File:Eclipse Magnitude.png
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| Description | The magnitude of a solar eclipse, as defined by the Bureau des Longitudes, is the ratio of a) the line connecting the centers of the Sun and the Moon and extending from that limb of the Sun which is closer to the center of the Moon to that limb of the Moon which is closer to the center of the Sun, and b) the diameter of the Sun (see J. Meeus: Mathematical Astronomy Morsels III, Richmond 2004, ch. 20) |
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| Source | Own work |
| Author | Sch |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 23:28, 21 January 2008 | | 800 × 800 (5 KB) | Sch (talk | contribs) | {{Information |Description=The magnitude of a solar eclipse, as defined by the Bureau des Longitudes, is the ratio of a) the line connecting the centers of the Sun and the Moon and extending from that limb of the Sun which is closer to the center of the M |
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