| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.92 | 64.24 | 21.02 | 35.53 | 17.77 | 214.13 | -21.29 | 50.91 | 0.4470 | 471.9 | 60.2 | |
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back to the solar disc SDO HMI 2011-11-25 17:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 0.92 | 17.56 | 217.88 | -17.54 | 46.15 | 0.4002 | 723.0 | 615.5 | |
| 0.00 | 2.05 | 0.00 | 1.12 | 18.52 | 217.32 | -18.10 | 45.24 | 0.4166 | 835.0 | 735.8 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 19.28 | 216.41 | -19.01 | 45.23 | 0.4350 | 463.0 | 526.1 | |
| 7.36 | 9.67 | 4.01 | 5.27 | 17.21 | 215.86 | -19.56 | 49.79 | 0.4207 | -1042.2 | -914.7 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 19.27 | 215.45 | -19.98 | 46.59 | 0.4458 | 865.0 | 716.4 | |
| 1.03 | 1.28 | 0.56 | 0.70 | 17.27 | 215.52 | -19.90 | 50.14 | 0.4253 | -820.1 | -669.3 | |
| 0.00 | 3.59 | 0.00 | 1.97 | 17.17 | 215.23 | -20.19 | 50.70 | 0.4279 | -247.0 | -509.6 | |
| 1.37 | 4.45 | 0.75 | 2.45 | 17.91 | 214.95 | -20.47 | 49.69 | 0.4383 | -864.1 | -753.9 | |
| 0.00 | 3.17 | 0.00 | 1.75 | 18.15 | 214.85 | -20.57 | 49.37 | 0.4417 | -642.0 | -629.6 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 17.96 | 213.68 | -21.74 | 51.20 | 0.4541 | 704.0 | 580.1 | |
| 1.03 | 1.71 | 0.57 | 0.95 | 17.98 | 213.34 | -22.08 | 51.56 | 0.4585 | 759.1 | 837.4 | |
| 3.17 | 32.51 | 1.76 | 18.13 | 17.61 | 213.22 | -22.20 | 52.37 | 0.4567 | 1075.7 | 821.7 | |
| 23.96 | -12.00 | 13.37 | -12.00 | 17.83 | 212.85 | -22.57 | 52.41 | 0.4630 | 1002.7 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 18.16 | 212.67 | -22.75 | 52.01 | 0.4681 | 547.0 | 436.7 | |
| 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. | |