SDO HMI 2011-11-19 05:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.98 | 204.85 | 17.24 | 114.21 | -18.87 | 337.38 | 16.30 | 216.17 | 0.4607 | 122.0 | 221.4 | |
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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 | 0.77 | 0.00 | 0.45 | -17.49 | 344.82 | 23.74 | 228.76 | 0.5127 | 692.0 | 592.2 | |
| 0.00 | 1.37 | 0.00 | 0.79 | -17.94 | 343.46 | 22.38 | 226.44 | 0.5018 | 614.0 | 519.1 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -17.75 | 343.40 | 22.32 | 226.66 | 0.4993 | 820.0 | 564.0 | |
| 0.00 | 2.06 | 0.00 | 1.18 | -18.03 | 343.14 | 22.05 | 225.90 | 0.4992 | 832.0 | 606.5 | |
| 1.37 | 2.23 | 0.78 | 1.27 | -17.77 | 343.04 | 21.95 | 226.17 | 0.4955 | 883.6 | 795.9 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -16.73 | 342.64 | 21.55 | 227.30 | 0.4808 | 764.0 | 637.1 | |
| 0.00 | 2.49 | 0.00 | 1.41 | -17.04 | 342.54 | 21.46 | 226.68 | 0.4828 | 855.0 | 801.0 | |
| 0.00 | 1.20 | 0.00 | 0.68 | -17.48 | 342.60 | 21.51 | 226.05 | 0.4878 | 958.0 | 747.4 | |
| 0.00 | 1.72 | 0.00 | 0.99 | -19.42 | 342.75 | 21.67 | 223.37 | 0.5092 | 625.0 | 538.2 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -17.92 | 342.52 | 21.44 | 225.28 | 0.4914 | 790.0 | 639.8 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -17.00 | 342.24 | 21.16 | 226.34 | 0.4790 | 868.0 | 673.4 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -16.75 | 342.08 | 20.99 | 226.53 | 0.4747 | 766.0 | 759.1 | |
| 0.00 | 0.94 | 0.00 | 0.55 | -21.31 | 342.69 | 21.61 | 220.67 | 0.5285 | 670.0 | 598.1 | |
| 0.00 | 3.78 | 0.00 | 2.19 | -21.31 | 342.32 | 21.23 | 220.20 | 0.5248 | 969.0 | 767.2 | |
| 1.37 | 4.29 | 0.77 | 2.42 | -17.53 | 341.74 | 20.65 | 224.84 | 0.4789 | 777.1 | 643.2 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -17.15 | 341.63 | 20.54 | 225.29 | 0.4738 | 803.0 | 606.5 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -16.43 | 341.48 | 20.39 | 226.24 | 0.4647 | 867.0 | 701.9 | |
| 0.00 | 1.80 | 0.00 | 1.01 | -17.58 | 340.78 | 19.70 | 223.45 | 0.4692 | 818.0 | 595.5 | |
| 0.00 | 3.18 | 0.00 | 1.79 | -18.84 | 340.50 | 19.42 | 221.16 | 0.4800 | -673.0 | -588.2 | |
| 3.26 | 111.52 | 1.82 | 62.00 | -17.38 | 340.30 | 19.21 | 223.06 | 0.4619 | 947.5 | 512.1 | |
| 0.34 | 2.49 | 0.19 | 1.38 | -16.06 | 340.13 | 19.04 | 224.93 | 0.4459 | 807.8 | 827.6 | |
| 18.20 | -20.00 | 10.12 | -20.00 | -17.37 | 339.74 | 18.66 | 222.25 | 0.4559 | 1217.9 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.76 | -15.93 | 339.30 | 18.22 | 223.91 | 0.4353 | 859.0 | 766.4 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -15.88 | 338.26 | 17.18 | 222.34 | 0.4236 | -810.0 | -637.8 | |
| 1.80 | 2.32 | 0.98 | 1.27 | -16.75 | 337.27 | 16.19 | 219.30 | 0.4234 | -828.5 | -567.3 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -18.04 | 337.16 | 16.08 | 217.16 | 0.4378 | -914.0 | -695.3 | |
