SDO HMI 2011-11-20 10:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.56 | 114.86 | 14.52 | 73.04 | -18.34 | 338.24 | 33.07 | 235.77 | 0.6286 | 176.2 | 249.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.40 | 0.00 | 1.63 | -16.88 | 344.47 | 39.29 | 242.22 | 0.6873 | 653.0 | 464.7 | |
| 0.00 | 0.51 | 0.00 | 0.35 | -18.53 | 344.70 | 39.53 | 240.16 | 0.6980 | 517.0 | 438.8 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -17.12 | 344.09 | 38.91 | 241.69 | 0.6842 | 678.0 | 575.2 | |
| 1.80 | 3.00 | 1.22 | 2.02 | -17.49 | 343.66 | 38.49 | 240.96 | 0.6812 | 732.5 | 670.3 | |
| 0.00 | 0.94 | 0.00 | 0.63 | -16.99 | 343.54 | 38.36 | 241.58 | 0.6773 | 831.0 | 747.4 | |
| 0.00 | 1.63 | 0.00 | 1.09 | -16.48 | 343.41 | 38.24 | 242.20 | 0.6733 | 757.0 | 586.4 | |
| 0.00 | 1.89 | 0.00 | 1.27 | -17.36 | 343.35 | 38.18 | 240.97 | 0.6771 | 684.0 | 558.5 | |
| 1.80 | 2.57 | 1.19 | 1.70 | -17.05 | 342.45 | 37.28 | 240.86 | 0.6653 | 650.2 | 677.1 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -17.01 | 342.17 | 37.00 | 240.75 | 0.6618 | 847.0 | 696.2 | |
| 0.00 | 2.75 | 0.00 | 1.87 | -21.12 | 342.66 | 37.49 | 235.58 | 0.6906 | 786.0 | 607.4 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -16.24 | 341.15 | 35.97 | 241.22 | 0.6458 | -603.0 | -448.2 | |
| 9.18 | 68.37 | 5.91 | 43.81 | -17.06 | 340.33 | 35.16 | 239.54 | 0.6410 | 872.1 | 531.3 | |
| 0.00 | 0.51 | 0.00 | 0.35 | -22.46 | 341.75 | 36.57 | 233.28 | 0.6893 | 494.0 | 421.0 | |
| 5.66 | -12.00 | 3.63 | -12.00 | -17.05 | 339.92 | 34.74 | 239.28 | 0.6361 | 1092.2 | 999999 | |
| 2.92 | -12.00 | 1.86 | -12.00 | -17.11 | 339.59 | 34.42 | 238.98 | 0.6326 | 1008.9 | 999999 | |
| 0.00 | 2.57 | 0.00 | 1.61 | -18.50 | 337.20 | 32.03 | 235.27 | 0.6142 | -861.0 | -678.1 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -18.59 | 337.03 | 31.86 | 235.02 | 0.6129 | -621.0 | -530.1 | |
| 0.00 | 0.94 | 0.00 | 0.61 | -23.09 | 336.75 | 31.58 | 228.74 | 0.6431 | 728.0 | 600.6 | |
| 0.00 | 1.20 | 0.00 | 0.74 | -19.38 | 335.19 | 30.01 | 232.39 | 0.5979 | 750.0 | 587.3 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -19.80 | 335.16 | 29.99 | 231.79 | 0.6008 | 525.0 | 366.3 | |
| 0.00 | 1.46 | 0.00 | 0.87 | -21.56 | 330.22 | 25.05 | 224.53 | 0.5636 | -749.0 | -631.9 | |
| 0.00 | 1.46 | 0.00 | 0.87 | -21.56 | 329.72 | 24.55 | 224.00 | 0.5585 | -706.0 | -523.4 | |
| 0.00 | 1.63 | 0.00 | 0.97 | -21.33 | 329.58 | 24.41 | 224.14 | 0.5548 | -833.0 | -695.3 | |
| 0.00 | 1.20 | 0.00 | 0.71 | -21.07 | 329.43 | 24.26 | 224.33 | 0.5508 | -828.0 | -684.9 | |
| 1.20 | 1.46 | 0.71 | 0.86 | -23.27 | 326.99 | 21.82 | 218.58 | 0.5498 | -762.6 | -645.0 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -23.57 | 326.94 | 21.77 | 218.15 | 0.5525 | -880.0 | -784.0 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -23.33 | 326.76 | 21.59 | 218.21 | 0.5483 | -967.0 | -761.9 | |
| 0.00 | 1.37 | 0.00 | 0.82 | -24.35 | 326.73 | 21.56 | 216.94 | 0.5592 | -644.0 | -524.7 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -23.07 | 326.51 | 21.33 | 218.22 | 0.5431 | -789.0 | -676.3 | |
| 0.00 | 3.52 | 0.00 | 2.09 | -23.79 | 326.60 | 21.42 | 217.45 | 0.5518 | -818.0 | -714.5 | |
| 0.00 | 1.46 | 0.00 | 0.86 | -23.39 | 326.53 | 21.36 | 217.84 | 0.5469 | -909.0 | -796.2 | |
| 0.00 | 0.94 | 0.00 | 0.56 | -24.09 | 326.61 | 21.44 | 217.11 | 0.5552 | -580.0 | -448.7 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -21.07 | 325.31 | 20.14 | 219.23 | 0.5100 | -650.0 | -536.0 | |
| 0.00 | 0.69 | 0.00 | 0.40 | -23.94 | 325.65 | 20.48 | 216.07 | 0.5452 | -560.0 | -487.6 | |
| 0.00 | 1.29 | 0.00 | 0.76 | -23.54 | 325.48 | 20.31 | 216.33 | 0.5393 | -707.0 | -532.5 | |
| 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. | |