SOHO MDI 2000-11-01 05:36:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 103 | 756 | 56 | 419 | 2.64 | 271.52 | -26.56 | 92.66 | 0.4488 | 1550.7 | 582.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33 | 683 | 18 | 376 | 2.29 | 272.86 | -25.21 | 93.70 | 0.4283 | 2012.3 | 629.1 | |
| 10 | -1 | 5 | -1 | 2.12 | 272.31 | -25.76 | 93.98 | 0.4372 | 1465.1 | 999999 | |
| 10 | -1 | 6 | -1 | 3.41 | 271.85 | -26.22 | 90.96 | 0.4430 | 1607.9 | 999999 | |
| 0 | 6 | 0 | 3 | 0.83 | 271.90 | -26.17 | 96.77 | 0.4461 | 447.0 | 225.0 | |
| 5 | -1 | 3 | -1 | 2.28 | 271.58 | -26.50 | 93.45 | 0.4485 | 1187.1 | 999999 | |
| 29 | -1 | 16 | -1 | 2.90 | 271.44 | -26.64 | 92.06 | 0.4500 | 1591.1 | 999999 | |
| 8 | -1 | 4 | -1 | 2.92 | 271.13 | -26.94 | 91.95 | 0.4547 | 1212.2 | 999999 | |
| 4 | 22 | 2 | 12 | 4.52 | 270.51 | -27.56 | 88.41 | 0.4634 | 792.3 | 538.1 | |
| 4 | -8 | 2 | -8 | 4.51 | 270.21 | -27.87 | 88.43 | 0.4681 | 794.8 | 999999 | |
| 0 | 3 | 0 | 2 | 2.14 | 268.52 | -29.55 | 93.20 | 0.4957 | -621.0 | -569.1 | |
| 0 | 5 | 0 | 3 | 3.91 | 268.42 | -29.65 | 89.61 | 0.4956 | 567.0 | 468.9 | |
| 0 | 6 | 0 | 3 | 2.66 | 266.90 | -31.18 | 91.93 | 0.5195 | 294.0 | 447.2 | |
| 0 | 3 | 0 | 2 | 0.40 | 266.30 | -31.77 | 96.12 | 0.5317 | 615.0 | 574.0 | |
| 0 | 5 | 0 | 3 | -2.01 | 266.10 | -31.98 | 100.50 | 0.5404 | 416.0 | 429.9 | |
| 0 | 6 | 0 | 4 | 0.41 | 265.71 | -32.36 | 95.95 | 0.5403 | 384.0 | 412.0 | |
| 0 | 4 | 0 | 3 | 2.74 | 264.15 | -33.93 | 91.45 | 0.5599 | -628.0 | -595.5 | |
| 0 | 6 | 0 | 3 | 3.54 | 262.99 | -35.08 | 89.93 | 0.5759 | -501.0 | -555.5 | |
| 0 | 4 | 0 | 3 | 3.22 | 260.12 | -37.96 | 90.25 | 0.6164 | -370.0 | -335.5 | |
| 0 | 3 | 0 | 2 | 5.22 | 258.41 | -39.67 | 86.97 | 0.6389 | -532.0 | -501.4 | |
| 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. | |