers and thunderstorms are largely governed by the vertical temperature-structure of the atmosphere.
What is the formula to convert °F to °C.
T(c) = (T(f) -32) x 5/9
Describe absolute zero.
The Kelvin scale has its zero at -273.2 °C. At this temp a body is said to contain no heat energy.
Describe how observed temperature is recorded.
A temp sensor is placed in a louvered shelter called a Stevenson screen, set at a height of about 1.5 m above a grassed surface. This shelters it from direct radiation and precipitation but exposed to the wind flow. This is the temp reported in the METARs.
Is runway temp likely to be the same as observed?
No.
Define solar radiation.
Short wavelength radiation from the sun that warms our earth/atmosphere system. The temp of the surface of the sun is very hot. It averages around 6000 °C, about 1 billionth of the sun’s total output reaches the earth’s atmosphere.
Define terrestrial radiation.
Radiation emitted by the earth and its atmosphere to space. As the earth’s average temperature is only 15 °C, it emits radiation in long wavelengths which carry much less energy than short wavelengths do.
Describe the balance of solar versus outgoing terrestrial radiation.
Incoming solar radiation must balance outgoing terrestrial radiation for the temperature of the earth’s atmosphere to remain at an average temperature of 15 °C at mean sea level.
Describe how solar and terrestrial radiation affects the daily minimum temperature.
The rate at which long-wave terrestrial radiation is emitted from the earth depends on the amount of incoming solar radiation heating it. Incoming short-wave solar radiation is weak when the sun first rises, but the earth has been losing heat to space through terrestrial radiation all night, so that the min temp occurs just after dawn.
Describe how solar and terrestrial radiation affects the daily maximum temperature.
Solar radiation increases with the sun’s elevation. As the ground warms, the rate of loss by long-wave radiation also increases. After midday, the short-wave intensity starts to decrease whilst long-wave radiation is still increasing. The two rates become equal about three hours after midday on land, so the is the time of max temp.
Describe the effect of latitude on daily air temperature.
Near the equator, the midday rays from the sun strike the earth almost perpendicular to its surface. This results in maximum heating per unit area of the surface and consequently the daily maximum temperature is very warm.
Near the poles, the suns angle, even at the height of summer is very low. Thus, heating per unit area is low resulting in much colder maximum temperatures.
Describe the effect of the seasons on daily temperature.
No matter the time of year, near the equator the sun beats relentlessly down during the day. Thus only small temp fluctuations occur here.
At the south pole, the sun is below the horizon for all winter months, so the temp falls rapidly due to constant outgoing terrestrial heat and no incoming solar radiation to offset it. Thus the temp gradient between the equator and south pole is more pronounced during the southern hemisphere winter and spring than autumn and summer.
Describe the effect of strong winds on daily temperature.
If it it windy, mixing of the air occurs through a deeper layer, and the gain of heat by day and loss by night is then shared by more molecules in the air through greater depth. Thus diurnal variation of surface temp tends to decrease during windy conditions.
Describe the effect of wind direction on daily temperature.
Certain winds will decrease or increase temperatures depending on the origin of the wind e.g. a southerly flow into NZ will be colder than a northernly flow and reduce ambient air temp.
Describe the effect of cloud cover on daily temperature.
Cloudiness reduces diurnal fluctuation of temp. During the day, thick clouds reflect much of the incoming solar radiation back into space but at night will absorb outgoing terrestrial radiation and then re-radiate much of this heat back to the earth’s surface. Acts like a blanket.
Describe the effect of coastal locations on daily temperature.
Sea surface temps are slow to change over a 24 hr period. Thus, temps at coastal locations will be moderated by the effect of the cooler sea by day and the warmer sea by night, reducing diurnal fluctuations.
Describe the effect of inland locations on daily temperature.
Inland, temps can be considerably warmer by day and colder by night as the tempering effect of the sea is non-existent (land is quicker to warm up and cool down).
Describe the effect of surface type on daily temperatures.
Different land surfaces may heat up at differing rates - mostly based on colour. Darker surfaces absorb incoming solar radiation much quicker than lighter surfaces.
List seven factors which can alter daily temperature fluctuations.
Latitude. Seasons. Strong winds. Wind direction. Cloud cover. Coastal/inland locations (proximity to the sea). Surface type (colour).
Recite how heat enters and leaves the earth’s atmosphere.
Heat enters and leaves the earth/atmosphere system via solar and terrestrial radiation respectively.
Recite how heat is transferred throughout the atmosphere.
Heat is transferred within the atmosphere by conduction, convection and advection.
Describe the process of radiation in relation to heat transfer in the atmosphere.
Short-wave, high energy electromagnetic solar radiation heats the earth/atmosphere, and low energy long-wave radiation is emitted by the earth (terrestrial radiation) which acts to cool the earth/atmosphere system.
Describe the process of conduction in relation to heat transfer in the atmosphere.
Conduction is heat transfer by contact or touch. Air is a very poor conductor of heat, so conduction only occurs within a shallow layer of about 10 cm above the earth’s surface (which includes both heating and cooling of the earth).
Describe the process of convection in relation to heat transfer in the atmosphere.
Convection is heat transfer by the vertical movement of mass e.g. the cumuliform cloud formation process. This process relies on the atmosphere changing density as the temp changes and is an important method of heat energy transfer in the atmosphere.