| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.89 | 165.84 | 27.04 | 118.16 | 15.77 | 233.45 | 44.17 | 291.02 | 0.7207 | -723.1 | -317.6 | |
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back to the solar disc SDO HMI 2011-11-29 05:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 1.20 | 16.68 | 235.28 | 46.00 | 291.66 | 0.7437 | -583.0 | -510.1 | |
| 0.00 | 2.74 | 0.00 | 2.03 | 17.58 | 235.38 | 46.10 | 292.79 | 0.7475 | -489.0 | -391.6 | |
| 1.28 | 2.57 | 0.95 | 1.90 | 17.74 | 235.21 | 45.93 | 293.05 | 0.7461 | -552.8 | -572.4 | |
| 1.80 | 3.76 | 1.33 | 2.78 | 17.95 | 235.02 | 45.74 | 293.40 | 0.7447 | -610.7 | -674.6 | |
| 0.00 | 1.54 | 0.00 | 1.14 | 18.17 | 234.91 | 45.63 | 293.72 | 0.7442 | -357.0 | -372.2 | |
| 1.20 | 131.62 | 0.85 | 93.51 | 15.20 | 233.71 | 44.43 | 290.18 | 0.7221 | -400.2 | -284.2 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 14.54 | 233.36 | 44.08 | 289.38 | 0.7162 | -203.0 | -179.2 | |
| 24.72 | -6.00 | 17.55 | -6.00 | 15.42 | 233.38 | 44.10 | 290.58 | 0.7189 | -1019.8 | 999999 | |
| 1.88 | 2.74 | 1.38 | 2.01 | 19.15 | 234.26 | 44.98 | 295.22 | 0.7405 | 498.6 | 413.5 | |
| 4.62 | 8.21 | 3.29 | 5.84 | 16.62 | 233.24 | 43.96 | 292.25 | 0.7210 | -621.5 | -529.2 | |
| 2.39 | -6.00 | 1.69 | -6.00 | 15.80 | 232.84 | 43.56 | 291.27 | 0.7139 | -890.0 | 999999 | |
| 0.00 | 5.90 | 0.00 | 4.17 | 16.29 | 232.85 | 43.57 | 291.93 | 0.7155 | -843.0 | -662.6 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 13.67 | 232.06 | 42.78 | 288.59 | 0.6986 | -540.0 | -484.2 | |
| 0.00 | 1.11 | 0.00 | 0.77 | 14.83 | 231.91 | 42.63 | 290.25 | 0.7003 | -507.0 | -459.4 | |
| 0.00 | 0.94 | 0.00 | 0.67 | 19.36 | 232.54 | 43.26 | 296.16 | 0.7227 | -535.0 | -413.5 | |
| 0.00 | 1.03 | 0.00 | 0.70 | 15.17 | 231.17 | 41.89 | 290.99 | 0.6926 | 431.0 | 341.2 | |
| 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. | |