SDO HMI 2011-08-31 21:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.38 | 227.37 | 22.18 | 113.67 | 13.84 | 291.62 | 3.83 | 330.61 | 0.1344 | -691.2 | -372.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.03 | 0.00 | 2.05 | 18.62 | 293.66 | 5.88 | 333.98 | 0.2222 | 554.0 | 614.2 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 18.04 | 293.35 | 5.57 | 333.94 | 0.2110 | 1072.0 | 868.4 | |
| 0.00 | 1.25 | 0.00 | 0.64 | 18.44 | 293.30 | 5.52 | 335.00 | 0.2168 | 849.0 | 634.5 | |
| 0.00 | 4.38 | 0.00 | 2.19 | 13.55 | 292.36 | 4.57 | 325.11 | 0.1361 | -584.0 | -384.6 | |
| 6.35 | 206.61 | 3.18 | 103.23 | 14.16 | 291.90 | 4.12 | 330.24 | 0.1408 | -1198.6 | -474.0 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 14.59 | 291.91 | 4.12 | 331.67 | 0.1473 | -42.0 | -53.7 | |
| 11.10 | -5.00 | 5.54 | -5.00 | 13.25 | 291.85 | 4.07 | 326.88 | 0.1270 | -1229.5 | 999999 | |
| 21.65 | -5.00 | 10.82 | -5.00 | 13.59 | 291.61 | 3.82 | 329.86 | 0.1297 | -1343.6 | 999999 | |
| 5.28 | -5.00 | 2.64 | -5.00 | 14.01 | 291.49 | 3.71 | 332.22 | 0.1352 | -1171.9 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 15.61 | 290.39 | 2.60 | 343.38 | 0.1536 | 670.0 | 608.0 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 11.20 | 289.41 | 1.63 | 338.27 | 0.0757 | 984.0 | 792.8 | |
| 0.00 | 3.67 | 0.00 | 1.84 | 15.13 | 287.68 | -0.10 | 0.69 | 0.1387 | 826.0 | 776.2 | |
| 0.00 | 2.42 | 0.00 | 1.21 | 16.50 | 286.86 | -0.92 | 5.43 | 0.1633 | 901.0 | 633.2 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 16.59 | 286.23 | -1.55 | 9.02 | 0.1662 | 782.0 | 720.1 | |
| 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. | |