SDO HMI 2014-08-09 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.54 | 71.30 | 0.29 | 38.22 | 9.57 | 173.74 | 21.66 | 281.06 | 0.3716 | 273.5 | 278.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.58 | 5.60 | 184.10 | 32.02 | 270.38 | 0.5298 | -647.0 | -480.3 | |
| 0.00 | 1.44 | 0.00 | 0.83 | 6.71 | 182.89 | 30.81 | 272.42 | 0.5111 | -838.0 | -750.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 11.39 | 182.05 | 29.97 | 281.79 | 0.5022 | -630.0 | -517.2 | |
| 0.00 | 1.72 | 0.00 | 0.98 | 11.72 | 181.58 | 29.50 | 282.57 | 0.4960 | -782.0 | -540.3 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 9.10 | 180.46 | 28.38 | 277.38 | 0.4753 | -614.0 | -471.6 | |
| 0.00 | 1.62 | 0.00 | 0.92 | 11.64 | 180.37 | 28.29 | 282.73 | 0.4778 | -807.0 | -554.1 | |
| 0.00 | 1.44 | 0.00 | 0.81 | 12.49 | 180.36 | 28.28 | 284.51 | 0.4798 | -716.0 | -621.5 | |
| 0.00 | 1.53 | 0.00 | 0.86 | 9.73 | 179.44 | 27.36 | 278.90 | 0.4604 | -924.0 | -748.8 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 5.87 | 179.16 | 27.08 | 270.45 | 0.4547 | -785.0 | -643.1 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 8.97 | 178.72 | 26.64 | 277.35 | 0.4484 | -751.0 | -579.5 | |
| 0.00 | 2.17 | 0.00 | 1.20 | 9.11 | 178.35 | 26.27 | 277.72 | 0.4428 | -600.0 | -607.0 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 8.69 | 177.67 | 25.59 | 276.86 | 0.4318 | -763.0 | -545.0 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 9.21 | 177.60 | 25.52 | 278.07 | 0.4314 | -703.0 | -587.4 | |
| 0.00 | 2.98 | 0.00 | 1.61 | 9.37 | 175.52 | 23.44 | 278.90 | 0.3989 | -684.0 | -483.5 | |
| 0.00 | 1.35 | 0.00 | 0.73 | 9.90 | 174.38 | 22.30 | 280.60 | 0.3820 | 693.0 | 520.4 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 10.10 | 174.17 | 22.09 | 281.18 | 0.3789 | 825.0 | 516.3 | |
| 0.00 | 2.44 | 0.00 | 1.30 | 8.62 | 173.87 | 21.79 | 277.32 | 0.3715 | 570.0 | 403.5 | |
| 0.00 | 5.15 | 0.00 | 2.75 | 10.05 | 173.86 | 21.78 | 281.16 | 0.3740 | 689.0 | 565.2 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 9.29 | 173.68 | 21.60 | 279.20 | 0.3696 | 690.0 | 541.2 | |
| 0.54 | 1.90 | 0.29 | 1.01 | 10.31 | 173.55 | 21.47 | 281.97 | 0.3697 | 967.3 | 777.1 | |
| 0.00 | 2.26 | 0.00 | 1.20 | 9.30 | 173.48 | 21.40 | 279.28 | 0.3664 | 875.0 | 733.6 | |
| 0.00 | 3.34 | 0.00 | 1.77 | 8.50 | 173.00 | 20.92 | 277.18 | 0.3575 | 853.0 | 691.4 | |
| 0.00 | 5.33 | 0.00 | 2.82 | 8.90 | 172.96 | 20.88 | 278.31 | 0.3574 | 1039.0 | 802.3 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 9.23 | 172.98 | 20.90 | 279.23 | 0.3583 | 849.0 | 644.4 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 9.81 | 172.92 | 20.84 | 280.87 | 0.3585 | 867.0 | 693.7 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 9.51 | 172.83 | 20.75 | 280.06 | 0.3564 | 818.0 | 672.4 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 9.09 | 172.74 | 20.66 | 278.91 | 0.3542 | 1010.0 | 841.6 | |
| 0.00 | 2.08 | 0.00 | 1.10 | 8.79 | 172.69 | 20.61 | 278.07 | 0.3528 | 873.0 | 704.3 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 9.79 | 172.62 | 20.54 | 280.93 | 0.3537 | 618.0 | 463.4 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 7.86 | 172.34 | 20.26 | 275.47 | 0.3461 | 823.0 | 696.6 | |
| 0.00 | 3.16 | 0.00 | 1.67 | 9.32 | 172.36 | 20.28 | 279.68 | 0.3485 | 780.0 | 739.1 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 8.92 | 172.30 | 20.22 | 278.56 | 0.3468 | 881.0 | 772.3 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 8.64 | 171.83 | 19.75 | 277.86 | 0.3387 | 710.0 | 626.3 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 13.65 | 171.69 | 19.61 | 292.20 | 0.3538 | 707.0 | 618.6 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 13.48 | 171.32 | 19.24 | 292.07 | 0.3472 | 815.0 | 655.2 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 7.16 | 167.86 | 15.78 | 273.84 | 0.2716 | 762.0 | 610.0 | |
| 0.00 | 2.08 | 0.00 | 1.05 | 11.64 | 163.23 | 11.15 | 296.41 | 0.2123 | 704.0 | 446.1 | |
| 0.00 | 1.90 | 0.00 | 0.95 | 8.35 | 161.89 | 9.81 | 282.14 | 0.1732 | 802.0 | 645.0 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 9.01 | 158.83 | 6.75 | 292.00 | 0.1258 | 1030.0 | 754.0 | |
| 0.00 | 1.53 | 0.00 | 0.77 | 14.05 | 157.95 | 5.87 | 323.56 | 0.1678 | 733.0 | 636.2 | |
| 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. | |