SDO HMI 2014-05-15 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 130.41 | 423.57 | 87.34 | 281.22 | 10.14 | 179.53 | -39.88 | 71.53 | 0.6673 | 39.4 | -131.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.80 | 10.01 | 182.06 | -37.35 | 70.65 | 0.6355 | -315.0 | -290.4 | |
| 6.11 | 8.89 | 3.94 | 5.73 | 10.67 | 181.77 | -37.64 | 69.79 | 0.6418 | -820.2 | -558.2 | |
| 0.00 | 1.98 | 0.00 | 1.28 | 10.46 | 181.61 | -37.80 | 70.18 | 0.6430 | -857.0 | -652.9 | |
| 3.05 | 209.08 | 1.97 | 134.90 | 10.18 | 181.57 | -37.84 | 70.61 | 0.6424 | -840.0 | -401.5 | |
| 35.21 | -4.00 | 22.70 | -4.00 | 9.35 | 181.33 | -38.08 | 71.96 | 0.6424 | -1131.9 | 999999 | |
| 4.67 | -4.00 | 3.04 | -4.00 | 9.31 | 180.67 | -38.75 | 72.30 | 0.6506 | -716.3 | 999999 | |
| 2.42 | -4.00 | 1.58 | -4.00 | 9.62 | 180.62 | -38.79 | 71.85 | 0.6523 | -399.6 | 999999 | |
| 0.45 | 13.92 | 0.29 | 9.16 | 10.52 | 180.49 | -38.92 | 70.57 | 0.6572 | -650.8 | -397.8 | |
| 2.34 | -8.00 | 1.54 | -8.00 | 10.68 | 180.35 | -39.06 | 70.40 | 0.6596 | -653.1 | 999999 | |
| 2.42 | -8.00 | 1.60 | -8.00 | 10.47 | 180.22 | -39.19 | 70.77 | 0.6604 | -803.7 | 999999 | |
| 1.71 | -4.00 | 1.12 | -4.00 | 9.13 | 180.33 | -39.08 | 72.69 | 0.6542 | -389.7 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.25 | 10.73 | 179.82 | -39.59 | 70.56 | 0.6663 | 312.0 | 218.8 | |
| 0.00 | 1.08 | 0.00 | 0.71 | 8.74 | 180.10 | -39.31 | 73.36 | 0.6558 | -425.0 | -347.2 | |
| 0.45 | 3.23 | 0.30 | 2.14 | 10.42 | 179.79 | -39.62 | 71.02 | 0.6655 | -552.8 | -388.0 | |
| 0.00 | 1.53 | 0.00 | 1.01 | 9.58 | 179.87 | -39.54 | 72.21 | 0.6615 | 386.0 | 388.9 | |
| 0.00 | 2.07 | 0.00 | 1.37 | 10.09 | 179.36 | -40.05 | 71.67 | 0.6697 | -255.0 | -244.3 | |
| 0.00 | 0.72 | 0.00 | 0.48 | 11.63 | 179.03 | -40.38 | 69.61 | 0.6793 | 646.0 | 522.9 | |
| 1.62 | 3.14 | 1.09 | 2.13 | 11.85 | 178.83 | -40.59 | 69.38 | 0.6826 | 851.4 | 733.2 | |
| 0.45 | 1.53 | 0.30 | 1.03 | 9.96 | 178.65 | -40.76 | 72.14 | 0.6780 | -548.4 | -472.5 | |
| 0.00 | 1.44 | 0.00 | 0.97 | 10.18 | 178.61 | -40.80 | 71.84 | 0.6791 | -267.0 | -238.2 | |
| 1.80 | 68.71 | 1.22 | 47.22 | 11.71 | 178.32 | -41.10 | 69.79 | 0.6882 | 885.8 | 216.0 | |
| 0.00 | 0.72 | 0.00 | 0.48 | 8.97 | 178.67 | -40.75 | 73.55 | 0.6745 | 796.0 | 709.8 | |
| 8.44 | 14.46 | 5.68 | 9.72 | 9.59 | 178.50 | -40.91 | 72.72 | 0.6786 | 384.4 | 242.1 | |
| 1.71 | -21.00 | 1.17 | -21.00 | 11.72 | 178.07 | -41.35 | 69.88 | 0.6912 | 844.1 | 999999 | |
| 1.35 | 2.51 | 0.91 | 1.69 | 9.13 | 178.40 | -41.01 | 73.41 | 0.6783 | 788.0 | 651.8 | |
| 0.00 | 0.90 | 0.00 | 0.60 | 8.95 | 178.34 | -41.07 | 73.70 | 0.6785 | 706.0 | 628.6 | |
| 4.49 | -21.00 | 3.08 | -21.00 | 11.67 | 177.83 | -41.58 | 70.05 | 0.6938 | 1001.3 | 999999 | |
| 1.35 | 4.76 | 0.91 | 3.22 | 9.17 | 178.07 | -41.35 | 73.47 | 0.6826 | 666.4 | 516.9 | |
| 9.25 | -21.00 | 6.36 | -21.00 | 11.48 | 177.65 | -41.76 | 70.38 | 0.6952 | 976.4 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.98 | 10.58 | 177.64 | -41.77 | 71.64 | 0.6922 | 703.0 | 594.2 | |
| 0.00 | 2.42 | 0.00 | 1.66 | 10.40 | 177.51 | -41.90 | 71.94 | 0.6933 | 712.0 | 636.1 | |
| 0.00 | 1.08 | 0.00 | 0.74 | 10.77 | 177.40 | -42.01 | 71.46 | 0.6958 | 574.0 | 494.5 | |
| 3.50 | 74.81 | 2.41 | 51.95 | 10.50 | 177.28 | -42.13 | 71.88 | 0.6963 | 962.5 | 338.5 | |
| 7.36 | -33.00 | 5.06 | -33.00 | 10.13 | 177.22 | -42.19 | 72.42 | 0.6959 | 895.5 | 999999 | |
| 27.12 | -33.00 | 18.88 | -33.00 | 10.92 | 176.66 | -42.75 | 71.52 | 0.7050 | 832.5 | 999999 | |
| 3.14 | -33.00 | 2.19 | -33.00 | 10.37 | 176.47 | -42.95 | 72.36 | 0.7056 | 629.9 | 999999 | |
| 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. | |