SDO HMI 2011-11-29 08:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.95 | 370.91 | 40.48 | 195.38 | 20.05 | 192.37 | 4.73 | 346.07 | 0.3402 | -162.4 | -201.5 | |
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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 |
| 42.33 | 231.47 | 22.21 | 121.51 | 19.12 | 194.68 | 7.04 | 339.46 | 0.3314 | -1383.8 | -431.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 22.49 | 194.49 | 6.85 | 343.18 | 0.3822 | -761.0 | -611.9 | |
| 3.33 | 8.55 | 1.74 | 4.46 | 18.54 | 193.91 | 6.26 | 340.93 | 0.3180 | -1051.3 | -684.5 | |
| 0.00 | 2.31 | 0.00 | 1.20 | 18.29 | 193.58 | 5.94 | 341.58 | 0.3124 | -866.0 | -635.0 | |
| 0.00 | 1.71 | 0.00 | 0.91 | 21.10 | 193.66 | 6.01 | 344.03 | 0.3568 | -836.0 | -609.5 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 20.41 | 193.50 | 5.86 | 343.84 | 0.3453 | -710.0 | -507.2 | |
| 2.05 | 3.25 | 1.06 | 1.68 | 17.61 | 192.84 | 5.20 | 343.07 | 0.2979 | -925.3 | -811.4 | |
| 0.00 | 4.45 | 0.00 | 2.35 | 21.03 | 192.83 | 5.18 | 346.09 | 0.3523 | -644.0 | -722.0 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.75 | 192.78 | 5.14 | 345.21 | 0.3317 | -941.0 | -709.9 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.60 | 192.59 | 4.95 | 344.77 | 0.3125 | -869.0 | -652.2 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.69 | 192.56 | 4.92 | 345.77 | 0.3298 | -872.0 | -715.6 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 20.78 | 192.60 | 4.95 | 346.51 | 0.3474 | -914.0 | -763.6 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 20.94 | 192.47 | 4.83 | 346.94 | 0.3495 | -854.0 | -646.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 20.56 | 192.11 | 4.47 | 347.63 | 0.3421 | -834.0 | -578.9 | |
| 0.00 | 2.14 | 0.00 | 1.12 | 20.19 | 192.01 | 4.36 | 347.66 | 0.3357 | -1073.0 | -834.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 20.91 | 191.84 | 4.19 | 348.59 | 0.3468 | -656.0 | -557.1 | |
| 4.36 | 5.73 | 2.29 | 3.01 | 20.19 | 191.57 | 3.92 | 348.88 | 0.3343 | -1029.2 | -904.3 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 20.41 | 191.22 | 3.58 | 349.95 | 0.3368 | -688.0 | -555.7 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 20.22 | 190.49 | 2.85 | 351.88 | 0.3318 | -803.0 | -594.2 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.69 | 190.39 | 2.75 | 351.93 | 0.3229 | -929.0 | -686.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.72 | 190.23 | 2.59 | 352.40 | 0.3230 | -691.0 | -566.8 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 19.94 | 190.21 | 2.56 | 352.58 | 0.3266 | -690.0 | -579.9 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 17.37 | 189.33 | 1.69 | 354.27 | 0.2822 | -931.0 | -710.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.47 | 189.01 | 1.37 | 356.13 | 0.3334 | 799.0 | 645.2 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 20.79 | 188.76 | 1.12 | 356.89 | 0.3383 | 769.0 | 625.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 22.21 | 188.52 | 0.88 | 357.75 | 0.3614 | 881.0 | 725.6 | |
