SDO HMI 2011-09-02 18:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.46 | 73.38 | 15.00 | 41.44 | 13.44 | 291.50 | 28.48 | 284.94 | 0.4821 | -563.9 | -367.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.98 | 0.00 | 0.57 | 14.14 | 293.47 | 30.45 | 285.63 | 0.5123 | -683.0 | -592.4 | |
| 0.00 | 1.07 | 0.00 | 0.62 | 13.48 | 293.30 | 30.28 | 284.40 | 0.5082 | -672.0 | -460.3 | |
| 0.00 | 4.38 | 0.00 | 2.49 | 12.85 | 292.11 | 29.08 | 283.49 | 0.4893 | -763.0 | -578.7 | |
| 5.90 | 48.27 | 3.35 | 27.31 | 13.24 | 292.12 | 29.10 | 284.29 | 0.4905 | -926.6 | -627.4 | |
| 3.13 | -4.00 | 1.77 | -4.00 | 13.14 | 291.86 | 28.84 | 284.16 | 0.4864 | -952.5 | 999999 | |
| 4.47 | 6.97 | 2.54 | 3.95 | 14.05 | 291.91 | 28.89 | 285.99 | 0.4895 | -859.7 | -720.1 | |
| 8.40 | -4.00 | 4.76 | -4.00 | 13.57 | 291.81 | 28.79 | 285.05 | 0.4867 | -973.5 | 999999 | |
| 4.56 | -4.00 | 2.58 | -4.00 | 13.19 | 291.58 | 28.56 | 284.34 | 0.4824 | -1095.4 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.11 | 13.82 | 291.63 | 28.61 | 285.63 | 0.4848 | -808.0 | -594.9 | |
| 0.00 | 2.32 | 0.00 | 1.30 | 11.03 | 290.46 | 27.44 | 280.09 | 0.4612 | 905.0 | 804.0 | |
| 0.00 | 1.52 | 0.00 | 0.84 | 10.30 | 289.97 | 26.95 | 278.58 | 0.4528 | 823.0 | 711.2 | |
| 0.00 | 2.59 | 0.00 | 1.43 | 14.84 | 288.12 | 25.10 | 289.39 | 0.4365 | 573.0 | 486.2 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 15.79 | 287.55 | 24.53 | 291.85 | 0.4322 | 866.0 | 560.9 | |
| 0.00 | 2.06 | 0.00 | 1.13 | 16.30 | 287.17 | 24.14 | 293.24 | 0.4290 | 659.0 | 554.6 | |
| 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. | |