SDO HMI 2011-08-08 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 |
| 4.51 | 32.95 | 2.43 | 17.89 | -16.29 | 243.42 | 7.79 | 198.98 | 0.4086 | 40.3 | 0.5 | |
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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 | 0.54 | -14.16 | 246.56 | 10.93 | 207.93 | 0.3942 | 801.0 | 640.2 | |
| 4.06 | 9.39 | 2.19 | 5.07 | -14.80 | 246.02 | 10.39 | 206.00 | 0.3994 | 1035.7 | 749.0 | |
| 0.00 | 1.72 | 0.00 | 0.93 | -15.34 | 245.66 | 10.03 | 204.63 | 0.4048 | 837.0 | 659.9 | |
| 0.00 | 2.71 | 0.00 | 1.46 | -14.59 | 245.59 | 9.97 | 205.30 | 0.3935 | 826.0 | 729.1 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -16.13 | 245.38 | 9.75 | 203.22 | 0.4144 | 792.0 | 639.5 | |
| 0.00 | 2.71 | 0.00 | 1.47 | -16.22 | 245.00 | 9.37 | 202.32 | 0.4134 | 862.0 | 688.7 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -17.20 | 242.12 | 6.50 | 195.22 | 0.4134 | -874.0 | -655.7 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -17.33 | 241.96 | 6.34 | 194.79 | 0.4148 | -702.0 | -459.7 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -16.76 | 241.27 | 5.65 | 193.58 | 0.4033 | -760.0 | -554.7 | |
| 0.00 | 1.45 | 0.00 | 0.78 | -17.02 | 240.93 | 5.31 | 192.63 | 0.4061 | -913.0 | -745.7 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -25.10 | 240.62 | 5.00 | 188.63 | 0.5279 | -732.0 | -611.1 | |
| 0.45 | 5.69 | 0.24 | 3.08 | -17.24 | 240.20 | 4.58 | 190.84 | 0.4072 | -908.8 | -938.4 | |
| 0.00 | 2.53 | 0.00 | 1.36 | -16.83 | 238.51 | 2.88 | 187.00 | 0.3965 | -697.0 | -589.4 | |
| 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. | |