SDO HMI 2011-08-25 17:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.33 | 0.00 | 12.35 | 16.69 | 330.33 | -38.93 | 72.18 | 0.6339 | -278.1 | -247.4 | |
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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 | 0.59 | 13.60 | 335.23 | -34.03 | 76.09 | 0.5625 | -674.0 | -440.0 | |
| 0.00 | 2.51 | 0.00 | 1.50 | 13.87 | 335.15 | -34.11 | 75.63 | 0.5642 | -748.0 | -613.4 | |
| 0.00 | 1.26 | 0.00 | 0.77 | 15.48 | 333.43 | -35.83 | 73.31 | 0.5911 | -725.0 | -578.9 | |
| 0.00 | 0.72 | 0.00 | 0.44 | 14.32 | 333.23 | -36.03 | 75.30 | 0.5914 | -537.0 | -429.1 | |
| 0.00 | 1.26 | 0.00 | 0.79 | 17.84 | 331.88 | -37.38 | 69.90 | 0.6176 | -738.0 | -646.4 | |
| 0.00 | 0.90 | 0.00 | 0.56 | 17.68 | 331.80 | -37.46 | 70.18 | 0.6182 | -729.0 | -632.3 | |
| 0.00 | 3.77 | 0.00 | 2.42 | 18.45 | 330.42 | -38.84 | 69.40 | 0.6378 | -650.0 | -467.0 | |
| 0.00 | 1.35 | 0.00 | 0.89 | 18.76 | 328.67 | -40.59 | 69.44 | 0.6603 | -657.0 | -480.9 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 18.33 | 328.37 | -40.89 | 70.16 | 0.6629 | -662.0 | -578.5 | |
| 0.00 | 1.08 | 0.00 | 0.71 | 18.22 | 328.23 | -41.03 | 70.35 | 0.6643 | -536.0 | -395.6 | |
| 0.00 | 0.99 | 0.00 | 0.66 | 16.09 | 327.20 | -42.06 | 73.74 | 0.6727 | 679.0 | 590.7 | |
| 0.00 | 0.90 | 0.00 | 0.60 | 15.92 | 326.69 | -42.57 | 74.08 | 0.6788 | 774.0 | 669.0 | |
| 0.00 | 1.62 | 0.00 | 1.09 | 16.62 | 326.46 | -42.80 | 73.11 | 0.6827 | 810.0 | 686.3 | |
| 0.00 | 1.08 | 0.00 | 0.74 | 15.80 | 325.60 | -43.66 | 74.43 | 0.6919 | 500.0 | 357.9 | |
| 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. | |