SDO HMI 2014-07-07 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.95 | 357.63 | 26.98 | 192.22 | 14.94 | 260.33 | 19.57 | 302.63 | 0.3849 | -381.2 | -267.7 | |
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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 | 0.73 | 0.00 | 0.41 | 15.93 | 267.41 | 26.65 | 297.18 | 0.4867 | -654.0 | -633.6 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 12.60 | 266.56 | 25.80 | 291.11 | 0.4572 | -729.0 | -608.0 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 16.54 | 266.89 | 26.13 | 298.74 | 0.4835 | -753.0 | -606.3 | |
| 0.00 | 1.91 | 0.00 | 1.08 | 17.85 | 266.17 | 25.41 | 301.82 | 0.4826 | -554.0 | -436.2 | |
| 0.00 | 1.73 | 0.00 | 0.95 | 12.95 | 264.84 | 24.08 | 293.07 | 0.4340 | -790.0 | -686.8 | |
| 0.00 | 2.00 | 0.00 | 1.09 | 14.37 | 263.93 | 23.17 | 296.89 | 0.4291 | -737.0 | -548.5 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 12.82 | 262.69 | 21.92 | 294.53 | 0.4019 | -734.0 | -629.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 13.10 | 262.51 | 21.75 | 295.35 | 0.4010 | -703.0 | -546.7 | |
| 0.00 | 1.91 | 0.00 | 1.03 | 12.73 | 262.41 | 21.65 | 294.58 | 0.3973 | -966.0 | -858.2 | |
| 3.09 | 5.36 | 1.65 | 2.86 | 8.87 | 262.05 | 21.28 | 285.22 | 0.3733 | -941.1 | -655.8 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 11.35 | 262.06 | 21.29 | 291.56 | 0.3845 | -819.0 | -579.8 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 12.94 | 261.62 | 20.86 | 295.80 | 0.3871 | -871.0 | -748.6 | |
| 42.50 | 260.92 | 23.00 | 141.25 | 15.20 | 261.71 | 20.95 | 300.92 | 0.4038 | -1337.8 | -424.8 | |
| 2.00 | -13.00 | 1.08 | -13.00 | 14.65 | 261.41 | 20.65 | 300.00 | 0.3957 | -852.7 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 17.14 | 261.69 | 20.93 | 305.07 | 0.4188 | 441.0 | 364.9 | |
| 0.00 | 2.45 | 0.00 | 1.31 | 12.70 | 261.13 | 20.37 | 295.71 | 0.3785 | -808.0 | -658.5 | |
| 0.45 | -13.00 | 0.24 | -13.00 | 14.81 | 261.03 | 20.27 | 300.81 | 0.3916 | -1040.6 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 12.52 | 260.79 | 20.02 | 295.63 | 0.3723 | -946.0 | -826.7 | |
| 1.18 | -13.00 | 0.63 | -13.00 | 14.69 | 260.78 | 20.02 | 300.83 | 0.3872 | -1002.6 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 16.88 | 260.87 | 20.11 | 305.51 | 0.4060 | -779.0 | -578.1 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 13.52 | 260.41 | 19.64 | 298.49 | 0.3735 | -824.0 | -750.2 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 16.16 | 260.56 | 19.80 | 304.38 | 0.3959 | -651.0 | -609.0 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 13.56 | 260.04 | 19.28 | 299.00 | 0.3686 | -775.0 | -664.1 | |
| 0.00 | 6.90 | 0.00 | 3.71 | 16.11 | 260.25 | 19.49 | 304.65 | 0.3913 | -203.0 | -179.6 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 9.20 | 259.14 | 18.38 | 288.21 | 0.3291 | 812.0 | 592.2 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 14.41 | 259.42 | 18.66 | 301.83 | 0.3662 | -748.0 | -617.7 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 14.44 | 259.26 | 18.49 | 302.12 | 0.3642 | -845.0 | -752.2 | |
| 0.00 | 2.82 | 0.00 | 1.49 | 14.02 | 258.92 | 18.16 | 301.51 | 0.3562 | -946.0 | -759.0 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 13.77 | 258.70 | 17.94 | 301.19 | 0.3512 | -943.0 | -784.2 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 16.29 | 258.69 | 17.93 | 307.19 | 0.3725 | 666.0 | 458.9 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 13.53 | 258.35 | 17.59 | 301.05 | 0.3445 | -880.0 | -725.8 | |
| 0.73 | 3.27 | 0.38 | 1.72 | 14.26 | 257.56 | 16.79 | 304.03 | 0.3394 | 805.6 | 574.2 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 17.63 | 257.49 | 16.73 | 311.96 | 0.3704 | 838.0 | 706.8 | |
| 0.00 | 1.73 | 0.00 | 0.92 | 17.89 | 257.48 | 16.72 | 312.50 | 0.3729 | 804.0 | 768.3 | |
| 0.00 | 3.54 | 0.00 | 1.86 | 14.58 | 256.86 | 16.10 | 305.93 | 0.3328 | 636.0 | 588.2 | |
| 0.00 | 1.82 | 0.00 | 0.97 | 17.84 | 256.67 | 15.91 | 313.75 | 0.3628 | 818.0 | 596.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 12.76 | 254.85 | 14.09 | 304.40 | 0.2890 | 707.0 | 620.9 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 10.79 | 252.61 | 11.85 | 302.40 | 0.2400 | 792.0 | 551.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 11.47 | 252.26 | 11.50 | 305.58 | 0.2413 | 873.0 | 703.8 | |
| 0.00 | 3.63 | 0.00 | 1.86 | 13.60 | 252.23 | 11.47 | 312.39 | 0.2629 | 950.0 | 726.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.00 | 251.98 | 11.22 | 319.30 | 0.2880 | 317.0 | 340.8 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 13.64 | 251.76 | 10.99 | 313.68 | 0.2574 | 749.0 | 607.6 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 13.45 | 251.49 | 10.73 | 313.83 | 0.2521 | 901.0 | 788.5 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 13.39 | 251.27 | 10.50 | 314.25 | 0.2487 | 986.0 | 834.0 | |
| 0.00 | 3.81 | 0.00 | 1.94 | 11.97 | 251.21 | 10.44 | 309.90 | 0.2322 | 877.0 | 528.0 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 12.96 | 251.06 | 10.29 | 313.51 | 0.2412 | 892.0 | 647.7 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 13.98 | 251.10 | 10.34 | 316.39 | 0.2537 | 664.0 | 555.0 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 13.77 | 250.96 | 10.20 | 316.16 | 0.2495 | 907.0 | 772.3 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 14.27 | 250.64 | 9.87 | 318.47 | 0.2518 | 881.0 | 677.9 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 14.61 | 250.52 | 9.76 | 319.70 | 0.2548 | 921.0 | 823.0 | |
| 0.00 | 3.81 | 0.00 | 1.96 | 15.36 | 250.21 | 9.45 | 322.51 | 0.2611 | 822.0 | 646.0 | |
| 0.00 | 2.72 | 0.00 | 1.40 | 16.71 | 249.82 | 9.06 | 326.65 | 0.2756 | 815.0 | 664.1 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 17.15 | 249.49 | 8.73 | 328.50 | 0.2787 | 947.0 | 742.8 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 14.80 | 246.94 | 6.17 | 332.08 | 0.2231 | 848.0 | 740.8 | |
| 0.00 | 3.45 | 0.00 | 1.80 | 21.07 | 245.99 | 5.23 | 344.29 | 0.3152 | 958.0 | 746.0 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 19.24 | 244.79 | 4.03 | 346.26 | 0.2805 | 785.0 | 628.2 | |
| 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. | |