SDO HMI 2011-06-02 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.96 | 296.78 | 21.91 | 167.64 | 17.19 | 19.95 | -22.84 | 50.55 | 0.4809 | -303.5 | -285.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.59 | 18.24 | 25.72 | -17.06 | 40.94 | 0.4271 | -745.0 | -560.0 | |
| 0.00 | 2.44 | 0.00 | 1.40 | 21.46 | 21.90 | -20.89 | 41.59 | 0.5019 | -817.0 | -590.7 | |
| 0.00 | 4.97 | 0.00 | 2.78 | 18.41 | 22.28 | -20.50 | 45.73 | 0.4660 | -517.0 | -483.0 | |
| 17.80 | 228.99 | 9.91 | 127.71 | 16.46 | 21.32 | -21.46 | 50.27 | 0.4581 | -1251.0 | -463.0 | |
| 8.86 | -4.00 | 4.96 | -4.00 | 17.07 | 20.98 | -21.81 | 49.65 | 0.4679 | -889.5 | 999999 | |
| 4.43 | -4.00 | 2.47 | -4.00 | 16.50 | 20.94 | -21.84 | 50.68 | 0.4630 | -1027.0 | 999999 | |
| 2.26 | -4.00 | 1.26 | -4.00 | 16.78 | 20.81 | -21.98 | 50.35 | 0.4672 | -937.4 | 999999 | |
| 1.36 | -4.00 | 0.76 | -4.00 | 16.50 | 20.67 | -22.11 | 51.01 | 0.4663 | -762.3 | 999999 | |
| 0.00 | 2.26 | 0.00 | 1.28 | 18.52 | 20.10 | -22.69 | 48.32 | 0.4916 | -385.0 | -397.7 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 18.29 | 19.78 | -23.00 | 49.06 | 0.4932 | -502.0 | -385.1 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 18.10 | 19.77 | -23.01 | 49.38 | 0.4915 | -638.0 | -439.3 | |
| 0.00 | 1.72 | 0.00 | 0.98 | 17.78 | 19.54 | -23.25 | 50.18 | 0.4913 | -735.0 | -652.1 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 17.84 | 19.29 | -23.50 | 50.36 | 0.4949 | -610.0 | -469.9 | |
| 0.00 | 0.72 | 0.00 | 0.41 | 17.56 | 19.33 | -23.46 | 50.79 | 0.4918 | -575.0 | -417.2 | |
| 0.00 | 1.17 | 0.00 | 0.67 | 17.49 | 18.78 | -24.01 | 51.50 | 0.4978 | -610.0 | -483.7 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 17.66 | 18.19 | -24.59 | 51.87 | 0.5061 | -716.0 | -516.0 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 17.85 | 17.92 | -24.87 | 51.85 | 0.5110 | -567.0 | -428.7 | |
| 0.63 | 2.71 | 0.37 | 1.58 | 18.46 | 17.19 | -25.60 | 51.62 | 0.5248 | 925.9 | 805.1 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 18.43 | 16.80 | -25.99 | 52.06 | 0.5291 | 796.0 | 633.1 | |
| 0.00 | 1.08 | 0.00 | 0.63 | 18.15 | 16.70 | -26.08 | 52.62 | 0.5279 | 732.0 | 568.2 | |
| 0.00 | 2.44 | 0.00 | 1.43 | 18.44 | 16.26 | -26.52 | 52.59 | 0.5354 | -716.0 | -594.0 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 19.37 | 15.70 | -27.08 | 51.68 | 0.5496 | 586.0 | 502.4 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 19.83 | 15.51 | -27.28 | 51.18 | 0.5555 | 730.0 | 618.1 | |
| 0.00 | 1.45 | 0.00 | 0.85 | 17.93 | 15.38 | -27.41 | 54.23 | 0.5419 | 906.0 | 772.7 | |
| 0.00 | 0.90 | 0.00 | 0.55 | 21.14 | 14.74 | -28.05 | 49.99 | 0.5748 | 690.0 | 587.4 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 16.65 | 14.90 | -27.88 | 56.70 | 0.5382 | 748.0 | 578.1 | |
| 0.00 | 1.27 | 0.00 | 0.77 | 21.44 | 13.93 | -28.85 | 50.30 | 0.5860 | 736.0 | 549.1 | |
| 0.00 | 2.26 | 0.00 | 1.38 | 21.67 | 13.77 | -29.02 | 50.12 | 0.5896 | 757.0 | 579.9 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 19.84 | 14.15 | -28.63 | 52.42 | 0.5710 | 773.0 | 585.5 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 19.67 | 14.04 | -28.75 | 52.76 | 0.5710 | 775.0 | 589.8 | |
| 2.26 | 10.30 | 1.36 | 6.20 | 19.09 | 13.89 | -28.89 | 53.76 | 0.5683 | 900.8 | 674.9 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 19.38 | 13.76 | -29.02 | 53.43 | 0.5720 | 652.0 | 548.0 | |
| 0.00 | 1.81 | 0.00 | 1.08 | 18.45 | 13.76 | -29.03 | 54.85 | 0.5651 | 655.0 | 595.2 | |
| 0.00 | 8.77 | 0.00 | 5.28 | 18.64 | 13.42 | -29.36 | 54.84 | 0.5704 | 481.0 | 624.0 | |
| 1.36 | 4.61 | 0.82 | 2.79 | 19.00 | 13.28 | -29.50 | 54.42 | 0.5747 | 750.3 | 495.1 | |
| 0.00 | 0.72 | 0.00 | 0.45 | 21.12 | 12.23 | -30.55 | 52.21 | 0.6022 | 664.0 | 529.5 | |
| 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. | |