SDO HMI 2011-08-31 22:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.20 | 232.93 | 22.10 | 116.49 | 13.75 | 291.62 | 4.38 | 326.98 | 0.1377 | -726.5 | -372.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.40 | 13.62 | 293.65 | 6.42 | 316.06 | 0.1572 | -734.0 | -524.0 | |
| 0.00 | 1.79 | 0.00 | 0.91 | 18.74 | 293.59 | 6.36 | 332.42 | 0.2276 | 888.0 | 693.0 | |
| 0.00 | 2.95 | 0.00 | 1.50 | 18.09 | 293.34 | 6.11 | 331.92 | 0.2161 | 826.0 | 692.7 | |
| 6.98 | 218.00 | 3.49 | 108.99 | 14.13 | 291.91 | 4.68 | 326.87 | 0.1453 | -1177.2 | -454.2 | |
| 10.02 | -4.00 | 5.01 | -4.00 | 13.25 | 291.86 | 4.63 | 323.43 | 0.1324 | -1221.7 | 999999 | |
| 21.48 | -4.00 | 10.74 | -4.00 | 13.61 | 291.62 | 4.38 | 326.48 | 0.1352 | -1320.6 | 999999 | |
| 4.56 | -4.00 | 2.28 | -4.00 | 14.01 | 291.50 | 4.27 | 328.76 | 0.1399 | -1152.8 | 999999 | |
| 1.16 | -4.00 | 0.58 | -4.00 | 13.31 | 291.39 | 4.16 | 326.55 | 0.1287 | -1072.3 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 14.05 | 290.84 | 3.61 | 332.93 | 0.1349 | -127.0 | -169.7 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 10.95 | 290.06 | 2.83 | 323.61 | 0.0820 | 862.0 | 630.4 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 11.17 | 289.44 | 2.21 | 331.38 | 0.0795 | 863.0 | 734.6 | |
| 0.00 | 2.86 | 0.00 | 1.43 | 15.13 | 287.73 | 0.49 | 356.55 | 0.1389 | 642.0 | 726.4 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 14.43 | 287.26 | 0.02 | 359.81 | 0.1265 | 832.0 | 655.0 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 16.50 | 286.85 | -0.39 | 2.28 | 0.1627 | 1015.0 | 763.9 | |
| 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. | |