SDO HMI 2014-08-18 02:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.47 | 268.66 | 27.49 | 137.63 | 14.29 | 57.15 | 12.48 | 303.33 | 0.2533 | -385.9 | -231.5 | |
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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 |
| 0.00 | 0.81 | 0.00 | 0.44 | 21.98 | 63.30 | 18.63 | 312.13 | 0.4011 | -623.0 | -532.4 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 24.21 | 63.03 | 18.36 | 316.72 | 0.4207 | -677.0 | -565.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 9.59 | 60.72 | 16.05 | 281.09 | 0.2790 | -909.0 | -727.4 | |
| 5.76 | 24.40 | 2.99 | 12.64 | 13.93 | 60.34 | 15.67 | 296.14 | 0.2932 | -946.9 | -489.3 | |
| 0.00 | 1.44 | 0.00 | 0.75 | 16.23 | 60.45 | 15.78 | 302.82 | 0.3120 | -775.0 | -608.7 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 11.34 | 60.05 | 15.37 | 287.84 | 0.2742 | -791.0 | -665.0 | |
| 2.16 | -4.00 | 1.12 | -4.00 | 13.81 | 60.14 | 15.46 | 296.04 | 0.2894 | -1094.4 | 999999 | |
| 4.14 | -4.00 | 2.14 | -4.00 | 14.09 | 60.12 | 15.45 | 296.94 | 0.2911 | -998.7 | 999999 | |
| 4.23 | -4.00 | 2.19 | -4.00 | 13.97 | 60.08 | 15.41 | 296.61 | 0.2897 | -1282.2 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 11.71 | 59.94 | 15.26 | 289.24 | 0.2743 | -794.0 | -548.5 | |
| 0.00 | 1.98 | 0.00 | 1.02 | 11.88 | 59.37 | 14.70 | 290.46 | 0.2662 | -935.0 | -780.1 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 10.37 | 59.13 | 14.46 | 285.08 | 0.2555 | -945.0 | -737.7 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 11.73 | 59.20 | 14.53 | 290.12 | 0.2628 | -1012.0 | -912.5 | |
| 0.00 | 2.25 | 0.00 | 1.16 | 12.04 | 59.15 | 14.48 | 291.29 | 0.2636 | -982.0 | -840.7 | |
| 0.00 | 4.05 | 0.00 | 2.08 | 12.44 | 59.11 | 14.44 | 292.76 | 0.2653 | -792.0 | -587.6 | |
| 0.99 | 3.96 | 0.51 | 2.03 | 11.89 | 59.02 | 14.35 | 290.91 | 0.2607 | -1177.5 | -894.1 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 10.16 | 58.87 | 14.19 | 284.51 | 0.2504 | -920.0 | -704.0 | |
| 0.00 | 6.12 | 0.00 | 3.24 | 21.26 | 59.60 | 14.92 | 316.58 | 0.3507 | -11.0 | -4.1 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 15.90 | 59.05 | 14.38 | 304.15 | 0.2899 | -671.0 | -534.2 | |
| 0.00 | 3.15 | 0.00 | 1.63 | 16.73 | 58.20 | 13.53 | 308.13 | 0.2860 | -675.0 | -643.0 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 17.56 | 58.26 | 13.59 | 310.32 | 0.2951 | -646.0 | -534.0 | |
| 0.00 | 1.53 | 0.00 | 0.78 | 8.61 | 57.69 | 13.02 | 278.92 | 0.2265 | -833.0 | -656.4 | |
| 0.00 | 3.15 | 0.00 | 1.63 | 17.01 | 58.09 | 13.42 | 309.14 | 0.2874 | -1070.0 | -847.6 | |
| 20.17 | 137.60 | 10.33 | 70.43 | 13.85 | 57.85 | 13.18 | 299.66 | 0.2558 | -1242.4 | -492.7 | |
| 5.94 | -24.00 | 3.04 | -24.00 | 13.54 | 57.83 | 13.16 | 298.62 | 0.2532 | -1293.8 | 999999 | |
| 8.28 | -24.00 | 4.25 | -24.00 | 14.22 | 57.68 | 13.00 | 301.25 | 0.2563 | -1001.8 | 999999 | |
| 1.80 | 4.50 | 0.92 | 2.31 | 14.93 | 57.69 | 13.02 | 303.60 | 0.2624 | -841.8 | -694.7 | |
