SDO HMI 2014-07-06 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.07 | 104.37 | 13.88 | 57.73 | 10.97 | 279.29 | 25.30 | 288.29 | 0.4443 | -507.7 | -327.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.59 | 16.21 | 284.15 | 30.15 | 295.44 | 0.5362 | -633.0 | -460.8 | |
| 0.00 | 1.73 | 0.00 | 0.98 | 11.90 | 282.70 | 28.71 | 288.24 | 0.4968 | -614.0 | -497.0 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 11.72 | 282.47 | 28.47 | 288.01 | 0.4928 | -647.0 | -522.9 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 11.35 | 282.32 | 28.32 | 287.35 | 0.4893 | -618.0 | -568.7 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 11.60 | 282.35 | 28.35 | 287.83 | 0.4906 | -678.0 | -615.2 | |
| 0.00 | 1.09 | 0.00 | 0.62 | 11.51 | 282.16 | 28.17 | 287.75 | 0.4876 | -777.0 | -657.6 | |
| 0.00 | 2.00 | 0.00 | 1.14 | 12.28 | 282.22 | 28.22 | 289.25 | 0.4913 | -650.0 | -579.2 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 9.89 | 281.72 | 27.72 | 284.65 | 0.4755 | -670.0 | -548.1 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 10.54 | 281.67 | 27.68 | 286.01 | 0.4770 | -851.0 | -729.2 | |
| 0.00 | 5.00 | 0.00 | 2.81 | 10.05 | 281.56 | 27.56 | 285.05 | 0.4736 | -634.0 | -666.0 | |
| 0.00 | 0.73 | 0.00 | 0.41 | 7.27 | 281.30 | 27.30 | 279.25 | 0.4628 | -491.0 | -445.6 | |
| 0.00 | 2.00 | 0.00 | 1.11 | 7.40 | 281.06 | 27.07 | 279.59 | 0.4595 | -692.0 | -682.0 | |
| 0.00 | 2.63 | 0.00 | 1.46 | 8.26 | 280.75 | 26.75 | 281.56 | 0.4565 | -631.0 | -507.0 | |
| 0.00 | 2.00 | 0.00 | 1.13 | 14.64 | 281.17 | 27.17 | 294.49 | 0.4875 | -644.0 | -520.5 | |
| 0.00 | 1.82 | 0.00 | 1.01 | 8.33 | 280.41 | 26.41 | 281.83 | 0.4515 | -737.0 | -569.8 | |
| 0.00 | 0.73 | 0.00 | 0.40 | 7.24 | 280.23 | 26.23 | 279.46 | 0.4463 | -657.0 | -554.0 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 8.28 | 280.23 | 26.23 | 281.77 | 0.4486 | -180.0 | -187.9 | |
| 20.53 | 44.77 | 11.38 | 24.84 | 10.87 | 279.79 | 25.80 | 287.63 | 0.4503 | -1011.6 | -431.2 | |
| 0.82 | -18.00 | 0.45 | -18.00 | 10.56 | 279.73 | 25.73 | 287.00 | 0.4482 | -826.6 | 999999 | |
| 1.36 | 4.09 | 0.75 | 2.26 | 11.43 | 279.61 | 25.61 | 288.94 | 0.4497 | -820.7 | -648.3 | |
| 1.00 | 2.18 | 0.55 | 1.20 | 11.22 | 279.10 | 25.11 | 288.80 | 0.4415 | -986.3 | -851.4 | |
| 0.00 | 2.36 | 0.00 | 1.28 | 4.30 | 278.25 | 24.25 | 272.92 | 0.4119 | -686.0 | -602.8 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 11.12 | 278.24 | 24.24 | 289.11 | 0.4281 | -645.0 | -519.2 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 11.37 | 278.19 | 24.20 | 289.69 | 0.4285 | -918.0 | -781.2 | |
| 1.36 | 3.81 | 0.75 | 2.09 | 11.78 | 277.96 | 23.96 | 290.76 | 0.4269 | -965.1 | -775.4 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 12.15 | 277.82 | 23.83 | 291.70 | 0.4268 | -795.0 | -696.2 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 12.16 | 277.45 | 23.45 | 291.99 | 0.4213 | -703.0 | -588.9 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 12.42 | 276.96 | 22.97 | 292.95 | 0.4156 | -640.0 | -510.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 12.32 | 275.87 | 21.88 | 293.63 | 0.3990 | 816.0 | 643.8 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 12.23 | 274.53 | 20.53 | 294.63 | 0.3787 | 809.0 | 611.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 11.43 | 274.36 | 20.37 | 292.79 | 0.3716 | 722.0 | 559.8 | |
| 0.00 | 3.36 | 0.00 | 1.79 | 11.40 | 274.10 | 20.10 | 292.97 | 0.3675 | 861.0 | 726.8 | |
| 0.00 | 1.91 | 0.00 | 1.03 | 14.46 | 274.33 | 20.33 | 300.16 | 0.3907 | 1002.0 | 818.8 | |
| 0.00 | 3.18 | 0.00 | 1.71 | 13.75 | 274.26 | 20.26 | 298.58 | 0.3847 | 774.0 | 593.5 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 8.57 | 273.19 | 19.19 | 286.02 | 0.3397 | 630.0 | 508.4 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 15.54 | 273.43 | 19.43 | 303.68 | 0.3868 | 875.0 | 693.4 | |
| 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. | |