| 7.01 | 8.55 | 3.70 | 4.51 | 21.26 | 188.35 | 0.71 | 358.08 | 0.3458 | 1088.3 | 810.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.44 | 187.85 | 0.20 | 359.43 | 0.3321 | -983.0 | -806.2 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 20.98 | 187.72 | 0.08 | 359.79 | 0.3409 | 666.0 | 577.7 | |
| 0.00 | 1.80 | 0.00 | 0.95 | 21.67 | 187.69 | 0.04 | 359.88 | 0.3523 | 923.0 | 771.8 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 22.81 | 187.43 | -0.21 | 0.53 | 0.3710 | 914.0 | 711.9 | |
| 3.42 | 10.60 | 1.81 | 5.61 | 21.73 | 187.34 | -0.31 | 0.81 | 0.3534 | 1159.2 | 909.0 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 22.52 | 187.34 | -0.31 | 0.78 | 0.3664 | 461.0 | 493.5 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 21.07 | 187.31 | -0.34 | 0.92 | 0.3425 | 836.0 | 640.7 | |
| 0.00 | 11.54 | 0.00 | 6.13 | 22.21 | 187.24 | -0.40 | 1.04 | 0.3612 | 903.0 | 796.2 | |
| 1.54 | -32.00 | 0.81 | -32.00 | 21.64 | 187.08 | -0.56 | 1.49 | 0.3519 | 984.4 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 24.86 | 186.91 | -0.74 | 1.66 | 0.4043 | 864.0 | 628.9 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 21.13 | 186.90 | -0.75 | 2.04 | 0.3437 | 904.0 | 703.1 | |
| 12.91 | 16.67 | 6.86 | 8.86 | 22.30 | 186.79 | -0.85 | 2.18 | 0.3630 | 1006.4 | 755.7 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 24.86 | 186.52 | -1.13 | 2.54 | 0.4046 | 892.0 | 754.2 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 21.92 | 186.45 | -1.20 | 3.13 | 0.3570 | 817.0 | 723.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 21.45 | 186.39 | -1.26 | 3.37 | 0.3493 | 1071.0 | 900.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 21.48 | 186.23 | -1.42 | 3.79 | 0.3500 | 849.0 | 700.9 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 22.43 | 186.22 | -1.43 | 3.63 | 0.3655 | 790.0 | 625.0 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 22.62 | 186.02 | -1.62 | 4.08 | 0.3688 | 1026.0 | 899.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 22.65 | 185.67 | -1.97 | 4.95 | 0.3698 | 854.0 | 645.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 20.63 | 185.70 | -1.95 | 5.44 | 0.3368 | 835.0 | 630.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.82 | 185.66 | -1.98 | 5.48 | 0.3399 | 722.0 | 644.6 | |
| 0.00 | 2.39 | 0.00 | 1.30 | 25.64 | 185.56 | -2.09 | 4.52 | 0.4179 | 551.0 | 590.8 | |
| 0.00 | 2.48 | 0.00 | 1.33 | 23.26 | 185.53 | -2.11 | 5.14 | 0.3798 | 766.0 | 652.5 | |
| 0.00 | 2.05 | 0.00 | 1.10 | 23.03 | 185.41 | -2.24 | 5.50 | 0.3764 | 890.0 | 773.1 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 25.84 | 185.29 | -2.35 | 5.05 | 0.4214 | 459.0 | 413.8 | |
| 0.00 | 1.71 | 0.00 | 0.92 | 23.29 | 184.92 | -2.72 | 6.60 | 0.3813 | 828.0 | 682.0 | |
| 0.00 | 4.36 | 0.00 | 2.37 | 25.22 | 184.71 | -2.93 | 6.46 | 0.4125 | 837.0 | 727.1 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 24.38 | 184.67 | -2.97 | 6.83 | 0.3992 | 835.0 | 672.1 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 22.43 | 184.10 | -3.54 | 8.93 | 0.3693 | 718.0 | 611.1 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 22.14 | 183.60 | -4.04 | 10.33 | 0.3660 | 661.0 | 530.4 | |
| 0.00 | 2.22 | 0.00 | 1.21 | 25.57 | 182.90 | -4.75 | 10.22 | 0.4223 | 609.0 | 453.7 | |
| 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. | |