| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.38 | 175.08 | 35.60 | 110.57 | 34.03 | 267.61 | 10.61 | 345.76 | 0.6230 | -20.5 | -71.7 | |
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back to the solar disc SDO HMI 2010-12-31 20:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.89 | 95.19 | 13.22 | 60.26 | 33.67 | 269.62 | 12.61 | 343.03 | 0.6249 | -1094.5 | -375.7 | |
| 0.00 | 1.10 | 0.00 | 0.69 | 32.97 | 269.23 | 12.22 | 343.13 | 0.6143 | -793.0 | -709.2 | |
| 1.95 | -1.00 | 1.23 | -1.00 | 33.48 | 269.01 | 12.01 | 343.69 | 0.6201 | -805.0 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.75 | 34.14 | 268.78 | 11.77 | 344.33 | 0.6277 | -569.0 | -393.9 | |
| 1.53 | 2.12 | 0.96 | 1.34 | 33.73 | 268.68 | 11.68 | 344.24 | 0.6221 | -649.4 | -632.6 | |
| 1.10 | 1.95 | 0.70 | 1.24 | 33.99 | 268.50 | 11.50 | 344.60 | 0.6247 | -542.9 | -335.3 | |
| 0.00 | 1.10 | 0.00 | 0.70 | 34.47 | 268.24 | 11.24 | 345.17 | 0.6300 | -571.0 | -483.4 | |
| 0.00 | 1.27 | 0.00 | 0.79 | 33.05 | 266.66 | 9.65 | 346.54 | 0.6061 | 633.0 | 526.3 | |
| 0.00 | 1.95 | 0.00 | 1.24 | 34.52 | 266.54 | 9.53 | 347.35 | 0.6253 | -315.0 | -398.5 | |
| 2.12 | 61.23 | 1.32 | 38.47 | 33.44 | 265.52 | 8.52 | 348.23 | 0.6079 | 761.4 | 568.5 | |
| 0.00 | 1.19 | 0.00 | 0.76 | 35.11 | 265.26 | 8.25 | 349.21 | 0.6295 | 596.0 | 492.4 | |
| 5.52 | -10.00 | 3.46 | -10.00 | 34.17 | 264.98 | 7.98 | 349.22 | 0.6163 | 895.9 | 999999 | |
| 3.82 | 6.79 | 2.44 | 4.33 | 35.33 | 264.92 | 7.91 | 349.72 | 0.6316 | 703.9 | 478.9 | |
| 19.45 | -10.00 | 12.27 | -10.00 | 34.66 | 264.70 | 7.70 | 349.76 | 0.6221 | 880.6 | 999999 | |
| 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. | |