SOHO MDI 2000-09-26 22:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28 | 158 | 24 | 142 | -12.16 | 350.14 | -53.36 | 109.65 | 0.8329 | -160.8 | -10.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 42 | 5 | 33 | -12.02 | 356.77 | -46.73 | 111.94 | 0.7701 | -843.0 | -642.8 | |
| 0 | 3 | 0 | 2 | -11.16 | 356.84 | -46.65 | 110.91 | 0.7661 | -432.0 | -395.6 | |
| 9 | -1 | 7 | -1 | -11.57 | 356.28 | -47.21 | 111.19 | 0.7734 | -824.3 | 999999 | |
| 0 | 4 | 0 | 3 | -10.94 | 356.13 | -47.37 | 110.34 | 0.7727 | -571.0 | -416.9 | |
| 0 | 10 | 0 | 9 | -12.30 | 351.14 | -52.36 | 110.09 | 0.8259 | -441.0 | -275.2 | |
| 0 | 5 | 0 | 5 | -13.53 | 349.14 | -54.36 | 110.79 | 0.8473 | -270.0 | -217.9 | |
| 0 | 5 | 0 | 4 | -12.31 | 349.39 | -54.10 | 109.50 | 0.8417 | 359.0 | 392.2 | |
| 0 | 5 | 0 | 5 | -10.95 | 349.58 | -53.92 | 108.00 | 0.8364 | -192.0 | -116.2 | |
| 1 | 6 | 1 | 5 | -13.85 | 348.40 | -55.10 | 110.90 | 0.8545 | -202.0 | -119.1 | |
| 0 | 17 | 0 | 17 | -13.95 | 347.43 | -56.06 | 110.69 | 0.8627 | 635.0 | 426.0 | |
| 0 | 11 | 0 | 10 | -11.30 | 348.17 | -55.33 | 107.94 | 0.8498 | 811.0 | 622.7 | |
| 0 | 6 | 0 | 6 | -13.27 | 346.81 | -56.69 | 109.74 | 0.8662 | 435.0 | 191.8 | |
| 11 | 34 | 11 | 33 | -11.79 | 346.87 | -56.62 | 108.11 | 0.8621 | 522.4 | 220.9 | |
| 0 | 4 | 0 | 4 | -12.43 | 346.66 | -56.83 | 108.75 | 0.8653 | 311.0 | 152.6 | |
| 0 | 6 | 0 | 6 | -10.48 | 346.25 | -57.25 | 106.45 | 0.8643 | 490.0 | 397.5 | |
| 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. | |