The structure and length of tail-associated phenomena in the solar wind downstream from the Earth-Reference-Cited by-同舟云学术

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The structure and length of tail-associated phenomena in the solar wind downstream from the Earth

Published:1991-07 Issue:7 Volume:39 Page:1039-1043
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Cowley S.W.H.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference30 articles.

1. Plasma regimes in the deep geomagnetic tail : ISEE-3;Bame;Geophys. Res. Lett.,1983

2. Far magnetospheric field observations by Pioneer 8 : the distant bow shock and extended tail;Bavassano;Space Res.,1974

3. Solar wind control of magnetospheric convection;Cowley,1984

4. The distant geomagnetic tail in theory and observation;Cowley,1984

5. Energetic ion regimes in the deep geomagnetic tail : ISEE-3;Cowley;Geophys. Res. Lett.,1984

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2. Space Plasma Physics: A Review;IEEE Transactions on Plasma Science;2022

3. Generation of By in Earth’s magnetotail with the effect of IMF By during southward interplanetary magnetic field;AIP Advances;2021-04-01

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5. Magnetotail;Magnetotails in the Solar System;2015-01-09

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