SDO HMI 2011-10-27 09:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 279.94 | 1401.42 | 142.57 | 712.83 | 7.59 | 250.81 | -11.34 | 76.10 | 0.2013 | -218.8 | -111.6 | |
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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 | 1.30 | 0.00 | 0.65 | 12.84 | 261.14 | -1.01 | 7.08 | 0.1407 | -765.0 | -634.5 | |
| 0.00 | 1.13 | 0.00 | 0.56 | 12.20 | 258.58 | -3.57 | 25.44 | 0.1425 | -832.0 | -671.3 | |
| 0.00 | 1.91 | 0.00 | 0.95 | 4.61 | 256.79 | -5.36 | 92.45 | 0.0937 | 739.0 | 474.6 | |
| 0.00 | 2.86 | 0.00 | 1.44 | 12.82 | 256.45 | -5.70 | 34.86 | 0.1701 | -799.0 | -581.0 | |
| 1.48 | 815.73 | 0.73 | 407.00 | 5.67 | 256.18 | -5.97 | 81.90 | 0.1051 | -1179.0 | -432.8 | |
| 0.00 | 1.74 | 0.00 | 0.87 | 7.91 | 255.91 | -6.24 | 63.49 | 0.1209 | -14.0 | 64.1 | |
| 133.16 | -5.00 | 66.39 | -5.00 | 6.33 | 255.75 | -6.40 | 76.71 | 0.1144 | -1422.9 | 999999 | |
| 0.87 | -5.00 | 0.43 | -5.00 | 6.47 | 254.96 | -7.19 | 76.97 | 0.1282 | -993.9 | 999999 | |
| 2.86 | -5.00 | 1.43 | -5.00 | 5.81 | 254.64 | -7.51 | 82.41 | 0.1318 | -1116.2 | 999999 | |
| 15.45 | -5.00 | 7.72 | -5.00 | 6.08 | 254.57 | -7.58 | 80.47 | 0.1335 | -1151.9 | 999999 | |
| 5.73 | -5.00 | 2.86 | -5.00 | 6.58 | 254.54 | -7.61 | 76.81 | 0.1358 | -756.4 | 999999 | |
| 0.00 | 1.56 | 0.00 | 0.78 | 3.84 | 254.51 | -7.64 | 97.29 | 0.1344 | 1094.0 | 825.9 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 4.97 | 254.50 | -7.65 | 88.80 | 0.1333 | -845.0 | -653.2 | |
| 0.00 | 2.17 | 0.00 | 1.09 | 12.02 | 254.26 | -7.89 | 46.93 | 0.1846 | -905.0 | -793.7 | |
| 0.00 | 1.74 | 0.00 | 0.87 | 4.70 | 254.41 | -7.74 | 90.81 | 0.1348 | -657.0 | -463.2 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 7.68 | 253.70 | -8.45 | 71.02 | 0.1547 | -779.0 | -610.7 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 5.17 | 253.68 | -8.47 | 87.50 | 0.1475 | -689.0 | -479.8 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 13.69 | 253.40 | -8.75 | 43.70 | 0.2148 | -745.0 | -591.2 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 13.96 | 253.11 | -9.04 | 43.74 | 0.2214 | -692.0 | -542.6 | |
| 0.00 | 1.74 | 0.00 | 0.88 | 11.37 | 252.99 | -9.16 | 53.72 | 0.1945 | -866.0 | -662.3 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 10.86 | 252.52 | -9.63 | 57.25 | 0.1963 | -746.0 | -422.8 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 11.31 | 252.44 | -9.71 | 55.54 | 0.2015 | -863.0 | -662.2 | |
| 0.00 | 2.69 | 0.00 | 1.35 | 6.41 | 252.48 | -9.67 | 80.40 | 0.1701 | -1049.0 | -825.1 | |
| 2.86 | 3.91 | 1.44 | 1.96 | 5.45 | 252.43 | -9.72 | 86.05 | 0.1692 | -964.8 | -716.3 | |
| 0.00 | 3.82 | 0.00 | 1.92 | 6.25 | 252.24 | -9.91 | 81.48 | 0.1738 | -707.0 | -648.2 | |
| 2.00 | 12.15 | 1.01 | 6.13 | 5.68 | 251.49 | -10.66 | 85.10 | 0.1856 | -1102.8 | -816.0 | |
| 0.69 | -26.00 | 0.35 | -26.00 | 5.61 | 251.28 | -10.87 | 85.51 | 0.1892 | -833.0 | 999999 | |
