Heating and Energetics of the Solar Corona and Solar Wind
These altitudes have been estimated assuming that all kernels were situated vertically above the aquot;neutralaquot; line (HAl = 0). ... a sequence of SXT images; the solid line is the magnetic aquot;neutralaquot; line (Hii=0) taken from the Kitt Peak magnetograms. ... B, C and D was the result of this expansion and is explained in more detail in another paper of this issue (Jakimiec, 2001). ... 1986; 1987; 1992) a method of investigating the flare evolution in the temperature-density diagnostic diagrams hasanbsp;...
| Title | : | Heating and Energetics of the Solar Corona and Solar Wind |
| Author | : | COSPAR. Scientific Assembly |
| Publisher | : | - 2002 |
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