SDO HMI 2011-09-02 19:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.78 | 315.62 | 49.56 | 206.19 | 24.03 | 300.78 | 38.31 | 299.42 | 0.6500 | 32.8 | -64.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.32 | 184.59 | 23.22 | 125.10 | 23.10 | 304.01 | 41.54 | 296.40 | 0.6833 | -1063.4 | -246.6 | |
| 2.77 | 11.17 | 1.86 | 7.47 | 23.69 | 303.09 | 40.62 | 297.57 | 0.6749 | -816.0 | -676.4 | |
| 0.00 | 1.07 | 0.00 | 0.71 | 23.70 | 302.53 | 40.06 | 297.80 | 0.6686 | -747.0 | -552.5 | |
| 1.34 | 1.70 | 0.89 | 1.13 | 23.98 | 302.59 | 40.12 | 298.18 | 0.6703 | -781.5 | -653.0 | |
| 0.00 | 2.06 | 0.00 | 1.34 | 24.71 | 300.59 | 38.12 | 300.09 | 0.6504 | -803.0 | -608.6 | |
| 0.00 | 1.61 | 0.00 | 1.04 | 24.86 | 300.35 | 37.88 | 300.42 | 0.6483 | -898.0 | -671.3 | |
| 0.00 | 2.06 | 0.00 | 1.33 | 26.20 | 299.65 | 37.18 | 302.71 | 0.6468 | -556.0 | -454.5 | |
| 1.43 | 5.90 | 0.92 | 3.80 | 25.88 | 299.12 | 36.65 | 302.52 | 0.6391 | -666.7 | -664.1 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 25.27 | 297.66 | 35.19 | 302.40 | 0.6195 | 567.0 | 407.4 | |
| 1.43 | 1.97 | 0.90 | 1.23 | 25.00 | 297.41 | 34.94 | 302.13 | 0.6151 | 668.4 | 614.5 | |
| 0.00 | 3.22 | 0.00 | 2.00 | 25.11 | 296.71 | 34.24 | 302.70 | 0.6077 | 458.0 | 433.3 | |
| 0.00 | 1.25 | 0.00 | 0.78 | 25.20 | 296.37 | 33.90 | 303.03 | 0.6042 | 514.0 | 523.5 | |
| 0.00 | 0.89 | 0.00 | 0.55 | 25.43 | 296.25 | 33.78 | 303.46 | 0.6040 | 470.0 | 378.6 | |
| 0.72 | 9.30 | 0.44 | 5.75 | 25.42 | 295.96 | 33.49 | 303.61 | 0.6007 | 964.0 | 614.8 | |
| 0.00 | 0.89 | 0.00 | 0.55 | 25.44 | 295.69 | 33.22 | 303.81 | 0.5976 | 663.0 | 587.2 | |
| 3.22 | 17.07 | 2.00 | 10.60 | 26.71 | 295.90 | 33.43 | 305.61 | 0.6075 | 517.0 | 269.7 | |
| 0.00 | 1.61 | 0.00 | 0.99 | 25.45 | 295.49 | 33.02 | 303.95 | 0.5954 | 668.0 | 614.4 | |
| 0.00 | 3.40 | 0.00 | 2.10 | 25.99 | 295.54 | 33.07 | 304.75 | 0.5991 | 478.0 | 415.8 | |
| 0.00 | 1.34 | 0.00 | 0.82 | 25.18 | 295.21 | 32.74 | 303.71 | 0.5905 | 798.0 | 600.9 | |
| 8.76 | -16.00 | 5.43 | -16.00 | 26.67 | 295.56 | 33.09 | 305.76 | 0.6034 | 795.8 | 999999 | |
| 2.23 | 5.63 | 1.37 | 3.45 | 25.42 | 295.00 | 32.53 | 304.21 | 0.5895 | 855.2 | 767.1 | |
| 2.15 | 7.78 | 1.32 | 4.78 | 25.86 | 295.14 | 32.67 | 304.80 | 0.5937 | 847.5 | 672.6 | |
| 1.34 | 4.20 | 0.83 | 2.60 | 26.87 | 295.06 | 32.59 | 306.38 | 0.5990 | 590.5 | 127.7 | |
| 0.00 | 1.52 | 0.00 | 0.93 | 26.49 | 294.78 | 32.31 | 306.01 | 0.5935 | 754.0 | 623.6 | |
| 3.84 | 6.26 | 2.34 | 3.81 | 25.67 | 294.48 | 32.01 | 304.95 | 0.5851 | 871.8 | 720.4 | |
| 6.17 | 11.53 | 3.73 | 6.98 | 25.32 | 293.94 | 31.47 | 304.76 | 0.5767 | 1058.3 | 596.2 | |
| 2.50 | 6.08 | 1.53 | 3.72 | 26.78 | 294.39 | 31.92 | 306.70 | 0.5909 | 816.9 | 650.9 | |
| 4.56 | 5.99 | 2.78 | 3.65 | 26.15 | 294.15 | 31.68 | 305.90 | 0.5842 | 908.0 | 741.5 | |
| 0.00 | 1.34 | 0.00 | 0.82 | 27.00 | 294.42 | 31.95 | 307.02 | 0.5927 | 518.0 | 473.9 | |
| 0.00 | 1.16 | 0.00 | 0.71 | 26.53 | 294.27 | 31.80 | 306.40 | 0.5879 | 913.0 | 717.0 | |
| 0.00 | 1.07 | 0.00 | 0.66 | 26.69 | 294.20 | 31.73 | 306.70 | 0.5882 | 941.0 | 883.4 | |
| 0.00 | 1.34 | 0.00 | 0.80 | 25.16 | 293.00 | 30.53 | 305.16 | 0.5645 | 782.0 | 613.1 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 25.79 | 293.10 | 30.63 | 306.09 | 0.5698 | 725.0 | 623.7 | |
| 0.00 | 0.89 | 0.00 | 0.53 | 25.08 | 292.71 | 30.24 | 305.24 | 0.5606 | 687.0 | 544.0 | |
| 0.00 | 0.80 | 0.00 | 0.46 | 22.00 | 289.34 | 26.87 | 302.58 | 0.4993 | 768.0 | 645.3 | |
| 0.00 | 1.52 | 0.00 | 0.84 | 21.12 | 285.09 | 22.62 | 304.79 | 0.4388 | 867.0 | 634.9 | |
| 0.00 | 2.23 | 0.00 | 1.21 | 22.60 | 281.97 | 19.50 | 311.43 | 0.4128 | 695.0 | 485.4 | |
| 0.00 | 3.22 | 0.00 | 1.74 | 22.72 | 281.43 | 18.96 | 312.39 | 0.4075 | 781.0 | 699.2 | |
| 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. | |