SDO HMI 2011-11-11 18:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81.31 | 311.44 | 57.59 | 225.98 | -17.68 | 101.94 | 42.52 | 241.82 | 0.7311 | -190.2 | 68.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 1.15 | -14.66 | 110.43 | 51.01 | 249.08 | 0.8073 | -531.0 | -424.0 | |
| 0.00 | 1.55 | 0.00 | 1.19 | -16.86 | 105.65 | 46.23 | 244.65 | 0.7671 | 563.0 | 446.6 | |
| 10.50 | 97.93 | 8.19 | 76.18 | -18.13 | 105.94 | 46.52 | 243.22 | 0.7748 | 761.3 | 293.9 | |
| 0.00 | 1.20 | 0.00 | 0.91 | -17.42 | 104.14 | 44.72 | 243.30 | 0.7539 | 570.0 | 530.0 | |
| 0.00 | 1.03 | 0.00 | 0.76 | -15.66 | 103.41 | 43.99 | 245.19 | 0.7391 | -598.0 | -464.8 | |
| 2.50 | 15.15 | 1.87 | 11.30 | -17.69 | 103.83 | 44.41 | 242.82 | 0.7518 | 778.4 | 537.3 | |
| 3.36 | -6.00 | 2.51 | -6.00 | -17.88 | 103.85 | 44.43 | 242.59 | 0.7528 | 566.9 | 999999 | |
| 1.12 | -6.00 | 0.83 | -6.00 | -17.61 | 103.46 | 44.04 | 242.74 | 0.7477 | 790.3 | 999999 | |
| 1.55 | 1.98 | 1.16 | 1.48 | -18.38 | 103.66 | 44.24 | 241.88 | 0.7530 | 651.4 | 552.0 | |
| 1.20 | 41.05 | 0.89 | 30.08 | -16.84 | 103.14 | 43.72 | 243.57 | 0.7411 | -436.6 | 353.2 | |
| 0.00 | 3.27 | 0.00 | 2.43 | -18.12 | 103.31 | 43.89 | 242.05 | 0.7483 | 795.0 | 708.4 | |
| 1.03 | -10.00 | 0.76 | -10.00 | -17.30 | 102.76 | 43.34 | 242.81 | 0.7390 | 843.2 | 999999 | |
| 6.80 | -10.00 | 4.98 | -10.00 | -17.58 | 102.63 | 43.21 | 242.39 | 0.7389 | 858.5 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.42 | -16.97 | 101.64 | 42.23 | 242.69 | 0.7258 | 776.0 | 715.8 | |
| 0.00 | 1.98 | 0.00 | 1.42 | -17.54 | 101.59 | 42.18 | 241.94 | 0.7279 | 724.0 | 632.5 | |
| 0.00 | 1.20 | 0.00 | 0.85 | -16.87 | 100.66 | 41.24 | 242.32 | 0.7147 | 657.0 | 542.6 | |
| 0.00 | 1.12 | 0.00 | 0.78 | -16.02 | 99.86 | 40.45 | 243.02 | 0.7020 | 593.0 | 468.0 | |
| 0.00 | 1.03 | 0.00 | 0.73 | -18.35 | 100.36 | 40.95 | 240.27 | 0.7187 | -591.0 | -488.8 | |
| 0.00 | 3.10 | 0.00 | 2.21 | -18.73 | 100.39 | 40.98 | 239.80 | 0.7209 | -785.0 | -551.5 | |
| 4.73 | 6.45 | 3.39 | 4.62 | -19.28 | 100.52 | 41.10 | 239.17 | 0.7250 | -633.7 | -259.5 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -17.15 | 99.74 | 40.33 | 241.48 | 0.7062 | -314.0 | -200.3 | |
| 0.77 | 92.17 | 0.54 | 62.63 | -16.76 | 99.36 | 39.94 | 241.78 | 0.7000 | -369.7 | -397.9 | |
| 1.20 | 3.61 | 0.83 | 2.48 | -16.37 | 99.02 | 39.60 | 242.12 | 0.6943 | -620.4 | -503.8 | |
| 5.77 | -22.00 | 3.94 | -22.00 | -17.01 | 98.49 | 39.08 | 240.97 | 0.6917 | -771.7 | 999999 | |
| 3.10 | 4.39 | 2.10 | 2.97 | -16.33 | 98.13 | 38.71 | 241.67 | 0.6842 | -791.2 | -388.7 | |
| 0.00 | 0.86 | 0.00 | 0.59 | -18.30 | 98.47 | 39.05 | 239.26 | 0.6983 | -412.0 | -299.5 | |
| 0.00 | 0.95 | 0.00 | 0.64 | -16.58 | 97.91 | 38.49 | 241.22 | 0.6830 | 378.0 | 425.5 | |
| 7.57 | -22.00 | 5.13 | -22.00 | -16.89 | 97.87 | 38.45 | 240.77 | 0.6842 | -746.2 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.47 | -17.97 | 98.10 | 38.68 | 239.47 | 0.6925 | -633.0 | -520.0 | |
| 3.18 | 22.55 | 2.19 | 15.43 | -18.58 | 98.18 | 38.76 | 238.73 | 0.6967 | -461.9 | -514.1 | |
| 17.90 | -22.00 | 12.10 | -22.00 | -17.29 | 97.57 | 38.15 | 240.06 | 0.6830 | -979.4 | 999999 | |
| 5.42 | -30.00 | 3.71 | -30.00 | -18.44 | 97.86 | 38.45 | 238.72 | 0.6925 | -720.0 | 999999 | |
| 3.61 | -30.00 | 2.47 | -30.00 | -18.15 | 97.79 | 38.37 | 239.05 | 0.6901 | -905.6 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.76 | -18.20 | 97.36 | 37.94 | 238.73 | 0.6857 | -673.0 | -582.0 | |
| 0.00 | 2.75 | 0.00 | 1.84 | -16.97 | 96.70 | 37.29 | 239.97 | 0.6716 | -593.0 | -651.1 | |
| 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. | |