SDO HMI 2011-02-09 20:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.89 | 55.65 | 11.47 | 33.95 | 19.66 | 65.86 | -24.44 | 41.95 | 0.5842 | -195.1 | -186.4 | |
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back to the solar disc SDO HMI 2011-02-09 20:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.70 | 23.76 | 2.81 | 14.28 | 19.42 | 67.74 | -22.57 | 40.10 | 0.5641 | -835.5 | -710.3 | |
| 5.47 | -1.00 | 3.28 | -1.00 | 19.34 | 67.38 | -22.93 | 40.64 | 0.5666 | -1024.8 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.02 | 18.66 | 67.34 | -22.97 | 41.53 | 0.5598 | -825.0 | -674.2 | |
| 0.94 | -1.00 | 0.57 | -1.00 | 19.52 | 67.08 | -23.23 | 40.79 | 0.5713 | -793.8 | 999999 | |
| 2.91 | 10.94 | 1.76 | 6.64 | 19.90 | 66.74 | -23.56 | 40.73 | 0.5783 | -647.1 | -445.2 | |
| 0.00 | 2.14 | 0.00 | 1.29 | 19.28 | 66.70 | -23.60 | 41.53 | 0.5723 | -752.0 | -569.7 | |
| 0.00 | 2.22 | 0.00 | 1.38 | 20.78 | 64.44 | -25.87 | 42.29 | 0.6085 | 840.0 | 745.3 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 20.70 | 64.07 | -26.24 | 42.78 | 0.6113 | 560.0 | 608.6 | |
| 1.28 | 2.91 | 0.80 | 1.82 | 20.08 | 63.30 | -27.01 | 44.33 | 0.6127 | 758.5 | 661.9 | |
| 1.45 | 1.54 | 0.91 | 0.96 | 19.67 | 62.91 | -27.39 | 45.22 | 0.6126 | 910.2 | 761.0 | |
| 2.14 | 6.58 | 1.34 | 4.12 | 19.49 | 62.63 | -27.68 | 45.74 | 0.6138 | 857.0 | 597.3 | |
| 0.00 | 1.71 | 0.00 | 1.08 | 20.24 | 62.09 | -28.22 | 45.35 | 0.6258 | 777.0 | 533.4 | |
| 0.00 | 1.03 | 0.00 | 0.67 | 20.78 | 60.28 | -30.03 | 46.44 | 0.6480 | 709.0 | 607.3 | |
| 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. | |