| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24 | 168 | 40 | 544 | 10.01 | 312.17 | 80.86 | 280.36 | 0.9825 | -532.4 | -26.6 | |
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previous
or next observation for the same group /
back to the solar disc SOHO MDI 1999-12-15 01:35:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 49 | 0 | 350 | 9.73 | 317.12 | 85.81 | 279.82 | 0.9979 | -50.0 | -20.0 | |
| 6 | 116 | 10 | 190 | 10.20 | 303.52 | 72.20 | 280.99 | 0.9559 | -407.6 | -45.2 | |
| 18 | -2 | 30 | -2 | 10.63 | 303.25 | 71.93 | 281.45 | 0.9547 | -613.9 | 999999 | |
| 0 | 3 | 0 | 4 | 10.14 | 299.95 | 68.64 | 281.22 | 0.9362 | 183.0 | 111.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |