SOHO MDI 2000-09-27 05:56:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 201 | 34 | 170 | -12.28 | 349.53 | -49.82 | 111.08 | 0.8005 | -5.9 | 69.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 23 | 5 | 17 | -11.95 | 356.69 | -42.65 | 113.74 | 0.7265 | -946.3 | -598.7 | |
| 11 | 20 | 8 | 15 | -11.59 | 356.16 | -43.18 | 113.01 | 0.7307 | -842.8 | -565.3 | |
| 0 | 4 | 0 | 3 | -10.95 | 356.07 | -43.28 | 112.14 | 0.7290 | -527.0 | -371.5 | |
| 0 | 7 | 0 | 6 | -11.56 | 352.32 | -47.02 | 111.24 | 0.7713 | -684.0 | -469.0 | |
| 0 | 4 | 0 | 4 | -11.41 | 351.29 | -48.05 | 110.64 | 0.7814 | 264.0 | 245.3 | |
| 0 | 6 | 0 | 5 | -13.50 | 349.54 | -49.81 | 112.43 | 0.8058 | -250.0 | -146.0 | |
| 0 | 4 | 0 | 3 | -12.86 | 349.28 | -50.07 | 111.58 | 0.8062 | -159.0 | -38.5 | |
| 1 | 8 | 1 | 7 | -13.69 | 348.79 | -50.56 | 112.36 | 0.8135 | -374.3 | -281.3 | |
| 0 | 3 | 0 | 3 | -12.09 | 349.23 | -50.11 | 110.65 | 0.8040 | 391.0 | 435.0 | |
| 0 | 3 | 0 | 2 | -11.90 | 348.65 | -50.69 | 110.21 | 0.8090 | 515.0 | 417.0 | |
| 0 | 3 | 0 | 2 | -11.68 | 348.40 | -50.95 | 109.85 | 0.8108 | 321.0 | 411.1 | |
| 0 | 13 | 0 | 12 | -14.10 | 347.57 | -51.78 | 112.36 | 0.8261 | 638.0 | 478.2 | |
| 0 | 13 | 0 | 11 | -12.88 | 347.81 | -51.53 | 111.05 | 0.8200 | 482.0 | 455.2 | |
| 5 | 11 | 4 | 9 | -11.03 | 347.92 | -51.42 | 108.92 | 0.8134 | 639.6 | 531.3 | |
| 0 | 3 | 0 | 3 | -10.43 | 347.87 | -51.47 | 108.19 | 0.8121 | 459.0 | 460.4 | |
| 4 | 29 | 4 | 26 | -13.59 | 346.88 | -52.47 | 111.52 | 0.8308 | 546.9 | 391.8 | |
| 0 | 3 | 0 | 3 | -12.47 | 346.56 | -52.79 | 110.12 | 0.8303 | 146.0 | 150.9 | |
| 12 | 35 | 10 | 31 | -11.64 | 346.66 | -52.69 | 109.20 | 0.8270 | 565.5 | 99.4 | |
| 2 | 9 | 2 | 8 | -10.62 | 346.33 | -53.01 | 107.90 | 0.8272 | 456.9 | 319.4 | |
| 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. | |