| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.30 | 189.67 | 21.25 | 127.86 | 14.37 | 251.79 | 41.08 | 289.96 | 0.6792 | -562.3 | -282.5 | |
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back to the solar disc SDO HMI 2011-11-27 14:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.60 | 0.00 | 0.41 | 13.01 | 253.89 | 43.17 | 287.34 | 0.7007 | 556.0 | 392.3 | |
| 28.99 | 170.77 | 19.70 | 116.02 | 14.28 | 252.43 | 41.72 | 289.57 | 0.6868 | -1066.1 | -350.1 | |
| 2.31 | -2.00 | 1.55 | -2.00 | 14.56 | 251.76 | 41.05 | 290.20 | 0.6796 | -817.0 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.63 | 13.59 | 251.27 | 40.55 | 288.98 | 0.6706 | -703.0 | -583.3 | |
| 0.00 | 0.60 | 0.00 | 0.41 | 17.23 | 251.69 | 40.97 | 294.00 | 0.6879 | -522.0 | -433.0 | |
| 0.00 | 0.94 | 0.00 | 0.63 | 16.28 | 251.20 | 40.48 | 292.87 | 0.6787 | -534.0 | -453.8 | |
| 0.00 | 0.94 | 0.00 | 0.64 | 18.00 | 251.66 | 40.94 | 295.09 | 0.6905 | -548.0 | -404.0 | |
| 0.00 | 1.11 | 0.00 | 0.74 | 17.13 | 250.00 | 39.28 | 294.58 | 0.6677 | -648.0 | -495.9 | |
| 0.00 | 1.37 | 0.00 | 0.86 | 11.80 | 247.63 | 36.91 | 287.54 | 0.6189 | 840.0 | 726.8 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 17.07 | 245.18 | 34.46 | 296.92 | 0.6089 | 562.0 | 358.8 | |
| 0.00 | 1.88 | 0.00 | 1.17 | 17.66 | 244.59 | 33.87 | 298.17 | 0.6047 | 584.0 | 482.6 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 10.60 | 243.09 | 32.38 | 287.31 | 0.5535 | 681.0 | 496.5 | |
| 0.00 | 1.97 | 0.00 | 1.18 | 13.65 | 242.90 | 32.18 | 292.67 | 0.5631 | 254.0 | 305.0 | |
| 0.00 | 1.71 | 0.00 | 1.01 | 10.10 | 242.43 | 31.72 | 286.70 | 0.5425 | 651.0 | 581.1 | |
| 0.00 | 3.59 | 0.00 | 2.20 | 17.67 | 243.55 | 32.83 | 298.83 | 0.5920 | 714.0 | 608.6 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 13.93 | 241.90 | 31.19 | 293.72 | 0.5512 | 558.0 | 489.8 | |
| 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. | |