SOHO MDI 2000-10-28 04:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 88 | 583 | 72 | 461 | -22.70 | 306.98 | -44.25 | 124.28 | 0.7811 | -846.2 | -231.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 63 | 10 | 48 | -23.76 | 310.07 | -41.17 | 127.22 | 0.7589 | -851.5 | -545.7 | |
| 19 | 90 | 15 | 70 | -23.56 | 308.27 | -42.96 | 125.95 | 0.7740 | -911.1 | -305.1 | |
| 18 | 169 | 14 | 130 | -21.95 | 308.56 | -42.68 | 124.25 | 0.7630 | -1357.7 | -480.4 | |
| 11 | -3 | 9 | -3 | -22.11 | 307.92 | -43.31 | 124.09 | 0.7697 | -794.6 | 999999 | |
| 0 | 6 | 0 | 5 | -20.41 | 307.98 | -43.25 | 122.12 | 0.7606 | -224.0 | -40.6 | |
| 2 | 9 | 2 | 7 | -22.33 | 306.50 | -44.73 | 123.57 | 0.7837 | -656.7 | -561.0 | |
| 0 | 9 | 0 | 7 | -22.87 | 306.04 | -45.20 | 123.96 | 0.7905 | -558.0 | -431.7 | |
| 0 | 3 | 0 | 3 | -21.73 | 306.51 | -44.73 | 122.89 | 0.7808 | -239.0 | -341.7 | |
| 10 | 126 | 9 | 104 | -24.05 | 305.21 | -46.02 | 124.86 | 0.8032 | -729.3 | -223.3 | |
| 12 | -9 | 10 | -9 | -23.63 | 304.91 | -46.32 | 124.25 | 0.8038 | -765.1 | 999999 | |
| 0 | 3 | 0 | 2 | -19.92 | 306.20 | -45.03 | 120.62 | 0.7753 | 484.0 | 538.1 | |
| 0 | 4 | 0 | 3 | -22.11 | 305.04 | -46.20 | 122.59 | 0.7959 | -4.0 | -137.2 | |
| 0 | 5 | 0 | 4 | -20.47 | 305.53 | -45.71 | 120.93 | 0.7841 | 696.0 | 551.7 | |
| 0 | 6 | 0 | 5 | -23.34 | 304.06 | -47.17 | 123.50 | 0.8098 | -107.0 | -243.2 | |
| 3 | 71 | 3 | 57 | -21.10 | 304.92 | -46.31 | 121.37 | 0.7924 | 462.1 | 680.8 | |
| 0 | 4 | 0 | 3 | -20.38 | 304.85 | -46.39 | 120.50 | 0.7900 | 551.0 | 376.6 | |
| 0 | 3 | 0 | 3 | -21.74 | 303.55 | -47.68 | 121.45 | 0.8074 | -589.0 | -481.9 | |
| 0 | 12 | 0 | 10 | -21.57 | 302.88 | -48.35 | 120.95 | 0.8126 | -708.0 | -557.9 | |
| 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. | |