SOHO MDI 2000-11-01 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67 | 465 | 40 | 272 | -23.24 | 305.93 | 17.95 | 211.74 | 0.5405 | -1332.8 | -595.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 4 | -23.89 | 311.68 | 23.70 | 218.32 | 0.5951 | -536.0 | -536.2 | |
| 0 | 5 | 0 | 3 | -20.54 | 310.06 | 22.08 | 220.42 | 0.5451 | -636.0 | -578.2 | |
| 0 | 4 | 0 | 2 | -22.68 | 310.19 | 22.20 | 217.96 | 0.5691 | -699.0 | -638.0 | |
| 4 | 11 | 2 | 6 | -23.31 | 308.27 | 20.29 | 214.83 | 0.5598 | -603.1 | -422.3 | |
| 20 | 113 | 12 | 66 | -22.43 | 307.38 | 19.40 | 214.65 | 0.5421 | -1573.2 | -697.5 | |
| 0 | 5 | 0 | 3 | -24.15 | 306.97 | 18.99 | 212.22 | 0.5591 | -556.0 | -441.9 | |
| 0 | 4 | 0 | 2 | -23.31 | 306.40 | 18.42 | 212.34 | 0.5446 | -568.0 | -418.5 | |
| 3 | 12 | 2 | 7 | -22.61 | 305.91 | 17.93 | 212.41 | 0.5323 | -1197.8 | -843.9 | |
| 0 | 13 | 0 | 8 | -25.23 | 306.07 | 18.08 | 209.92 | 0.5652 | -375.0 | -123.0 | |
| 23 | 171 | 14 | 101 | -23.90 | 305.60 | 17.62 | 210.61 | 0.5457 | -1336.4 | -578.8 | |
| 0 | 5 | 0 | 3 | -22.85 | 305.19 | 17.21 | 211.13 | 0.5297 | -829.0 | -672.6 | |
| 0 | 4 | 0 | 2 | -24.94 | 305.31 | 17.33 | 209.17 | 0.5563 | -376.0 | -316.2 | |
| 12 | -10 | 7 | -10 | -23.54 | 305.02 | 17.04 | 210.16 | 0.5369 | -1496.2 | 999999 | |
| 0 | 5 | 0 | 3 | -22.49 | 304.71 | 16.73 | 210.80 | 0.5216 | -1009.0 | -898.2 | |
| 0 | 17 | 0 | 10 | -25.56 | 305.04 | 17.06 | 208.22 | 0.5620 | 532.0 | 256.7 | |
| 2 | 78 | 1 | 45 | -22.96 | 304.51 | 16.53 | 210.01 | 0.5259 | -1223.1 | -805.4 | |
| 3 | -16 | 2 | -16 | -22.14 | 304.15 | 16.17 | 210.33 | 0.5128 | -1251.6 | 999999 | |
| 0 | 7 | 0 | 4 | -25.33 | 304.56 | 16.58 | 207.77 | 0.5559 | -593.0 | -442.2 | |
| 0 | 5 | 0 | 3 | -22.11 | 303.15 | 15.17 | 208.81 | 0.5052 | 45.0 | 24.8 | |
| 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. | |