SDO HMI 2011-08-21 02:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.91 | 184.79 | 30.93 | 108.09 | -21.16 | 54.65 | -15.72 | 151.70 | 0.5329 | 85.0 | 36.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.61 | 0.00 | 1.46 | -19.04 | 60.67 | -9.70 | 159.93 | 0.4659 | 926.0 | 712.3 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -18.92 | 59.86 | -10.51 | 158.31 | 0.4686 | 722.0 | 583.0 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -18.83 | 58.20 | -12.17 | 155.19 | 0.4774 | 717.0 | 614.3 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -19.31 | 58.13 | -12.24 | 155.50 | 0.4844 | 805.0 | 552.1 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -17.53 | 58.13 | -12.24 | 153.81 | 0.4598 | 694.0 | 486.3 | |
| 0.00 | 1.89 | 0.00 | 1.05 | -17.20 | 57.89 | -12.48 | 153.03 | 0.4570 | 677.0 | 526.5 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.34 | 57.62 | -12.75 | 152.68 | 0.4608 | 627.0 | 521.2 | |
| 4.68 | 73.67 | 2.71 | 42.73 | -21.52 | 57.25 | -13.12 | 155.94 | 0.5200 | 832.7 | 431.3 | |
| 0.00 | 2.79 | 0.00 | 1.56 | -17.62 | 57.08 | -13.29 | 152.00 | 0.4685 | 941.0 | 751.9 | |
| 16.19 | -8.00 | 9.39 | -8.00 | -21.40 | 56.62 | -13.75 | 154.83 | 0.5223 | 1161.6 | 999999 | |
| 1.71 | 2.07 | 1.00 | 1.21 | -21.76 | 55.95 | -14.42 | 154.09 | 0.5314 | 744.7 | 771.0 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -17.58 | 56.26 | -14.11 | 150.52 | 0.4740 | 737.0 | 597.5 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -21.77 | 55.71 | -14.66 | 153.73 | 0.5330 | 698.0 | 576.3 | |
| 4.05 | 16.10 | 2.35 | 9.38 | -20.48 | 54.36 | -16.01 | 150.44 | 0.5257 | 904.7 | 320.6 | |
| 3.42 | 5.85 | 2.00 | 3.42 | -20.96 | 54.24 | -16.13 | 150.74 | 0.5327 | 793.9 | 619.0 | |
| 3.51 | -14.00 | 2.05 | -14.00 | -20.62 | 54.11 | -16.26 | 150.20 | 0.5294 | 628.7 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.16 | -21.15 | 53.75 | -16.62 | 150.18 | 0.5387 | 621.0 | 435.7 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -21.47 | 53.37 | -17.00 | 149.95 | 0.5455 | -546.0 | -323.9 | |
| 0.00 | 2.61 | 0.00 | 1.53 | -20.96 | 53.26 | -17.11 | 149.28 | 0.5399 | -806.0 | -574.9 | |
| 0.00 | 1.62 | 0.00 | 0.94 | -19.87 | 53.25 | -17.12 | 148.14 | 0.5265 | -859.0 | -785.5 | |
| 5.40 | 47.86 | 3.19 | 28.30 | -21.42 | 52.96 | -17.40 | 149.32 | 0.5478 | -704.5 | -639.1 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -19.88 | 53.01 | -17.36 | 147.79 | 0.5285 | -766.0 | -634.3 | |
| 7.56 | -21.00 | 4.46 | -21.00 | -21.16 | 52.69 | -17.68 | 148.66 | 0.5466 | -983.2 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -20.44 | 52.64 | -17.73 | 147.85 | 0.5382 | -839.0 | -638.2 | |
| 6.39 | -21.00 | 3.78 | -21.00 | -20.97 | 52.10 | -18.27 | 147.63 | 0.5489 | -1035.9 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.80 | -21.27 | 51.51 | -18.86 | 147.13 | 0.5571 | -703.0 | -534.5 | |
| 0.00 | 1.62 | 0.00 | 0.97 | -22.02 | 50.92 | -19.45 | 147.11 | 0.5705 | -746.0 | -539.8 | |
| 0.00 | 2.07 | 0.00 | 1.25 | -21.67 | 50.21 | -20.16 | 145.81 | 0.5721 | -894.0 | -691.0 | |
| 0.00 | 1.17 | 0.00 | 0.72 | -23.83 | 49.44 | -20.93 | 147.04 | 0.6026 | -783.0 | -653.4 | |
| 0.00 | 2.16 | 0.00 | 1.32 | -22.71 | 49.38 | -20.99 | 145.84 | 0.5905 | -629.0 | -431.2 | |
| 0.00 | 0.90 | 0.00 | 0.57 | -24.96 | 48.92 | -21.45 | 147.49 | 0.6191 | -675.0 | -554.1 | |
| 0.00 | 0.90 | 0.00 | 0.57 | -24.81 | 48.88 | -21.49 | 147.31 | 0.6179 | -747.0 | -575.0 | |
| 0.00 | 1.17 | 0.00 | 0.72 | -23.26 | 48.86 | -21.50 | 145.76 | 0.6007 | -661.0 | -488.2 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -24.55 | 48.53 | -21.84 | 146.64 | 0.6175 | -763.0 | -613.8 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -23.91 | 48.46 | -21.90 | 145.93 | 0.6110 | -641.0 | -490.4 | |
| 0.00 | 1.35 | 0.00 | 0.85 | -24.68 | 48.04 | -22.33 | 146.19 | 0.6226 | -547.0 | -418.5 | |
| 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. | |