SDO HMI 2011-06-15 17:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98.69 | 543.39 | 109.52 | 601.67 | 16.50 | 166.15 | -62.35 | 71.93 | 0.8931 | -125.0 | 4.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.46 | 278.85 | 26.57 | 271.43 | 17.16 | 170.55 | -57.96 | 70.56 | 0.8609 | -946.4 | -184.5 | |
| 0.82 | -1.00 | 0.79 | -1.00 | 16.87 | 170.26 | -58.24 | 70.95 | 0.8629 | 163.0 | 999999 | |
| 21.84 | -1.00 | 21.27 | -1.00 | 16.52 | 170.19 | -58.32 | 71.36 | 0.8630 | -712.6 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.95 | 16.40 | 168.44 | -60.07 | 71.78 | 0.8772 | -188.0 | -143.8 | |
| 0.00 | 1.99 | 0.00 | 2.00 | 14.83 | 168.89 | -59.62 | 73.51 | 0.8717 | -600.0 | -449.4 | |
| 0.00 | 1.27 | 0.00 | 1.37 | 16.92 | 166.71 | -61.80 | 71.47 | 0.8912 | 636.0 | 546.6 | |
| 0.00 | 0.36 | 0.00 | 0.39 | 16.69 | 166.77 | -61.74 | 71.71 | 0.8905 | 542.0 | 553.0 | |
| 0.00 | 1.00 | 0.00 | 1.11 | 16.11 | 165.79 | -62.72 | 72.49 | 0.8972 | -236.0 | -183.1 | |
| 0.00 | 0.91 | 0.00 | 1.05 | 16.85 | 164.78 | -63.73 | 71.80 | 0.9052 | 456.0 | 395.9 | |
| 0.00 | 3.17 | 0.00 | 3.55 | 15.31 | 165.46 | -63.05 | 73.41 | 0.8989 | -473.0 | -454.3 | |
| 0.00 | 4.08 | 0.00 | 5.00 | 18.56 | 163.41 | -65.10 | 70.12 | 0.9161 | 368.0 | 307.8 | |
| 0.00 | 1.72 | 0.00 | 1.92 | 14.34 | 165.55 | -62.96 | 74.49 | 0.8974 | -571.0 | -497.6 | |
| 1.63 | 2.63 | 1.87 | 3.01 | 15.18 | 164.75 | -63.76 | 73.65 | 0.9039 | -357.5 | -290.7 | |
| 0.00 | 1.00 | 0.00 | 1.13 | 14.55 | 165.09 | -63.42 | 74.30 | 0.9010 | -483.0 | -391.1 | |
| 5.35 | 66.25 | 6.81 | 84.48 | 18.22 | 162.32 | -66.19 | 70.62 | 0.9228 | 586.9 | 386.7 | |
| 0.00 | 17.49 | 0.00 | 21.46 | 16.70 | 163.08 | -65.43 | 72.18 | 0.9167 | 641.0 | 532.0 | |
| 0.00 | 1.90 | 0.00 | 2.49 | 18.63 | 161.68 | -66.83 | 70.26 | 0.9272 | -176.0 | -118.4 | |
| 8.97 | 54.10 | 10.54 | 64.22 | 14.79 | 164.09 | -64.41 | 74.15 | 0.9083 | -544.6 | -61.2 | |
| 4.53 | -15.00 | 5.80 | -15.00 | 17.42 | 162.11 | -66.40 | 71.51 | 0.9236 | 738.5 | 999999 | |
| 0.00 | 1.72 | 0.00 | 2.24 | 17.89 | 161.76 | -66.75 | 71.04 | 0.9261 | 361.0 | 324.8 | |
| 0.00 | 0.63 | 0.00 | 0.79 | 16.63 | 162.66 | -65.85 | 72.30 | 0.9194 | 566.0 | 535.6 | |
| 1.00 | -18.00 | 1.19 | -18.00 | 14.94 | 163.56 | -64.95 | 74.05 | 0.9121 | 389.6 | 999999 | |
| 0.00 | 1.00 | 0.00 | 1.27 | 16.85 | 162.27 | -66.24 | 72.11 | 0.9221 | 640.0 | 584.4 | |
| 2.54 | -15.00 | 3.31 | -15.00 | 17.60 | 161.65 | -66.86 | 71.37 | 0.9266 | 269.4 | 999999 | |
| 0.63 | 5.08 | 0.78 | 6.22 | 15.94 | 162.80 | -65.71 | 73.04 | 0.9179 | 615.0 | 534.7 | |
| 0.00 | 5.98 | 0.00 | 7.95 | 18.08 | 161.20 | -67.31 | 70.91 | 0.9297 | -357.0 | -231.5 | |
| 1.00 | 2.63 | 1.22 | 3.21 | 15.49 | 162.92 | -65.58 | 73.51 | 0.9168 | 590.5 | 552.8 | |
| 3.53 | -15.00 | 4.59 | -15.00 | 17.19 | 161.71 | -66.80 | 71.80 | 0.9259 | 423.5 | 999999 | |
| 0.00 | 5.08 | 0.00 | 6.53 | 16.68 | 161.91 | -66.60 | 72.33 | 0.9243 | 553.0 | 402.2 | |
| 0.00 | 1.54 | 0.00 | 1.92 | 15.62 | 162.62 | -65.89 | 73.41 | 0.9190 | 530.0 | 479.5 | |
| 9.24 | 12.78 | 11.77 | 16.28 | 16.02 | 162.12 | -66.39 | 73.02 | 0.9225 | 550.7 | 284.8 | |
| 0.00 | 1.63 | 0.00 | 2.01 | 14.86 | 162.84 | -65.66 | 74.20 | 0.9169 | 516.0 | 436.0 | |
| 0.00 | 0.82 | 0.00 | 1.01 | 14.64 | 162.74 | -65.77 | 74.45 | 0.9175 | 403.0 | 362.8 | |
| 10.15 | 62.62 | 13.01 | 81.43 | 15.51 | 161.81 | -66.70 | 73.60 | 0.9241 | 564.7 | 12.1 | |
| 0.00 | 3.26 | 0.00 | 4.25 | 14.62 | 161.32 | -67.19 | 74.61 | 0.9267 | 525.0 | 381.6 | |
| 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. | |