SDO HMI 2011-08-21 06:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.43 | 220.46 | 32.66 | 127.72 | -21.15 | 54.41 | -13.76 | 154.71 | 0.5199 | 111.5 | -54.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.34 | 0.00 | 1.29 | -18.52 | 61.45 | -6.73 | 165.46 | 0.4444 | 765.0 | 602.5 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -19.00 | 60.78 | -7.39 | 164.40 | 0.4544 | 759.0 | 618.5 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -17.63 | 58.49 | -9.69 | 158.81 | 0.4454 | 660.0 | 494.9 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -19.22 | 58.14 | -10.04 | 159.43 | 0.4703 | 560.0 | 445.8 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.51 | 58.14 | -10.03 | 158.01 | 0.4456 | 825.0 | 700.9 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.32 | 57.64 | -10.54 | 156.84 | 0.4459 | 772.0 | 680.7 | |
| 4.32 | 77.11 | 2.48 | 44.37 | -21.60 | 57.02 | -11.16 | 159.25 | 0.5101 | 769.6 | 406.0 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -17.53 | 57.14 | -11.04 | 156.07 | 0.4520 | 886.0 | 858.0 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -17.77 | 56.89 | -11.28 | 155.83 | 0.4569 | 706.0 | 571.8 | |
| 14.85 | -7.00 | 8.54 | -7.00 | -21.44 | 56.60 | -11.58 | 158.42 | 0.5101 | 1179.7 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -19.09 | 56.45 | -11.73 | 156.21 | 0.4783 | 712.0 | 463.3 | |
| 2.34 | 3.87 | 1.35 | 2.24 | -21.84 | 55.86 | -12.32 | 157.51 | 0.5197 | 766.4 | 653.8 | |
| 3.51 | 13.68 | 2.02 | 7.87 | -20.43 | 54.58 | -13.59 | 154.22 | 0.5084 | 1001.8 | 547.5 | |
| 4.23 | -13.00 | 2.44 | -13.00 | -20.68 | 54.46 | -13.71 | 154.24 | 0.5125 | 736.3 | 999999 | |
| 4.59 | 5.22 | 2.65 | 3.02 | -21.03 | 54.30 | -13.88 | 154.29 | 0.5182 | 734.7 | 578.7 | |
| 1.17 | -13.00 | 0.67 | -13.00 | -20.51 | 54.24 | -13.93 | 153.74 | 0.5117 | 607.3 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -21.11 | 53.95 | -14.22 | 153.81 | 0.5215 | 674.0 | 460.8 | |
| 0.00 | 2.34 | 0.00 | 1.35 | -20.83 | 53.95 | -14.23 | 153.55 | 0.5179 | -120.0 | -26.9 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -21.01 | 53.86 | -14.31 | 153.58 | 0.5207 | 513.0 | 401.3 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -21.15 | 53.71 | -14.46 | 153.47 | 0.5236 | 543.0 | 346.4 | |
| 0.00 | 2.25 | 0.00 | 1.30 | -20.70 | 53.66 | -14.52 | 152.97 | 0.5181 | -206.0 | -307.1 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -19.96 | 53.33 | -14.85 | 151.74 | 0.5107 | -895.0 | -709.7 | |
| 3.42 | 88.99 | 2.00 | 51.96 | -21.45 | 53.01 | -15.17 | 152.65 | 0.5322 | -731.7 | -525.0 | |
| 8.10 | -23.00 | 4.73 | -23.00 | -21.19 | 52.53 | -15.65 | 151.68 | 0.5322 | -1015.4 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.94 | -20.54 | 52.53 | -15.64 | 151.05 | 0.5238 | -437.0 | -191.1 | |
| 9.90 | -23.00 | 5.78 | -23.00 | -20.96 | 52.18 | -15.99 | 150.94 | 0.5317 | -1180.9 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -21.93 | 51.94 | -16.24 | 151.50 | 0.5458 | -826.0 | -716.6 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -22.32 | 51.86 | -16.32 | 151.74 | 0.5512 | -755.0 | -631.9 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -22.71 | 51.64 | -16.54 | 151.78 | 0.5576 | -638.0 | -444.4 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -20.47 | 51.46 | -16.72 | 149.36 | 0.5309 | -727.0 | -562.1 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -22.04 | 50.97 | -17.21 | 150.20 | 0.5540 | -747.0 | -509.4 | |
| 0.00 | 1.26 | 0.00 | 0.79 | -26.11 | 50.00 | -18.18 | 152.55 | 0.6100 | -642.0 | -397.5 | |
| 0.00 | 1.53 | 0.00 | 0.91 | -21.72 | 50.18 | -17.99 | 148.78 | 0.5559 | -889.0 | -605.5 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -23.78 | 49.30 | -18.87 | 149.59 | 0.5870 | -506.0 | -471.1 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -24.49 | 48.49 | -19.69 | 149.20 | 0.6011 | -660.0 | -449.1 | |
| 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. | |