SDO HMI 2011-11-25 17:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102.23 | 368.78 | 73.69 | 263.07 | 19.49 | 192.09 | -43.33 | 64.08 | 0.7200 | -136.7 | -152.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 0.84 | 16.97 | 197.15 | -38.27 | 65.45 | 0.6536 | -682.0 | -542.5 | |
| 1.11 | 201.50 | 0.76 | 137.27 | 19.06 | 194.73 | -40.69 | 63.57 | 0.6905 | -893.4 | -433.4 | |
| 8.13 | -2.00 | 5.55 | -2.00 | 18.84 | 194.63 | -40.79 | 63.92 | 0.6908 | -879.5 | 999999 | |
| 27.55 | -2.00 | 18.78 | -2.00 | 18.28 | 194.55 | -40.88 | 64.73 | 0.6895 | -1106.3 | 999999 | |
| 1.37 | 29.26 | 0.95 | 20.40 | 19.13 | 193.58 | -41.84 | 63.96 | 0.7037 | -649.8 | -506.3 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 18.64 | 193.65 | -41.77 | 64.61 | 0.7011 | -53.0 | -114.0 | |
| 8.90 | -5.00 | 6.19 | -5.00 | 18.76 | 193.36 | -42.06 | 64.57 | 0.7048 | -858.5 | 999999 | |
| 2.74 | -5.00 | 1.92 | -5.00 | 18.66 | 192.93 | -42.50 | 64.88 | 0.7093 | -527.3 | 999999 | |
| 3.94 | 5.99 | 2.78 | 4.23 | 19.34 | 192.71 | -42.71 | 64.05 | 0.7142 | -577.6 | -228.6 | |
| 1.28 | 1.54 | 0.90 | 1.08 | 18.99 | 192.65 | -42.77 | 64.53 | 0.7136 | -428.8 | -433.3 | |
| 6.84 | 12.49 | 4.87 | 8.90 | 19.83 | 192.29 | -43.13 | 63.56 | 0.7206 | -571.9 | 17.6 | |
| 0.00 | 1.37 | 0.00 | 0.97 | 19.11 | 192.48 | -42.94 | 64.44 | 0.7159 | -362.0 | -321.9 | |
| 0.00 | 0.94 | 0.00 | 0.67 | 18.99 | 192.26 | -43.16 | 64.69 | 0.7178 | -378.0 | -283.7 | |
| 1.20 | 4.28 | 0.87 | 3.11 | 20.31 | 191.33 | -44.09 | 63.31 | 0.7327 | -422.7 | -9.3 | |
| 0.00 | 1.20 | 0.00 | 0.87 | 19.40 | 190.99 | -44.43 | 64.63 | 0.7331 | 612.0 | 516.6 | |
| 1.45 | 4.02 | 1.05 | 2.91 | 19.18 | 191.02 | -44.40 | 64.91 | 0.7320 | 777.2 | 431.8 | |
| 0.00 | 2.22 | 0.00 | 1.63 | 20.11 | 190.69 | -44.73 | 63.81 | 0.7387 | 439.0 | 402.1 | |
| 5.13 | 7.36 | 3.75 | 5.38 | 19.64 | 190.60 | -44.82 | 64.46 | 0.7381 | 707.2 | 642.3 | |
| 1.71 | 29.69 | 1.27 | 22.10 | 20.32 | 190.12 | -45.30 | 63.76 | 0.7455 | 768.8 | 439.5 | |
| 2.99 | -19.00 | 2.22 | -19.00 | 20.19 | 189.95 | -45.47 | 63.99 | 0.7469 | 904.9 | 999999 | |
| 1.11 | 2.57 | 0.82 | 1.90 | 19.85 | 189.99 | -45.44 | 64.42 | 0.7453 | 650.3 | 396.0 | |
| 0.00 | 0.86 | 0.00 | 0.65 | 21.44 | 189.18 | -46.24 | 62.68 | 0.7590 | 598.0 | 538.3 | |
| 10.27 | -19.00 | 7.68 | -19.00 | 20.28 | 189.51 | -45.91 | 64.04 | 0.7518 | 691.7 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.57 | 21.65 | 188.77 | -46.65 | 62.57 | 0.7639 | 672.0 | 490.4 | |
| 2.57 | 5.65 | 2.04 | 4.49 | 21.83 | 186.74 | -48.68 | 63.05 | 0.7844 | 769.2 | 654.5 | |
| 2.48 | 45.86 | 1.99 | 37.11 | 22.33 | 186.41 | -49.01 | 62.54 | 0.7891 | 886.9 | 532.8 | |
| 0.00 | 1.03 | 0.00 | 0.82 | 21.54 | 186.44 | -48.98 | 63.50 | 0.7865 | 564.0 | 531.7 | |
| 8.98 | -26.00 | 7.27 | -26.00 | 22.29 | 185.99 | -49.44 | 62.73 | 0.7930 | 824.5 | 999999 | |
| 0.94 | -26.00 | 0.77 | -26.00 | 22.64 | 185.72 | -49.70 | 62.40 | 0.7966 | 648.0 | 999999 | |
| 1.54 | -26.00 | 1.26 | -26.00 | 22.83 | 185.57 | -49.85 | 62.22 | 0.7985 | 452.7 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.35 | 21.94 | 185.86 | -49.56 | 63.20 | 0.7932 | 534.0 | 497.0 | |
| 0.00 | 2.48 | 0.00 | 2.05 | 22.62 | 185.02 | -50.40 | 62.64 | 0.8030 | 387.0 | 234.9 | |
| 0.00 | 1.28 | 0.00 | 1.05 | 21.90 | 185.28 | -50.14 | 63.44 | 0.7985 | 533.0 | 427.1 | |
| 0.00 | 1.54 | 0.00 | 1.28 | 22.37 | 184.90 | -50.52 | 62.99 | 0.8034 | 435.0 | 357.2 | |
| 0.00 | 0.86 | 0.00 | 0.73 | 22.82 | 183.69 | -51.73 | 62.82 | 0.8158 | 444.0 | 353.0 | |
| 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. | |