SDO HMI 2014-07-07 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.05 | 352.67 | 28.23 | 190.16 | 14.84 | 260.32 | 20.10 | 301.74 | 0.3913 | -374.8 | -285.8 | |
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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 | 1.63 | 0.00 | 0.93 | 15.99 | 267.40 | 27.19 | 296.87 | 0.4944 | -809.0 | -654.1 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 12.56 | 266.57 | 26.35 | 290.67 | 0.4650 | -750.0 | -590.6 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 16.53 | 266.91 | 26.70 | 298.26 | 0.4910 | -762.0 | -571.0 | |
| 0.00 | 2.00 | 0.00 | 1.10 | 14.39 | 263.97 | 23.76 | 296.41 | 0.4375 | -757.0 | -662.0 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 12.78 | 262.71 | 22.50 | 293.94 | 0.4100 | -672.0 | -555.2 | |
| 3.00 | 4.54 | 1.61 | 2.43 | 8.86 | 262.13 | 21.92 | 284.82 | 0.3831 | -971.5 | -756.7 | |
| 0.00 | 3.81 | 0.00 | 2.07 | 12.76 | 262.43 | 22.22 | 294.11 | 0.4058 | -1035.0 | -778.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 12.46 | 261.73 | 21.52 | 294.04 | 0.3939 | -813.0 | -652.0 | |
| 0.00 | 2.45 | 0.00 | 1.32 | 12.90 | 261.61 | 21.39 | 295.19 | 0.3946 | -857.0 | -751.7 | |
| 44.05 | 256.58 | 23.93 | 139.40 | 15.19 | 261.73 | 21.52 | 300.27 | 0.4116 | -1321.2 | -417.2 | |
| 0.00 | 0.73 | 0.00 | 0.40 | 17.32 | 261.78 | 21.57 | 304.68 | 0.4285 | 691.0 | 536.5 | |
| 2.18 | -10.00 | 1.18 | -10.00 | 14.64 | 261.44 | 21.23 | 299.36 | 0.4036 | -819.0 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 12.66 | 261.18 | 20.97 | 295.02 | 0.3870 | -876.0 | -681.3 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 13.10 | 261.12 | 20.91 | 296.12 | 0.3888 | -729.0 | -613.6 | |
| 0.27 | -10.00 | 0.15 | -10.00 | 15.36 | 261.21 | 21.00 | 301.20 | 0.4057 | -1260.0 | 999999 | |
| 0.00 | 2.27 | 0.00 | 1.22 | 12.49 | 260.80 | 20.59 | 294.96 | 0.3803 | -998.0 | -788.9 | |
| 0.91 | -10.00 | 0.49 | -10.00 | 14.84 | 260.99 | 20.77 | 300.29 | 0.3987 | -1054.2 | 999999 | |
| 0.91 | -10.00 | 0.49 | -10.00 | 14.69 | 260.70 | 20.49 | 300.27 | 0.3937 | -1056.7 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 13.51 | 260.45 | 20.24 | 297.80 | 0.3819 | -817.0 | -705.2 | |
| 0.00 | 2.91 | 0.00 | 1.55 | 13.42 | 260.28 | 20.07 | 297.77 | 0.3788 | -953.0 | -731.4 | |
| 0.00 | 2.09 | 0.00 | 1.12 | 13.49 | 260.02 | 19.81 | 298.22 | 0.3756 | -668.0 | -680.7 | |
| 0.00 | 3.18 | 0.00 | 1.72 | 16.01 | 260.23 | 20.02 | 303.76 | 0.3975 | -207.0 | -79.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 9.20 | 259.12 | 18.90 | 287.75 | 0.3373 | 840.0 | 595.6 | |
| 0.00 | 2.72 | 0.00 | 1.45 | 14.50 | 259.34 | 19.13 | 301.43 | 0.3734 | -854.0 | -712.4 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 14.94 | 259.22 | 19.01 | 302.61 | 0.3751 | -766.0 | -691.3 | |
| 0.00 | 3.91 | 0.00 | 2.08 | 14.07 | 259.01 | 18.79 | 300.82 | 0.3654 | -832.0 | -708.8 | |
