SOHO MDI 2000-09-26 23:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28 | 158 | 24 | 138 | -12.20 | 349.74 | -52.87 | 109.86 | 0.8288 | -15.1 | 53.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5 | 18 | 4 | 13 | -12.02 | 356.76 | -45.85 | 112.32 | 0.7610 | -810.2 | -773.5 | |
| 10 | 22 | 7 | 17 | -11.61 | 356.27 | -46.34 | 111.61 | 0.7645 | -768.8 | -468.7 | |
| 0 | 4 | 0 | 3 | -10.94 | 356.07 | -46.55 | 110.69 | 0.7642 | -432.0 | -473.2 | |
| 0 | 5 | 0 | 4 | -12.41 | 351.27 | -51.34 | 110.57 | 0.8168 | -435.0 | -266.5 | |
| 0 | 6 | 0 | 6 | -13.55 | 349.22 | -53.40 | 111.15 | 0.8390 | -136.0 | -145.7 | |
| 0 | 5 | 0 | 4 | -12.35 | 349.39 | -53.23 | 109.83 | 0.8340 | 353.0 | 425.0 | |
| 1 | 7 | 1 | 6 | -13.83 | 348.51 | -54.11 | 111.22 | 0.8459 | -240.8 | -149.0 | |
| 0 | 6 | 0 | 5 | -13.20 | 348.65 | -53.96 | 110.55 | 0.8429 | 493.0 | 367.5 | |
| 0 | 4 | 0 | 4 | -11.81 | 348.67 | -53.95 | 108.97 | 0.8389 | 449.0 | 393.9 | |
| 0 | 7 | 0 | 6 | -13.88 | 347.58 | -55.03 | 110.96 | 0.8540 | 623.0 | 566.4 | |
| 2 | 11 | 2 | 10 | -11.29 | 348.13 | -54.48 | 108.20 | 0.8424 | 801.9 | 607.0 | |
| 0 | 4 | 0 | 4 | -13.59 | 347.27 | -55.35 | 110.52 | 0.8559 | 346.0 | 375.1 | |
| 0 | 11 | 0 | 10 | -13.31 | 346.72 | -55.90 | 110.03 | 0.8597 | 112.0 | 219.9 | |
| 10 | 42 | 10 | 40 | -11.83 | 346.85 | -55.76 | 108.41 | 0.8549 | 649.9 | 233.6 | |
| 0 | 6 | 0 | 6 | -10.54 | 346.30 | -56.31 | 106.79 | 0.8565 | 468.0 | 346.7 | |
| 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. | |