Observation of a non-uniform component in the distribution of coronal bright points |
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| Authors: | L Golub A S Krieger G S Vaiana |
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| Institution: | 1. American Science and Engineering, 02139, Cambridge, Mass., U.S.A.
2. Center for Astrophysics, Harvard College Observatory - Smithsonian Astrophysical Observatory, 02138, Cambridge, Mass., U.S.A.
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| Abstract: | The longitude distribution of X-ray bright points shows very strong variations when plotted in a heliocentric (Carrington) coordinate system. In addition, the latitude distribution can be interpreted as having two components : a uniformly distributed component and one having a distribution similar to that of active regions, occurring mostly within ±30° of the equator. |
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