SDO HMI 2011-11-20 21:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.31 | 105.53 | 16.24 | 73.68 | -17.85 | 339.60 | 40.48 | 241.32 | 0.7063 | 327.5 | 375.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.84 | -17.16 | 344.35 | 45.24 | 244.69 | 0.7528 | 538.0 | 402.9 | |
| 0.00 | 1.46 | 0.00 | 1.09 | -17.37 | 344.11 | 45.00 | 244.33 | 0.7511 | 612.0 | 542.1 | |
| 0.00 | 0.77 | 0.00 | 0.57 | -16.93 | 343.97 | 44.86 | 244.83 | 0.7480 | 619.0 | 604.9 | |
| 0.00 | 0.86 | 0.00 | 0.64 | -16.83 | 343.81 | 44.70 | 244.88 | 0.7459 | 580.0 | 568.2 | |
| 0.00 | 1.46 | 0.00 | 1.08 | -17.05 | 343.84 | 44.72 | 244.61 | 0.7470 | 707.0 | 608.9 | |
| 0.00 | 0.77 | 0.00 | 0.57 | -17.46 | 343.92 | 44.81 | 244.13 | 0.7494 | 583.0 | 471.0 | |
| 0.00 | 1.11 | 0.00 | 0.85 | -19.40 | 344.48 | 45.37 | 241.96 | 0.7629 | 532.0 | 500.5 | |
| 0.00 | 0.69 | 0.00 | 0.52 | -18.64 | 344.22 | 45.10 | 242.79 | 0.7571 | 588.0 | 559.9 | |
| 0.00 | 1.11 | 0.00 | 0.83 | -17.67 | 343.59 | 44.48 | 243.72 | 0.7468 | 589.0 | 514.5 | |
| 4.54 | 6.77 | 3.34 | 4.97 | -17.16 | 343.17 | 44.06 | 244.19 | 0.7404 | 735.4 | 585.7 | |
| 0.00 | 1.80 | 0.00 | 1.36 | -19.70 | 343.83 | 44.72 | 241.30 | 0.7576 | 129.0 | 214.1 | |
| 0.00 | 1.29 | 0.00 | 0.93 | -16.61 | 342.62 | 43.51 | 244.66 | 0.7324 | 704.0 | 593.1 | |
| 0.00 | 1.37 | 0.00 | 0.98 | -15.60 | 342.18 | 43.07 | 245.77 | 0.7235 | -564.0 | -415.1 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -15.75 | 341.92 | 42.81 | 245.47 | 0.7213 | -581.0 | -554.3 | |
| 0.00 | 2.06 | 0.00 | 1.48 | -17.78 | 341.64 | 42.53 | 242.71 | 0.7267 | 679.0 | 512.2 | |
| 0.00 | 1.46 | 0.00 | 1.04 | -18.11 | 341.32 | 42.21 | 242.12 | 0.7247 | 534.0 | 500.2 | |
| 7.89 | 58.05 | 5.53 | 40.49 | -16.96 | 340.41 | 41.30 | 243.18 | 0.7097 | 791.8 | 533.0 | |
| 0.00 | 1.63 | 0.00 | 1.14 | -17.33 | 340.43 | 41.32 | 242.69 | 0.7116 | 0.0 | 4.0 | |
| 5.14 | -17.00 | 3.58 | -17.00 | -16.92 | 340.03 | 40.91 | 243.04 | 0.7053 | 1060.2 | 999999 | |
| 1.03 | -17.00 | 0.71 | -17.00 | -17.03 | 339.73 | 40.62 | 242.74 | 0.7026 | 828.9 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.66 | -18.33 | 339.96 | 40.85 | 241.16 | 0.7112 | 614.0 | 472.6 | |
| 0.00 | 1.80 | 0.00 | 1.26 | -18.61 | 339.71 | 40.60 | 240.67 | 0.7098 | 497.0 | 353.5 | |
| 0.00 | 1.20 | 0.00 | 0.83 | -18.06 | 339.39 | 40.28 | 241.21 | 0.7037 | 646.0 | 550.8 | |
| 0.00 | 1.37 | 0.00 | 0.94 | -18.78 | 337.89 | 38.77 | 239.43 | 0.6910 | 735.0 | 582.8 | |
| 1.63 | 1.80 | 1.10 | 1.21 | -18.07 | 337.14 | 38.03 | 239.95 | 0.6789 | -590.8 | -466.0 | |
| 1.11 | 1.63 | 0.75 | 1.10 | -18.38 | 337.18 | 38.07 | 239.55 | 0.6811 | -515.2 | -536.0 | |
| 0.00 | 1.80 | 0.00 | 1.21 | -18.72 | 336.91 | 37.80 | 238.94 | 0.6800 | -445.0 | -388.4 | |
| 0.00 | 0.43 | 0.00 | 0.30 | -23.59 | 336.81 | 37.69 | 232.64 | 0.7074 | 491.0 | 377.8 | |
| 0.00 | 1.11 | 0.00 | 0.73 | -20.16 | 334.31 | 35.20 | 235.35 | 0.6601 | 540.0 | 368.8 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -22.74 | 328.21 | 29.09 | 227.06 | 0.6149 | -523.0 | -490.7 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -23.07 | 326.86 | 27.74 | 225.36 | 0.6042 | -734.0 | -606.6 | |
| 1.97 | 3.60 | 1.23 | 2.24 | -23.53 | 326.78 | 27.66 | 224.70 | 0.6075 | -865.0 | -649.8 | |
| 0.00 | 0.77 | 0.00 | 0.48 | -23.10 | 326.68 | 27.57 | 225.15 | 0.6027 | -746.0 | -561.1 | |
| 0.00 | 1.20 | 0.00 | 0.75 | -24.14 | 326.01 | 26.89 | 223.17 | 0.6056 | -377.0 | -401.6 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -26.99 | 326.45 | 27.34 | 220.21 | 0.6361 | -587.0 | -436.1 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -24.25 | 325.05 | 25.94 | 222.05 | 0.5976 | -664.0 | -587.7 | |
| 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. | |