SDO HMI 2011-06-05 21:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.29 | 273.97 | 42.78 | 181.30 | -21.99 | 34.75 | 36.11 | 235.60 | 0.6645 | 15.4 | -37.3 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.95 | -19.12 | 40.04 | 41.39 | 242.45 | 0.7069 | -397.0 | -363.3 | |
| 0.00 | 0.36 | 0.00 | 0.25 | -18.19 | 39.50 | 40.86 | 243.46 | 0.6970 | -487.0 | -485.5 | |
| 0.00 | 0.99 | 0.00 | 0.70 | -20.45 | 39.59 | 40.95 | 240.48 | 0.7079 | 392.0 | 333.8 | |
| 1.90 | 2.80 | 1.30 | 1.91 | -18.45 | 38.77 | 40.13 | 242.76 | 0.6899 | -422.0 | -230.3 | |
| 14.11 | 42.15 | 9.71 | 29.01 | -19.38 | 39.00 | 40.35 | 241.61 | 0.6966 | 899.4 | 445.1 | |
| 0.00 | 1.27 | 0.00 | 0.86 | -18.58 | 38.39 | 39.74 | 242.40 | 0.6861 | -243.0 | -238.6 | |
| 0.00 | 1.27 | 0.00 | 0.89 | -21.82 | 39.15 | 40.50 | 238.47 | 0.7097 | 618.0 | 534.0 | |
| 0.00 | 2.26 | 0.00 | 1.57 | -21.07 | 38.89 | 40.25 | 239.32 | 0.7033 | 442.0 | 264.7 | |
| 0.00 | 1.27 | 0.00 | 0.86 | -19.28 | 38.01 | 39.36 | 241.24 | 0.6851 | 678.0 | 642.4 | |
| 0.00 | 0.99 | 0.00 | 0.67 | -18.86 | 37.80 | 39.16 | 241.71 | 0.6808 | 661.0 | 637.2 | |
| 0.00 | 1.27 | 0.00 | 0.86 | -19.19 | 37.85 | 39.20 | 241.30 | 0.6829 | 667.0 | 635.3 | |
| 0.00 | 1.45 | 0.00 | 1.03 | -24.30 | 38.87 | 40.23 | 235.15 | 0.7195 | 683.0 | 539.2 | |
| 0.00 | 1.90 | 0.00 | 1.28 | -20.64 | 36.82 | 38.18 | 238.76 | 0.6787 | 735.0 | 578.4 | |
| 8.68 | 12.75 | 5.86 | 8.60 | -20.97 | 36.88 | 38.23 | 238.36 | 0.6811 | 611.7 | 380.9 | |
| 0.00 | 1.27 | 0.00 | 0.85 | -20.06 | 36.61 | 37.96 | 239.44 | 0.6733 | 669.0 | 571.3 | |
| 0.00 | 1.36 | 0.00 | 0.91 | -20.12 | 36.46 | 37.82 | 239.27 | 0.6721 | 689.0 | 592.6 | |
| 0.00 | 2.44 | 0.00 | 1.64 | -20.68 | 36.46 | 37.81 | 238.51 | 0.6749 | 767.0 | 640.0 | |
| 0.00 | 1.81 | 0.00 | 1.21 | -21.13 | 36.43 | 37.78 | 237.88 | 0.6770 | 816.0 | 595.2 | |
| 0.00 | 1.27 | 0.00 | 0.85 | -21.33 | 36.41 | 37.76 | 237.60 | 0.6778 | 651.0 | 536.1 | |
| 0.00 | 0.99 | 0.00 | 0.67 | -20.87 | 36.27 | 37.62 | 238.14 | 0.6739 | 650.0 | 583.5 | |
| 0.00 | 5.34 | 0.00 | 3.55 | -20.64 | 36.04 | 37.39 | 238.32 | 0.6701 | 396.0 | 453.5 | |
| 0.00 | 1.54 | 0.00 | 1.01 | -19.48 | 35.43 | 36.78 | 239.57 | 0.6570 | -559.0 | -512.7 | |
| 0.00 | 1.81 | 0.00 | 1.18 | -19.35 | 35.24 | 36.59 | 239.63 | 0.6541 | -702.0 | -555.9 | |