| 0.00 | 2.92 | 0.00 | 1.59 | -16.96 | 337.03 | 15.95 | 218.55 | 0.4236 | -745.0 | -568.6 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -16.74 | 337.01 | 15.93 | 218.86 | 0.4207 | -966.0 | -731.3 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -14.77 | 336.73 | 15.65 | 221.61 | 0.3944 | 873.0 | 680.9 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -19.54 | 335.10 | 14.01 | 211.51 | 0.4385 | 817.0 | 611.1 | |
| 0.00 | 1.37 | 0.00 | 0.76 | -20.10 | 333.75 | 12.67 | 208.36 | 0.4355 | 1003.0 | 831.1 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -21.58 | 328.76 | 7.68 | 197.02 | 0.4263 | -907.0 | -732.8 | |
| 0.00 | 2.83 | 0.00 | 1.55 | -21.25 | 328.59 | 7.50 | 196.89 | 0.4206 | -851.0 | -699.8 | |
| 0.00 | 2.15 | 0.00 | 1.17 | -21.67 | 328.25 | 7.17 | 195.89 | 0.4254 | -875.0 | -698.3 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -23.21 | 328.14 | 7.06 | 194.65 | 0.4481 | -761.0 | -686.4 | |
| 0.00 | 0.77 | 0.00 | 0.43 | -23.30 | 327.95 | 6.87 | 194.22 | 0.4489 | -917.0 | -845.8 | |
| 1.55 | 3.09 | 0.86 | 1.72 | -23.96 | 327.95 | 6.87 | 193.84 | 0.4588 | -808.7 | -663.4 | |
| 0.00 | 5.07 | 0.00 | 2.82 | -24.06 | 327.66 | 6.58 | 193.22 | 0.4592 | -715.0 | -681.5 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -23.63 | 327.41 | 6.33 | 192.97 | 0.4518 | -1054.0 | -831.3 | |
| 0.00 | 1.72 | 0.00 | 0.98 | -26.68 | 327.31 | 6.22 | 191.28 | 0.4972 | -779.0 | -530.7 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -26.40 | 327.19 | 6.11 | 191.20 | 0.4928 | -757.0 | -584.2 | |
| 3.09 | 4.46 | 1.72 | 2.48 | -23.83 | 326.97 | 5.88 | 191.99 | 0.4533 | -1000.3 | -863.6 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -24.49 | 326.87 | 5.78 | 191.47 | 0.4631 | -790.0 | -656.3 | |
| 0.00 | 2.58 | 0.00 | 1.43 | -23.99 | 326.65 | 5.56 | 191.28 | 0.4548 | -851.0 | -812.7 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -28.66 | 326.68 | 5.59 | 189.41 | 0.5248 | -807.0 | -523.5 | |
| 0.00 | 1.46 | 0.00 | 0.81 | -24.39 | 326.44 | 5.35 | 190.68 | 0.4602 | -806.0 | -676.9 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -24.69 | 326.25 | 5.17 | 190.20 | 0.4643 | -672.0 | -518.8 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -24.62 | 326.05 | 4.97 | 189.84 | 0.4627 | -589.0 | -602.7 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -23.92 | 325.67 | 4.58 | 189.36 | 0.4510 | -885.0 | -748.5 | |
| 0.00 | 0.77 | 0.00 | 0.43 | -23.76 | 325.60 | 4.51 | 189.29 | 0.4483 | -599.0 | -571.6 | |
| 0.00 | 2.15 | 0.00 | 1.20 | -24.52 | 325.53 | 4.44 | 188.86 | 0.4598 | -799.0 | -699.0 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -23.19 | 325.06 | 3.98 | 188.40 | 0.4383 | -702.0 | -571.0 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -23.19 | 324.80 | 3.72 | 187.86 | 0.4377 | -839.0 | -602.5 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -25.78 | 323.99 | 2.91 | 185.52 | 0.4763 | -695.0 | -573.5 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -26.66 | 323.65 | 2.56 | 184.71 | 0.4892 | -616.0 | -530.7 | |
| 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. | |