| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.68 | 24.39 | 0.36 | 12.97 | 17.94 | 214.54 | 13.17 | 323.11 | 0.3630 | 645.9 | 476.7 | |
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back to the solar disc SDO HMI 2011-11-28 07:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.68 | 0.00 | 0.37 | 18.06 | 218.63 | 17.26 | 315.78 | 0.4063 | 1029.0 | 728.5 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 16.37 | 218.08 | 16.71 | 313.47 | 0.3818 | -915.0 | -758.9 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 17.85 | 217.67 | 16.30 | 316.98 | 0.3933 | 751.0 | 505.7 | |
| 0.00 | 2.31 | 0.00 | 1.24 | 17.73 | 217.33 | 15.96 | 317.33 | 0.3883 | 915.0 | 698.9 | |
| 0.00 | 1.88 | 0.00 | 1.02 | 20.38 | 216.29 | 14.92 | 323.67 | 0.4091 | 907.0 | 745.5 | |
| 0.00 | 2.40 | 0.00 | 1.27 | 16.33 | 215.49 | 14.12 | 318.06 | 0.3518 | -748.0 | -674.4 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 17.47 | 213.95 | 12.58 | 323.38 | 0.3499 | 825.0 | 554.4 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 17.44 | 213.60 | 12.23 | 324.09 | 0.3461 | 814.0 | 671.3 | |
| 0.68 | 1.63 | 0.36 | 0.86 | 17.84 | 213.28 | 11.91 | 325.50 | 0.3483 | 866.1 | 722.3 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 17.38 | 213.21 | 11.85 | 324.83 | 0.3416 | 1046.0 | 883.2 | |
| 0.00 | 2.31 | 0.00 | 1.22 | 17.91 | 213.00 | 11.63 | 326.23 | 0.3465 | 900.0 | 739.2 | |
| 0.00 | 2.31 | 0.00 | 1.22 | 17.75 | 212.89 | 11.52 | 326.21 | 0.3435 | 973.0 | 811.3 | |
| 0.00 | 2.40 | 0.00 | 1.26 | 17.48 | 212.52 | 11.16 | 326.57 | 0.3365 | 780.0 | 687.4 | |
| 0.00 | 1.80 | 0.00 | 0.96 | 21.18 | 211.72 | 10.35 | 333.84 | 0.3816 | 820.0 | 595.5 | |
| 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. | |