SOHO MDI 2000-10-05 01:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 552 | 68 | 519 | -12.21 | 351.32 | 55.12 | 250.98 | 0.8463 | 80.7 | 91.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15 | 168 | 17 | 192 | -11.10 | 358.49 | 62.29 | 254.39 | 0.9038 | -461.6 | -198.8 | |
| 9 | -1 | 10 | -1 | -11.23 | 357.86 | 61.66 | 254.09 | 0.8995 | -877.3 | 999999 | |
| 0 | 8 | 0 | 8 | -11.82 | 356.84 | 60.63 | 253.20 | 0.8930 | -268.0 | -172.1 | |
| 0 | 3 | 0 | 3 | -12.74 | 351.35 | 55.15 | 250.60 | 0.8508 | -280.0 | -310.2 | |
| 0 | 25 | 0 | 23 | -12.81 | 350.75 | 54.54 | 250.33 | 0.8457 | -624.0 | -335.3 | |
| 0 | 8 | 0 | 7 | -12.58 | 350.13 | 53.93 | 250.38 | 0.8396 | -579.0 | -655.5 | |
| 7 | 14 | 6 | 13 | -11.82 | 349.83 | 53.63 | 251.15 | 0.8349 | -627.3 | -534.5 | |
| 0 | 4 | 0 | 4 | -13.10 | 349.95 | 53.75 | 249.73 | 0.8394 | -352.0 | -339.1 | |
| 0 | 13 | 0 | 11 | -12.80 | 349.39 | 53.18 | 249.88 | 0.8336 | -474.0 | -475.0 | |
| 0 | 13 | 0 | 12 | -13.20 | 348.91 | 52.71 | 249.25 | 0.8304 | -85.0 | -148.9 | |
| 5 | 82 | 4 | 70 | -12.94 | 347.85 | 51.65 | 249.17 | 0.8199 | -191.7 | 323.5 | |
| 8 | -11 | 7 | -11 | -13.37 | 347.66 | 51.45 | 248.60 | 0.8194 | 627.3 | 999999 | |
| 0 | 8 | 0 | 7 | -14.04 | 347.73 | 51.53 | 247.86 | 0.8222 | -90.0 | -117.6 | |
| 0 | 10 | 0 | 9 | -11.68 | 347.00 | 50.79 | 250.35 | 0.8080 | -154.0 | 2.2 | |
| 6 | -11 | 5 | -11 | -13.54 | 347.19 | 50.99 | 248.24 | 0.8156 | 747.2 | 999999 | |
| 3 | -11 | 2 | -11 | -13.56 | 346.57 | 50.36 | 247.97 | 0.8098 | 748.8 | 999999 | |
| 9 | 128 | 7 | 104 | -12.42 | 345.69 | 49.49 | 248.98 | 0.7976 | 1085.0 | 681.4 | |
| 6 | -17 | 5 | -17 | -11.96 | 345.02 | 48.82 | 249.29 | 0.7895 | 1202.1 | 999999 | |
| 6 | 62 | 5 | 51 | -13.71 | 345.49 | 49.29 | 247.37 | 0.8000 | 804.7 | 387.7 | |
| 0 | 6 | 0 | 5 | -13.77 | 344.77 | 48.57 | 247.01 | 0.7933 | 646.0 | 570.5 | |
| 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. | |