SOHO MDI 2000-07-15 23:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66 | 348 | 33 | 180 | 3.05 | 271.03 | -16.67 | 94.60 | 0.2884 | -740.1 | -275.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 7 | 0 | 4 | 1.68 | 278.44 | -9.26 | 106.69 | 0.1687 | 599.0 | 631.2 | |
| 0 | 5 | 0 | 2 | 4.20 | 277.54 | -10.17 | 91.33 | 0.1769 | 969.0 | 783.9 | |
| 7 | 16 | 4 | 8 | 2.69 | 276.87 | -10.83 | 99.17 | 0.1911 | 1188.7 | 827.4 | |
| 0 | 15 | 0 | 8 | 3.62 | 275.52 | -12.18 | 93.73 | 0.2119 | 1261.0 | 1019.1 | |
| 0 | 3 | 0 | 2 | 2.90 | 275.21 | -12.49 | 96.90 | 0.2186 | 757.0 | 705.8 | |
| 0 | 13 | 0 | 7 | 3.81 | 275.20 | -12.51 | 92.73 | 0.2173 | 939.0 | 885.6 | |
| 9 | 28 | 4 | 14 | 3.33 | 275.04 | -12.66 | 94.85 | 0.2206 | 1231.5 | 854.5 | |
| 0 | 6 | 0 | 3 | 2.81 | 274.93 | -12.78 | 97.11 | 0.2236 | 868.0 | 765.1 | |
| 0 | 6 | 0 | 3 | 2.57 | 274.40 | -13.30 | 97.85 | 0.2331 | 625.0 | 557.7 | |
| 0 | 7 | 0 | 4 | 3.86 | 271.51 | -16.19 | 91.69 | 0.2795 | -790.0 | -605.5 | |
| 0 | 7 | 0 | 3 | 3.50 | 271.35 | -16.35 | 92.94 | 0.2826 | -710.0 | -684.1 | |
| 0 | 6 | 0 | 3 | 1.59 | 269.43 | -18.27 | 98.51 | 0.3183 | -745.0 | -568.2 | |
| 8 | 198 | 4 | 103 | 2.97 | 269.29 | -18.41 | 94.12 | 0.3177 | -1862.9 | -701.9 | |
| 6 | -13 | 3 | -13 | 3.41 | 269.24 | -18.46 | 92.74 | 0.3179 | -1715.8 | 999999 | |
| 13 | -13 | 7 | -13 | 3.05 | 269.04 | -18.67 | 93.82 | 0.3217 | -1532.9 | 999999 | |
| 8 | -13 | 4 | -13 | 3.76 | 269.02 | -18.68 | 91.60 | 0.3211 | -1385.7 | 999999 | |
| 4 | -13 | 2 | -13 | 2.88 | 268.79 | -18.91 | 94.26 | 0.3261 | -1002.3 | 999999 | |
| 9 | 31 | 4 | 16 | 1.69 | 268.64 | -19.07 | 97.81 | 0.3310 | -1081.0 | -848.1 | |
| 2 | -18 | 1 | -18 | 1.41 | 268.60 | -19.11 | 98.62 | 0.3324 | -1136.7 | 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. | |