SDO HMI 2011-12-05 19:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.93 | 44.85 | 13.16 | 25.72 | -17.93 | 78.08 | -24.45 | 128.55 | 0.5050 | -46.2 | 100.1 | |
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back to the solar disc SDO HMI 2011-12-05 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 |
| 7.67 | 12.53 | 4.31 | 7.04 | -17.53 | 80.41 | -22.11 | 130.49 | 0.4740 | 1006.5 | 642.7 | |
| 0.00 | 1.71 | 0.00 | 0.97 | -17.38 | 79.22 | -23.30 | 128.83 | 0.4867 | 975.0 | 824.3 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -17.13 | 78.68 | -23.84 | 127.81 | 0.4910 | 966.0 | 821.1 | |
| 2.81 | 6.40 | 1.61 | 3.65 | -17.23 | 78.13 | -24.40 | 127.37 | 0.4985 | 869.8 | 766.7 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -17.07 | 77.84 | -24.68 | 126.81 | 0.5007 | 704.0 | 545.5 | |
| 1.53 | 4.09 | 0.89 | 2.36 | -18.41 | 77.51 | -25.02 | 128.65 | 0.5159 | -876.9 | -773.7 | |
| 0.77 | -6.00 | 0.44 | -6.00 | -18.35 | 77.38 | -25.15 | 128.42 | 0.5169 | -848.7 | 999999 | |
| 2.13 | 12.96 | 1.24 | 7.55 | -18.63 | 76.92 | -25.61 | 128.39 | 0.5246 | -858.0 | -743.9 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -18.19 | 76.89 | -25.64 | 127.66 | 0.5214 | 413.0 | 195.1 | |
| 0.00 | 1.28 | 0.00 | 0.74 | -17.73 | 76.82 | -25.71 | 126.84 | 0.5184 | -942.0 | -839.2 | |
| 8.02 | -8.00 | 4.67 | -8.00 | -18.63 | 76.57 | -25.95 | 128.05 | 0.5287 | -864.5 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.95 | -18.07 | 75.73 | -26.80 | 126.33 | 0.5342 | -899.0 | -699.6 | |
| 0.00 | 1.19 | 0.00 | 0.70 | -18.67 | 75.35 | -27.18 | 126.91 | 0.5434 | -830.0 | -730.9 | |
| 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. | |