SOHO MDI 2000-09-29 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 172 | 1049 | 92 | 558 | -11.18 | 352.41 | -10.63 | 150.58 | 0.3616 | -181.6 | 47.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 407 | 8 | 212 | -10.24 | 357.65 | -5.38 | 162.42 | 0.3071 | -2338.4 | -746.3 | |
| 33 | -1 | 17 | -1 | -10.82 | 357.40 | -5.63 | 162.24 | 0.3175 | -2076.8 | 999999 | |
| 7 | -1 | 4 | -1 | -10.37 | 357.17 | -5.86 | 161.10 | 0.3116 | -2124.4 | 999999 | |
| 9 | -1 | 5 | -1 | -10.62 | 356.89 | -6.15 | 160.52 | 0.3171 | -1677.5 | 999999 | |
| 8 | -1 | 4 | -1 | -10.87 | 356.61 | -6.43 | 159.97 | 0.3225 | -1129.9 | 999999 | |
| 0 | 16 | 0 | 8 | -11.33 | 356.00 | -7.04 | 158.76 | 0.3332 | -389.0 | -379.2 | |
| 0 | 10 | 0 | 5 | -12.44 | 355.77 | -7.27 | 159.33 | 0.3516 | -745.0 | -586.8 | |
| 0 | 3 | 0 | 2 | -11.21 | 355.44 | -7.60 | 157.11 | 0.3348 | -787.0 | -568.5 | |
| 0 | 5 | 0 | 3 | -12.03 | 355.42 | -7.62 | 157.98 | 0.3474 | -439.0 | -302.8 | |
| 0 | 6 | 0 | 3 | -12.82 | 355.23 | -7.80 | 158.35 | 0.3605 | -753.0 | -448.6 | |
| 0 | 4 | 0 | 2 | -10.69 | 355.21 | -7.82 | 155.85 | 0.3284 | -398.0 | -316.8 | |
| 0 | 6 | 0 | 3 | -11.06 | 354.76 | -8.27 | 155.11 | 0.3370 | -792.0 | -639.5 | |
| 0 | 6 | 0 | 3 | -10.33 | 354.62 | -8.41 | 153.77 | 0.3272 | -561.0 | -545.5 | |
| 0 | 4 | 0 | 2 | -10.62 | 354.42 | -8.62 | 153.61 | 0.3329 | -658.0 | -473.6 | |
| 0 | 5 | 0 | 2 | -11.77 | 354.02 | -9.02 | 154.10 | 0.3528 | 713.0 | 636.3 | |
| 0 | 7 | 0 | 4 | -12.27 | 353.84 | -9.20 | 154.27 | 0.3613 | 929.0 | 764.9 | |
| 0 | 5 | 0 | 3 | -11.08 | 353.60 | -9.44 | 152.14 | 0.3458 | -310.0 | -204.1 | |
| 0 | 4 | 0 | 2 | -10.15 | 353.55 | -9.49 | 150.67 | 0.3327 | -741.0 | -632.5 | |
| 0 | 2 | 0 | 1 | -11.55 | 352.94 | -10.10 | 151.15 | 0.3576 | -51.0 | -116.0 | |
| 0 | 9 | 0 | 5 | -11.06 | 352.75 | -10.28 | 150.03 | 0.3522 | 1041.0 | 696.8 | |
| 0 | 3 | 0 | 2 | -10.01 | 352.31 | -10.73 | 147.35 | 0.3413 | -546.0 | -436.2 | |
| 0 | 5 | 0 | 3 | -15.30 | 351.91 | -11.12 | 153.49 | 0.4186 | -638.0 | -560.1 | |
| 7 | 234 | 4 | 125 | -11.45 | 351.69 | -11.35 | 148.11 | 0.3665 | 1352.2 | 605.9 | |
| 3 | -23 | 2 | -23 | -11.59 | 351.20 | -11.84 | 147.20 | 0.3726 | 1426.3 | 999999 | |
| 9 | -23 | 5 | -23 | -11.26 | 351.05 | -11.99 | 146.39 | 0.3696 | 1772.9 | 999999 | |
| 7 | -23 | 4 | -23 | -12.17 | 350.85 | -12.19 | 147.29 | 0.3836 | 772.2 | 999999 | |
| 11 | -23 | 6 | -23 | -11.80 | 350.70 | -12.34 | 146.44 | 0.3800 | -778.9 | 999999 | |
| 9 | -23 | 5 | -23 | -11.35 | 350.68 | -12.36 | 145.72 | 0.3741 | 686.6 | 999999 | |
| 13 | -23 | 7 | -23 | -12.27 | 350.23 | -12.81 | 146.14 | 0.3904 | 973.7 | 999999 | |
| 0 | 7 | 0 | 4 | -13.13 | 349.08 | -13.96 | 145.07 | 0.4120 | 722.0 | 497.2 | |
| 0 | 7 | 0 | 4 | -11.93 | 349.06 | -13.98 | 143.27 | 0.3968 | 750.0 | 651.4 | |
| 4 | 11 | 2 | 6 | -11.41 | 348.72 | -14.32 | 141.78 | 0.3935 | 1210.3 | 904.1 | |
| 0 | 7 | 0 | 4 | -10.46 | 347.91 | -15.13 | 138.64 | 0.3901 | 930.0 | 859.6 | |
| 4 | 259 | 2 | 141 | -11.99 | 347.33 | -15.71 | 140.10 | 0.4146 | 934.0 | 714.2 | |
| 0 | 4 | 0 | 2 | -13.37 | 346.74 | -16.29 | 141.17 | 0.4371 | 431.0 | 413.8 | |
| 0 | 13 | 0 | 7 | -12.38 | 346.77 | -16.27 | 139.71 | 0.4250 | 1078.0 | 771.0 | |
| 23 | -34 | 12 | -34 | -11.28 | 346.55 | -16.49 | 137.56 | 0.4143 | 1663.8 | 999999 | |
| 9 | -34 | 5 | -34 | -10.67 | 346.33 | -16.70 | 136.17 | 0.4096 | 1622.1 | 999999 | |
| 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. | |