| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.36 | 226.39 | 16.61 | 132.66 | 28.37 | 42.39 | 20.87 | 324.07 | 0.5361 | -879.1 | -434.8 | |
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back to the solar disc SDO HMI 2011-11-14 15:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.72 | 0.00 | 1.07 | 29.34 | 48.94 | 27.41 | 318.24 | 0.6049 | -727.0 | -546.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 23.98 | 43.66 | 22.14 | 316.47 | 0.5020 | -538.0 | -456.8 | |
| 0.00 | 1.46 | 0.00 | 0.90 | 32.21 | 45.12 | 23.60 | 325.48 | 0.6000 | -707.0 | -562.9 | |
| 0.00 | 1.03 | 0.00 | 0.66 | 35.15 | 45.68 | 24.16 | 328.05 | 0.6347 | -506.0 | -422.2 | |
| 0.00 | 1.12 | 0.00 | 0.71 | 34.90 | 45.48 | 23.96 | 328.00 | 0.6308 | -443.0 | -416.8 | |
| 1.89 | 208.60 | 1.11 | 122.10 | 28.14 | 42.77 | 21.24 | 323.31 | 0.5369 | -1078.9 | -453.3 | |
| 9.63 | -6.00 | 5.65 | -6.00 | 28.40 | 42.53 | 21.01 | 323.93 | 0.5377 | -1113.1 | 999999 | |
| 12.46 | -6.00 | 7.28 | -6.00 | 28.05 | 42.39 | 20.86 | 323.66 | 0.5325 | -1384.8 | 999999 | |
| 1.89 | -6.00 | 1.11 | -6.00 | 28.38 | 42.09 | 20.57 | 324.44 | 0.5337 | -987.8 | 999999 | |
| 2.49 | -6.00 | 1.46 | -6.00 | 28.61 | 42.10 | 20.58 | 324.71 | 0.5363 | -860.9 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.81 | 28.88 | 41.80 | 20.28 | 325.42 | 0.5368 | -595.0 | -438.8 | |
| 0.00 | 1.29 | 0.00 | 0.77 | 30.20 | 42.04 | 20.52 | 326.68 | 0.5537 | 545.0 | 358.5 | |
| 0.00 | 1.89 | 0.00 | 1.11 | 29.02 | 41.54 | 20.02 | 325.91 | 0.5361 | -569.0 | -486.6 | |
| 0.00 | 2.84 | 0.00 | 1.66 | 29.70 | 40.34 | 18.82 | 328.24 | 0.5344 | -839.0 | -564.7 | |
| 0.00 | 1.20 | 0.00 | 0.70 | 30.04 | 39.50 | 17.98 | 329.72 | 0.5322 | -752.0 | -614.1 | |
| 0.00 | 3.09 | 0.00 | 1.73 | 26.60 | 36.49 | 14.97 | 330.17 | 0.4663 | 780.0 | 705.5 | |
| 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. | |