| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.02 | 183.40 | 17.11 | 108.62 | 19.40 | 104.25 | -27.95 | 53.88 | 0.5499 | -716.8 | -348.1 | |
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back to the solar disc SDO HMI 2011-12-03 13:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 0.79 | 24.97 | 104.55 | -27.65 | 45.49 | 0.5921 | -766.0 | -557.1 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 23.57 | 104.04 | -28.16 | 47.87 | 0.5855 | -640.0 | -528.1 | |
| 0.00 | 3.07 | 0.00 | 1.79 | 17.41 | 104.97 | -27.23 | 56.39 | 0.5263 | 817.0 | 569.4 | |
| 28.51 | 167.36 | 16.81 | 98.69 | 19.05 | 104.44 | -27.76 | 54.20 | 0.5449 | -1110.8 | -375.4 | |
| 0.00 | 1.02 | 0.00 | 0.66 | 27.88 | 101.77 | -30.42 | 44.25 | 0.6438 | -560.0 | -465.4 | |
| 0.00 | 1.37 | 0.00 | 0.86 | 25.48 | 102.25 | -29.95 | 46.89 | 0.6195 | -793.0 | -590.8 | |
| 0.00 | 1.54 | 0.00 | 0.97 | 25.87 | 102.06 | -30.13 | 46.54 | 0.6245 | -758.0 | -652.4 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 24.96 | 102.16 | -30.03 | 47.65 | 0.6162 | -512.0 | -489.9 | |
| 0.00 | 0.85 | 0.00 | 0.57 | 30.54 | 100.31 | -31.88 | 42.28 | 0.6785 | -667.0 | -569.7 | |
| 0.51 | 1.54 | 0.30 | 0.91 | 17.93 | 102.76 | -29.43 | 57.41 | 0.5571 | 783.5 | 666.1 | |
| 0.00 | 1.45 | 0.00 | 0.98 | 30.02 | 99.17 | -33.03 | 43.77 | 0.6845 | -698.0 | -450.9 | |
| 0.00 | 1.02 | 0.00 | 0.62 | 17.79 | 100.37 | -31.83 | 59.41 | 0.5856 | 726.0 | 533.4 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 15.09 | 100.61 | -31.59 | 63.56 | 0.5670 | 640.0 | 525.2 | |
| 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. | |