SOHO MDI 2000-07-26 22:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 372 | 26 | 235 | -30.69 | 130.62 | -12.34 | 162.91 | 0.6204 | -1197.8 | -285.2 | |
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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 | -36.17 | 132.83 | -10.13 | 167.91 | 0.6806 | -728.0 | -537.6 | |
| 33 | 294 | 20 | 183 | -30.33 | 132.98 | -9.98 | 165.63 | 0.6048 | -1612.4 | -487.6 | |
| 6 | -2 | 4 | -2 | -30.73 | 132.85 | -10.11 | 165.63 | 0.6105 | -1017.1 | 999999 | |
| -2 | -2 | -2 | -2 | -30.49 | 132.60 | -10.37 | 165.17 | 0.6082 | 999999 | 999999 | |
| 0 | 10 | 0 | 7 | -30.96 | 127.05 | -15.92 | 158.29 | 0.6380 | -419.0 | -423.2 | |
| 0 | 5 | 0 | 3 | -29.93 | 124.01 | -18.95 | 153.91 | 0.6423 | 607.0 | 609.6 | |
| 0 | 3 | 0 | 2 | -33.04 | 122.84 | -20.12 | 154.97 | 0.6840 | 372.0 | 345.6 | |
| 3 | 12 | 2 | 8 | -29.96 | 123.23 | -19.73 | 153.03 | 0.6472 | 921.9 | 776.5 | |
| 0 | 4 | 0 | 2 | -30.90 | 122.74 | -20.22 | 153.23 | 0.6608 | 267.0 | 255.6 | |
| 0 | 10 | 0 | 7 | -32.52 | 121.96 | -21.00 | 153.65 | 0.6831 | 421.0 | 616.7 | |
| 0 | 13 | 0 | 9 | -31.12 | 122.20 | -20.77 | 152.80 | 0.6665 | 934.0 | 743.5 | |
| 0 | 3 | 0 | 2 | -30.60 | 121.67 | -21.29 | 151.81 | 0.6639 | 454.0 | 615.1 | |
| 0 | 3 | 0 | 2 | -30.11 | 121.74 | -21.23 | 151.47 | 0.6581 | 668.0 | 604.6 | |
| 0 | 5 | 0 | 3 | -30.28 | 121.16 | -21.81 | 150.98 | 0.6636 | 583.0 | 527.2 | |
| 0 | 7 | 0 | 5 | -34.29 | 117.17 | -25.80 | 150.35 | 0.7291 | 320.0 | 393.5 | |
| 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. | |