SDO HMI 2011-12-13 07:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.56 | 196.39 | 18.99 | 99.42 | 8.73 | 356.57 | -7.13 | 36.48 | 0.2065 | -668.1 | -383.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.47 | 9.02 | 0.01 | -3.69 | 20.73 | 0.1804 | -955.0 | -716.4 | |
| 1.96 | 175.35 | 0.99 | 88.65 | 9.08 | 357.67 | -6.03 | 31.55 | 0.1992 | -930.7 | -486.0 | |
| 32.87 | -2.00 | 16.62 | -2.00 | 8.82 | 357.05 | -6.66 | 34.88 | 0.2012 | -1312.2 | 999999 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 8.76 | 356.15 | -7.56 | 38.52 | 0.2097 | -800.0 | -703.4 | |
| 0.00 | 1.70 | 0.00 | 0.86 | 8.73 | 355.39 | -8.31 | 41.27 | 0.2176 | -677.0 | -605.3 | |
| 2.73 | 2.90 | 1.38 | 1.47 | 8.43 | 355.31 | -8.39 | 42.49 | 0.2148 | -719.5 | -713.5 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 8.76 | 355.03 | -8.67 | 42.39 | 0.2221 | 375.0 | 277.6 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 8.91 | 354.78 | -8.92 | 42.72 | 0.2268 | 1032.0 | 943.6 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 9.69 | 354.16 | -9.55 | 42.36 | 0.2437 | 842.0 | 731.2 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 9.36 | 353.38 | -10.33 | 45.53 | 0.2490 | 924.0 | 713.6 | |
| 0.00 | 1.02 | 0.00 | 0.52 | 6.74 | 350.65 | -13.05 | 60.22 | 0.2595 | 876.0 | 592.7 | |
| 0.00 | 5.20 | 0.00 | 2.68 | 6.63 | 348.85 | -14.85 | 63.63 | 0.2855 | 538.0 | 635.5 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 6.18 | 348.50 | -15.21 | 65.56 | 0.2878 | 825.0 | 625.1 | |
| 0.00 | 1.70 | 0.00 | 0.88 | 6.57 | 348.30 | -15.40 | 64.62 | 0.2934 | 708.0 | 647.5 | |
| 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. | |