SOHO MDI 2000-11-02 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70 | 411 | 42 | 253 | -22.95 | 305.34 | 24.38 | 220.16 | 0.5910 | -1067.9 | -593.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21 | 109 | 13 | 68 | -22.51 | 307.44 | 26.48 | 223.01 | 0.6062 | -1401.7 | -579.3 | |
| 0 | 4 | 0 | 2 | -22.86 | 306.11 | 25.16 | 221.20 | 0.5971 | -865.0 | -762.5 | |
| 16 | 179 | 10 | 111 | -23.98 | 305.83 | 24.88 | 219.57 | 0.6057 | -1191.5 | -601.4 | |
| 6 | -3 | 4 | -3 | -23.83 | 305.38 | 24.43 | 219.25 | 0.6002 | -1372.1 | 999999 | |
| 8 | -3 | 5 | -3 | -23.64 | 304.98 | 24.02 | 219.01 | 0.5947 | -1397.0 | 999999 | |
| 0 | 13 | 0 | 8 | -22.98 | 304.44 | 23.48 | 219.17 | 0.5831 | -1143.0 | -863.7 | |
| 2 | 9 | 1 | 5 | -21.81 | 304.23 | 23.28 | 220.33 | 0.5690 | 312.8 | 116.0 | |
| 0 | 41 | 0 | 25 | -22.44 | 303.80 | 22.84 | 219.06 | 0.5717 | -1210.0 | -863.0 | |
| 0 | 5 | 0 | 3 | -22.96 | 303.89 | 22.94 | 218.55 | 0.5780 | -682.0 | -655.7 | |
| 0 | 4 | 0 | 3 | -20.68 | 303.32 | 22.37 | 220.66 | 0.5487 | -530.0 | -403.1 | |
| 0 | 2 | 0 | 1 | -20.37 | 303.06 | 22.10 | 220.71 | 0.5429 | -594.0 | -581.2 | |
| 0 | 4 | 0 | 2 | -20.31 | 302.47 | 21.52 | 220.05 | 0.5367 | -677.0 | -616.9 | |
| 6 | 30 | 3 | 18 | -21.03 | 302.31 | 21.36 | 218.95 | 0.5430 | -1146.8 | -790.3 | |
| 6 | -13 | 3 | -13 | -21.50 | 302.21 | 21.25 | 218.24 | 0.5471 | -811.9 | 999999 | |
| 5 | 11 | 3 | 7 | -21.99 | 299.76 | 18.81 | 214.39 | 0.5314 | 988.5 | 679.6 | |
| 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. | |