Nature, Volume 454Sir Norman Lockyer Macmillan Journals Limited, 2008 |
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Página 63
... solar wind blows outward from the Sun and forms a bubble of solar material in the interstellar medium . The termination shock occurs where the solar wind changes from being supersonic ( with respect to the surrounding interstellar ...
... solar wind blows outward from the Sun and forms a bubble of solar material in the interstellar medium . The termination shock occurs where the solar wind changes from being supersonic ( with respect to the surrounding interstellar ...
Página 64
... solar wind pressure : stronger solar wind pushes the termination shock farther from the Sun. We use the solar wind pressures observed by Voyager 2 before the termination shock crossing and a two - dimensional magnetohydrodynamics model1 ...
... solar wind pressure : stronger solar wind pushes the termination shock farther from the Sun. We use the solar wind pressures observed by Voyager 2 before the termination shock crossing and a two - dimensional magnetohydrodynamics model1 ...
Página 74
... solar wind termination shock . Science 309 , 2025-2027 ( 2005 ) . 5. Opher , M. , Stone , E. C. & Liewer , P. C. The effects of a local interstellar magnetic field on Voyager 1 and 2 observations . Astrophys . J. 640 , L71 - L74 ( 2006 ) ...
... solar wind termination shock . Science 309 , 2025-2027 ( 2005 ) . 5. Opher , M. , Stone , E. C. & Liewer , P. C. The effects of a local interstellar magnetic field on Voyager 1 and 2 observations . Astrophys . J. 640 , L71 - L74 ( 2006 ) ...
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More CO2 means more | 46 |
ARTICLES | 49 |
SMAD proteins control DROSHAmediated microRNA maturation | 56 |
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