SOHO MDI 2000-11-24 04:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 220 | 1507 | 117 | 790 | 20.36 | 357.73 | 2.24 | 353.50 | 0.3232 | 1310.9 | 429.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | 13.44 | 1.75 | 6.26 | 332.62 | 0.2317 | 574.0 | 450.8 | |
| 6 | 1112 | 3 | 581 | 19.43 | 1.38 | 5.89 | 342.45 | 0.3222 | -1107.4 | 656.2 | |
| 0 | 6 | 0 | 3 | 22.19 | 1.36 | 5.87 | 344.91 | 0.3655 | -747.0 | -443.4 | |
| 10 | 46 | 5 | 24 | 21.21 | 1.28 | 5.79 | 344.33 | 0.3497 | -722.0 | -76.9 | |
| 0 | 10 | 0 | 5 | 22.36 | 0.91 | 5.42 | 346.14 | 0.3662 | 437.0 | 328.8 | |
| 0 | 13 | 0 | 7 | 22.81 | 0.76 | 5.27 | 346.81 | 0.3728 | -779.0 | -467.7 | |
| 0 | 13 | 0 | 7 | 21.50 | 0.34 | 4.85 | 346.97 | 0.3505 | 474.0 | 339.6 | |
| 3 | 8 | 2 | 4 | 17.99 | 0.03 | 4.54 | 345.03 | 0.2929 | -836.5 | -741.6 | |
| 0 | 8 | 0 | 4 | 18.43 | 0.05 | 4.55 | 345.40 | 0.3001 | -23.0 | -0.5 | |
| 0 | 4 | 0 | 2 | 21.70 | 359.98 | 4.48 | 348.05 | 0.3524 | 316.0 | 232.9 | |
| 117 | -2 | 61 | -2 | 20.08 | 359.19 | 3.70 | 349.16 | 0.3237 | 1920.5 | 999999 | |
| 0 | 3 | 0 | 1 | 22.81 | 358.85 | 3.35 | 351.51 | 0.3670 | 483.0 | 310.4 | |
| 0 | 6 | 0 | 3 | 23.02 | 358.56 | 3.07 | 352.31 | 0.3696 | -579.0 | -571.2 | |
| 17 | -2 | 9 | -2 | 19.68 | 358.24 | 2.75 | 351.70 | 0.3145 | 2160.8 | 999999 | |
| 3 | 8 | 2 | 4 | 22.28 | 358.25 | 2.76 | 352.80 | 0.3570 | 576.6 | 494.6 | |
| 3 | 13 | 2 | 7 | 22.24 | 357.63 | 2.14 | 354.40 | 0.3552 | 694.6 | 569.3 | |
| 32 | -2 | 17 | -2 | 19.48 | 357.51 | 2.02 | 353.82 | 0.3097 | 2113.1 | 999999 | |
| 0 | 3 | 0 | 2 | 23.10 | 357.35 | 1.86 | 355.34 | 0.3689 | 659.0 | 568.3 | |
| 6 | 55 | 3 | 29 | 21.87 | 356.80 | 1.31 | 356.50 | 0.3481 | 959.4 | 374.6 | |
| 6 | -2 | 3 | -2 | 19.24 | 356.69 | 1.20 | 356.25 | 0.3045 | 1581.4 | 999999 | |
| 3 | -19 | 2 | -19 | 22.16 | 356.55 | 1.06 | 357.20 | 0.3526 | -410.0 | 999999 | |
| 0 | 12 | 0 | 6 | 20.90 | 356.38 | 0.89 | 357.49 | 0.3317 | -65.0 | -67.2 | |
| 0 | 5 | 0 | 3 | 18.72 | 355.84 | 0.35 | 358.88 | 0.2952 | 414.0 | 335.2 | |
| 0 | 4 | 0 | 2 | 20.45 | 355.48 | -0.02 | 0.05 | 0.3240 | -547.0 | -445.3 | |
| 0 | 3 | 0 | 2 | 18.88 | 355.36 | -0.14 | 0.44 | 0.2978 | 600.0 | 410.2 | |
| 0 | 27 | 0 | 14 | 19.68 | 355.27 | -0.22 | 0.67 | 0.3112 | 10.0 | -79.5 | |
| 0 | 11 | 0 | 6 | 18.48 | 355.15 | -0.34 | 1.11 | 0.2911 | -1138.0 | -672.8 | |
| 0 | 7 | 0 | 3 | 19.32 | 352.96 | -2.53 | 7.82 | 0.3080 | 739.0 | 649.0 | |
| 0 | 4 | 0 | 2 | 19.43 | 350.43 | -5.06 | 15.22 | 0.3184 | -854.0 | -753.7 | |
| 0 | 6 | 0 | 3 | 23.26 | 350.17 | -5.32 | 13.01 | 0.3801 | -698.0 | -601.8 | |
| 0 | 5 | 0 | 3 | 23.14 | 349.80 | -5.69 | 13.97 | 0.3795 | -1054.0 | -924.3 | |
| 0 | 9 | 0 | 5 | 23.26 | 349.46 | -6.03 | 14.68 | 0.3828 | -901.0 | -829.1 | |
| 0 | 4 | 0 | 2 | 23.67 | 349.10 | -6.39 | 15.19 | 0.3907 | -1049.0 | -891.7 | |
| 0 | 5 | 0 | 3 | 21.50 | 348.87 | -6.62 | 17.51 | 0.3581 | -625.0 | -585.2 | |
| 0 | 19 | 0 | 10 | 23.88 | 348.71 | -6.78 | 15.91 | 0.3956 | -1159.0 | -885.5 | |
| 0 | 22 | 0 | 12 | 24.00 | 347.95 | -7.55 | 17.49 | 0.4010 | -831.0 | -717.1 | |
| 0 | 5 | 0 | 3 | 23.13 | 347.74 | -7.75 | 18.68 | 0.3888 | -702.0 | -528.5 | |
| 0 | 4 | 0 | 2 | 26.09 | 347.17 | -8.32 | 17.43 | 0.4360 | -621.0 | -512.2 | |
| 0 | 7 | 0 | 4 | 22.88 | 346.71 | -8.78 | 21.20 | 0.3907 | -674.0 | -603.0 | |
| 14 | 27 | 8 | 14 | 22.35 | 346.66 | -8.83 | 21.86 | 0.3831 | -1250.9 | -834.7 | |
| 0 | 7 | 0 | 4 | 21.32 | 346.43 | -9.06 | 23.51 | 0.3694 | -1036.0 | -727.0 | |
| 0 | 3 | 0 | 2 | 25.05 | 341.11 | -14.38 | 29.47 | 0.4593 | -678.0 | -567.5 | |
| 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. | |