SDO HMI 2011-08-26 18:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 30.77 | 0.00 | 15.71 | 19.02 | 355.67 | 0.17 | 356.88 | 0.2371 | -24.9 | -102.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.35 | 0.00 | 0.68 | 15.22 | 5.51 | 10.02 | 310.55 | 0.2219 | -875.0 | -754.5 | |
| 0.00 | 4.84 | 0.00 | 2.46 | 18.07 | 2.54 | 7.04 | 328.69 | 0.2253 | -824.0 | -687.9 | |
| 0.00 | 3.86 | 0.00 | 1.96 | 17.98 | 1.76 | 6.27 | 331.34 | 0.2176 | -917.0 | -783.3 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 17.68 | 1.05 | 5.56 | 333.47 | 0.2075 | -798.0 | -666.2 | |
| 0.00 | 2.51 | 0.00 | 1.28 | 19.89 | 0.38 | 4.89 | 340.18 | 0.2374 | -787.0 | -676.4 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 18.59 | 359.96 | 4.46 | 339.77 | 0.2143 | -828.0 | -631.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 19.56 | 358.70 | 3.20 | 346.34 | 0.2238 | -804.0 | -662.4 | |
| 0.00 | 1.52 | 0.00 | 0.78 | 20.25 | 353.32 | -2.18 | 8.87 | 0.2319 | 852.0 | 664.5 | |
| 0.00 | 3.14 | 0.00 | 1.59 | 18.73 | 352.80 | -2.70 | 12.43 | 0.2080 | 716.0 | 565.7 | |
| 0.00 | 2.33 | 0.00 | 1.19 | 18.93 | 348.36 | -7.14 | 29.65 | 0.2386 | 1076.0 | 817.1 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.77 | 348.20 | -7.29 | 30.52 | 0.2377 | 663.0 | 551.3 | |
| 0.00 | 2.60 | 0.00 | 1.36 | 23.32 | 347.31 | -8.19 | 24.95 | 0.3113 | 549.0 | 356.5 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 18.60 | 345.53 | -9.97 | 39.11 | 0.2612 | 782.0 | 587.9 | |
| 0.00 | 2.06 | 0.00 | 1.07 | 20.02 | 344.95 | -10.55 | 37.26 | 0.2853 | 847.0 | 591.4 | |
| 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. | |