Add to ORKGA one-dimensional theoretical model of the Saturn upper atmosphere and ionosphere was developed and used to study the effects of various free parameters on the structure and composition of the ionosphere. The model was used to solve the diffusion equations for all the major neutral species aboPhDPhysics, Atmospheric ScienceUniversity of Michiganhttp://deepblue.lib.umich.edu/bitstream/2027.42/158364/1/8116353.pd
We present a semianalytical photochemical model of Saturn's near-equatorial ionosphere and adapt it ...
The atmosphere of Saturn exhibits dynamical structures (jets, bands, spots, eddies) with horizontal...
The dynamics of Saturn's magnetosphere are driven internally by the planet's strong magnetic field, ...
A time-dependent one-dimensional model of Saturn’s ionosphere has been developed as an intermediate ...
The giant planets in our solar system such as Saturn and Jupiter represent fascinating worlds which ...
The high latitude ionosphere and polar wind outflow at Saturn were studied with a sophisticated nume...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/62878/1/292682a0.pd
Numerical modeling tools can be used for a number of reasons yielding many benefits in their applica...
Model ionospheres are calculated for Saturn, Uranus, and Neptune. P ro tons are the maj or ions ab...
[1] We have calculated self-consistent electron and ion temperatures in Saturn’s ionosphere using a ...
This chapter summarizes our current understanding of the ionosphere of Saturn. We give an overview o...
We present the first results from a newly developed 3-D Jupiter Global Ionosphere-Thermosphere Model...
We present new models of Saturn's equatorial ionosphere based on the first in situ measurements of i...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94859/1/jgra18429.pd
An edited version of this paper was published by AGU. Copyright 2018 American Geophysical Union.The ...
We present a semianalytical photochemical model of Saturn's near-equatorial ionosphere and adapt it ...
The atmosphere of Saturn exhibits dynamical structures (jets, bands, spots, eddies) with horizontal...
The dynamics of Saturn's magnetosphere are driven internally by the planet's strong magnetic field, ...
A time-dependent one-dimensional model of Saturn’s ionosphere has been developed as an intermediate ...
The giant planets in our solar system such as Saturn and Jupiter represent fascinating worlds which ...
The high latitude ionosphere and polar wind outflow at Saturn were studied with a sophisticated nume...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/62878/1/292682a0.pd
Numerical modeling tools can be used for a number of reasons yielding many benefits in their applica...
Model ionospheres are calculated for Saturn, Uranus, and Neptune. P ro tons are the maj or ions ab...
[1] We have calculated self-consistent electron and ion temperatures in Saturn’s ionosphere using a ...
This chapter summarizes our current understanding of the ionosphere of Saturn. We give an overview o...
We present the first results from a newly developed 3-D Jupiter Global Ionosphere-Thermosphere Model...
We present new models of Saturn's equatorial ionosphere based on the first in situ measurements of i...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94859/1/jgra18429.pd
An edited version of this paper was published by AGU. Copyright 2018 American Geophysical Union.The ...
We present a semianalytical photochemical model of Saturn's near-equatorial ionosphere and adapt it ...
The atmosphere of Saturn exhibits dynamical structures (jets, bands, spots, eddies) with horizontal...
The dynamics of Saturn's magnetosphere are driven internally by the planet's strong magnetic field, ...