SDO HMI 2014-08-10 08:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 50.04 | 0.00 | 27.88 | 10.11 | 173.38 | 26.24 | 281.16 | 0.4441 | 298.5 | 284.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.50 | 8.02 | 183.11 | 35.97 | 274.88 | 0.5859 | -583.0 | -467.4 | |
| 0.00 | 3.79 | 0.00 | 2.25 | 11.96 | 180.40 | 33.26 | 282.09 | 0.5508 | -831.0 | -538.0 | |
| 0.00 | 1.35 | 0.00 | 0.79 | 5.89 | 179.63 | 32.49 | 270.94 | 0.5364 | -714.0 | -598.3 | |
| 0.00 | 1.81 | 0.00 | 1.07 | 12.76 | 180.22 | 33.08 | 283.59 | 0.5498 | -490.0 | -437.2 | |
| 0.00 | 1.26 | 0.00 | 0.75 | 11.30 | 180.01 | 32.88 | 280.98 | 0.5443 | -670.0 | -506.6 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 9.79 | 179.68 | 32.55 | 278.24 | 0.5377 | -679.0 | -560.0 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 11.43 | 179.88 | 32.75 | 281.24 | 0.5426 | -621.0 | -438.6 | |
| 0.00 | 0.72 | 0.00 | 0.42 | 8.98 | 179.49 | 32.35 | 276.73 | 0.5343 | -651.0 | -571.5 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 11.52 | 178.98 | 31.84 | 281.58 | 0.5297 | -725.0 | -626.1 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 9.20 | 177.81 | 30.67 | 277.31 | 0.5097 | -605.0 | -566.8 | |
| 0.00 | 0.36 | 0.00 | 0.21 | 13.19 | 177.06 | 29.92 | 285.32 | 0.5055 | -577.0 | -552.2 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 9.63 | 175.62 | 28.48 | 278.46 | 0.4772 | -803.0 | -602.0 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 10.01 | 174.67 | 27.53 | 279.45 | 0.4634 | 730.0 | 590.2 | |
| 0.00 | 2.35 | 0.00 | 1.31 | 10.15 | 174.34 | 27.20 | 279.82 | 0.4585 | 772.0 | 677.1 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 10.59 | 174.10 | 26.96 | 280.84 | 0.4556 | 651.0 | 533.6 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 10.49 | 173.81 | 26.67 | 280.67 | 0.4510 | 831.0 | 698.9 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 9.80 | 173.47 | 26.34 | 279.22 | 0.4447 | 659.0 | 515.2 | |
| 0.00 | 1.35 | 0.00 | 0.75 | 9.50 | 173.28 | 26.14 | 278.60 | 0.4412 | 806.0 | 622.2 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 9.90 | 173.31 | 26.17 | 279.48 | 0.4423 | 585.0 | 514.6 | |
| 0.00 | 5.87 | 0.00 | 3.23 | 9.18 | 173.15 | 26.01 | 277.87 | 0.4388 | 741.0 | 756.4 | |
| 0.00 | 2.08 | 0.00 | 1.14 | 8.60 | 173.07 | 25.93 | 276.57 | 0.4370 | 845.0 | 740.0 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 8.82 | 173.02 | 25.88 | 277.07 | 0.4364 | 856.0 | 697.5 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 9.58 | 172.97 | 25.84 | 278.83 | 0.4367 | 778.0 | 633.1 | |
| 0.00 | 1.26 | 0.00 | 0.69 | 8.98 | 172.76 | 25.62 | 277.49 | 0.4325 | 872.0 | 761.1 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 9.87 | 172.72 | 25.59 | 279.54 | 0.4332 | 784.0 | 671.2 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 9.32 | 172.65 | 25.51 | 278.30 | 0.4312 | 890.0 | 707.4 | |
| 0.00 | 0.54 | 0.00 | 0.30 | 9.07 | 172.22 | 25.08 | 277.78 | 0.4242 | 856.0 | 844.5 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 9.32 | 172.00 | 24.86 | 278.43 | 0.4211 | 770.0 | 806.2 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 9.11 | 171.91 | 24.77 | 277.95 | 0.4195 | 847.0 | 718.4 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 8.85 | 168.98 | 21.84 | 277.88 | 0.3727 | 728.0 | 609.9 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 7.37 | 167.84 | 20.70 | 273.98 | 0.3529 | 867.0 | 687.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 7.22 | 167.80 | 20.66 | 273.56 | 0.3522 | 713.0 | 598.6 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 12.61 | 165.75 | 18.61 | 290.12 | 0.3331 | 799.0 | 649.6 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 11.16 | 162.34 | 15.20 | 288.71 | 0.2728 | 640.0 | 550.6 | |
| 0.00 | 2.53 | 0.00 | 1.29 | 14.05 | 158.24 | 11.10 | 305.95 | 0.2317 | 929.0 | 727.6 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 13.72 | 156.09 | 8.95 | 310.49 | 0.1997 | 747.0 | 533.7 | |
| 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. | |