SDO HMI 2011-08-10 05:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.32 | 0.00 | 10.99 | 19.19 | 223.73 | 9.60 | 325.38 | 0.2755 | -210.5 | -180.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.52 | 20.00 | 226.90 | 12.78 | 318.91 | 0.3175 | -634.0 | -573.5 | |
| 0.00 | 2.17 | 0.00 | 1.13 | 20.04 | 226.61 | 12.48 | 319.63 | 0.3148 | -861.0 | -744.9 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 19.58 | 226.05 | 11.92 | 319.88 | 0.3032 | -974.0 | -741.2 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 20.30 | 226.10 | 11.97 | 321.33 | 0.3127 | -806.0 | -716.8 | |
| 0.00 | 2.89 | 0.00 | 1.50 | 20.10 | 225.42 | 11.29 | 322.46 | 0.3032 | -775.0 | -781.8 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 17.82 | 224.13 | 10.00 | 320.43 | 0.2607 | -861.0 | -727.9 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 17.98 | 223.82 | 9.69 | 321.71 | 0.2594 | -848.0 | -615.7 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 18.73 | 223.66 | 9.53 | 323.94 | 0.2677 | -1197.0 | -995.4 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 19.32 | 221.91 | 7.78 | 330.42 | 0.2599 | 552.0 | 519.7 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.95 | 221.43 | 7.31 | 331.18 | 0.2506 | 1035.0 | 833.8 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 19.26 | 221.35 | 7.22 | 332.08 | 0.2546 | 948.0 | 780.2 | |
| 0.00 | 2.08 | 0.00 | 1.06 | 18.09 | 220.62 | 6.50 | 332.18 | 0.2314 | 848.0 | 716.1 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 18.19 | 220.27 | 6.15 | 333.65 | 0.2302 | 836.0 | 636.8 | |
| 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. | |