Nature, Volume 454Sir Norman Lockyer Macmillan Journals Limited, 2008 |
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Página 63
... termination shock John D. Richardson 12 , Justin C. Kasper3 , Chi Wang2 , John W. Belcher1 & Alan J. Lazarus1 The solar wind blows outward from the Sun and forms a bubble of solar material in the interstellar medium . The termination shock ...
... termination shock John D. Richardson 12 , Justin C. Kasper3 , Chi Wang2 , John W. Belcher1 & Alan J. Lazarus1 The solar wind blows outward from the Sun and forms a bubble of solar material in the interstellar medium . The termination shock ...
Página 64
... termination shock 10 AU closer to the Sun than did Voyager 1 . However , the termination shock position changes with the solar wind pressure : stronger solar wind pushes the termination shock farther from the Sun. We use the solar wind ...
... termination shock 10 AU closer to the Sun than did Voyager 1 . However , the termination shock position changes with the solar wind pressure : stronger solar wind pushes the termination shock farther from the Sun. We use the solar wind ...
Página 74
... termination shock region and the heliosheath beyond . Science 309 , 2017-2020 ( 2005 ) . 2. Burlaga , L. F. et al . Crossing the termination shock into the heliosheath : Magnetic fields . Science 309 , 2027-2029 ( 2005 ) . 3 . Decker ...
... termination shock region and the heliosheath beyond . Science 309 , 2017-2020 ( 2005 ) . 2. Burlaga , L. F. et al . Crossing the termination shock into the heliosheath : Magnetic fields . Science 309 , 2027-2029 ( 2005 ) . 3 . Decker ...
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More CO2 means more | 46 |
ARTICLES | 49 |
SMAD proteins control DROSHAmediated microRNA maturation | 56 |
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