Planetary Ionospheres

1975 ◽  
pp. 635-653
Author(s):  
Rocco S. Narcisi
Keyword(s):  
Planetary Ionospheres

Dissociative recombination in the interstellar medium and planetary ionospheres

2008 ◽  
Vol 106 (16-18) ◽  
pp. 2199-2226 ◽  
Author(s):  
W.D. Geppert ◽  
M. Larsson
Keyword(s):  
Interstellar Medium ◽  
Dissociative Recombination ◽  
Planetary Ionospheres

scholarly journals A study of the reactions of Al+ions with O3, N2, O2, CO2and H2O: influence on Al+chemistry in planetary ionospheres

2019 ◽  
Vol 21 (26) ◽  
pp. 14080-14089 ◽  
Author(s):  
Shane M. Daly ◽  
David L. Bones ◽  
John M. C. Plane
Keyword(s):  
Reaction Kinetics ◽  
Metal Chemistry ◽  
Planetary Ionospheres

First measurements of Al+ion reaction kinetics relevant to meteor-ablated metal chemistry in planetary upper atmospheres.

Beaming of electromagnetic radiation by planetary ionospheres

Icarus ◽  
1970 ◽  
Vol 12 (3) ◽  
pp. 431-434
Author(s):  
Vassilios Kerdemelidis
Keyword(s):  
Electromagnetic Radiation ◽  
Planetary Ionospheres

scholarly journals Planetary ionospheres – sources and dynamic drivers

2008 ◽  
Vol 4 (S257) ◽  
pp. 499-510 ◽  
Author(s):  
Joseph M. Grebowsky ◽  
Arthur C. Aikin
Keyword(s):  
Carbon Dioxide ◽  
Solar Wind ◽  
Magnetic Fields ◽  
Lower Atmosphere ◽  
Dust Particles ◽  
X Rays ◽  
Interplanetary Dust Particles ◽  
Carbon Dioxide Atmosphere ◽  
Energy Inputs ◽  
Planetary Ionospheres

AbstractExternal energy inputs into all planetary upper atmospheres (including more than a half dozen moons with atmospheres) are comprised of combinations of solar EUV, soft x-rays, solar energetic particles, solar wind charged particles, magnetospherically accelerated particles, solar wind electric field, interplanetary dust particles as well as propagating lower atmosphere disturbances. Each input has analogous physical interactions with all planetary ionospheres and upper atmospheres, but the integrated consequences of the multiple energy inputs vary from planet to planet. The Earth forms the framework for most fundamental processes because of extensive measurements of the effects of each of the inputs. However the conditions at Earth are far different from those at the carbon dioxide atmosphere of magnetic field-free, slow-rotating Venus, the carbon dioxide atmosphere of Mars with patchy remnant magnetic fields, while the outer planets have hydrogen atmospheres, are fast rotating with intrinsic magnetic fields, and encompass moons that interact with the magnetospheres and have exotic atmospheres. Although the physical processes are known, our understanding of our solar system's ionospheres diminishes with increasing distance from the Sun.

Planetary ionospheres

Ionospheres ◽  
2010 ◽  
pp. 482-516
Author(s):  
Robert Schunk ◽  
Andrew Nagy
Keyword(s):  
Planetary Ionospheres
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