| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.58 | 328.34 | 27.71 | 180.37 | 28.07 | 43.32 | -5.67 | 11.53 | 0.4331 | -894.8 | -376.3 | |
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back to the solar disc SDO HMI 2011-11-12 13:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 0.75 | 34.38 | 46.09 | -2.90 | 4.61 | 0.5219 | -660.0 | -491.7 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 32.04 | 45.18 | -3.81 | 6.65 | 0.4882 | -765.0 | -624.7 | |
| 48.18 | 314.23 | 26.39 | 172.19 | 27.94 | 43.79 | -5.20 | 10.82 | 0.4285 | -1274.7 | -401.4 | |
| 0.34 | -3.00 | 0.19 | -3.00 | 28.63 | 43.62 | -5.37 | 10.82 | 0.4397 | -708.5 | 999999 | |
| 0.60 | -3.00 | 0.33 | -3.00 | 28.14 | 43.30 | -5.68 | 11.69 | 0.4330 | -896.9 | 999999 | |
| 1.46 | -3.00 | 0.80 | -3.00 | 28.10 | 42.97 | -6.02 | 12.37 | 0.4336 | -744.8 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 29.28 | 41.22 | -7.77 | 14.99 | 0.4578 | -863.0 | -732.0 | |
| 0.00 | 2.24 | 0.00 | 1.24 | 28.58 | 40.69 | -8.30 | 16.44 | 0.4497 | -801.0 | -683.3 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 27.37 | 37.43 | -11.56 | 23.42 | 0.4496 | 743.0 | 583.6 | |
| 0.00 | 1.63 | 0.00 | 0.94 | 30.27 | 34.45 | -14.54 | 25.38 | 0.5079 | 463.0 | 299.9 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 30.77 | 29.60 | -19.39 | 31.47 | 0.5484 | 632.0 | 547.2 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 28.45 | 26.71 | -22.28 | 37.74 | 0.5468 | 637.0 | 504.7 | |
| 0.00 | 2.24 | 0.00 | 1.33 | 28.24 | 26.06 | -22.93 | 38.75 | 0.5504 | 635.0 | 500.4 | |
| 0.00 | 2.07 | 0.00 | 1.27 | 30.80 | 24.45 | -24.54 | 37.31 | 0.5907 | 718.0 | 622.5 | |
| 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. | |