Meteor showers - Modeled and measured effects in the atmosphere

Author:

Grebowsky J.1,Pesnell W.2

Affiliation:

1. NASA, Goddard Space Flight Center, Greenbelt, MD

2. Nomad Research, Inc., Bowie, MD

Publisher

American Institute of Aeronautics and Astronautics

Reference24 articles.

1. While Figures 4 and 5 show the results of a dry chemistry (reactions Nl-N7 and 11-114 in Table 1). a wet chemistry (adding N8-Nll) rearranges the molecular compounds below 80 km, but leaves the ion layer intact (Figure 7). A small decrease in the peak concentration of Mg' can be seen in this figure where the Mg' profile from Figure 4 is plotted as a dashed line along with the wet chemistry. The peak altitude moves up a little, but not a significant amount.

2. Ion Concentration Figure 6. Results of the 1-D model plotted with the averaged data. 701 I I I IOIII I I I I ,111 I I I I, 0.01 0.10 1.00 10.00 100.00 - 1000.00 10000.0~

3. N9 MgOH+H+ Mg+H,O 4x10-"exp(-5501 r) B N10 MgO + H,O + N, + Mg(OH), + N, 1.7x 10-2'(T / 20q)-3.7 C Nl 1 Mg(OH), + H 3 MgOH + H,O 5x10-`"exp(-2500/ r) C

4. Mg+ 0; + Mg++O, 1.2x 1o-9 C

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