Meteorology Exam 1 (Ch 1,2,3,4)

0.0(0)
Studied by 6 people
call kaiCall Kai
Locked
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/58

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 5:52 PM on 9/16/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai
Chat

No analytics yet

Send a link to your students to track their progress

59 Terms

1
New cards

What does a high percentage of hot colors (red, orange, yellow) in clouds indicate on a satellite map?

The cloud is colder and located at a higher altitude.

2
New cards

What percentage of scenarios would produce rainfall if there’s an '80% chance of rain'?

80 scenarios out of 100 would likely produce rainfall.

3
New cards

How far is Earth from the Sun?

93 million miles.

4
New cards

How long does it take for light to travel from the Sun to Earth?

8 minutes.

5
New cards

What fraction of the Sun's total energy output does Earth intercept?

very small fraction

6
New cards

What are the two most important greenhouse gases?

Water vapor and CO2.

7
New cards

What replaced CFCs according to the Montreal Protocol?

Hydrofluorocarbons (HFCs).

8
New cards

How is ozone thickness measured?

In Dobson Units (DU).

9
New cards

What is the typical thickness of the ozone layer?

300 Dobson Units (DU) or approximately 1/8 inch.

10
New cards

What is said about ozone in the stratosphere compared to the troposphere?

Good in the stratosphere for UV absorption, but bad in the troposphere due to health effects.

11
New cards

What are the dimensions of density?

Density = mass/volume, measured in kg/m³.

12
New cards

What is the average air pressure at sea level?

1013 mb or 1013 hPa.

13
New cards

What is the definition of 'Weather'?

The condition of the atmosphere at any particular time or place.

14
New cards

What is the definition of 'Climate'?

Collection of all possible weather and their likelihoods of occurrence over a long time.

15
New cards

What is the formula for calculating kinetic energy?

Kinetic energy = 1/2mv², where m is mass and v is velocity.

16
New cards

What does Stefan-Boltzmann Law of Radiation state?

The total radiant energy emitted is proportional to the temperature to the fourth power.

17
New cards

What is the unit of energy?

Joules (J).

18
New cards

What is the definition of specific heat capacity?

The amount of energy required to raise the temperature of 1 kg by 1 unit Kelvin.

19
New cards

What is the primary role of the ozone layer?

To absorb UV radiation.

20
New cards

What type of scattering occurs with particles smaller than the wavelength of light?

Rayleigh scattering.

21
New cards

What is the average heat capacity of dry air?

1000 J/(kg·K).

22
New cards

What is the greenhouse effect primarily caused by?

The absorption and emission of infrared radiation by water vapor and CO2.

23
New cards

What is wind shear?

The difference in wind speed and direction at different altitudes.

24
New cards

What is the albedo effect?

The fraction of solar energy reflected back into space by Earth's surface and atmosphere.

25
New cards

How can you determine the wavelength of radiation?

Wavelength = wave speed/frequency.

26
New cards

What is Wien's Law of Displacement?

Hotter bodies emit most radiation at shorter wavelengths.

27
New cards

Dobson Unit (DU)

A unit of measure for ozone layer thickness compressed to sea level pressure, where 1 DU=0.01 mm1\,\text{DU} = 0.01\,\text{mm}.

28
New cards

Radiosonde

An instrument package launched twice daily (1 hour before midnight UTC and noon) from 108 sites in the United States to measure air properties.

29
New cards

Weather

The condition of the atmosphere at any particular time or place, characterized by variables such as pressure, temperature, humidity, clouds, precipitation, wind, visibility, and air quality.

30
New cards

Climate

The collection of all possible weather conditions and their likelihoods of occurrence over a long period of time.

31
New cards

Work

The active process of transferring or converting energy from one form to another by applying a force over a distance.

32
New cards

Kinetic Energy

The energy possessed by an object in motion, directly related to its speed and calculated as 12mv2\frac{1}{2}mv^2.

33
New cards

Potential Energy

The energy stored in an object due to its position, represented by work done against gravity (ghgh).

34
New cards

Temperature

The measure of the average kinetic energy of the molecules within a substance.

