SDO HMI 2011-05-31 14:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.02 | 188.17 | 28.91 | 149.07 | -20.11 | 20.10 | -48.59 | 115.47 | 0.7822 | 292.3 | 262.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.42 | 7.86 | 3.97 | 5.75 | -17.60 | 23.61 | -45.09 | 113.49 | 0.7383 | -698.9 | -579.7 | |
| 0.00 | 1.26 | 0.00 | 0.94 | -19.42 | 22.99 | -45.71 | 115.62 | 0.7509 | -680.0 | -603.6 | |
| 2.89 | 3.34 | 2.13 | 2.46 | -17.82 | 23.36 | -45.34 | 113.69 | 0.7417 | -588.5 | -522.0 | |
| 0.00 | 1.17 | 0.00 | 0.88 | -19.39 | 22.73 | -45.97 | 115.47 | 0.7536 | -550.0 | -390.0 | |
| 0.00 | 1.26 | 0.00 | 0.95 | -19.38 | 22.49 | -46.21 | 115.39 | 0.7560 | -267.0 | -292.2 | |
| 0.00 | 1.08 | 0.00 | 0.82 | -19.35 | 22.13 | -46.57 | 115.21 | 0.7596 | -474.0 | -433.3 | |
| 0.00 | 0.81 | 0.00 | 0.61 | -18.80 | 22.28 | -46.42 | 114.58 | 0.7563 | -478.0 | -412.2 | |
| 3.43 | 6.50 | 2.62 | 4.96 | -18.54 | 21.53 | -47.17 | 113.99 | 0.7633 | -616.6 | -420.2 | |
| 0.00 | 4.70 | 0.00 | 3.61 | -18.86 | 21.32 | -47.38 | 114.32 | 0.7664 | -73.0 | -84.2 | |
| 1.26 | 2.17 | 0.98 | 1.68 | -18.95 | 20.90 | -47.80 | 114.29 | 0.7710 | 551.9 | 396.0 | |
| 0.00 | 1.17 | 0.00 | 0.91 | -18.89 | 20.64 | -48.06 | 114.13 | 0.7734 | 406.0 | 341.4 | |
| 19.05 | 155.59 | 15.19 | 124.47 | -20.36 | 19.84 | -48.85 | 115.69 | 0.7857 | 1002.9 | 331.8 | |
| 4.97 | -12.00 | 4.02 | -12.00 | -20.68 | 19.16 | -49.54 | 115.86 | 0.7933 | 586.8 | 999999 | |
| 0.00 | 1.26 | 0.00 | 1.03 | -19.77 | 18.40 | -50.30 | 114.51 | 0.7980 | 413.0 | 290.4 | |
| 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. | |