SDO HMI 2011-12-17 04:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.47 | 27.33 | 5.48 | 14.36 | -17.12 | 323.77 | 11.13 | 213.73 | 0.3343 | -173.5 | 76.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.59 | -17.02 | 326.80 | 14.17 | 220.48 | 0.3621 | 555.0 | 466.5 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -20.18 | 326.43 | 13.79 | 214.40 | 0.3978 | -649.0 | -537.7 | |
| 0.00 | 2.21 | 0.00 | 1.17 | -16.99 | 326.01 | 13.37 | 218.94 | 0.3535 | 1027.0 | 812.4 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -14.22 | 325.64 | 13.00 | 223.87 | 0.3161 | 770.0 | 557.7 | |
| 1.87 | 2.38 | 0.99 | 1.26 | -17.49 | 325.16 | 12.52 | 216.25 | 0.3512 | 884.9 | 769.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -17.70 | 324.92 | 12.28 | 215.36 | 0.3517 | 980.0 | 797.5 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -17.61 | 324.72 | 12.08 | 215.09 | 0.3486 | 985.0 | 782.0 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -18.48 | 324.15 | 11.51 | 212.38 | 0.3549 | 833.0 | 628.8 | |
| 5.28 | 5.28 | 2.75 | 2.75 | -15.44 | 323.68 | 11.04 | 216.72 | 0.3101 | -999.4 | 0.0 | |
| 0.00 | 2.04 | 0.00 | 1.07 | -17.25 | 322.37 | 9.73 | 210.16 | 0.3228 | -824.0 | -665.4 | |
| 3.32 | 3.66 | 1.74 | 1.91 | -17.38 | 322.00 | 9.36 | 209.02 | 0.3215 | -1062.9 | -939.0 | |
| 0.00 | 2.38 | 0.00 | 1.25 | -17.84 | 321.49 | 8.85 | 207.00 | 0.3242 | -963.0 | -696.3 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -18.33 | 321.42 | 8.78 | 206.11 | 0.3309 | -1071.0 | -872.4 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -18.80 | 321.23 | 8.59 | 204.97 | 0.3364 | -781.0 | -609.2 | |
| 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. | |