SDO HMI 2014-08-09 22:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.37 | 45.13 | 5.69 | 24.98 | -18.82 | 160.97 | 8.33 | 197.95 | 0.4481 | 714.6 | 650.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.81 | 0.00 | 1.01 | -18.52 | 165.00 | 12.37 | 205.90 | 0.4669 | 654.0 | 434.0 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -18.30 | 164.43 | 11.80 | 205.06 | 0.4601 | 733.0 | 474.9 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -19.24 | 161.39 | 8.75 | 198.44 | 0.4561 | 819.0 | 748.9 | |
| 0.00 | 2.98 | 0.00 | 1.65 | -18.94 | 161.31 | 8.67 | 198.51 | 0.4512 | 935.0 | 785.8 | |
| 1.08 | 15.98 | 0.60 | 8.88 | -19.37 | 161.13 | 8.50 | 197.85 | 0.4568 | 871.1 | 759.8 | |
| 6.41 | 12.91 | 3.50 | 7.05 | -17.20 | 160.93 | 8.30 | 199.09 | 0.4234 | 962.4 | 785.6 | |
| 0.81 | -5.00 | 0.45 | -5.00 | -19.23 | 160.87 | 8.23 | 197.42 | 0.4534 | 932.4 | 999999 | |
| 0.99 | -6.00 | 0.54 | -6.00 | -17.26 | 160.71 | 8.08 | 198.56 | 0.4232 | 989.3 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -23.24 | 160.56 | 7.92 | 194.41 | 0.5110 | 558.0 | 375.0 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -20.85 | 159.87 | 7.23 | 194.46 | 0.4732 | -813.0 | -678.9 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -19.38 | 159.67 | 7.04 | 194.93 | 0.4505 | 831.0 | 677.6 | |
| 1.08 | 2.71 | 0.60 | 1.51 | -19.85 | 159.04 | 6.41 | 193.39 | 0.4551 | 806.8 | 651.1 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -20.08 | 158.50 | 5.86 | 192.18 | 0.4567 | 519.0 | 473.7 | |
| 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. | |