Solar Corona: Revision history

Diff selection: Mark the radio buttons of the revisions to compare and hit enter or the button at the bottom.
Legend: (cur) = difference with latest revision, (prev) = difference with preceding revision, m = minor edit.

8 May 2024

  • curprev 10:3010:30, 8 May 2024Ai talk contribs 3,343 bytes +220 No edit summary
  • curprev 10:2910:29, 8 May 2024Ai talk contribs 3,123 bytes −1 No edit summary
  • curprev 10:2710:27, 8 May 2024Ai talk contribs 3,124 bytes +3,124 Created page with "== Introduction == The solar corona is the outermost part of the Sun's atmosphere, characterized by high temperatures and low densities. This region of the Sun extends millions of kilometers into space, far beyond the visible disc of the Sun, and is most easily seen during a total solar eclipse, when it is visible as a pearly white crown surrounding the Sun. == Physical Properties == The solar corona is a plasma, a state of matter..."