| 0.00 | 1.26 | 0.00 | 0.65 | 16.74 | 57.81 | 13.14 | 308.93 | 0.2810 | -772.0 | -645.0 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 14.81 | 57.36 | 12.69 | 303.86 | 0.2568 | -934.0 | -794.9 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 12.13 | 56.99 | 12.32 | 294.69 | 0.2306 | -843.0 | -679.2 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 15.04 | 57.05 | 12.38 | 305.22 | 0.2546 | -727.0 | -481.9 | |
| 0.00 | 18.19 | 0.00 | 9.26 | 13.43 | 56.32 | 11.65 | 301.02 | 0.2302 | 774.0 | 332.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 12.67 | 56.13 | 11.45 | 298.43 | 0.2213 | 887.0 | 731.1 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 13.59 | 55.98 | 11.31 | 302.36 | 0.2266 | 779.0 | 652.4 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 11.57 | 54.85 | 10.17 | 296.24 | 0.1938 | 707.0 | 544.9 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 12.92 | 54.68 | 10.01 | 302.67 | 0.2021 | -396.0 | -365.2 | |
| 0.00 | 3.60 | 0.00 | 1.82 | 14.80 | 52.22 | 7.55 | 317.86 | 0.1902 | 600.0 | 584.0 | |
| 0.00 | 2.52 | 0.00 | 1.27 | 14.44 | 52.02 | 7.35 | 317.27 | 0.1834 | 788.0 | 743.0 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 15.48 | 51.93 | 7.26 | 321.32 | 0.1957 | 724.0 | 541.6 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 14.62 | 51.74 | 7.07 | 319.05 | 0.1826 | 1041.0 | 926.1 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 15.43 | 51.45 | 6.78 | 323.00 | 0.1900 | 861.0 | 686.4 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 15.06 | 51.32 | 6.64 | 322.33 | 0.1836 | 927.0 | 782.2 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 16.17 | 51.10 | 6.43 | 326.72 | 0.1968 | 838.0 | 646.5 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 15.28 | 50.69 | 6.02 | 325.73 | 0.1804 | 895.0 | 726.3 | |
| 0.00 | 2.70 | 0.00 | 1.36 | 15.01 | 50.59 | 5.91 | 325.28 | 0.1755 | 876.0 | 753.2 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 14.00 | 50.53 | 5.85 | 321.89 | 0.1611 | 852.0 | 679.8 | |
| 0.00 | 1.44 | 0.00 | 0.72 | 14.98 | 50.33 | 5.66 | 326.35 | 0.1727 | 958.0 | 747.9 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 16.15 | 50.37 | 5.69 | 329.72 | 0.1899 | 674.0 | 546.2 | |
| 0.00 | 2.97 | 0.00 | 1.50 | 16.00 | 50.14 | 5.47 | 330.30 | 0.1857 | 1035.0 | 796.8 | |
| 0.00 | 2.34 | 0.00 | 1.19 | 17.51 | 50.16 | 5.48 | 333.97 | 0.2085 | 937.0 | 809.4 | |
| 0.00 | 2.61 | 0.00 | 1.32 | 17.26 | 50.15 | 5.47 | 333.45 | 0.2047 | 854.0 | 717.7 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 17.75 | 50.07 | 5.39 | 334.86 | 0.2117 | 740.0 | 611.7 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 15.91 | 49.63 | 4.96 | 332.40 | 0.1803 | 901.0 | 720.1 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 17.92 | 49.27 | 4.60 | 338.48 | 0.2089 | 921.0 | 818.9 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 17.90 | 47.83 | 3.16 | 344.79 | 0.2009 | 870.0 | 713.7 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 18.62 | 45.41 | 0.74 | 356.59 | 0.2065 | 949.0 | 688.3 | |
| 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. | |