Nature, Volume 454Sir Norman Lockyer Macmillan Journals Limited, 2008 - Electronic journals |
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Page 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 ...
Page 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 ...
Page 69
... termination shock Edward C. Stone1 ,. 75.3 76.9 78.4 80.0 81.6 83.2 -25.7 -26.1 -26.4 -26.8 -27.1 -27.4 i : 0.04-0.08 MeV 102 101 Interplanetary shock TS - 1 Day 242 of 2007 R = 83.65 AU L = -27.5 ° 102 2002.5 2003.5 2004.5 i : 0.14-0.22 ...
... termination shock Edward C. Stone1 ,. 75.3 76.9 78.4 80.0 81.6 83.2 -25.7 -26.1 -26.4 -26.8 -27.1 -27.4 i : 0.04-0.08 MeV 102 101 Interplanetary shock TS - 1 Day 242 of 2007 R = 83.65 AU L = -27.5 ° 102 2002.5 2003.5 2004.5 i : 0.14-0.22 ...
Contents
More CO2 means more | 46 |
ARTICLES | 49 |
SMAD proteins control DROSHAmediated microRNA maturation | 56 |
Copyright | |
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