| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.52 | 169.27 | 19.76 | 97.03 | 18.53 | 103.24 | 24.31 | 309.04 | 0.5045 | -400.6 | -245.5 | |
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back to the solar disc SDO HMI 2011-12-07 14:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.03 | 8.01 | 2.87 | 4.56 | 17.03 | 103.61 | 24.68 | 306.13 | 0.4963 | 882.5 | 767.8 | |
| 0.00 | 3.58 | 0.00 | 2.04 | 17.31 | 103.38 | 24.44 | 306.85 | 0.4957 | 727.0 | 511.9 | |
| 23.35 | 133.82 | 13.43 | 76.99 | 18.77 | 103.53 | 24.59 | 309.11 | 0.5099 | -1256.2 | -361.8 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 17.31 | 103.04 | 24.10 | 307.21 | 0.4916 | -649.0 | -442.8 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 16.97 | 102.52 | 23.58 | 307.19 | 0.4824 | 669.0 | 504.7 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 17.93 | 102.21 | 23.28 | 309.18 | 0.4870 | -567.0 | -424.8 | |
| 2.05 | 2.81 | 1.15 | 1.59 | 17.44 | 102.01 | 23.07 | 308.57 | 0.4802 | 877.9 | 774.7 | |
| 0.00 | 1.19 | 0.00 | 0.68 | 18.99 | 102.09 | 23.16 | 311.06 | 0.4952 | -752.0 | -593.4 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 15.01 | 101.41 | 22.48 | 304.88 | 0.4520 | 815.0 | 614.5 | |
| 0.00 | 1.53 | 0.00 | 0.86 | 17.53 | 101.58 | 22.65 | 309.22 | 0.4759 | 819.0 | 626.3 | |
| 4.09 | 7.76 | 2.31 | 4.37 | 18.18 | 101.43 | 22.50 | 310.50 | 0.4801 | -896.3 | -424.1 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 19.24 | 101.28 | 22.35 | 312.42 | 0.4883 | 403.0 | 474.4 | |
| 0.00 | 2.81 | 0.00 | 1.58 | 18.24 | 101.07 | 22.14 | 311.04 | 0.4765 | 287.0 | 434.2 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 18.06 | 99.94 | 21.01 | 312.14 | 0.4617 | 672.0 | 538.5 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 18.49 | 99.57 | 20.63 | 313.36 | 0.4616 | 651.0 | 585.1 | |
| 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. | |