SOHO MDI 2000-11-27 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 67 | 264 | 39 | 151 | 15.82 | 336.02 | 24.44 | 302.65 | 0.4744 | |
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next day for the same group /
back to the solar disc SOHO MDI 2000-11-27 12:47:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 3 | 10 | 2 | 6 | 15.03 | 338.45 | 26.87 | 298.90 | 0.5007 | |
| 19 | 94 | 11 | 54 | 15.95 | 338.00 | 26.42 | 300.93 | 0.5008 | |
| 0 | 5 | 0 | 3 | 15.08 | 337.83 | 26.25 | 299.50 | 0.4928 | |
| 0 | 6 | 0 | 4 | 14.65 | 337.51 | 25.93 | 298.98 | 0.4857 | |
| 11 | -2 | 6 | -2 | 16.07 | 337.30 | 25.73 | 301.78 | 0.4927 | |
| 0 | 8 | 0 | 5 | 15.76 | 336.78 | 25.20 | 301.70 | 0.4836 | |
| 0 | 7 | 0 | 4 | 14.34 | 336.47 | 24.89 | 299.32 | 0.4696 | |
| 0 | 7 | 0 | 4 | 14.62 | 336.11 | 24.53 | 300.18 | 0.4666 | |
| 0 | 3 | 0 | 2 | 16.95 | 336.41 | 24.83 | 304.21 | 0.4878 | |
| 5 | 39 | 3 | 22 | 14.70 | 335.33 | 23.76 | 301.09 | 0.4569 | |
| 0 | 6 | 0 | 3 | 17.08 | 335.59 | 24.01 | 305.27 | 0.4784 | |
| 3 | -10 | 2 | -10 | 14.78 | 335.04 | 23.46 | 301.54 | 0.4536 | |
| 5 | -10 | 3 | -10 | 15.34 | 334.98 | 23.40 | 302.68 | 0.4569 | |
| 0 | 11 | 0 | 6 | 16.09 | 335.07 | 23.49 | 304.00 | 0.4639 | |
| 5 | 17 | 3 | 10 | 16.57 | 334.87 | 23.29 | 305.10 | 0.4652 | |
| 0 | 9 | 0 | 5 | 17.41 | 333.93 | 22.35 | 307.69 | 0.4606 | |
| 0 | 5 | 0 | 3 | 16.03 | 333.07 | 21.50 | 306.12 | 0.4379 | |
| 0 | 3 | 0 | 2 | 16.31 | 332.76 | 21.18 | 307.03 | 0.4363 | |
| 7 | 15 | 4 | 8 | 15.71 | 332.61 | 21.03 | 306.07 | 0.4293 | |
| 9 | 19 | 5 | 10 | 16.67 | 332.46 | 20.88 | 308.09 | 0.4358 | |
| 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 | |