SOHO MDI 2000-11-08 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52 | 399 | 30 | 219 | -12.55 | 176.48 | -19.26 | 130.28 | 0.4242 | 1190.7 | 385.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 2 | 0 | 1 | -12.51 | 178.75 | -16.99 | 133.65 | 0.3961 | 549.0 | 466.9 | |
| 0 | 4 | 0 | 2 | -11.87 | 178.71 | -17.03 | 132.37 | 0.3897 | 756.0 | 651.9 | |
| 14 | 289 | 8 | 157 | -13.45 | 177.77 | -17.97 | 133.79 | 0.4175 | 1342.6 | 687.6 | |
| 19 | -3 | 11 | -3 | -12.45 | 177.48 | -18.27 | 131.50 | 0.4105 | 1757.8 | 999999 | |
| 11 | -3 | 6 | -3 | -12.59 | 176.84 | -18.90 | 130.79 | 0.4195 | 1398.6 | 999999 | |
| 5 | -3 | 3 | -3 | -13.11 | 176.80 | -18.95 | 131.69 | 0.4253 | 977.3 | 999999 | |
| 0 | 7 | 0 | 4 | -13.63 | 176.76 | -18.99 | 132.56 | 0.4311 | -438.0 | -226.9 | |
| 0 | 10 | 0 | 6 | -11.61 | 175.79 | -19.96 | 127.46 | 0.4230 | 863.0 | 693.2 | |
| 0 | 4 | 0 | 2 | -12.41 | 175.56 | -20.19 | 128.65 | 0.4334 | 542.0 | 390.5 | |
| 0 | 6 | 0 | 3 | -9.89 | 174.79 | -20.96 | 122.74 | 0.4208 | -443.0 | -422.9 | |
| 0 | 4 | 0 | 3 | -16.81 | 174.10 | -21.65 | 134.08 | 0.4937 | -398.0 | -408.1 | |
| 0 | 11 | 0 | 6 | -15.06 | 174.00 | -21.75 | 131.19 | 0.4775 | -863.0 | -719.8 | |
| 0 | 3 | 0 | 2 | -10.81 | 174.22 | -21.53 | 123.88 | 0.4361 | -712.0 | -597.2 | |
| 0 | 5 | 0 | 3 | -8.92 | 174.01 | -21.74 | 119.84 | 0.4236 | -983.0 | -860.8 | |
| 0 | 38 | 0 | 21 | -10.83 | 173.50 | -22.25 | 123.06 | 0.4456 | -1163.0 | -617.3 | |
| 3 | 7 | 2 | 4 | -10.93 | 172.81 | -22.94 | 122.46 | 0.4554 | -905.2 | -673.2 | |
| 0 | 5 | 0 | 3 | -11.41 | 172.30 | -23.45 | 122.81 | 0.4660 | -841.0 | -637.1 | |
| 0 | 4 | 0 | 2 | -11.83 | 171.62 | -24.13 | 122.83 | 0.4782 | -731.0 | -635.0 | |
| 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. | |