SDO HMI 2011-06-22 09:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81.69 | 497.72 | 47.91 | 291.52 | 17.13 | 169.01 | 28.74 | 300.43 | 0.5343 | -630.8 | -284.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.00 | 0.00 | 1.23 | 14.15 | 175.19 | 34.92 | 291.51 | 0.5988 | -584.0 | -466.5 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 12.95 | 172.80 | 32.53 | 290.64 | 0.5622 | -819.0 | -599.0 | |
| 0.00 | 3.18 | 0.00 | 1.91 | 14.26 | 172.89 | 32.63 | 292.81 | 0.5690 | -609.0 | -615.3 | |
| 75.16 | 426.37 | 44.34 | 251.45 | 17.10 | 169.89 | 29.63 | 299.48 | 0.5449 | -1455.0 | -395.5 | |
| 0.00 | 2.09 | 0.00 | 1.20 | 12.60 | 169.04 | 28.78 | 292.07 | 0.5089 | -596.0 | -535.4 | |
| 0.00 | 1.72 | 0.00 | 1.00 | 16.62 | 168.21 | 27.95 | 299.93 | 0.5202 | -974.0 | -833.1 | |
| 0.00 | 1.72 | 0.00 | 0.99 | 14.58 | 167.84 | 27.57 | 296.56 | 0.5028 | -595.0 | -536.2 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 17.54 | 168.29 | 28.02 | 301.45 | 0.5272 | -821.0 | -612.8 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 18.44 | 167.39 | 27.13 | 303.73 | 0.5222 | -750.0 | -584.6 | |
| 0.00 | 2.72 | 0.00 | 1.58 | 18.79 | 167.13 | 26.86 | 304.56 | 0.5215 | 875.0 | 732.7 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 14.15 | 165.57 | 25.30 | 297.52 | 0.4692 | -626.0 | -446.0 | |
| 0.00 | 1.63 | 0.00 | 0.94 | 18.04 | 166.07 | 25.81 | 304.26 | 0.5028 | 606.0 | 418.2 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 16.69 | 165.27 | 25.00 | 302.61 | 0.4826 | 560.0 | 506.6 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 18.13 | 164.28 | 24.02 | 306.19 | 0.4812 | 710.0 | 560.5 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 18.83 | 164.39 | 24.12 | 307.30 | 0.4882 | 351.0 | 346.0 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 18.61 | 164.32 | 24.05 | 306.99 | 0.4855 | 652.0 | 513.7 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 18.71 | 163.81 | 23.54 | 307.72 | 0.4801 | 648.0 | 421.6 | |
| 0.00 | 2.63 | 0.00 | 1.47 | 17.70 | 163.49 | 23.22 | 306.26 | 0.4677 | 946.0 | 694.3 | |
| 1.36 | 4.72 | 0.75 | 2.61 | 15.59 | 162.91 | 22.64 | 302.90 | 0.4435 | 961.3 | 712.6 | |
| 0.00 | 2.36 | 0.00 | 1.32 | 18.76 | 162.69 | 22.43 | 309.05 | 0.4671 | 758.0 | 656.2 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 17.36 | 162.51 | 22.24 | 306.74 | 0.4526 | 801.0 | 677.5 | |
| 0.00 | 3.00 | 0.00 | 1.67 | 17.68 | 162.51 | 22.25 | 307.32 | 0.4554 | 804.0 | 666.5 | |
| 0.00 | 2.36 | 0.00 | 1.32 | 18.53 | 162.56 | 22.29 | 308.82 | 0.4635 | 811.0 | 648.2 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 17.84 | 162.33 | 22.06 | 307.83 | 0.4545 | 857.0 | 677.6 | |
| 0.00 | 2.54 | 0.00 | 1.41 | 17.55 | 162.25 | 21.99 | 307.39 | 0.4512 | 687.0 | 670.6 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 19.24 | 162.00 | 21.73 | 310.74 | 0.4632 | 595.0 | 565.6 | |
| 0.00 | 2.45 | 0.00 | 1.37 | 19.28 | 161.65 | 21.39 | 311.22 | 0.4595 | 951.0 | 813.7 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 19.50 | 161.68 | 21.42 | 311.57 | 0.4620 | 679.0 | 547.6 | |
| 3.54 | 6.54 | 1.94 | 3.58 | 17.77 | 160.12 | 19.86 | 310.48 | 0.4270 | 938.7 | 670.7 | |
| 0.00 | 2.18 | 0.00 | 1.19 | 17.01 | 160.04 | 19.77 | 309.14 | 0.4188 | 896.0 | 733.2 | |
| 0.00 | 3.09 | 0.00 | 1.69 | 18.02 | 159.74 | 19.48 | 311.48 | 0.4250 | 802.0 | 629.1 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 18.44 | 159.76 | 19.49 | 312.22 | 0.4292 | 728.0 | 537.1 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 19.21 | 158.90 | 18.63 | 314.84 | 0.4272 | 751.0 | 613.7 | |
| 0.00 | 3.36 | 0.00 | 1.79 | 17.66 | 154.75 | 14.48 | 318.91 | 0.3642 | 909.0 | 711.5 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 20.02 | 154.79 | 14.53 | 322.99 | 0.3932 | 860.0 | 680.6 | |
| 1.63 | 2.00 | 0.88 | 1.08 | 20.47 | 154.70 | 14.44 | 323.89 | 0.3980 | 796.1 | 692.2 | |
| 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. | |