Energy balance and heating mechanisms of the Martian Upper atmosphere with the NASA Ames MGCM.

2021 ◽  
Author(s):  
Leonardos Gkouvelis ◽  
Amanda Brecht ◽  
Alexandre Kling ◽  
Robert Wilson ◽  
Sonny Harman ◽  
...  
Keyword(s):  
Energy Balance ◽  
Upper Atmosphere

The thermal structure and energy balance of the Uranian upper atmosphere

Icarus ◽  
1983 ◽  
Vol 53 (3) ◽  
pp. 399-414 ◽  
Author(s):  
R.G. French ◽  
J.L. Elliot ◽  
E.W. Dunham ◽  
D.A. Allen ◽  
J.H. Elias ◽  
...  
Keyword(s):  
Energy Balance ◽  
Thermal Structure ◽  
Upper Atmosphere

scholarly journals Passive Remote Study of the Aerosol in the Upper Atmosphere of the Earth

2019 ◽  
pp. 1-6
Author(s):  
Oleksandr Zbrutskyi ◽  
◽  
Nevodovskyi P ◽  
Anatoliy Vid’machenko ◽  
◽  
...  
Keyword(s):  
Global Warming ◽  
Energy Balance ◽  
Climate Changes ◽  
Upper Atmosphere ◽  
Anthropogenic Factors ◽  
The Sun ◽  
Earth System ◽  
Relative Contribution ◽  
The Earth

Climate changes on planet Earth are mainly caused by disturbances in the energy balance of the Sun-Earth system. This process is the result of both natural changes in nature and the influence of anthropogenic factors. The combined effect of these factors can lead to threatening phenomena for mankind - a decrease in the power of the ozone layer, the formation of “ozone holes” and global warming on the planet and other disasters. The study of the causes of these factors and the determination of their relative contribution is one of the pressing problems of our time.

Estimated energy balance in the jovian upper atmosphere during an auroral heating event

Icarus ◽  
2006 ◽  
Vol 181 (1) ◽  
pp. 256-265 ◽  
Author(s):  
H MELIN ◽  
S MILLER ◽  
T STALLARD ◽  
C SMITH ◽  
D GRODENT
Keyword(s):  
Energy Balance ◽  
Upper Atmosphere ◽  
Heating Event

Effects of Ambipolar Diffusion on Prominence Thread Models

1994 ◽  
Vol 144 ◽  
pp. 315-321 ◽  
Author(s):  
M. G. Rovira ◽  
J. M. Fontenla ◽  
J.-C. Vial ◽  
P. Gouttebroze
Keyword(s):  
Energy Balance ◽  
Transition Region ◽  
Ambipolar Diffusion ◽  
Line Profiles ◽  
Balance Equations ◽  
Model Calculations ◽  
Partial Frequency ◽  
Frequency Redistribution ◽  
Partial Frequency Redistribution ◽  
Theoretical Structure

AbstractWe have improved previous model calculations of the prominence-corona transition region including the effect of the ambipolar diffusion in the statistical equilibrium and energy balance equations. We show its influence on the different parameters that characterize the resulting prominence theoretical structure. We take into account the effect of the partial frequency redistribution (PRD) in the line profiles and total intensities calculations.

Influence of Magnetic Fields on Solar Hydrodynamics: Experimental Results

1977 ◽  
Vol 36 ◽  
pp. 143-180 ◽  
Author(s):  
J.O. Stenflo
Keyword(s):  
Solar Activity ◽  
Energy Balance ◽  
Magnetic Fields ◽  
Solar Atmosphere ◽  
General Problem ◽  
Solar Rotation ◽  
Active Regions ◽  
Physical Conditions ◽  
Dynamic Phenomena

It is well-known that solar activity is basically caused by the Interaction of magnetic fields with convection and solar rotation, resulting in a great variety of dynamic phenomena, like flares, surges, sunspots, prominences, etc. Many conferences have been devoted to solar activity, including the role of magnetic fields. Similar attention has not been paid to the role of magnetic fields for the overall dynamics and energy balance of the solar atmosphere, related to the general problem of chromospheric and coronal heating. To penetrate this problem we have to focus our attention more on the physical conditions in the ‘quiet’ regions than on the conspicuous phenomena in active regions.

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