Model for the production of CO Cameron band emission in Comet 1P/Halley

Author:

Raghuram Susarla,Bhardwaj Anil

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference57 articles.

1. Emission cross sections of CO2 by electron impact in the interval 1260–4500Å, II;Ajello;Journal of Chemical Physics,1971

2. Avakyan, S.V., II'in, R.N., Lavrov, V.M., Ogurtsov, G.N. (Eds.), 1998. Collision Processes and Excitation of UV Emission from Planetary Atmospheric Gases: A Handbook of Cross Sections. Gordon and Breach Science Publishers.

3. On the role of solar EUV, photoelectrons, and auroral electrons in the chemistry of C(1D) and the production of C I 1931Å in the inner cometary coma: a case for comet P/Halley;Bhardwaj;Journal of Geophysical Research,1999

4. On the solar EUV deposition in the inner coma of comets with large gas production rates;Bhardwaj;Geophysical Research Letters,2003

5. Optical thin H Lyman alpha production on outer planets: low energy proton acceleration in parallel electric fields and neutral H atom precipitation from ring current;Bhardwaj;Journal of Geophysical Research,1993

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