SOHO MDI 2000-07-03 05:51:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89 | 506 | 74 | 409 | -19.12 | 48.72 | -47.86 | 117.40 | 0.7893 | -468.0 | -122.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18 | 322 | 14 | 244 | -18.20 | 52.05 | -44.53 | 117.68 | 0.7546 | -1559.9 | -413.3 | |
| 4 | -1 | 3 | -1 | -19.06 | 51.58 | -45.00 | 118.53 | 0.7630 | -826.6 | 999999 | |
| -1 | -1 | -1 | -1 | -17.82 | 51.88 | -44.70 | 117.14 | 0.7548 | 999999 | 999999 | |
| 11 | -1 | 8 | -1 | -18.48 | 51.37 | -45.21 | 117.72 | 0.7627 | -824.2 | 999999 | |
| 15 | -1 | 12 | -1 | -18.02 | 51.29 | -45.30 | 117.11 | 0.7616 | -983.7 | 999999 | |
| 0 | 4 | 0 | 3 | -17.38 | 50.42 | -46.16 | 115.95 | 0.7679 | -504.0 | -365.1 | |
| 0 | 3 | 0 | 3 | -18.31 | 48.44 | -48.15 | 116.26 | 0.7908 | 583.0 | 497.7 | |
| 13 | 23 | 12 | 20 | -21.62 | 46.25 | -50.33 | 119.26 | 0.8224 | -494.1 | -330.9 | |
| 3 | 73 | 2 | 63 | -19.28 | 46.64 | -49.94 | 116.71 | 0.8110 | 919.5 | 571.4 | |
| 7 | -9 | 6 | -9 | -19.69 | 46.00 | -50.58 | 116.94 | 0.8181 | 664.6 | 999999 | |
| 11 | -9 | 10 | -9 | -19.46 | 45.36 | -51.22 | 116.44 | 0.8231 | 480.6 | 999999 | |
| 0 | 9 | 0 | 9 | -22.22 | 43.44 | -53.14 | 118.88 | 0.8480 | 453.0 | 529.9 | |
| 0 | 6 | 0 | 5 | -20.03 | 44.14 | -52.44 | 116.66 | 0.8355 | 458.0 | 404.8 | |
| 2 | 66 | 2 | 62 | -21.17 | 42.79 | -53.79 | 117.47 | 0.8502 | 628.5 | 228.5 | |
| 5 | -14 | 5 | -14 | -21.11 | 42.16 | -54.42 | 117.20 | 0.8551 | 309.7 | 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. | |