SDO HMI 2011-08-09 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 |
| 0.00 | 37.20 | 0.00 | 18.94 | 19.31 | 224.81 | 2.41 | 350.13 | 0.2309 | -704.1 | -627.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.44 | 0.00 | 0.74 | 17.45 | 229.94 | 7.53 | 327.20 | 0.2319 | -845.0 | -555.9 | |
| 0.00 | 3.61 | 0.00 | 1.84 | 19.61 | 225.92 | 3.51 | 345.92 | 0.2383 | -1168.0 | -855.5 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 20.67 | 225.91 | 3.50 | 347.02 | 0.2558 | -854.0 | -720.9 | |
| 0.00 | 4.51 | 0.00 | 2.30 | 19.76 | 225.63 | 3.23 | 347.19 | 0.2398 | -615.0 | -757.7 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 19.98 | 225.57 | 3.17 | 347.63 | 0.2432 | -893.0 | -787.7 | |
| 0.00 | 6.86 | 0.00 | 3.50 | 20.08 | 225.31 | 2.91 | 348.68 | 0.2439 | -519.0 | -647.7 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 20.43 | 224.54 | 2.14 | 351.85 | 0.2475 | -779.0 | -484.7 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 18.21 | 224.35 | 1.95 | 351.11 | 0.2097 | -915.0 | -732.6 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 18.46 | 224.32 | 1.92 | 351.43 | 0.2139 | -1004.0 | -660.4 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 19.02 | 224.26 | 1.86 | 352.06 | 0.2232 | -1005.0 | -769.9 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 18.31 | 224.09 | 1.69 | 352.32 | 0.2107 | -612.0 | -534.9 | |
| 0.00 | 5.96 | 0.00 | 3.02 | 18.34 | 223.52 | 1.12 | 354.93 | 0.2102 | -977.0 | -781.1 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 20.90 | 221.78 | -0.62 | 2.31 | 0.2532 | -710.0 | -567.6 | |
| 0.00 | 1.90 | 0.00 | 0.96 | 19.06 | 221.56 | -0.84 | 3.60 | 0.2220 | 1038.0 | 852.3 | |
| 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. | |