SDO HMI 2011-10-20 23:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93.46 | 441.78 | 112.37 | 553.70 | 9.40 | 53.68 | 66.92 | 277.96 | 0.9165 | -109.1 | -75.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 1.53 | 5.57 | 57.38 | 70.62 | 273.97 | 0.9426 | -71.0 | -30.1 | |
| 2.44 | 248.19 | 3.46 | 344.77 | 7.61 | 56.78 | 70.02 | 276.11 | 0.9384 | 283.9 | -78.4 | |
| 4.88 | -2.00 | 6.88 | -2.00 | 7.41 | 56.70 | 69.95 | 275.88 | 0.9380 | -361.1 | 999999 | |
| 1.31 | -2.00 | 1.85 | -2.00 | 7.94 | 56.82 | 70.06 | 276.46 | 0.9385 | 245.1 | 999999 | |
| 2.87 | -2.00 | 4.02 | -2.00 | 7.90 | 56.53 | 69.78 | 276.41 | 0.9368 | -346.3 | 999999 | |
| 2.26 | -2.00 | 3.16 | -2.00 | 8.54 | 56.52 | 69.76 | 277.09 | 0.9366 | 107.4 | 999999 | |
| 20.90 | -2.00 | 28.54 | -2.00 | 8.47 | 55.97 | 69.21 | 276.98 | 0.9332 | -585.7 | 999999 | |
| 3.22 | -2.00 | 4.26 | -2.00 | 8.80 | 55.25 | 68.49 | 277.31 | 0.9286 | -700.4 | 999999 | |
| 5.40 | -2.00 | 6.99 | -2.00 | 8.87 | 54.78 | 68.03 | 277.37 | 0.9255 | -661.9 | 999999 | |
| 0.00 | 0.78 | 0.00 | 1.04 | 10.94 | 55.45 | 68.70 | 279.62 | 0.9294 | -316.0 | -274.2 | |
| 0.00 | 2.09 | 0.00 | 2.65 | 8.29 | 54.24 | 67.49 | 276.71 | 0.9221 | -590.0 | -525.6 | |
| 3.05 | 6.01 | 3.89 | 7.67 | 9.30 | 54.46 | 67.71 | 277.81 | 0.9233 | -595.2 | -572.3 | |
| 0.00 | 0.70 | 0.00 | 0.87 | 8.67 | 53.99 | 67.23 | 277.11 | 0.9203 | -570.0 | -518.9 | |
| 0.00 | 1.13 | 0.00 | 1.42 | 9.18 | 54.10 | 67.34 | 277.67 | 0.9209 | -545.0 | -488.6 | |
| 6.01 | 35.62 | 7.53 | 44.59 | 9.79 | 54.03 | 67.27 | 278.33 | 0.9203 | -724.2 | -578.0 | |
| 0.00 | 0.78 | 0.00 | 0.98 | 9.50 | 53.91 | 67.15 | 278.01 | 0.9195 | -621.0 | -588.7 | |
| 0.00 | 1.22 | 0.00 | 1.51 | 9.18 | 53.70 | 66.95 | 277.66 | 0.9182 | -565.0 | -523.9 | |
| 0.87 | 2.26 | 1.05 | 2.73 | 9.18 | 53.01 | 66.25 | 277.63 | 0.9134 | -697.0 | -605.2 | |
| 0.00 | 0.96 | 0.00 | 1.13 | 10.12 | 52.32 | 65.56 | 278.64 | 0.9083 | -512.0 | -548.2 | |
| 0.00 | 3.05 | 0.00 | 3.42 | 9.53 | 51.02 | 64.26 | 277.96 | 0.8988 | -159.0 | -207.2 | |
| 0.61 | 3.83 | 0.67 | 4.23 | 9.81 | 50.56 | 63.80 | 278.26 | 0.8953 | -136.4 | 112.0 | |
| 2.53 | 4.62 | 2.76 | 5.04 | 10.60 | 50.22 | 63.47 | 279.13 | 0.8926 | 206.8 | 35.4 | |
| 7.23 | 13.06 | 7.48 | 13.55 | 10.52 | 48.66 | 61.90 | 279.02 | 0.8801 | 400.3 | 92.0 | |
| 2.35 | 5.31 | 2.40 | 5.42 | 10.38 | 48.16 | 61.40 | 278.86 | 0.8760 | 615.0 | 465.8 | |
| 0.00 | 0.78 | 0.00 | 0.84 | 15.10 | 49.73 | 62.98 | 284.20 | 0.8891 | -365.0 | -341.0 | |
| 0.00 | 3.05 | 0.00 | 3.03 | 10.57 | 47.34 | 60.58 | 279.07 | 0.8691 | 406.0 | 331.7 | |
| 0.00 | 1.05 | 0.00 | 1.03 | 10.62 | 47.05 | 60.29 | 279.13 | 0.8666 | 660.0 | 570.3 | |
| 0.00 | 1.83 | 0.00 | 1.80 | 10.78 | 46.91 | 60.16 | 279.32 | 0.8655 | 615.0 | 536.4 | |
| 18.64 | 89.26 | 18.54 | 89.18 | 12.20 | 47.36 | 60.61 | 280.95 | 0.8694 | 651.5 | 171.9 | |
| 5.49 | -29.00 | 5.49 | -29.00 | 12.71 | 47.50 | 60.74 | 281.54 | 0.8706 | 576.6 | 999999 | |
| 1.92 | 3.05 | 1.93 | 3.07 | 13.21 | 47.71 | 60.95 | 282.11 | 0.8724 | 377.0 | 325.1 | |
| 0.00 | 2.18 | 0.00 | 2.23 | 14.33 | 48.21 | 61.46 | 283.38 | 0.8768 | 203.0 | 60.6 | |
| 0.00 | 1.74 | 0.00 | 1.75 | 13.01 | 47.56 | 60.80 | 281.88 | 0.8712 | 474.0 | 422.2 | |
| 0.00 | 3.57 | 0.00 | 3.60 | 13.84 | 47.80 | 61.04 | 282.83 | 0.8733 | 444.0 | 356.1 | |
| 0.00 | 1.65 | 0.00 | 1.68 | 14.14 | 47.93 | 61.17 | 283.17 | 0.8745 | 22.0 | 99.3 | |
| 1.48 | 2.18 | 1.47 | 2.16 | 13.30 | 47.31 | 60.55 | 282.23 | 0.8691 | 538.8 | 502.8 | |
| 0.00 | 0.78 | 0.00 | 0.78 | 13.07 | 47.21 | 60.45 | 281.96 | 0.8682 | 485.0 | 500.6 | |
| 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. | |