SDO HMI 2011-11-30 20:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.30 | 304.98 | 25.13 | 176.91 | 20.18 | 192.87 | 25.01 | 310.10 | 0.5212 | -243.8 | -223.7 | |
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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 | 0.94 | 0.00 | 0.56 | 20.69 | 196.70 | 28.84 | 306.95 | 0.5668 | -279.0 | -307.8 | |
| 33.91 | 230.79 | 19.84 | 135.04 | 19.55 | 194.66 | 26.80 | 307.01 | 0.5342 | -1199.9 | -391.3 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 22.29 | 194.38 | 26.51 | 311.48 | 0.5535 | -538.0 | -478.3 | |
| 0.00 | 1.62 | 0.00 | 0.97 | 22.64 | 194.38 | 26.51 | 311.99 | 0.5565 | -703.0 | -592.5 | |
| 0.00 | 1.96 | 0.00 | 1.13 | 19.18 | 192.79 | 24.92 | 308.28 | 0.5091 | -792.0 | -668.5 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 17.39 | 192.48 | 24.61 | 305.56 | 0.4906 | -734.0 | -533.7 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 21.85 | 192.98 | 25.11 | 312.26 | 0.5344 | -644.0 | -560.8 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 19.98 | 191.16 | 23.29 | 311.34 | 0.4970 | -763.0 | -652.5 | |
| 0.00 | 1.62 | 0.00 | 0.93 | 20.20 | 190.99 | 23.12 | 311.89 | 0.4971 | -921.0 | -718.5 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 20.35 | 190.88 | 23.01 | 312.27 | 0.4973 | -722.0 | -647.1 | |
| 0.00 | 1.79 | 0.00 | 1.03 | 21.17 | 190.97 | 23.11 | 313.44 | 0.5061 | -825.0 | -696.3 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 20.60 | 190.85 | 22.98 | 312.70 | 0.4994 | -839.0 | -650.4 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 17.50 | 189.96 | 22.10 | 308.53 | 0.4605 | -819.0 | -644.2 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 15.48 | 189.09 | 21.23 | 305.79 | 0.4320 | -754.0 | -624.6 | |
| 0.00 | 2.73 | 0.00 | 1.49 | 14.99 | 188.74 | 20.88 | 305.25 | 0.4234 | -936.0 | -770.4 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 21.12 | 188.57 | 20.71 | 316.33 | 0.4797 | 695.0 | 536.5 | |
| 1.02 | 2.56 | 0.58 | 1.45 | 22.23 | 187.75 | 19.89 | 319.10 | 0.4830 | 801.2 | 755.8 | |
| 5.21 | 6.58 | 2.93 | 3.69 | 22.27 | 186.71 | 18.84 | 320.61 | 0.4730 | 839.9 | 649.1 | |
| 2.65 | 3.33 | 1.49 | 1.87 | 22.59 | 186.25 | 18.38 | 321.74 | 0.4722 | 793.5 | 556.8 | |
| 0.00 | 2.56 | 0.00 | 1.44 | 22.72 | 185.96 | 18.10 | 322.34 | 0.4710 | 632.0 | 618.3 | |
| 0.00 | 1.96 | 0.00 | 1.10 | 22.27 | 185.83 | 17.97 | 321.90 | 0.4646 | 747.0 | 655.0 | |
| 0.00 | 3.67 | 0.00 | 2.05 | 22.50 | 185.73 | 17.87 | 322.37 | 0.4662 | 842.0 | 764.6 | |
| 0.51 | 4.53 | 0.29 | 2.53 | 22.82 | 185.17 | 17.30 | 323.67 | 0.4647 | 967.5 | 838.0 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 24.29 | 185.37 | 17.50 | 325.34 | 0.4841 | 573.0 | 428.5 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 23.39 | 185.04 | 17.18 | 324.65 | 0.4705 | 809.0 | 648.9 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 19.60 | 184.52 | 16.65 | 319.86 | 0.4206 | 848.0 | 683.1 | |
| 0.00 | 1.96 | 0.00 | 1.13 | 26.50 | 185.32 | 17.46 | 328.12 | 0.5105 | 830.0 | 712.4 | |
| 0.00 | 2.48 | 0.00 | 1.38 | 22.98 | 184.82 | 16.95 | 324.43 | 0.4635 | 916.0 | 836.2 | |
| 0.00 | 2.99 | 0.00 | 1.68 | 23.59 | 184.83 | 16.97 | 325.23 | 0.4709 | 870.0 | 707.8 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 23.36 | 184.70 | 16.84 | 325.13 | 0.4670 | 796.0 | 685.4 | |
| 0.00 | 2.14 | 0.00 | 1.22 | 25.95 | 184.96 | 17.10 | 327.99 | 0.5008 | 803.0 | 701.8 | |
| 0.00 | 4.01 | 0.00 | 2.29 | 25.72 | 184.89 | 17.03 | 327.82 | 0.4974 | 939.0 | 778.1 | |
| 0.00 | 2.65 | 0.00 | 1.48 | 22.98 | 184.52 | 16.65 | 324.90 | 0.4608 | 956.0 | 761.2 | |
| 0.00 | 3.67 | 0.00 | 2.06 | 23.84 | 184.33 | 16.46 | 326.35 | 0.4697 | 828.0 | 754.4 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 23.27 | 184.22 | 16.35 | 325.76 | 0.4617 | 756.0 | 657.7 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 25.43 | 184.30 | 16.44 | 328.35 | 0.4891 | 809.0 | 664.5 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 20.96 | 182.86 | 15.00 | 324.79 | 0.4208 | 901.0 | 620.2 | |
| 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. | |