SDO HMI 2014-05-16 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 99.12 | 329.41 | 55.97 | 186.21 | 10.33 | 178.75 | -25.80 | 62.91 | 0.4823 | -26.9 | -45.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.51 | 17.11 | 182.20 | -22.34 | 47.51 | 0.4948 | 509.0 | 388.9 | |
| 2.96 | 4.40 | 1.63 | 2.42 | 10.45 | 182.06 | -22.49 | 59.54 | 0.4382 | -1033.0 | -795.4 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 10.68 | 181.27 | -23.28 | 59.92 | 0.4506 | -754.0 | -585.3 | |
| 3.68 | 139.08 | 2.03 | 76.95 | 9.26 | 181.31 | -23.24 | 62.74 | 0.4398 | -1130.5 | -528.2 | |
| 11.41 | -4.00 | 6.32 | -4.00 | 10.07 | 181.08 | -23.46 | 61.33 | 0.4486 | -1154.1 | 999999 | |
| 2.79 | 6.11 | 1.55 | 3.40 | 10.78 | 180.92 | -23.62 | 60.08 | 0.4560 | -814.9 | -687.0 | |
| 9.43 | -4.00 | 5.21 | -4.00 | 9.32 | 181.00 | -23.54 | 62.90 | 0.4446 | -1163.4 | 999999 | |
| 2.52 | -4.00 | 1.40 | -4.00 | 10.35 | 180.93 | -23.62 | 60.93 | 0.4528 | -783.9 | 999999 | |
| 7.82 | -4.00 | 4.33 | -4.00 | 9.91 | 180.89 | -23.65 | 61.82 | 0.4502 | -1107.3 | 999999 | |
| 8.00 | -4.00 | 4.43 | -4.00 | 9.48 | 180.69 | -23.86 | 62.88 | 0.4500 | -1000.4 | 999999 | |
| 2.70 | 4.76 | 1.50 | 2.65 | 10.54 | 180.57 | -23.97 | 60.90 | 0.4590 | -645.1 | -311.3 | |
| 0.00 | 1.89 | 0.00 | 1.05 | 10.33 | 180.52 | -24.02 | 61.37 | 0.4581 | -608.0 | -504.8 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 8.75 | 180.51 | -24.04 | 64.55 | 0.4477 | -716.0 | -541.2 | |
| 2.16 | -4.00 | 1.20 | -4.00 | 9.43 | 180.39 | -24.15 | 63.27 | 0.4538 | -568.2 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.10 | 10.11 | 180.30 | -24.24 | 62.00 | 0.4597 | -226.0 | -149.0 | |
| 0.00 | 0.45 | 0.00 | 0.25 | 7.46 | 180.18 | -24.36 | 67.50 | 0.4445 | 512.0 | 476.6 | |
| 0.00 | 1.44 | 0.00 | 0.81 | 10.28 | 179.71 | -24.83 | 62.23 | 0.4689 | -619.0 | -438.8 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 10.50 | 179.63 | -24.92 | 61.89 | 0.4716 | -673.0 | -621.6 | |
| 0.36 | 1.89 | 0.20 | 1.05 | 9.01 | 179.47 | -25.07 | 64.92 | 0.4640 | 475.8 | 265.1 | |
| 0.00 | 1.89 | 0.00 | 1.06 | 8.81 | 178.91 | -25.63 | 65.79 | 0.4706 | 417.0 | 378.4 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 10.03 | 178.40 | -26.14 | 63.87 | 0.4852 | 853.0 | 651.7 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 11.03 | 178.14 | -26.40 | 62.24 | 0.4953 | 884.0 | 821.8 | |
| 0.00 | 1.17 | 0.00 | 0.67 | 11.09 | 177.93 | -26.62 | 62.30 | 0.4986 | 930.0 | 785.7 | |
| 0.00 | 1.44 | 0.00 | 0.82 | 9.85 | 178.01 | -26.54 | 64.53 | 0.4896 | 733.0 | 596.6 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 8.18 | 178.10 | -26.44 | 67.66 | 0.4785 | 645.0 | 454.7 | |
| 2.70 | 45.37 | 1.54 | 26.04 | 11.16 | 177.61 | -26.94 | 62.44 | 0.5033 | 1074.2 | 384.0 | |
| 1.71 | -26.00 | 0.98 | -26.00 | 11.38 | 177.55 | -26.99 | 62.10 | 0.5055 | 987.5 | 999999 | |
| 1.80 | -26.00 | 1.03 | -26.00 | 11.42 | 177.27 | -27.28 | 62.27 | 0.5095 | 892.8 | 999999 | |
| 4.04 | -26.00 | 2.33 | -26.00 | 11.36 | 177.10 | -27.44 | 62.51 | 0.5114 | 925.8 | 999999 | |
| 0.00 | 2.61 | 0.00 | 1.50 | 10.21 | 176.93 | -27.61 | 64.71 | 0.5065 | 624.0 | 552.0 | |
| 3.05 | 99.19 | 1.76 | 57.47 | 10.47 | 176.67 | -27.88 | 64.45 | 0.5117 | 1001.8 | 316.5 | |
| 10.06 | -31.00 | 5.82 | -31.00 | 10.82 | 176.42 | -28.12 | 64.02 | 0.5171 | 1054.3 | 999999 | |
| 2.88 | -31.00 | 1.66 | -31.00 | 10.57 | 176.31 | -28.24 | 64.55 | 0.5171 | 962.8 | 999999 | |
| 1.44 | 8.09 | 0.83 | 4.67 | 10.33 | 176.12 | -28.42 | 65.12 | 0.5182 | 894.4 | 632.5 | |
| 17.61 | -31.00 | 10.22 | -31.00 | 10.76 | 175.97 | -28.57 | 64.46 | 0.5228 | 941.0 | 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. | |