SDO HMI 2011-12-05 06:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.33 | 261.06 | 38.55 | 140.92 | 19.48 | 123.32 | 13.66 | 326.10 | 0.3986 | 298.5 | 268.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 0.53 | 19.50 | 141.93 | 32.26 | 303.13 | 0.6032 | 565.0 | 422.7 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 19.06 | 140.22 | 30.55 | 303.76 | 0.5802 | 780.0 | 636.7 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 17.40 | 135.71 | 26.05 | 304.99 | 0.5135 | 685.0 | 532.0 | |
| 0.00 | 0.43 | 0.00 | 0.25 | 20.17 | 134.01 | 24.35 | 311.23 | 0.5167 | 769.0 | 675.4 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 20.44 | 128.03 | 18.36 | 319.30 | 0.4546 | -505.0 | -386.9 | |
| 1.62 | 4.61 | 0.90 | 2.55 | 20.25 | 127.94 | 18.27 | 319.14 | 0.4516 | -816.7 | -683.4 | |
| 0.00 | 1.88 | 0.00 | 1.04 | 19.62 | 127.63 | 17.97 | 318.62 | 0.4414 | -670.0 | -511.1 | |
| 4.10 | 6.40 | 2.26 | 3.54 | 20.03 | 127.61 | 17.95 | 319.29 | 0.4458 | -1023.2 | -759.5 | |
| 5.80 | 7.68 | 3.20 | 4.23 | 19.81 | 127.22 | 17.56 | 319.55 | 0.4393 | -1003.4 | -904.1 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 19.75 | 126.85 | 17.19 | 320.03 | 0.4349 | -311.0 | -378.5 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 20.50 | 126.91 | 17.24 | 321.11 | 0.4441 | -657.0 | -549.0 | |
| 1.37 | 2.73 | 0.75 | 1.51 | 20.56 | 126.72 | 17.05 | 321.51 | 0.4430 | -965.4 | -822.6 | |
| 0.00 | 2.22 | 0.00 | 1.22 | 19.68 | 126.62 | 16.95 | 320.31 | 0.4317 | -1093.0 | -971.0 | |
| 0.00 | 2.56 | 0.00 | 1.41 | 20.34 | 126.62 | 16.96 | 321.32 | 0.4395 | -891.0 | -746.2 | |
| 4.69 | 6.14 | 2.60 | 3.40 | 21.10 | 126.61 | 16.95 | 322.47 | 0.4483 | -817.9 | -626.0 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 18.06 | 126.29 | 16.62 | 318.18 | 0.4097 | -788.0 | -626.9 | |
| 0.00 | 4.95 | 0.00 | 2.71 | 19.97 | 126.19 | 16.52 | 321.45 | 0.4308 | -935.0 | -890.7 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 19.69 | 125.64 | 15.97 | 321.93 | 0.4220 | -864.0 | -647.1 | |
| 0.00 | 1.62 | 0.00 | 0.90 | 21.70 | 125.29 | 15.63 | 325.47 | 0.4435 | -692.0 | -471.3 | |
| 0.00 | 1.37 | 0.00 | 0.75 | 21.58 | 124.65 | 14.99 | 326.38 | 0.4363 | -855.0 | -662.5 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 20.28 | 124.52 | 14.86 | 324.77 | 0.4188 | -551.0 | -364.8 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 19.47 | 124.41 | 14.75 | 323.74 | 0.4075 | 610.0 | 382.5 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 20.07 | 122.85 | 13.18 | 327.56 | 0.4010 | 392.0 | 309.9 | |
| 3.07 | 180.25 | 1.66 | 96.56 | 19.75 | 122.76 | 13.09 | 327.28 | 0.3961 | 911.3 | 461.0 | |
| 3.67 | -24.00 | 1.98 | -24.00 | 19.91 | 122.57 | 12.91 | 327.86 | 0.3966 | 852.6 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 26.22 | 123.21 | 13.55 | 334.27 | 0.4860 | 712.0 | 606.5 | |
| 3.07 | -24.00 | 1.65 | -24.00 | 19.31 | 122.43 | 12.77 | 327.28 | 0.3875 | 748.0 | 999999 | |
| 0.68 | 4.27 | 0.37 | 2.30 | 19.63 | 122.46 | 12.79 | 327.69 | 0.3919 | 847.4 | 679.5 | |
| 27.82 | -24.00 | 14.89 | -24.00 | 18.91 | 122.24 | 12.57 | 327.06 | 0.3804 | 1196.1 | 999999 | |
| 9.81 | -24.00 | 5.27 | -24.00 | 19.44 | 122.05 | 12.39 | 328.22 | 0.3859 | 964.9 | 999999 | |
| 5.63 | 13.31 | 3.02 | 7.14 | 19.82 | 121.67 | 12.00 | 329.55 | 0.3878 | 889.6 | 361.3 | |
| 0.00 | 2.13 | 0.00 | 1.16 | 22.22 | 121.70 | 12.04 | 332.57 | 0.4210 | 887.0 | 674.8 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 20.73 | 121.29 | 11.62 | 331.55 | 0.3973 | 1018.0 | 802.5 | |
| 0.00 | 2.39 | 0.00 | 1.29 | 20.92 | 121.17 | 11.51 | 332.03 | 0.3990 | 904.0 | 702.4 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 17.51 | 120.68 | 11.02 | 328.27 | 0.3480 | -737.0 | -597.2 | |
| 0.00 | 1.19 | 0.00 | 0.62 | 16.87 | 115.74 | 6.08 | 340.36 | 0.3027 | -873.0 | -586.7 | |
| 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. | |