SDO HMI 2011-02-13 04:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.53 | 38.38 | 9.33 | 21.75 | 19.48 | 33.96 | -12.46 | 24.74 | 0.4869 | -133.2 | 11.7 | |
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back to the solar disc SDO HMI 2011-02-13 04:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.93 | 19.87 | 7.28 | 11.19 | 19.60 | 35.48 | -10.94 | 22.04 | 0.4785 | -976.6 | -554.1 | |
| 0.00 | 2.31 | 0.00 | 1.30 | 19.24 | 35.22 | -11.20 | 22.82 | 0.4750 | -921.0 | -746.6 | |
| 0.43 | 1.03 | 0.24 | 0.58 | 18.68 | 35.23 | -11.20 | 23.30 | 0.4671 | -932.2 | -820.7 | |
| 1.11 | 1.88 | 0.63 | 1.06 | 19.21 | 35.03 | -11.39 | 23.19 | 0.4757 | -625.6 | -443.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 18.49 | 33.74 | -12.68 | 26.18 | 0.4740 | 749.0 | 541.8 | |
| 0.00 | 0.69 | 0.00 | 0.39 | 18.45 | 31.88 | -14.54 | 29.44 | 0.4867 | 752.0 | 555.8 | |
| 2.06 | 3.43 | 1.18 | 1.96 | 19.35 | 31.38 | -15.05 | 29.32 | 0.5022 | 868.2 | 709.1 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 19.09 | 31.40 | -15.02 | 29.56 | 0.4986 | 938.0 | 760.5 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 19.36 | 31.18 | -15.24 | 29.63 | 0.5037 | 815.0 | 566.9 | |
| 0.00 | 3.00 | 0.00 | 1.73 | 19.89 | 30.93 | -15.49 | 29.48 | 0.5125 | 823.0 | 518.9 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 19.67 | 30.79 | -15.63 | 29.93 | 0.5106 | 675.0 | 575.1 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 19.44 | 30.82 | -15.61 | 30.13 | 0.5074 | 652.0 | 560.1 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 20.24 | 30.54 | -15.89 | 29.74 | 0.5198 | 577.0 | 553.8 | |
| 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. | |