SDO HMI 2011-10-14 10:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 116.63 | 757.42 | 64.12 | 418.14 | 26.89 | 57.01 | -16.05 | 34.09 | 0.4410 | -743.9 | -349.0 | |
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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 | 2.10 | 0.00 | 1.16 | 28.82 | 59.16 | -13.90 | 28.26 | 0.4465 | 724.0 | 712.6 | |
| 2.27 | 666.68 | 1.24 | 366.49 | 26.94 | 58.96 | -14.11 | 31.02 | 0.4234 | -1116.2 | -394.3 | |
| 108.58 | -2.00 | 59.66 | -2.00 | 27.14 | 57.92 | -15.14 | 32.49 | 0.4345 | -1322.2 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 20.85 | 58.60 | -14.47 | 41.86 | 0.3514 | -768.0 | -698.7 | |
| 0.00 | 2.62 | 0.00 | 1.38 | 19.93 | 58.59 | -14.47 | 43.82 | 0.3409 | -786.0 | -710.9 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 19.52 | 58.43 | -14.63 | 45.00 | 0.3382 | -765.0 | -620.2 | |
| 1.14 | -2.00 | 0.63 | -2.00 | 26.86 | 57.06 | -16.01 | 34.29 | 0.4385 | -939.0 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 20.79 | 57.44 | -15.62 | 44.07 | 0.3635 | -658.0 | -428.5 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 19.62 | 57.57 | -15.50 | 46.34 | 0.3494 | -767.0 | -528.8 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 19.22 | 57.41 | -15.66 | 47.51 | 0.3471 | -867.0 | -633.6 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 28.15 | 55.91 | -17.16 | 34.24 | 0.4642 | -657.0 | -536.6 | |
| 0.00 | 2.45 | 0.00 | 1.36 | 27.73 | 55.76 | -17.30 | 35.04 | 0.4604 | -707.0 | -694.9 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 27.24 | 55.67 | -17.40 | 35.87 | 0.4555 | -853.0 | -664.6 | |
| 0.00 | 1.84 | 0.00 | 1.02 | 27.46 | 55.56 | -17.50 | 35.71 | 0.4591 | -563.0 | -512.7 | |
| 1.75 | 3.32 | 0.97 | 1.85 | 26.83 | 54.99 | -18.07 | 37.45 | 0.4571 | -943.7 | -784.6 | |
| 0.00 | 4.90 | 0.00 | 2.74 | 27.47 | 54.81 | -18.25 | 36.77 | 0.4661 | -1000.0 | -729.0 | |
| 0.00 | 1.84 | 0.00 | 0.98 | 19.73 | 55.87 | -17.20 | 48.90 | 0.3710 | -705.0 | -612.0 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 26.92 | 54.73 | -18.33 | 37.70 | 0.4605 | -686.0 | -567.9 | |
| 1.49 | 2.19 | 0.83 | 1.22 | 26.85 | 54.42 | -18.64 | 38.24 | 0.4626 | -736.2 | -658.4 | |
| 0.00 | 1.66 | 0.00 | 0.94 | 28.67 | 53.84 | -19.22 | 36.41 | 0.4886 | -739.0 | -594.9 | |
| 0.00 | 0.87 | 0.00 | 0.49 | 27.83 | 53.93 | -19.13 | 37.48 | 0.4783 | -672.0 | -566.9 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 27.41 | 53.93 | -19.13 | 38.08 | 0.4736 | -984.0 | -849.7 | |
| 0.00 | 1.92 | 0.00 | 1.09 | 27.92 | 53.63 | -19.44 | 37.76 | 0.4821 | -755.0 | -586.9 | |
| 1.40 | 3.23 | 0.79 | 1.82 | 27.63 | 53.64 | -19.42 | 38.15 | 0.4788 | -796.9 | -692.1 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 28.69 | 53.26 | -19.80 | 37.15 | 0.4940 | -520.0 | -472.0 | |
| 0.00 | 1.22 | 0.00 | 0.70 | 28.42 | 53.06 | -20.00 | 37.79 | 0.4929 | -641.0 | -593.4 | |
| 0.00 | 1.22 | 0.00 | 0.69 | 26.68 | 53.07 | -19.99 | 40.34 | 0.4739 | -827.0 | -624.6 | |
