SDO HMI 2011-12-12 02:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.31 | 213.21 | 20.24 | 115.70 | 9.13 | 357.37 | -22.24 | 65.93 | 0.4109 | -727.9 | -387.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.41 | 191.32 | 16.47 | 103.58 | 9.22 | 357.75 | -21.86 | 65.43 | 0.4058 | -1433.7 | -450.3 | |
| 2.13 | -1.00 | 1.16 | -1.00 | 8.87 | 357.32 | -22.29 | 66.64 | 0.4099 | -1009.4 | 999999 | |
| 0.51 | -1.00 | 0.28 | -1.00 | 8.96 | 357.12 | -22.49 | 66.61 | 0.4134 | -833.3 | 999999 | |
| 0.00 | 1.96 | 0.00 | 1.06 | 8.27 | 357.07 | -22.54 | 68.22 | 0.4103 | -563.0 | -503.0 | |
| 0.00 | 1.96 | 0.00 | 1.06 | 8.57 | 356.98 | -22.62 | 67.61 | 0.4132 | -873.0 | -691.3 | |
| 2.56 | 5.62 | 1.39 | 3.06 | 8.84 | 356.64 | -22.96 | 67.29 | 0.4197 | -880.6 | -613.7 | |
| 1.70 | 2.47 | 0.94 | 1.36 | 8.52 | 354.80 | -24.81 | 69.43 | 0.4450 | 922.1 | 670.3 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 8.49 | 354.41 | -25.20 | 69.77 | 0.4507 | 996.0 | 836.2 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 8.64 | 353.77 | -25.84 | 69.89 | 0.4608 | 882.0 | 676.9 | |
| 0.00 | 1.62 | 0.00 | 0.91 | 9.45 | 353.64 | -25.97 | 68.33 | 0.4667 | 823.0 | 672.1 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 8.88 | 352.85 | -26.76 | 70.00 | 0.4753 | 971.0 | 753.2 | |
| 0.00 | 2.04 | 0.00 | 1.16 | 8.86 | 352.25 | -27.36 | 70.44 | 0.4839 | 695.0 | 592.9 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 8.53 | 352.27 | -27.33 | 71.07 | 0.4820 | 681.0 | 546.1 | |
| 0.00 | 1.79 | 0.00 | 1.03 | 8.30 | 349.84 | -29.76 | 72.85 | 0.5162 | 585.0 | 479.9 | |
| 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. | |