| 0.00 | 1.36 | 0.00 | 0.92 | -23.10 | 35.80 | 37.16 | 234.89 | 0.6814 | 608.0 | 418.2 | |
| 0.00 | 1.72 | 0.00 | 1.15 | -23.77 | 34.90 | 36.25 | 233.45 | 0.6760 | -614.0 | -443.0 | |
| 3.35 | 38.71 | 2.20 | 25.55 | -22.61 | 34.17 | 35.52 | 234.50 | 0.6611 | 775.7 | 196.9 | |
| 0.00 | 0.81 | 0.00 | 0.52 | -19.80 | 33.36 | 34.71 | 237.84 | 0.6352 | -660.0 | -524.2 | |
| 2.71 | -26.00 | 1.79 | -26.00 | -22.87 | 33.97 | 35.32 | 234.01 | 0.6606 | 808.2 | 999999 | |
| 7.51 | 9.50 | 5.00 | 6.32 | -24.13 | 34.19 | 35.55 | 232.50 | 0.6710 | -711.0 | -507.0 | |
| 0.00 | 1.09 | 0.00 | 0.71 | -22.41 | 33.23 | 34.58 | 234.13 | 0.6497 | 494.0 | 398.2 | |
| 0.00 | 1.90 | 0.00 | 1.22 | -21.82 | 32.70 | 34.05 | 234.57 | 0.6403 | -782.0 | -687.7 | |
| 16.55 | 110.79 | 10.79 | 71.97 | -23.27 | 32.91 | 34.27 | 232.76 | 0.6520 | -378.1 | -330.0 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -21.23 | 32.19 | 33.54 | 235.03 | 0.6308 | -702.0 | -560.7 | |
| 0.00 | 2.53 | 0.00 | 1.62 | -21.79 | 32.26 | 33.61 | 234.30 | 0.6352 | -810.0 | -693.1 | |
| 2.08 | 2.35 | 1.34 | 1.51 | -22.15 | 32.32 | 33.67 | 233.85 | 0.6382 | -739.9 | -806.0 | |
| 0.63 | -32.00 | 0.41 | -32.00 | -23.44 | 32.60 | 33.95 | 232.31 | 0.6498 | -823.7 | 999999 | |
| 2.44 | -32.00 | 1.58 | -32.00 | -22.91 | 32.41 | 33.76 | 232.88 | 0.6442 | -920.9 | 999999 | |
| 0.54 | -32.00 | 0.35 | -32.00 | -23.57 | 32.52 | 33.87 | 232.08 | 0.6499 | -644.8 | 999999 | |
| 2.98 | -32.00 | 1.92 | -32.00 | -22.68 | 32.22 | 33.58 | 233.06 | 0.6407 | -839.5 | 999999 | |
| 0.00 | 2.17 | 0.00 | 1.39 | -22.21 | 32.02 | 33.37 | 233.54 | 0.6354 | -846.0 | -707.8 | |
| 0.81 | -32.00 | 0.53 | -32.00 | -23.40 | 32.31 | 33.66 | 232.15 | 0.6465 | -636.6 | 999999 | |
| 0.00 | 2.26 | 0.00 | 1.47 | -23.90 | 32.26 | 33.61 | 231.45 | 0.6494 | -418.0 | -319.4 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -21.79 | 31.63 | 32.98 | 233.85 | 0.6283 | -735.0 | -639.6 | |
| 0.00 | 3.71 | 0.00 | 2.38 | -22.77 | 31.86 | 33.21 | 232.66 | 0.6374 | -628.0 | -585.9 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -22.48 | 31.62 | 32.97 | 232.89 | 0.6328 | -816.0 | -686.9 | |
| 0.00 | 1.18 | 0.00 | 0.74 | -21.30 | 31.15 | 32.51 | 234.19 | 0.6197 | -674.0 | -597.1 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -22.05 | 29.84 | 31.19 | 232.11 | 0.6104 | -190.0 | -305.2 | |
| 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. | |