SDO HMI 2014-08-13 10:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.26 | 383.29 | 35.04 | 215.43 | 15.10 | 133.72 | 27.34 | 289.90 | 0.4735 | -870.1 | -357.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.62 | 16.82 | 135.60 | 29.22 | 292.37 | 0.5073 | 709.0 | 619.3 | |
| 0.00 | 1.35 | 0.00 | 0.77 | 16.17 | 135.09 | 28.71 | 291.38 | 0.4975 | -187.0 | -134.8 | |
| 61.36 | 363.19 | 34.57 | 204.66 | 15.24 | 134.02 | 27.64 | 290.08 | 0.4785 | -1442.1 | -408.1 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 13.27 | 133.30 | 26.92 | 286.34 | 0.4611 | 236.0 | 212.8 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 16.46 | 131.90 | 25.52 | 293.87 | 0.4536 | -716.0 | -543.8 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 12.60 | 127.45 | 21.07 | 287.82 | 0.3702 | 687.0 | 527.1 | |
| 0.00 | 2.17 | 0.00 | 1.15 | 12.67 | 127.13 | 20.75 | 288.24 | 0.3655 | 596.0 | 537.7 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 12.58 | 127.05 | 20.67 | 288.05 | 0.3640 | 886.0 | 759.7 | |
| 0.00 | 2.71 | 0.00 | 1.44 | 12.40 | 126.97 | 20.59 | 287.63 | 0.3620 | 959.0 | 712.1 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 11.52 | 125.98 | 19.60 | 285.84 | 0.3431 | 887.0 | 685.3 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 11.22 | 125.86 | 19.48 | 285.05 | 0.3401 | 807.0 | 634.3 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 6.81 | 125.05 | 18.67 | 271.90 | 0.3195 | 903.0 | 682.1 | |
| 0.90 | 2.62 | 0.47 | 1.36 | 10.33 | 124.33 | 17.95 | 283.28 | 0.3128 | 1100.0 | 920.7 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 11.22 | 123.38 | 17.00 | 286.77 | 0.3008 | 670.0 | 567.9 | |
| 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. | |