SOHO MDI 2000-07-15 01:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 440 | 42 | 253 | 3.01 | 270.00 | -30.06 | 91.66 | 0.5019 | -609.8 | -306.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 31 | 7 | 17 | 2.52 | 276.91 | -23.15 | 93.90 | 0.3954 | 1319.9 | 874.1 | |
| 0 | 9 | 0 | 5 | 1.93 | 276.87 | -23.19 | 95.40 | 0.3969 | 996.0 | 727.4 | |
| 0 | 4 | 0 | 2 | 4.13 | 276.30 | -23.76 | 89.79 | 0.4035 | 532.0 | 634.5 | |
| 0 | 13 | 0 | 7 | 3.70 | 275.45 | -24.61 | 90.75 | 0.4174 | 637.0 | 569.1 | |
| 0 | 5 | 0 | 3 | 2.65 | 274.73 | -25.33 | 93.13 | 0.4298 | 828.0 | 625.0 | |
| 6 | 12 | 3 | 7 | 2.88 | 274.33 | -25.73 | 92.54 | 0.4358 | 804.9 | 627.3 | |
| 0 | 4 | 0 | 2 | 3.28 | 273.48 | -26.58 | 91.49 | 0.4487 | 420.0 | 305.5 | |
| 0 | 6 | 0 | 3 | 2.91 | 272.87 | -27.19 | 92.24 | 0.4586 | 624.0 | 511.3 | |
| 0 | 9 | 0 | 5 | 4.08 | 271.39 | -28.67 | 89.57 | 0.4805 | -749.0 | -769.5 | |
| 0 | 6 | 0 | 4 | 2.66 | 270.49 | -29.57 | 92.39 | 0.4954 | -684.0 | -560.0 | |
| 0 | 2 | 0 | 1 | 2.26 | 270.36 | -29.70 | 93.18 | 0.4978 | 182.0 | 206.1 | |
| 0 | 5 | 0 | 3 | 1.52 | 269.73 | -30.33 | 94.52 | 0.5084 | 589.0 | 487.0 | |
| 14 | 334 | 8 | 194 | 3.51 | 268.99 | -31.07 | 90.53 | 0.5172 | -1368.3 | -542.3 | |
| 17 | -13 | 10 | -13 | 3.15 | 268.82 | -31.24 | 91.21 | 0.5201 | -1457.4 | 999999 | |
| -14 | -13 | -14 | -13 | 2.86 | 268.64 | -31.42 | 91.74 | 0.5230 | 999999 | 999999 | |
| 4 | -13 | 2 | -13 | 2.31 | 268.51 | -31.54 | 92.79 | 0.5254 | -1212.4 | 999999 | |
| 10 | -13 | 6 | -13 | 3.33 | 268.30 | -31.76 | 90.82 | 0.5276 | -956.7 | 999999 | |
| 7 | -13 | 4 | -13 | 2.41 | 268.23 | -31.83 | 92.54 | 0.5295 | -973.7 | 999999 | |
| 3 | -13 | 2 | -13 | 2.85 | 268.17 | -31.89 | 91.71 | 0.5299 | -789.5 | 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. | |