... TRACE looks at the region of the Sun between the "surface" that we see, called the photosphere , and the corona, the wispy ethereal atmosphere of the Sun seen in every solar eclipse picture. ...
... For smaller epochs the temperature of the ejecta is too high, or the photosphere must be at velocities so large that there is not enough material above it to form strong absorption lines. ...
... normal vector to the surface element), and the velocity of the photosphere, dr /dt ... of the line width with the photosphere velocity, and this effect was observed during ...
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Ссылки http://lnfm1.sai.msu.ru/~rastor/Papers/Rastorguev_Closing_remarks.pdf -- 141.9 Кб -- 12.01.2010 Похожие документы
... lines are basically formed in the photosphere, and their dynamical wavelet spectra ... of the velocity of matter in the photosphere corresponds to movement of features in ... These cannot be due to variations in the photosphere of Aa1 . ...
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Ссылки http://www.astro.spbu.ru/staff/afk/Papers/2006/delOriE.pdf -- 1677.9 Кб -- 19.11.2010 Похожие документы
... everywhere, from the Earth's surface to the Sun's photosphere and chromosphere ... the characteristics of magnetic fields transported away from the solar photosphere ...
... astro-ph/0410568 Ударные волны в спокойной солнечной фотосфере: необычные предположения (Shocks in the Quiet Solar Photosphere: A Rather Common Occurrence) . ...
... It will explore the magnetic structures responsible for carrying energy from the Sun's photosphere, or visible surface, through the thin chromosphere and out into the wispy corona. ...