Nature, Volume 454Sir Norman Lockyer Macmillan Journals Limited, 2008 - Electronic journals |
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Page 72
... intensity of termination shock particles ( TSPs ) observed by Voyager 1 in the heliosheath since mid- 2005. However , the intensity of helium nuclei with an energy of 1-1.5 MeV per nucleon and 4-5 MeV protons at Voyager 2 just after it ...
... intensity of termination shock particles ( TSPs ) observed by Voyager 1 in the heliosheath since mid- 2005. However , the intensity of helium nuclei with an energy of 1-1.5 MeV per nucleon and 4-5 MeV protons at Voyager 2 just after it ...
Page 73
... intensity of GCR He with 150–380 MeV per nucleon is twice the intensity bserved by Voyager 1 at 104 AU ( Fig . 3a ) , requiring a gradient of .2 % per AU if it were uniform between Voyager 1 and a heliopause at 35 AU . However , the ...
... intensity of GCR He with 150–380 MeV per nucleon is twice the intensity bserved by Voyager 1 at 104 AU ( Fig . 3a ) , requiring a gradient of .2 % per AU if it were uniform between Voyager 1 and a heliopause at 35 AU . However , the ...
Page 320
... intensity profiles , all with a central dip reduction near 0.6 % of the mean bright - field intensity ( Fig . 2e ) . By comparing the TEM image data for these additional features to adatom simulations , we rule out any adatom heavier ...
... intensity profiles , all with a central dip reduction near 0.6 % of the mean bright - field intensity ( Fig . 2e ) . By comparing the TEM image data for these additional features to adatom simulations , we rule out any adatom heavier ...
Contents
More CO2 means more | 46 |
ARTICLES | 49 |
SMAD proteins control DROSHAmediated microRNA maturation | 56 |
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