Collision Processes and Excitation of UV Emission from Planetary Atmospheric Gases
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A01=G N Ogurtsov
A01=R N Ii'In
A01=SV Avakyan
A01=V M Lavrov
aeronomy
atomic collision theory
Auger Effect
Auger Electron Spectra
Auger Electrons
Author_G N Ogurtsov
Author_R N Ii'In
Author_SV Avakyan
Author_V M Lavrov
Category=PHM
Category=PHVJ
Category=PNRL
Data Set
Differential Cross Sections
Electron Impact
electron impact excitation data
Electron Production
Electron Spectroscopy
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eq_isMigrated=1
eq_isMigrated=2
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Incident Electron Energy
Ion Production
Ionization Cross Section
Mass Spectroscopic Data
McLeod Gauge
Molecular Ion
molecular spectroscopy
Partial Cross Sections
Partial Ionization Cross Sections
Planetary Atmospheres
planetary ionospheres
plasma diagnostics
Proton Energies
Quiet Sun
Slow Ions
Solar EUV
Solar Flares
Total Cross Sections
Total Ionization Cross Section
upper atmosphere modelling
UV Emission
Product details
- ISBN 9789056991470
- Weight: 850g
- Dimensions: 174 x 246mm
- Publication Date: 27 Jan 1999
- Publisher: Taylor & Francis Ltd
- Publication City/Country: GB
- Product Form: Hardback
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Over the past few decades, the excitation and ionization of atmospheric gases has become an area of intense research. A large amount of data have been accumulated concerning the various elementary processes which occur when photons, electrons and ions collide with atoms and molecules. This scattered information has now been collected in a handbook for the first time, and the authors give a critical analysis of relevant data.
This book is a comprehensive and detailed study of the available information and is distinguished by the following outstanding features: the consideration of a large number of atmospheric constituents, including H^O2, H, N^O2, N, O^O2, O, CO, CO^O2, H^O2O, HCl and some hydrocarbons the maximum number of space particles, including magnetospheric particles, are considered as projectiles: photons, electrons, hydrogen atoms, protons and helium ionsthe energy range under study corresponds to the real spectrum of cosmic fluxes, from threshold values for elementary processes up to several thousand keV the recommended values of cross sections, obtained from analysis of the available experimental data, are given in the handbook and their accuracy is estimated.
These features make the handbook particularly valuable to specialists in the aeronomy of planets, comets and active perturbations, as well as to experimentalists and theoreticians working in the fields of plasma physics, atomic and molecular physics, physics of the upper atmosphere, chemical physics, optics and spectroscopy.
SV Avakyan (Author), R N Ii'In (Author), V M Lavrov (Author), G N Ogurtsov (Author)
