SOHO MDI 2000-10-27 14:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 99 | 536 | 93 | 496 | -22.72 | 307.22 | -51.92 | 120.76 | 0.8466 | -438.1 | -141.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11 | 59 | 10 | 52 | -23.91 | 309.93 | -49.21 | 123.22 | 0.8295 | -796.7 | -572.9 | |
| 22 | 88 | 20 | 80 | -23.58 | 308.40 | -50.74 | 122.18 | 0.8406 | -780.7 | -196.3 | |
| 23 | 155 | 21 | 138 | -22.02 | 308.54 | -50.60 | 120.51 | 0.8337 | -895.4 | -274.6 | |
| 0 | 10 | 0 | 9 | -20.29 | 309.09 | -50.05 | 118.79 | 0.8227 | 606.0 | 552.7 | |
| 0 | 5 | 0 | 5 | -20.56 | 308.12 | -51.02 | 118.71 | 0.8320 | 459.0 | 423.9 | |
| 1 | 8 | 1 | 7 | -22.33 | 306.56 | -52.58 | 120.05 | 0.8508 | -211.0 | -247.6 | |
| 0 | 2 | 0 | 2 | -22.95 | 306.21 | -52.93 | 120.59 | 0.8556 | -424.0 | -283.0 | |
| 0 | 5 | 0 | 5 | -21.15 | 306.97 | -52.17 | 118.90 | 0.8436 | 653.0 | 642.4 | |
| 0 | 3 | 0 | 2 | -21.39 | 306.57 | -52.57 | 119.02 | 0.8476 | 554.0 | 483.3 | |
| 9 | 127 | 9 | 126 | -23.99 | 304.88 | -54.26 | 121.21 | 0.8690 | -797.4 | -139.5 | |
| 0 | 3 | 0 | 3 | -22.43 | 305.67 | -53.48 | 119.81 | 0.8582 | -348.0 | -247.2 | |
| 18 | 48 | 17 | 44 | -20.58 | 306.57 | -52.57 | 118.12 | 0.8450 | 931.5 | 648.2 | |
| 0 | 5 | 0 | 4 | -21.39 | 305.88 | -53.26 | 118.76 | 0.8532 | 59.0 | 164.9 | |
| 15 | -10 | 15 | -10 | -23.58 | 304.55 | -54.59 | 120.65 | 0.8702 | -525.9 | 999999 | |
| 0 | 1 | 0 | 1 | -20.46 | 305.25 | -53.89 | 117.49 | 0.8554 | 226.0 | 309.0 | |
| 0 | 5 | 0 | 5 | -22.08 | 304.00 | -55.14 | 118.81 | 0.8699 | 13.0 | -20.2 | |
| 0 | 9 | 0 | 10 | -21.73 | 303.46 | -55.68 | 118.25 | 0.8729 | -721.0 | -544.0 | |
| 0 | 3 | 0 | 3 | -22.02 | 302.99 | -56.15 | 118.40 | 0.8772 | -497.0 | -488.9 | |
| 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. | |