| 0.00 | 5.18 | 0.00 | 2.75 | 13.77 | 258.75 | 18.54 | 300.40 | 0.3595 | -907.0 | -733.9 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 13.50 | 258.33 | 18.12 | 300.25 | 0.3515 | -757.0 | -620.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 14.06 | 257.98 | 17.77 | 302.13 | 0.3511 | 570.0 | 437.0 | |
| 0.73 | 3.36 | 0.38 | 1.77 | 14.26 | 257.57 | 17.35 | 303.19 | 0.3469 | 810.1 | 567.2 | |
| 0.00 | 1.91 | 0.00 | 1.02 | 17.91 | 257.47 | 17.26 | 311.69 | 0.3796 | 816.0 | 692.0 | |
| 0.00 | 1.91 | 0.00 | 1.02 | 17.73 | 257.38 | 17.17 | 311.43 | 0.3767 | 855.0 | 701.0 | |
| 0.00 | 2.09 | 0.00 | 1.10 | 14.58 | 256.93 | 16.72 | 304.93 | 0.3411 | 820.0 | 616.9 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 10.17 | 252.80 | 12.59 | 298.69 | 0.2456 | 858.0 | 659.1 | |
| 0.00 | 2.09 | 0.00 | 1.07 | 10.82 | 252.64 | 12.42 | 301.32 | 0.2485 | 781.0 | 529.7 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 11.47 | 252.25 | 12.04 | 304.36 | 0.2487 | 882.0 | 694.3 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 18.37 | 252.60 | 12.38 | 321.71 | 0.3299 | 627.0 | 456.6 | |
| 0.00 | 2.72 | 0.00 | 1.40 | 13.60 | 252.23 | 12.02 | 311.09 | 0.2697 | 919.0 | 730.0 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 10.40 | 251.38 | 11.17 | 302.44 | 0.2268 | 785.0 | 589.4 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 13.48 | 251.49 | 11.27 | 312.52 | 0.2591 | 865.0 | 761.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 13.21 | 251.41 | 11.20 | 311.89 | 0.2551 | 1005.0 | 791.3 | |
| 0.00 | 2.09 | 0.00 | 1.07 | 12.93 | 251.36 | 11.15 | 311.15 | 0.2515 | 832.0 | 623.4 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 13.39 | 251.29 | 11.08 | 312.74 | 0.2556 | 1016.0 | 814.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 13.74 | 250.99 | 10.78 | 314.52 | 0.2558 | 903.0 | 706.9 | |
| 0.00 | 2.54 | 0.00 | 1.30 | 14.05 | 250.75 | 10.53 | 316.04 | 0.2566 | 757.0 | 701.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 14.27 | 250.66 | 10.45 | 316.87 | 0.2583 | 929.0 | 683.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 14.64 | 250.52 | 10.31 | 318.26 | 0.2612 | 943.0 | 800.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 14.99 | 250.41 | 10.20 | 319.45 | 0.2642 | 821.0 | 695.4 | |
| 0.00 | 2.91 | 0.00 | 1.49 | 14.68 | 250.14 | 9.93 | 319.40 | 0.2574 | 706.0 | 612.3 | |
| 0.00 | 2.45 | 0.00 | 1.27 | 16.71 | 249.82 | 9.61 | 325.10 | 0.2806 | 938.0 | 686.0 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 17.18 | 249.49 | 9.28 | 326.99 | 0.2840 | 889.0 | 783.9 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.34 | 249.43 | 9.22 | 327.46 | 0.2857 | 686.0 | 568.3 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 14.80 | 246.99 | 6.78 | 329.82 | 0.2280 | 866.0 | 753.4 | |
| 0.00 | 2.63 | 0.00 | 1.38 | 21.08 | 245.96 | 5.75 | 342.80 | 0.3176 | 924.0 | 771.8 | |
| 0.00 | 2.00 | 0.00 | 1.02 | 16.36 | 242.07 | 1.86 | 352.02 | 0.2256 | 846.0 | 719.8 | |
| 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. | |