SDO HMI 2011-08-31 12:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.11 | 274.53 | 23.00 | 137.00 | 13.87 | 291.47 | -1.29 | 7.52 | 0.1201 | -561.1 | -322.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.58 | 0.00 | 1.81 | 17.96 | 293.35 | 0.59 | 357.00 | 0.1883 | 907.0 | 695.7 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 21.15 | 292.39 | -0.37 | 1.43 | 0.2428 | 803.0 | 624.4 | |
| 1.61 | 252.51 | 0.80 | 125.94 | 13.03 | 291.91 | -0.85 | 8.07 | 0.1037 | -761.4 | -429.1 | |
| 16.74 | -3.00 | 8.35 | -3.00 | 13.40 | 291.84 | -0.92 | 8.15 | 0.1101 | -1268.1 | 999999 | |
| 2.42 | -3.00 | 1.21 | -3.00 | 14.22 | 291.84 | -0.92 | 7.21 | 0.1243 | -1186.4 | 999999 | |
| 25.34 | -3.00 | 12.64 | -3.00 | 13.91 | 291.59 | -1.17 | 9.55 | 0.1197 | -1243.6 | 999999 | |
| 0.00 | 2.51 | 0.00 | 1.25 | 12.93 | 289.64 | -3.12 | 27.79 | 0.1143 | 896.0 | 559.9 | |
| 0.00 | 2.06 | 0.00 | 1.02 | 11.19 | 289.04 | -3.72 | 42.04 | 0.0954 | 890.0 | 705.7 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 15.73 | 288.62 | -4.13 | 24.94 | 0.1653 | 785.0 | 492.1 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 14.14 | 288.25 | -4.51 | 32.06 | 0.1443 | 772.0 | 545.2 | |
| 0.00 | 4.30 | 0.00 | 2.16 | 15.13 | 287.19 | -5.57 | 33.95 | 0.1685 | 790.0 | 718.7 | |
| 0.00 | 2.51 | 0.00 | 1.26 | 16.44 | 286.90 | -5.86 | 31.17 | 0.1900 | 922.0 | 681.1 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 15.68 | 286.76 | -5.99 | 34.07 | 0.1803 | 754.0 | 675.7 | |
| 0.00 | 1.79 | 0.00 | 0.90 | 16.62 | 286.38 | -6.37 | 32.80 | 0.1972 | 885.0 | 754.2 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 16.68 | 286.19 | -6.57 | 33.40 | 0.1999 | 871.0 | 731.8 | |
| 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. | |