| 0.00 | 1.56 | 0.00 | 0.79 | 8.10 | 250.05 | -12.10 | 74.28 | 0.2166 | -928.0 | -615.0 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 5.83 | 249.77 | -12.38 | 84.94 | 0.2150 | 856.0 | 718.8 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 8.21 | 249.52 | -12.63 | 74.38 | 0.2257 | -898.0 | -703.6 | |
| 0.00 | 2.52 | 0.00 | 1.28 | 5.67 | 249.19 | -12.96 | 85.82 | 0.2247 | 1005.0 | 780.0 | |
| 0.00 | 2.95 | 0.00 | 1.51 | 6.98 | 247.74 | -14.41 | 80.87 | 0.2513 | 1092.0 | 803.2 | |
| 0.00 | 2.60 | 0.00 | 1.33 | 7.39 | 247.54 | -14.61 | 79.37 | 0.2557 | 984.0 | 803.6 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 8.94 | 247.45 | -14.70 | 73.55 | 0.2626 | 1010.0 | 829.8 | |
| 0.00 | 3.47 | 0.00 | 1.78 | 7.12 | 247.46 | -14.69 | 80.46 | 0.2564 | 905.0 | 765.7 | |
| 0.00 | 1.74 | 0.00 | 0.89 | 8.01 | 247.30 | -14.85 | 77.15 | 0.2615 | 843.0 | 683.8 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 9.05 | 247.04 | -15.11 | 73.54 | 0.2697 | 1006.0 | 837.1 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 8.28 | 247.01 | -15.14 | 76.39 | 0.2671 | 999.0 | 816.6 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 9.07 | 246.41 | -15.74 | 74.04 | 0.2798 | 780.0 | 686.1 | |
| 0.00 | 1.56 | 0.00 | 0.81 | 9.25 | 246.37 | -15.78 | 73.46 | 0.2812 | 1005.0 | 824.9 | |
| 0.00 | 1.48 | 0.00 | 0.76 | 10.05 | 246.18 | -15.97 | 70.91 | 0.2880 | 820.0 | 636.5 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 9.69 | 246.07 | -16.08 | 72.23 | 0.2880 | 1022.0 | 903.5 | |
| 1.30 | 11.63 | 0.67 | 6.02 | 9.54 | 245.89 | -16.26 | 72.91 | 0.2902 | 1059.5 | 859.0 | |
| 0.78 | 4.60 | 0.41 | 2.39 | 10.22 | 245.63 | -16.52 | 70.90 | 0.2974 | 1035.6 | 869.5 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 9.64 | 245.13 | -17.02 | 73.23 | 0.3028 | -747.0 | -560.4 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 9.97 | 245.08 | -17.07 | 72.22 | 0.3050 | 701.0 | 467.9 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 10.29 | 245.00 | -17.15 | 71.26 | 0.3078 | 819.0 | 543.9 | |
| 9.55 | 483.87 | 5.00 | 253.90 | 11.02 | 244.00 | -18.15 | 69.98 | 0.3269 | 1077.6 | 376.3 | |
| 9.98 | -48.00 | 5.22 | -48.00 | 9.64 | 243.89 | -18.26 | 74.18 | 0.3225 | 1205.7 | 999999 | |
| 2.08 | -48.00 | 1.09 | -48.00 | 9.09 | 243.57 | -18.58 | 76.05 | 0.3256 | 1069.8 | 999999 | |
| 10.85 | -48.00 | 5.70 | -48.00 | 10.43 | 243.39 | -18.75 | 72.19 | 0.3336 | 1034.1 | 999999 | |
| 0.00 | 3.47 | 0.00 | 1.83 | 11.24 | 243.34 | -18.81 | 69.92 | 0.3382 | -14.0 | 76.8 | |
| 30.47 | -48.00 | 15.95 | -48.00 | 8.52 | 243.47 | -18.68 | 77.83 | 0.3254 | 1195.3 | 999999 | |
| 49.83 | -48.00 | 26.17 | -48.00 | 9.62 | 243.19 | -18.96 | 74.72 | 0.3336 | 1152.4 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.10 | 5.94 | 241.87 | -20.28 | 86.00 | 0.3472 | 726.0 | 536.1 | |
| 0.00 | 1.22 | 0.00 | 0.65 | 11.16 | 241.41 | -20.74 | 71.67 | 0.3676 | 649.0 | 479.5 | |
| 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. | |