ATM OCN (Meteorology) 100

Answers for Homework 3

Summer 1998


Date Due: Tuesday, 22 July 1998

The total maximum points were  100.  Point distribution for each question is noted below. 


PART 1. ATMOSPHERIC OPTICS

(36 pts for a and 6 pts for b)

a. For the following atmospheric optical phenomena, identify:

1. Mirage (Superior or inferior):

 
PHYSICAL CAUSE(S): Refraction of light by density differences in the atmosphere 
THE AGENT(S): Lower atmosphere with a strong vertical temperature -- and ultimately vertical density gradient. 
WHERE (WHEN) FOUND: Large vertical temperature and density gradients, such as the hot pavement and cool air immediately above, or the cold lake and warm overlying air mass. 
 

2. Halo (22°):

PHYSICAL CAUSE(S): Refraction (and dispersion) of light through ice crystals. 
THE AGENT(S): Airborne ice crystals. 
WHERE (WHEN) FOUND: Look toward the sun or the moon, with a thin veil of cirriform clouds (such as cirrostratus) in front of the illuminating source. 

3. Corona:

PHYSICAL CAUSE(S): Diffraction of light around liquid water droplets. 
THE AGENT(S): Airborne liquid cloud droplets (with a nearly uniform size for best results). 
WHERE (WHEN) FOUND: Look toward the sun or the moon, with a thin veil of warm clouds (such as altostratus or stratus) in front of the illuminating source. 

4. Rainbow (Primary):

 
PHYSICAL CAUSE(S): Refraction and dispersion of light entering the raindrop, the internal reflection of this light from the back surface of the drop and the refraction of the reflected light. 
THE AGENT(S): Falling liquid raindrops. 
WHERE (WHEN) FOUND: Look away from the low sun (due to geometry considerations, the sun should be no higher than 42 above the horizon) and toward a rain shaft of falling raindrops. 
 
b. What is the physical difference between Rayleigh and Mie scattering? Identify the characteristics of the particles responsible for each type of scatter.
 
Rayleigh scatter occurs when the incoming radiation (typically polychromatic sunlight) is scattered by gas molecules or other particles in the atmosphere that have a diameter typically less than one tenth the size of the wavelength of the incident radiation - or on the order of 0.05 micrometers. This type of scattering is wavelength dependent, with the short or blue and violet wavelengths preferentially scattered more than the longer wavelength red light. 
Mie scatter occurs when the incoming radiation is scattered by large aerosols or cloud droplets that have wavelengths at least as large as the wavelength of the incoming radiation. This type of radiation is independent of wavelength, meaning that the polychromatic white light is scattered and still appears as a milky white light. 
 

Cite an example of each of these two scattering processes.

 
Blue skies - an example of Rayleigh scatter 
White clouds (at least when viewed from the side or above) - an example of Mie scatter. 
Note that red sunsets in relatively clean air would represent Rayleigh scatter, but if sufficient aerosol loading of the atmosphere were present, vivid red sunsets would indicate additional Mie scatter. 
 

PART 2. ATMOSPHERIC MOTIONS

1. Identify the following characteristics associated with each of the force components in the atmospheric equation of motion:

[30 pts at 2 pts each]

A. VERTICAL PRESSURE GRADIENT FORCE

 
  • DIRECTION: 
Vertical and upward (from high pressure near the surface toward low pressure aloft, or opposite of down). 
  • MAGNITUDE depends upon: 
The preferable answer is that magnitude of vertical pressure gradient force depends upon the vertical spacing of the pressure surfaces, which depend upon the density or average temperature of the layer (see discussion below for #3). 
Altitude is acceptable. 
 
 

B. HORIZONTAL PRESSURE GRADIENT FORCE

 
  • DIRECTION: 
Horizontal and upward pointed from high pressure toward low pressure (as seen on a weather chart). 
  • MAGNITUDE depends upon: 
Packing of the isobars on a horizontal, constant altitude weather chart (which describe horizontal pressure gradient or difference in pressure over a given horizontal distance). 
 

C. GRAVITATIONAL FORCE or "GRAVITY"

 
  • DIRECTION: 
Vertical and downward (toward the center of the earth). 
  • MAGNITUDE depends upon: 
The masses of the earth and the object and upon the separation between their centers (according to I. Newton) 
or equivalently, upon the altitude above the earth's surface. 
 

D. CORIOLIS EFFECT or "FORCE" (Horizontal Component)

E. FRICTIONAL FORCE (Horizontal Component)

F. CENTRIPETAL FORCE


2. What is the primary physical significance of the hydrostatic balance relationship?

[4 pts]
 

The earth maintains an atmosphere, since large scale accelerations of air away from the earth's surface are inhibited by gravity. 

3. From this hydrostatic balance relationship, how does the magnitude of the vertical pressure gradient in a warm air column compare with the vertical pressure gradient in a column of cold air?

[4 pts]
 

The vertical pressure gradient in a warm air column is less than in a cold air column. 

4. a) What forces are balanced in the geostrophic wind model?

[2 pts.]
 

The horizontal components of the pressure gradient force and the Coriolis force.
b) Name three separate assumptions used to describe the geostrophic wind model.

[6 pts or 2 pts. each]
 

Select 3 of following 4: 

1. No net acceleration  

2. Frictionless  

3. Straight and parallel isobars  

4. Horizontal flow


5. On the horizontal surface pressure map in the Northern Hemisphere (within the friction layer), locate the regions of high and low pressure, placing a large block H and L, respectively. Make a force diagram by neatly drawing thin arrows to signify the direction and relative magnitudes of the horizontal pressure gradient force (FHPG), the Coriolis force (FCOR), the friction force (FFRC). Label each of these forces. Neatly draw a thick, double bladed arrow to represent the resultant wind (VRES); label this wind vector:

[12 pts]


 
 


Last revision: 22 July 1998
Produced by Edward J. Hopkins, Ph.D.
Department of Atmospheric and Oceanic Sciences
University of Wisconsin-Madison, Madison, WI 53706
hopkins@meteor.wisc.edu

URL Address: aos100/homework/98hmk03a.htm



 
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