SDO HMI 2011-10-11 12:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.57 | 96.29 | 13.05 | 49.21 | 20.08 | 109.62 | -1.92 | 7.39 | 0.2460 | 480.2 | 192.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.64 | 25.28 | 114.04 | 2.50 | 353.14 | 0.3320 | 741.0 | 591.9 | |
| 7.27 | 28.36 | 3.71 | 14.48 | 20.26 | 112.10 | 0.56 | 357.84 | 0.2453 | -890.7 | -935.2 | |
| 2.54 | -2.00 | 1.30 | -2.00 | 20.04 | 111.69 | 0.15 | 359.43 | 0.2415 | -935.4 | 999999 | |
| 0.00 | 3.68 | 0.00 | 1.88 | 19.95 | 111.28 | -0.27 | 1.05 | 0.2400 | -1051.0 | -784.1 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 24.97 | 110.61 | -0.94 | 2.63 | 0.3247 | 880.0 | 604.7 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 19.79 | 109.43 | -2.11 | 8.35 | 0.2398 | 724.0 | 635.0 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 18.99 | 109.31 | -2.23 | 9.37 | 0.2267 | 811.0 | 673.2 | |
| 0.00 | 1.75 | 0.00 | 0.89 | 19.70 | 109.31 | -2.24 | 8.90 | 0.2386 | 887.0 | 635.8 | |
| 0.00 | 2.10 | 0.00 | 1.07 | 19.52 | 109.12 | -2.42 | 9.77 | 0.2360 | 934.0 | 815.4 | |
| 0.00 | 1.75 | 0.00 | 0.89 | 19.33 | 109.09 | -2.45 | 10.03 | 0.2330 | 943.0 | 676.4 | |
| 0.00 | 2.71 | 0.00 | 1.38 | 19.02 | 108.78 | -2.77 | 11.55 | 0.2288 | 699.0 | 661.2 | |
| 15.76 | 48.59 | 8.04 | 24.78 | 19.54 | 108.42 | -3.12 | 12.48 | 0.2387 | 1116.6 | 718.8 | |
| 0.00 | 1.66 | 0.00 | 0.89 | 27.02 | 103.95 | -7.59 | 18.23 | 0.3779 | 806.0 | 558.8 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 26.12 | 103.14 | -8.41 | 20.95 | 0.3687 | 718.0 | 515.6 | |
| 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. | |