SDO HMI 2011-07-22 00:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.96 | 221.84 | 33.24 | 134.30 | 24.40 | 77.78 | -30.38 | 53.19 | 0.5768 | -195.0 | -150.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 0.52 | 22.54 | 82.20 | -25.96 | 52.50 | 0.5117 | -778.0 | -594.2 | |
| 14.51 | 97.95 | 8.59 | 57.99 | 24.00 | 80.02 | -28.15 | 52.07 | 0.5485 | -1118.7 | -502.4 | |
| 6.71 | -2.00 | 3.99 | -2.00 | 23.95 | 79.42 | -28.74 | 52.66 | 0.5549 | -762.6 | 999999 | |
| 3.72 | -2.00 | 2.22 | -2.00 | 24.09 | 78.97 | -29.20 | 52.80 | 0.5612 | -792.9 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.72 | 25.39 | 78.05 | -30.12 | 51.56 | 0.5809 | -924.0 | -740.2 | |
| 1.72 | 31.47 | 1.04 | 19.07 | 24.77 | 78.10 | -30.07 | 52.45 | 0.5759 | -536.3 | -533.9 | |
| 11.61 | -6.00 | 7.02 | -6.00 | 24.41 | 77.96 | -30.20 | 53.11 | 0.5749 | -906.5 | 999999 | |
| 0.00 | 0.73 | 0.00 | 0.44 | 25.34 | 77.63 | -30.53 | 51.96 | 0.5852 | -521.0 | -495.5 | |
| 0.00 | 1.72 | 0.00 | 1.05 | 25.01 | 77.60 | -30.56 | 52.47 | 0.5832 | -836.0 | -637.2 | |
| 0.45 | 9.80 | 0.28 | 6.01 | 25.68 | 77.26 | -30.91 | 51.73 | 0.5918 | -813.2 | -518.7 | |
| 0.00 | 1.18 | 0.00 | 0.72 | 24.71 | 77.49 | -30.67 | 53.00 | 0.5824 | -573.0 | -476.1 | |
| 0.00 | 1.27 | 0.00 | 0.78 | 25.26 | 77.26 | -30.90 | 52.36 | 0.5888 | -513.0 | -486.4 | |
| 2.36 | -6.00 | 1.44 | -6.00 | 24.73 | 77.25 | -30.91 | 53.15 | 0.5853 | -583.3 | 999999 | |
| 1.18 | -6.00 | 0.72 | -6.00 | 24.48 | 77.32 | -30.84 | 53.49 | 0.5827 | -550.4 | 999999 | |
| 0.00 | 10.61 | 0.00 | 6.50 | 24.52 | 76.72 | -31.44 | 53.87 | 0.5898 | -1.0 | -140.1 | |
| 0.00 | 2.45 | 0.00 | 1.50 | 24.26 | 76.71 | -31.45 | 54.26 | 0.5882 | -510.0 | -391.4 | |
| 0.00 | 2.81 | 0.00 | 1.76 | 26.81 | 75.91 | -32.25 | 51.10 | 0.6142 | 852.0 | 659.8 | |
| 0.00 | 1.09 | 0.00 | 0.67 | 24.72 | 76.23 | -31.93 | 53.91 | 0.5968 | -399.0 | -267.2 | |
| 0.00 | 7.44 | 0.00 | 4.58 | 24.49 | 76.10 | -32.07 | 54.35 | 0.5967 | 365.0 | 377.0 | |
| 0.00 | 1.00 | 0.00 | 0.61 | 22.30 | 76.30 | -31.86 | 57.57 | 0.5808 | 746.0 | 619.2 | |
| 0.00 | 2.81 | 0.00 | 1.75 | 24.85 | 75.43 | -32.73 | 54.27 | 0.6066 | 867.0 | 671.8 | |
| 0.00 | 0.36 | 0.00 | 0.23 | 26.79 | 74.82 | -33.34 | 51.89 | 0.6258 | 727.0 | 675.2 | |
| 5.17 | 17.05 | 3.20 | 10.54 | 24.24 | 75.58 | -32.59 | 55.08 | 0.6011 | 1013.2 | 755.9 | |
| 0.00 | 1.18 | 0.00 | 0.73 | 23.88 | 75.60 | -32.57 | 55.60 | 0.5987 | 808.0 | 736.0 | |
| 1.09 | 4.44 | 0.69 | 2.82 | 26.43 | 74.74 | -33.42 | 52.46 | 0.6243 | 840.9 | 706.2 | |
| 0.00 | 2.27 | 0.00 | 1.41 | 24.49 | 75.34 | -32.82 | 54.87 | 0.6053 | 524.0 | 485.1 | |
| 1.63 | 2.27 | 1.02 | 1.41 | 24.54 | 75.13 | -33.04 | 54.93 | 0.6081 | 871.8 | 727.4 | |
| 0.00 | 2.63 | 0.00 | 1.64 | 24.41 | 75.01 | -33.16 | 55.21 | 0.6086 | 865.0 | 634.2 | |
| 4.81 | 5.71 | 3.03 | 3.60 | 24.90 | 74.33 | -33.83 | 54.93 | 0.6192 | 878.2 | 533.0 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 25.35 | 74.15 | -34.01 | 54.39 | 0.6240 | 677.0 | 489.4 | |
| 0.00 | 3.17 | 0.00 | 1.98 | 23.64 | 74.59 | -33.57 | 56.62 | 0.6088 | 762.0 | 663.5 | |
| 0.00 | 2.63 | 0.00 | 1.66 | 24.95 | 74.03 | -34.13 | 55.04 | 0.6229 | 615.0 | 548.4 | |
| 0.00 | 1.81 | 0.00 | 1.13 | 23.63 | 74.36 | -33.81 | 56.78 | 0.6115 | 455.0 | 424.5 | |
| 0.00 | 1.00 | 0.00 | 0.64 | 26.11 | 73.53 | -34.63 | 53.71 | 0.6354 | 459.0 | 422.0 | |
| 0.00 | 1.00 | 0.00 | 0.63 | 25.19 | 73.63 | -34.53 | 54.95 | 0.6288 | 659.0 | 499.2 | |
| 0.00 | 0.63 | 0.00 | 0.41 | 25.25 | 73.33 | -34.84 | 55.06 | 0.6325 | 554.0 | 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. | |