SDO HMI 2011-08-09 08:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.01 | 0.00 | 13.38 | 20.18 | 221.88 | -3.83 | 11.52 | 0.2622 | -351.1 | -299.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.78 | 17.43 | 229.78 | 4.07 | 340.68 | 0.2056 | -789.0 | -650.7 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 20.63 | 226.48 | 0.77 | 357.09 | 0.2487 | -750.0 | -579.2 | |
| 0.00 | 5.06 | 0.00 | 2.58 | 19.56 | 225.92 | 0.22 | 359.11 | 0.2303 | -988.0 | -916.3 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 20.72 | 225.89 | 0.19 | 359.30 | 0.2500 | -984.0 | -816.9 | |
| 0.00 | 3.25 | 0.00 | 1.66 | 19.91 | 225.70 | -0.01 | 0.04 | 0.2361 | -738.0 | -719.5 | |
| 0.00 | 1.81 | 0.00 | 0.92 | 20.60 | 225.57 | -0.14 | 0.53 | 0.2479 | -889.0 | -711.7 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 18.04 | 224.26 | -1.45 | 6.74 | 0.2056 | -746.0 | -610.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 18.63 | 224.19 | -1.52 | 6.71 | 0.2158 | -895.0 | -766.9 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 15.15 | 221.98 | -3.73 | 22.18 | 0.1670 | -764.0 | -597.1 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 21.81 | 214.93 | -10.78 | 32.84 | 0.3216 | 804.0 | 606.1 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 20.92 | 214.30 | -11.41 | 36.01 | 0.3156 | 692.0 | 476.5 | |
| 0.00 | 4.34 | 0.00 | 2.28 | 22.20 | 213.86 | -11.85 | 34.56 | 0.3365 | 692.0 | 622.7 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 21.50 | 213.79 | -11.92 | 36.03 | 0.3282 | 791.0 | 622.5 | |
| 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. | |