SOHO MDI 2000-07-03 07:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94 | 527 | 72 | 415 | -19.17 | 48.76 | -46.64 | 118.00 | 0.7777 | -614.6 | -100.6 | |
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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 | -20.64 | 53.59 | -41.82 | 122.07 | 0.7386 | -313.0 | -197.9 | |
| 12 | 332 | 9 | 246 | -18.18 | 52.04 | -43.36 | 118.22 | 0.7426 | -1458.0 | -404.7 | |
| 5 | -2 | 4 | -2 | -19.05 | 51.65 | -43.76 | 119.11 | 0.7505 | -775.5 | 999999 | |
| 39 | -2 | 29 | -2 | -17.76 | 51.94 | -43.46 | 117.65 | 0.7418 | -1165.6 | 999999 | |
| -4 | -2 | -4 | -2 | -18.07 | 51.56 | -43.85 | 117.86 | 0.7472 | 999999 | 999999 | |
| -4 | -2 | -4 | -2 | -18.42 | 51.45 | -43.96 | 118.23 | 0.7498 | 999999 | 999999 | |
| 0 | 4 | 0 | 3 | -17.72 | 49.79 | -45.62 | 116.62 | 0.7638 | 66.0 | 78.1 | |
| 14 | 27 | 11 | 23 | -21.55 | 46.36 | -49.04 | 119.71 | 0.8109 | -637.4 | -276.0 | |
| 0 | 5 | 0 | 4 | -19.62 | 47.19 | -48.21 | 117.80 | 0.7962 | 732.0 | 520.0 | |
| 4 | 59 | 3 | 49 | -19.39 | 46.45 | -48.95 | 117.24 | 0.8023 | 1040.0 | 653.7 | |
| 8 | -10 | 6 | -10 | -19.67 | 46.08 | -49.32 | 117.41 | 0.8067 | 648.9 | 999999 | |
| 4 | -10 | 3 | -10 | -19.54 | 45.09 | -50.32 | 116.88 | 0.8153 | 320.6 | 999999 | |
| 0 | 6 | 0 | 5 | -20.05 | 44.19 | -51.21 | 117.13 | 0.8249 | 448.0 | 358.2 | |
| 5 | 91 | 4 | 83 | -21.15 | 42.76 | -52.64 | 117.86 | 0.8406 | 760.4 | 342.4 | |
| 3 | -14 | 3 | -14 | -21.09 | 42.16 | -53.25 | 117.58 | 0.8455 | 363.2 | 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. | |