| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98.89 | 397.52 | 52.04 | 209.15 | 19.62 | 123.70 | -5.18 | 14.62 | 0.3400 | 185.2 | 160.9 | |
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back to the solar disc SDO HMI 2011-12-03 19:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 0.90 | 20.03 | 136.78 | 7.89 | 338.80 | 0.3585 | 786.0 | 684.7 | |
| 0.00 | 2.13 | 0.00 | 1.12 | 19.84 | 133.92 | 5.04 | 345.92 | 0.3414 | 804.0 | 538.3 | |
| 0.26 | 20.14 | 0.13 | 10.59 | 20.31 | 127.32 | -1.56 | 4.34 | 0.3399 | -835.3 | -870.4 | |
| 2.05 | -3.00 | 1.08 | -3.00 | 20.16 | 127.23 | -1.66 | 4.63 | 0.3374 | -1083.4 | 999999 | |
| 1.28 | 3.50 | 0.67 | 1.84 | 19.91 | 126.98 | -1.90 | 5.40 | 0.3337 | -1029.7 | -935.7 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 21.01 | 126.84 | -2.05 | 5.46 | 0.3519 | -705.0 | -552.5 | |
| 5.20 | 24.06 | 2.74 | 12.66 | 20.25 | 126.63 | -2.26 | 6.26 | 0.3399 | -1072.0 | -886.0 | |
| 10.07 | -7.00 | 5.29 | -7.00 | 20.00 | 126.35 | -2.53 | 7.13 | 0.3363 | -1135.4 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.81 | 125.97 | -2.91 | 8.25 | 0.3341 | -1032.0 | -870.1 | |
| 2.73 | 15.19 | 1.44 | 8.02 | 20.56 | 125.93 | -2.95 | 8.04 | 0.3465 | -1045.8 | -810.9 | |
| 0.00 | 2.22 | 0.00 | 1.16 | 19.34 | 125.92 | -2.96 | 8.63 | 0.3266 | -1110.0 | -908.3 | |
| 2.82 | -10.00 | 1.49 | -10.00 | 20.91 | 125.83 | -3.06 | 8.16 | 0.3523 | -714.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.94 | 125.84 | -3.04 | 8.55 | 0.3364 | -541.0 | -531.5 | |
| 0.00 | 3.67 | 0.00 | 1.93 | 20.34 | 125.74 | -3.14 | 8.64 | 0.3433 | -975.0 | -835.0 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 20.53 | 125.58 | -3.30 | 8.99 | 0.3468 | -788.0 | -643.4 | |
| 3.75 | 26.11 | 1.97 | 13.69 | 19.53 | 125.57 | -3.31 | 9.52 | 0.3305 | -1088.3 | -450.4 | |
| 2.99 | 6.48 | 1.58 | 3.43 | 21.04 | 125.38 | -3.50 | 9.27 | 0.3555 | -765.5 | -343.0 | |
| 6.14 | -16.00 | 3.22 | -16.00 | 19.25 | 124.79 | -4.09 | 11.89 | 0.3284 | -937.6 | 999999 | |
| 2.30 | 5.63 | 1.22 | 2.98 | 20.69 | 124.06 | -4.82 | 12.90 | 0.3541 | -886.2 | -794.4 | |
| 0.00 | 1.96 | 0.00 | 1.04 | 20.15 | 124.07 | -4.81 | 13.22 | 0.3455 | -881.0 | -667.5 | |
| 0.00 | 3.92 | 0.00 | 2.08 | 21.00 | 124.05 | -4.83 | 12.71 | 0.3591 | -511.0 | -595.9 | |
| 0.00 | 0.43 | 0.00 | 0.23 | 21.22 | 124.01 | -4.87 | 12.67 | 0.3628 | -654.0 | -497.2 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 22.02 | 123.21 | -5.67 | 14.07 | 0.3782 | 936.0 | 780.8 | |
| 10.67 | 255.37 | 5.60 | 134.22 | 19.25 | 123.22 | -5.66 | 16.23 | 0.3346 | 1179.2 | 469.6 | |
| 0.00 | 2.39 | 0.00 | 1.28 | 21.98 | 123.06 | -5.83 | 14.47 | 0.3784 | 971.0 | 882.4 | |
| 0.00 | 2.39 | 0.00 | 1.27 | 20.85 | 122.72 | -6.16 | 16.16 | 0.3620 | 925.0 | 805.5 | |
| 0.00 | 2.30 | 0.00 | 1.23 | 21.63 | 122.65 | -6.23 | 15.69 | 0.3746 | 869.0 | 515.8 | |
| 40.96 | -24.00 | 21.54 | -24.00 | 19.22 | 122.53 | -6.35 | 18.11 | 0.3375 | 1268.2 | 999999 | |
| 2.47 | 3.16 | 1.32 | 1.68 | 20.94 | 122.43 | -6.45 | 16.80 | 0.3648 | 888.5 | 798.9 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 21.13 | 122.36 | -6.52 | 16.81 | 0.3681 | 638.0 | 455.7 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 20.84 | 122.05 | -6.83 | 17.80 | 0.3652 | 858.0 | 758.9 | |
| 4.18 | -24.00 | 2.21 | -24.00 | 19.93 | 122.06 | -6.82 | 18.63 | 0.3511 | 798.3 | 999999 | |
| 1.02 | 3.67 | 0.54 | 1.94 | 20.31 | 122.04 | -6.84 | 18.31 | 0.3570 | 636.1 | 649.0 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.17 | 121.58 | -7.30 | 23.06 | 0.3115 | -832.0 | -629.2 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 18.25 | 120.12 | -8.76 | 25.49 | 0.3376 | -846.0 | -660.6 | |
| 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. | |