SOHO MDI 2000-10-27 15:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90 | 530 | 79 | 482 | -22.74 | 307.29 | -50.97 | 121.17 | 0.8391 | -477.2 | -148.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 61 | 10 | 52 | -23.91 | 309.96 | -48.30 | 123.63 | 0.8220 | -776.4 | -501.5 | |
| 0 | 5 | 0 | 4 | -20.10 | 310.75 | -47.52 | 119.68 | 0.7994 | 541.0 | 441.6 | |
| 16 | 94 | 14 | 84 | -23.59 | 308.32 | -49.95 | 122.53 | 0.8342 | -786.0 | -228.0 | |
| 23 | 155 | 20 | 136 | -22.02 | 308.51 | -49.75 | 120.88 | 0.8266 | -960.8 | -308.2 | |
| 0 | 3 | 0 | 3 | -20.29 | 309.05 | -49.21 | 119.15 | 0.8154 | 755.0 | 641.6 | |
| 0 | 8 | 0 | 7 | -20.40 | 307.97 | -50.29 | 118.82 | 0.8252 | 635.0 | 492.1 | |
| 1 | 7 | 1 | 7 | -22.28 | 306.67 | -51.59 | 120.38 | 0.8427 | -284.0 | -320.9 | |
| 0 | 4 | 0 | 4 | -21.55 | 306.71 | -51.56 | 119.59 | 0.8399 | 194.0 | 150.5 | |
| 0 | 5 | 0 | 4 | -20.13 | 306.99 | -51.28 | 118.12 | 0.8327 | 904.0 | 756.3 | |
| 10 | 124 | 9 | 121 | -23.99 | 304.87 | -53.39 | 121.54 | 0.8625 | -625.2 | -121.2 | |
| 0 | 4 | 0 | 4 | -22.48 | 305.61 | -52.66 | 120.18 | 0.8519 | -41.0 | -159.5 | |
| 5 | -10 | 4 | -10 | -23.56 | 304.92 | -53.34 | 121.09 | 0.8608 | -1117.4 | 999999 | |
| 14 | 40 | 12 | 36 | -20.63 | 306.42 | -51.85 | 118.46 | 0.8392 | 981.8 | 730.3 | |
| 0 | 5 | 0 | 5 | -21.48 | 305.79 | -52.47 | 119.15 | 0.8472 | -45.0 | -19.0 | |
| 0 | 3 | 0 | 3 | -20.00 | 306.38 | -51.88 | 117.74 | 0.8374 | 554.0 | 401.8 | |
| 9 | -10 | 9 | -10 | -23.59 | 304.47 | -53.79 | 120.95 | 0.8642 | -287.3 | 999999 | |
| 0 | 9 | 0 | 9 | -21.68 | 303.50 | -54.76 | 118.52 | 0.8658 | -705.0 | -487.2 | |
| 0 | 3 | 0 | 3 | -21.79 | 302.56 | -55.71 | 118.30 | 0.8733 | -217.0 | -231.3 | |
| 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. | |