SDO HMI 2011-09-02 01:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.13 | 165.88 | 19.59 | 87.34 | 13.59 | 291.58 | 19.20 | 290.32 | 0.3425 | -581.3 | -424.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.42 | 0.00 | 1.29 | 14.42 | 293.22 | 20.84 | 291.15 | 0.3711 | -773.0 | -572.5 | |
| 8.86 | 152.29 | 4.68 | 80.25 | 13.19 | 292.01 | 19.64 | 288.76 | 0.3471 | -984.4 | -507.7 | |
| 8.41 | -2.00 | 4.44 | -2.00 | 14.01 | 291.92 | 19.54 | 291.12 | 0.3494 | -950.6 | 999999 | |
| 2.24 | -2.00 | 1.18 | -2.00 | 13.23 | 291.68 | 19.31 | 289.13 | 0.3422 | -1221.4 | 999999 | |
| 12.88 | -2.00 | 6.80 | -2.00 | 13.56 | 291.71 | 19.34 | 290.05 | 0.3442 | -1083.9 | 999999 | |
| 4.74 | -2.00 | 2.49 | -2.00 | 13.24 | 291.39 | 19.02 | 289.40 | 0.3377 | -1181.5 | 999999 | |
| 0.00 | 1.52 | 0.00 | 0.80 | 13.54 | 290.85 | 18.48 | 290.69 | 0.3309 | -797.0 | -628.2 | |
| 0.00 | 0.89 | 0.00 | 0.47 | 11.88 | 290.44 | 18.06 | 286.06 | 0.3171 | 598.0 | 497.0 | |
| 0.00 | 0.98 | 0.00 | 0.51 | 13.00 | 288.83 | 16.45 | 290.98 | 0.2969 | 623.0 | 493.5 | |
| 0.00 | 1.43 | 0.00 | 0.74 | 13.08 | 288.31 | 15.94 | 291.78 | 0.2894 | 851.0 | 646.6 | |
| 0.00 | 1.61 | 0.00 | 0.83 | 14.99 | 287.80 | 15.43 | 298.52 | 0.2937 | 842.0 | 717.2 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 15.39 | 287.60 | 15.23 | 300.05 | 0.2939 | 873.0 | 686.4 | |
| 0.00 | 1.88 | 0.00 | 0.97 | 16.28 | 286.76 | 14.39 | 304.07 | 0.2892 | 916.0 | 711.4 | |
| 0.00 | 0.89 | 0.00 | 0.46 | 16.61 | 286.78 | 14.41 | 305.01 | 0.2925 | 830.0 | 689.4 | |
| 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. | |