SOHO MDI 2000-07-15 22:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66 | 368 | 34 | 193 | 3.13 | 270.97 | -17.61 | 93.89 | 0.3039 | -948.2 | -268.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | 4.03 | 277.86 | -10.73 | 92.10 | 0.1867 | 663.0 | 621.3 | |
| 8 | 17 | 4 | 9 | 2.67 | 276.94 | -11.64 | 98.54 | 0.2048 | 1247.2 | 832.7 | |
| 0 | 10 | 0 | 5 | 3.73 | 276.40 | -12.18 | 93.16 | 0.2118 | 708.0 | 611.1 | |
| 4 | 55 | 2 | 28 | 3.39 | 275.07 | -13.52 | 94.20 | 0.2350 | 1327.3 | 911.7 | |
| 0 | 8 | 0 | 4 | 3.78 | 274.78 | -13.81 | 92.46 | 0.2394 | 810.0 | 722.2 | |
| 0 | 5 | 0 | 3 | 2.63 | 274.43 | -14.16 | 97.06 | 0.2473 | 744.0 | 632.3 | |
| 0 | 9 | 0 | 5 | 3.93 | 272.19 | -16.40 | 91.38 | 0.2830 | -740.0 | -659.0 | |
| 0 | 5 | 0 | 3 | 3.87 | 271.53 | -17.06 | 91.47 | 0.2941 | -902.0 | -708.2 | |
| 0 | 4 | 0 | 2 | 3.47 | 271.33 | -17.26 | 92.78 | 0.2978 | -721.0 | -669.0 | |
| 0 | 6 | 0 | 3 | 1.60 | 269.31 | -19.27 | 97.96 | 0.3346 | -769.0 | -684.3 | |
| 21 | 213 | 11 | 112 | 3.03 | 269.29 | -19.29 | 93.69 | 0.3321 | -1742.7 | -651.4 | |
| -11 | -11 | -11 | -11 | 3.38 | 269.24 | -19.34 | 92.61 | 0.3325 | 999999 | 999999 | |
| 6 | -11 | 3 | -11 | 3.77 | 269.02 | -19.56 | 91.40 | 0.3357 | -1288.9 | 999999 | |
| 15 | -11 | 8 | -11 | 3.06 | 268.95 | -19.63 | 93.51 | 0.3376 | -1441.6 | 999999 | |
| 12 | 30 | 6 | 16 | 1.62 | 268.64 | -19.95 | 97.59 | 0.3455 | -1131.4 | -799.7 | |
| 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. | |