Meteo 437
Atmospheric Physics II (Cloud
physics and chemistry)
Problem set 2
Assigned: 26 January 2004
Due: 2 February 2004
Use the constants in the Appendix in Bohren and Albrecht or in Rogers and Yau. You can work with others, but be sure that you understand how to do the problems.
The flux of molecules is given by F = ¼ n∙v, where n is the number density of molecules and v is the mean velocity of those molecules. Thus, the total number of molecules hitting the aerosols is F∙A, where A is the total aerosol surface area.
The mass of air, Mair, is about 0.029 kg mole-1. The energy of each molecule is thus about ½ mair∙v2. Thus, we need only multiply the molecular flux times the energy per each molecule to get the energy per unit surface area.
To do this problem absolutely correctly, we should look at the mean velocity and mass of each component of air and add them together; we should also use the root mean squared velocity when thinking about the energy and not the mean velocity. Ideally, we would even do the integral over the Boltzmann distribution. However, the differences caused by using the mass of air and the mean velocity of air are small.
This equals about 1.4x107 J. A kilowatt-hr is equal to 3.6x106 J, so that molecules strike you with the energy of about 4 kW-hr all the time. Why doesn’t this hurt?
Use the equation:
E = hc/l =
(1.98x10-16/ (nm)) J photon-1,
where l is in units of nm.
Note that 1 Joule = 6.242x1018 eV, 1 cal = 4.184 J; 1 eV = 23.06 kcal mol-1 = 96.48 kJ
mol-1 = 1.60x10-19 J molecule-1.
To break a
single bond requires the number of Joules per molecule, which is equal to:
Eb = (96.5x103 J/eV
5.12 eV)/mole x (1 mole/6.02x1023
molecules) = 8.2x10-19 J/molecule (one photon per molecule)
l = 1.98x10-16/8.21e-19
= 242 nm
In reality, because of other quantum mechanical considerations, the photodissociation of water vapor occurs with a reasonable cross section only for wavelengths below 200 nm.