Nearly sonic and trans-sonic convective motions in the solar atmosphere related to the solar wind origin

1996 ◽  
Author(s):  
I. S. Veselovsky
Keyword(s):  
Solar Wind ◽  
Solar Atmosphere ◽  
Convective Motions ◽  
Solar Wind Origin

The Sun

2015 ◽  
Author(s):  
Joanna D. Haigh ◽  
Peter Cargill
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Solar Atmosphere ◽  
Space Weather ◽  
Extreme Ultraviolet ◽  
The Sun ◽  
Base Level ◽  
Earth’S Climate ◽  
The Magnetic Field ◽  
Terrestrial Magnetic Field

This chapter discusses how there are four general factors that contribute to the Sun's potential role in variations in the Earth's climate. First, the fusion processes in the solar core determine the solar luminosity and hence the base level of radiation impinging on the Earth. Second, the presence of the solar magnetic field leads to radiation at ultraviolet (UV), extreme ultraviolet (EUV), and X-ray wavelengths which can affect certain layers of the atmosphere. Third, the variability of the magnetic field over a 22-year cycle leads to significant changes in the radiative output at some wavelengths. Finally, the interplanetary manifestation of the outer solar atmosphere (the solar wind) interacts with the terrestrial magnetic field, leading to effects commonly called space weather.

Turbulence in the Solar Atmosphere and Solar Wind

2010 ◽  
Vol 156 (1-4) ◽  
pp. 135-238 ◽  
Author(s):  
A. Petrosyan ◽  
A. Balogh ◽  
M. L. Goldstein ◽  
J. Léorat ◽  
E. Marsch ◽  
...  
Keyword(s):  
Solar Wind ◽  
Solar Atmosphere

Coexistence of Earth-origin O+and solar wind-origin H+/He++in the distant magnetotail

1996 ◽  
Vol 23 (9) ◽  
pp. 985-988 ◽  
Author(s):  
K. Seki ◽  
M. Hirahara ◽  
T. Terasawa ◽  
I. Shinohara ◽  
T. Mukai ◽  
...  
Keyword(s):  
Solar Wind ◽  
Solar Wind Origin
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