| 0.00 | 1.31 | 0.00 | 0.74 | 27.67 | 52.85 | -20.22 | 39.15 | 0.4868 | -605.0 | -508.9 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 18.53 | 53.00 | -20.06 | 55.44 | 0.3967 | -714.0 | -595.5 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 24.94 | 51.61 | -21.45 | 44.96 | 0.4713 | 474.0 | 286.9 | |
| 0.00 | 2.27 | 0.00 | 1.29 | 26.77 | 51.22 | -21.84 | 42.51 | 0.4936 | -649.0 | -572.1 | |
| 0.00 | 3.41 | 0.00 | 1.86 | 17.62 | 50.65 | -22.41 | 59.98 | 0.4215 | -889.0 | -563.9 | |
| 0.00 | 1.75 | 0.00 | 0.96 | 17.89 | 50.61 | -22.45 | 59.43 | 0.4239 | -770.0 | -572.7 | |
| 0.00 | 1.22 | 0.00 | 0.68 | 19.57 | 48.71 | -24.35 | 57.82 | 0.4609 | 970.0 | 781.6 | |
| 0.00 | 1.92 | 0.00 | 1.09 | 22.11 | 47.88 | -25.19 | 53.87 | 0.4901 | 904.0 | 639.3 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 19.36 | 48.12 | -24.94 | 58.76 | 0.4673 | 860.0 | 651.4 | |
| 0.00 | 2.45 | 0.00 | 1.37 | 19.53 | 47.81 | -25.25 | 58.70 | 0.4725 | 507.0 | 423.8 | |
| 0.00 | 1.66 | 0.00 | 0.99 | 27.53 | 45.94 | -27.12 | 46.91 | 0.5557 | 685.0 | 551.3 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 23.00 | 46.73 | -26.34 | 53.39 | 0.5108 | 588.0 | 536.8 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 27.89 | 45.24 | -27.83 | 47.03 | 0.5661 | 498.0 | 404.5 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 27.24 | 45.37 | -27.69 | 47.85 | 0.5594 | 773.0 | 649.1 | |
| 0.00 | 1.22 | 0.00 | 0.72 | 26.22 | 45.61 | -27.46 | 49.18 | 0.5487 | 605.0 | 412.0 | |
| 0.00 | 1.49 | 0.00 | 0.88 | 26.03 | 45.62 | -27.45 | 49.47 | 0.5470 | 696.0 | 507.4 | |
| 0.00 | 2.88 | 0.00 | 1.72 | 27.23 | 45.07 | -27.99 | 48.14 | 0.5625 | 569.0 | 540.0 | |
| 0.00 | 1.66 | 0.00 | 0.99 | 26.02 | 44.64 | -28.42 | 50.34 | 0.5578 | 704.0 | 614.3 | |
| 0.00 | 1.22 | 0.00 | 0.74 | 26.84 | 44.30 | -28.76 | 49.38 | 0.5678 | 660.0 | 489.1 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 26.25 | 44.16 | -28.90 | 50.38 | 0.5649 | 718.0 | 505.7 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 25.68 | 44.20 | -28.86 | 51.23 | 0.5602 | 742.0 | 604.6 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 26.21 | 43.90 | -29.16 | 50.66 | 0.5674 | 780.0 | 604.1 | |
| 0.00 | 6.38 | 0.00 | 3.84 | 26.40 | 43.78 | -29.29 | 50.48 | 0.5702 | 652.0 | 606.9 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 26.71 | 43.57 | -29.49 | 50.18 | 0.5748 | 642.0 | 502.0 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 26.60 | 43.29 | -29.77 | 50.57 | 0.5770 | 554.0 | 473.0 | |
| 0.00 | 1.49 | 0.00 | 0.90 | 26.71 | 43.03 | -30.03 | 50.60 | 0.5808 | 627.0 | 408.4 | |
| 0.00 | 1.05 | 0.00 | 0.65 | 29.23 | 41.96 | -31.10 | 47.82 | 0.6106 | 367.0 | 329.2 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 22.67 | 42.29 | -30.77 | 57.45 | 0.5623 | 717.0 | 566.6 | |
| 0.00 | 1.57 | 0.00 | 0.98 | 24.00 | 39.42 | -33.64 | 57.22 | 0.6043 | 654.0 | 572.0 | |
| 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. | |