SDO HMI 2011-12-15 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 |
| 71.01 | 376.78 | 37.83 | 200.67 | -18.17 | 352.17 | 13.18 | 216.08 | 0.3700 | 1083.9 | 409.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.55 | -19.24 | 354.21 | 15.23 | 218.16 | 0.4030 | -828.0 | -676.3 | |
| 53.04 | 342.83 | 28.23 | 182.60 | -17.86 | 352.36 | 13.37 | 216.98 | 0.3676 | 1410.6 | 410.6 | |
| 13.20 | -2.00 | 7.06 | -2.00 | -19.03 | 352.13 | 13.15 | 214.58 | 0.3805 | 992.0 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -17.00 | 351.47 | 12.48 | 216.65 | 0.3479 | 170.0 | 201.8 | |
| 2.30 | 4.17 | 1.22 | 2.22 | -18.79 | 351.41 | 12.42 | 213.49 | 0.3707 | 1103.1 | 803.1 | |
| 0.00 | 2.72 | 0.00 | 1.42 | -15.16 | 350.92 | 11.93 | 218.93 | 0.3189 | -1050.0 | -837.4 | |
| 0.00 | 3.66 | 0.00 | 1.95 | -19.07 | 351.17 | 12.19 | 212.57 | 0.3723 | 958.0 | 781.9 | |
| 2.47 | 12.51 | 1.32 | 6.68 | -19.50 | 351.02 | 12.03 | 211.58 | 0.3768 | 902.8 | 753.1 | |
| 0.00 | 2.47 | 0.00 | 1.29 | -16.33 | 350.58 | 11.59 | 215.88 | 0.3305 | -806.0 | -607.8 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -20.88 | 350.87 | 11.88 | 209.33 | 0.3943 | 651.0 | 519.9 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -19.32 | 350.33 | 11.34 | 210.39 | 0.3686 | 767.0 | 617.7 | |
| 0.00 | 1.28 | 0.00 | 0.69 | -20.66 | 350.30 | 11.31 | 208.46 | 0.3869 | 884.0 | 740.3 | |
| 0.00 | 1.70 | 0.00 | 0.92 | -22.76 | 346.74 | 7.75 | 198.46 | 0.3946 | 853.0 | 578.5 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -20.83 | 345.55 | 6.56 | 197.39 | 0.3592 | 884.0 | 687.2 | |
| 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. | |