35
New cards

Absolute Zero (0 K0\,\text{K})

The temperature at which molecular kinetic energy ceases and molecules become stationary.

36
New cards

Specific Heat Capacity

The amount of heat energy required to raise the temperature of 1 kg1\,\text{kg} of a mass by 1 K1\,\text{K}.

37
New cards

Latent Heat

Hidden energy absorbed or released by water molecules during a phase change without altering the temperature of the substance.

38
New cards

Sensible Heat

Heat transferrable by conduction or convection that changes the temperature of a substance without causing a phase change.

39
New cards

Conduction

The transfer of heat energy through direct physical contact.

40
New cards

Convection

The transfer of heat energy through the movement of air or buoyant turbulent currents.

41
New cards

Stefan-Boltzmann Law of Radiation

A radiation law stating that the total radiant energy emitted by an object per second is proportional to its absolute temperature raised to the fourth power (E=σT4E = \sigma T^4).

42
New cards

Wien's Law of Displacement

A radiation law stating that hotter objects emit their peak radiation at shorter wavelengths (λmax=constantT\lambda_{\text{max}} = \frac{\text{constant}}{T}).

43
New cards

Kirchhoff's Law of Radiation

A radiation law stating that at any particular wavelength, a good absorber of radiation is also a good emitter, and a poor absorber is a poor emitter.

44
New cards

Rayleigh Scattering

Selective scattering occurring when particles are much smaller than the wavelength of light (such as air gas molecules), causing shorter wavelengths like blue and violet to scatter most intensely.

45
New cards

Mie Scattering

Scattering occurring when particles are roughly equal in size to the wavelength of light (such as dust or cloud droplets), causing all visible wavelengths to scatter equally and producing white clouds.

46
New cards

Geometric Scattering

Scattering occurring when particles are much larger than the wavelength of light (such as large rain drops), where light reflects or refracts off boundaries independent of wavelength.

47
New cards

Atmospheric Phase Changes Chart

A reference chart categorizing water phase transitions into energy-absorbing processes (melting, evaporation, sublimation) and energy-releasing processes (freezing, condensation, deposition).

48
New cards

Saturation Vapor Pressure Exponential Growth Concept

The thermodynamic property where saturation vapor pressure rises rapidly and nonlinearly as temperature increases, and cooling lowers the saturation threshold prior to condensation.

49
New cards

Sublimation

The phase change of water directly from ice to vapor, which absorbs the greatest amount of energy from the surroundings among phase changes.

50
New cards

Deposition

The phase change of water directly from vapor to ice, which releases the greatest amount of latent energy to the surroundings among phase changes.

51
New cards

Absolute Humidity

The mass of water vapor contained within a fixed volume of air, expressed in g/m3\text{g/m}^3.

52
New cards

Specific Humidity (qq)

The mass of water vapor contained in a fixed total mass of moist air, expressed in g/kg\text{g/kg}.

53
New cards

Mixing Ratio (rr)

The mass of water vapor contained in a fixed mass of dry air, expressed in g/kg\text{g/kg}.

54
New cards

Vapor Pressure (ee)

The partial pressure contributed specifically by the water vapor molecules currently present in the atmosphere, measured in hPa\text{hPa}.

55
New cards

Saturation Vapor Pressure (es(T)e_s(T))

The partial vapor pressure at dynamic equilibrium for a given temperature TT, where the rate of evaporation equals the rate of condensation.

56
New cards

Relative Humidity (RH)

The percentage ratio of the actual vapor pressure to the saturation vapor pressure at a given temperature, calculated as RH=100×ees(T)\text{RH} = 100 \times \frac{e}{e_s(T)}.

57
New cards

Dew Point (TdT_d)

The temperature to which air must be cooled at constant pressure and moisture content to achieve full saturation.

58
New cards

Sling Psychrometer

An instrument equipped with both a dry-bulb and a ventilated wet-bulb thermometer used to determine atmospheric humidity.

59
New cards

Wet-Bulb Temperature (TwT_w)

The temperature measured by a wet, ventilated thermometer cooled by evaporation, which serves as an index for human discomfort and evaporative cooling capacity.