| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.27 | 201.48 | 26.00 | 113.34 | -16.59 | 266.12 | -21.47 | 132.30 | 0.4756 | -4.1 | -138.6 | |
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back to the solar disc SDO HMI 2011-11-21 18:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.97 | 0.00 | 1.09 | -18.25 | 269.70 | -17.89 | 139.88 | 0.4546 | 813.0 | 671.0 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -12.11 | 269.53 | -18.06 | 128.82 | 0.3906 | 1110.0 | 961.8 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -16.53 | 269.13 | -18.46 | 136.30 | 0.4413 | 893.0 | 666.6 | |
| 0.00 | 2.23 | 0.00 | 1.22 | -15.29 | 269.02 | -18.57 | 134.04 | 0.4292 | 812.0 | 706.3 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -15.33 | 268.59 | -19.00 | 133.47 | 0.4344 | 637.0 | 457.2 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -15.80 | 268.22 | -19.37 | 133.74 | 0.4435 | 654.0 | 548.6 | |
| 18.77 | 59.47 | 10.43 | 33.04 | -16.70 | 267.96 | -19.63 | 134.88 | 0.4559 | 1075.2 | 447.8 | |
| 0.00 | 3.77 | 0.00 | 2.07 | -14.99 | 268.11 | -19.48 | 132.17 | 0.4366 | -453.0 | -597.1 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -14.09 | 268.16 | -19.43 | 130.63 | 0.4270 | 661.0 | 504.5 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -15.58 | 267.98 | -19.61 | 133.03 | 0.4440 | 816.0 | 629.0 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -16.96 | 267.51 | -20.08 | 134.65 | 0.4636 | -1.0 | -8.7 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -17.18 | 267.42 | -20.17 | 134.88 | 0.4669 | 531.0 | 391.6 | |
| 0.00 | 1.20 | 0.00 | 0.65 | -12.72 | 267.69 | -19.90 | 127.38 | 0.4196 | 861.0 | 646.9 | |
| 1.37 | 15.68 | 0.77 | 8.79 | -16.75 | 266.94 | -20.65 | 133.53 | 0.4678 | 531.9 | -248.5 | |
| 0.00 | 3.00 | 0.00 | 1.70 | -17.52 | 265.78 | -21.81 | 133.25 | 0.4884 | 416.0 | 640.8 | |
| 2.83 | 4.80 | 1.59 | 2.70 | -16.55 | 265.80 | -21.79 | 131.72 | 0.4787 | -835.5 | -573.1 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -17.81 | 265.31 | -22.28 | 133.11 | 0.4965 | 706.0 | 536.8 | |
| 6.43 | 84.24 | 3.63 | 47.76 | -16.49 | 265.24 | -22.35 | 130.93 | 0.4846 | -1103.4 | -623.1 | |
| 3.77 | -18.00 | 2.13 | -18.00 | -15.93 | 265.21 | -22.38 | 129.97 | 0.4797 | -1015.6 | 999999 | |
| 1.97 | -18.00 | 1.12 | -18.00 | -17.31 | 264.84 | -22.75 | 131.76 | 0.4970 | 409.7 | 999999 | |
| 6.08 | -18.00 | 3.45 | -18.00 | -16.53 | 264.77 | -22.82 | 130.42 | 0.4905 | -1055.3 | 999999 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -14.73 | 264.85 | -22.74 | 127.49 | 0.4732 | 721.0 | 556.0 | |
| 3.68 | -18.00 | 2.10 | -18.00 | -16.97 | 264.44 | -23.15 | 130.75 | 0.4983 | -769.7 | 999999 | |
| 1.37 | -18.00 | 0.78 | -18.00 | -16.57 | 264.46 | -23.13 | 130.12 | 0.4944 | -817.8 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -16.48 | 263.70 | -23.89 | 129.11 | 0.5026 | -758.0 | -607.4 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -17.56 | 263.00 | -24.59 | 130.04 | 0.5202 | -803.0 | -542.9 | |
| 0.00 | 0.69 | 0.00 | 0.40 | -18.19 | 262.84 | -24.75 | 130.83 | 0.5277 | -713.0 | -520.8 | |
| 0.00 | 1.37 | 0.00 | 0.80 | -17.42 | 262.17 | -25.42 | 128.92 | 0.5286 | -812.0 | -634.1 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -18.72 | 261.58 | -26.01 | 130.28 | 0.5465 | -783.0 | -608.2 | |
| 0.00 | 1.80 | 0.00 | 1.06 | -18.34 | 261.54 | -26.05 | 129.67 | 0.5437 | -875.0 | -656.2 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -13.14 | 262.08 | -25.51 | 121.74 | 0.4951 | -766.0 | -580.4 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -16.37 | 261.12 | -26.47 | 126.21 | 0.5322 | -681.0 | -500.0 | |
| 0.00 | 0.94 | 0.00 | 0.57 | -20.05 | 259.97 | -27.62 | 130.59 | 0.5757 | -708.0 | -573.6 | |
| 0.00 | 1.11 | 0.00 | 0.68 | -20.28 | 259.89 | -27.70 | 130.83 | 0.5785 | -539.0 | -438.2 | |
| 0.00 | 1.20 | 0.00 | 0.73 | -19.15 | 258.68 | -28.91 | 128.10 | 0.5826 | -641.0 | -514.9 | |
| 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. | |