... separately compute the location of the bowshock, magnetopause, and the velocity and ... on the day side of Earth, especially along the bowshock and near the "nose" of the ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/geoCXgusts.pdf -- 1594.9 Кб -- 31.10.2014 Похожие документы
... ApJS, 163, 344. 2006 The X-ray Structure of the Pulsar BowShock G189.22+2.90 in the Supernova Remnant IC 443 (B. Gaensler et al.) - ApJ, 648, 1037. ...
... ApJ, 653, L37 . 2006 The X-ray Structure of the Pulsar BowShock G189.22+2.90 in the Supernova Remnant IC 443 (B. Gaensler et al.) - ApJ, 648, 1037. ...
... The alternative hypothesis, that the excess is due to the presence of a bowshock at the leading end of the lobe, seems unlikely both because Carilli and collaborators showed that the bowshock is hardly seen at energies less than 4 keV and because the ...
... We finally mention a brightness feature that looks like a bowshock leaving the merger site, first noted in the ROSAT image (Krivonos et al. 2003). ...
... Markevitch,б M.; Gonzalez,б A.б H.; David,б L.; Vikhlinin,б A.; Murray,б S.; Forman,б W.; Jones,б C.; Tucker,б W. A Textbook Example of a BowShock in the Merging Galaxy Cluster 1E 0657-56 . ...
... Currently, we can determine the species and charge state of the most abundant elements in the solar wind and roughly determine the morphology of the X-ray producing region behind the cometary bowshock. ...
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Ссылки http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf -- 258.4 Кб -- 28.06.2011 Похожие документы