SDO HMI 2014-07-11 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.88 | 146.68 | 16.71 | 78.92 | 5.99 | 204.45 | 22.66 | 276.25 | 0.3870 | -197.0 | -155.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.82 | 0.00 | 0.46 | 4.77 | 210.13 | 28.35 | 272.72 | 0.4756 | -681.0 | -619.9 | |
| 14.90 | 72.21 | 8.10 | 39.31 | 5.87 | 206.22 | 24.43 | 275.50 | 0.4150 | -1110.6 | -360.4 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 5.27 | 205.95 | 24.17 | 274.06 | 0.4104 | -852.0 | -749.8 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 4.79 | 205.80 | 24.01 | 272.89 | 0.4077 | -627.0 | -544.8 | |
| 6.36 | -2.00 | 3.45 | -2.00 | 5.83 | 205.78 | 23.99 | 275.44 | 0.4080 | -1180.3 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 4.91 | 205.64 | 23.85 | 273.21 | 0.4052 | -775.0 | -585.6 | |
| 2.54 | 5.63 | 1.38 | 3.05 | 4.37 | 205.58 | 23.80 | 271.85 | 0.4042 | -959.1 | -726.0 | |
| 0.00 | 1.82 | 0.00 | 0.98 | 4.89 | 205.37 | 23.58 | 273.17 | 0.4009 | -928.0 | -780.7 | |
| 0.00 | 5.36 | 0.00 | 2.89 | 3.31 | 205.15 | 23.36 | 269.19 | 0.3976 | -622.0 | -737.7 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 6.85 | 205.16 | 23.37 | 278.11 | 0.3995 | -655.0 | -573.3 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 7.56 | 204.96 | 23.18 | 279.93 | 0.3978 | 629.0 | 448.8 | |
| 0.00 | 5.18 | 0.00 | 2.78 | 6.27 | 204.26 | 22.48 | 276.82 | 0.3843 | -973.0 | -761.2 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 7.91 | 204.28 | 22.50 | 281.08 | 0.3878 | 53.0 | 119.9 | |
| 0.00 | 2.00 | 0.00 | 1.07 | 7.21 | 204.18 | 22.39 | 279.31 | 0.3846 | -964.0 | -720.9 | |
| 2.72 | 6.09 | 1.46 | 3.27 | 8.32 | 204.14 | 22.35 | 282.16 | 0.3866 | 943.9 | 560.5 | |
| 0.36 | 4.36 | 0.19 | 2.33 | 6.16 | 203.79 | 22.01 | 276.64 | 0.3767 | -1057.5 | -772.7 | |
| 2.91 | 4.45 | 1.55 | 2.38 | 8.12 | 203.43 | 21.64 | 281.97 | 0.3748 | 1074.0 | 815.4 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 7.91 | 203.42 | 21.63 | 281.41 | 0.3741 | 796.0 | 600.2 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 5.04 | 203.19 | 21.40 | 273.73 | 0.3658 | -919.0 | -764.6 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 5.20 | 203.13 | 21.34 | 274.16 | 0.3649 | -824.0 | -511.0 | |
| 1.09 | 2.63 | 0.58 | 1.40 | 6.30 | 203.14 | 21.35 | 277.16 | 0.3663 | -1001.4 | -781.2 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 6.45 | 202.95 | 21.16 | 277.65 | 0.3635 | -911.0 | -673.3 | |
| 0.00 | 2.27 | 0.00 | 1.20 | 7.08 | 202.39 | 20.60 | 279.56 | 0.3556 | 941.0 | 840.6 | |
| 0.00 | 4.72 | 0.00 | 2.50 | 4.86 | 202.20 | 20.41 | 273.29 | 0.3496 | 1092.0 | 767.5 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 5.19 | 202.08 | 20.29 | 274.28 | 0.3478 | 835.0 | 635.6 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 5.97 | 201.62 | 19.83 | 276.62 | 0.3411 | 872.0 | 736.0 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 6.85 | 201.62 | 19.84 | 279.20 | 0.3428 | 750.0 | 631.0 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 7.38 | 201.35 | 19.57 | 280.84 | 0.3396 | 778.0 | 631.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 5.76 | 200.05 | 18.27 | 276.39 | 0.3152 | 867.0 | 720.7 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 5.80 | 199.51 | 17.72 | 276.68 | 0.3062 | 849.0 | 627.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 8.31 | 199.45 | 17.66 | 284.75 | 0.3118 | 852.0 | 649.9 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 5.78 | 199.22 | 17.43 | 276.68 | 0.3014 | 819.0 | 738.6 | |
| 0.00 | 3.81 | 0.00 | 1.97 | 6.33 | 197.64 | 15.85 | 279.21 | 0.2762 | 927.0 | 666.3 | |
| 0.00 | 2.72 | 0.00 | 1.40 | 6.63 | 197.65 | 15.86 | 280.30 | 0.2771 | 714.0 | 719.0 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 6.48 | 196.24 | 14.46 | 280.54 | 0.2534 | 987.0 | 885.0 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 6.45 | 196.05 | 14.26 | 280.56 | 0.2502 | 957.0 | 713.1 | |
| 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. | |