SDO HMI 2014-08-09 08:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.17 | 104.51 | 0.60 | 53.70 | 9.39 | 175.41 | 15.05 | 283.02 | 0.2642 | 109.9 | 82.9 | |
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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 | 1.54 | 0.00 | 0.84 | 10.26 | 185.54 | 25.18 | 280.69 | 0.4278 | -687.0 | -582.2 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 5.42 | 184.31 | 23.95 | 269.10 | 0.4059 | -805.0 | -655.5 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 6.69 | 182.97 | 22.61 | 272.23 | 0.3838 | -864.0 | -630.1 | |
| 0.00 | 2.62 | 0.00 | 1.40 | 6.74 | 182.58 | 22.22 | 272.35 | 0.3774 | -1045.0 | -884.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 10.91 | 181.88 | 21.52 | 283.67 | 0.3723 | -843.0 | -642.7 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 11.44 | 181.69 | 21.33 | 285.16 | 0.3709 | -794.0 | -714.3 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 9.01 | 180.00 | 19.64 | 279.09 | 0.3377 | -802.0 | -627.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 9.38 | 179.83 | 19.47 | 280.26 | 0.3356 | -1062.0 | -864.9 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 8.41 | 179.58 | 19.22 | 277.44 | 0.3298 | -816.0 | -572.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 9.36 | 179.60 | 19.24 | 280.28 | 0.3319 | -761.0 | -586.7 | |
| 0.00 | 2.44 | 0.00 | 1.28 | 9.74 | 179.07 | 18.71 | 281.68 | 0.3242 | -655.0 | -649.1 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 8.86 | 179.02 | 18.66 | 278.98 | 0.3214 | -832.0 | -713.9 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 8.81 | 178.72 | 18.36 | 278.93 | 0.3165 | -796.0 | -626.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 11.86 | 178.85 | 18.49 | 288.19 | 0.3281 | -854.0 | -674.1 | |
| 0.00 | 3.61 | 0.00 | 1.89 | 12.11 | 178.57 | 18.21 | 289.17 | 0.3249 | -444.0 | -532.2 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 10.20 | 178.18 | 17.82 | 283.58 | 0.3113 | -899.0 | -735.2 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 8.47 | 177.99 | 17.63 | 278.08 | 0.3040 | -845.0 | -709.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 8.50 | 177.09 | 16.73 | 278.50 | 0.2892 | -965.0 | -866.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 8.63 | 176.94 | 16.58 | 279.00 | 0.2869 | -865.0 | -714.0 | |
| 0.00 | 3.16 | 0.00 | 1.63 | 8.73 | 176.66 | 16.30 | 279.48 | 0.2824 | -766.0 | -684.5 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 8.89 | 176.38 | 16.01 | 280.18 | 0.2782 | -513.0 | -508.1 | |
| 0.00 | 6.23 | 0.00 | 3.21 | 8.64 | 176.33 | 15.97 | 279.33 | 0.2769 | -993.0 | -875.0 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 13.74 | 176.40 | 16.04 | 296.41 | 0.3010 | -571.0 | -449.1 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 9.05 | 176.09 | 15.73 | 280.91 | 0.2739 | -785.0 | -557.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 13.57 | 176.07 | 15.70 | 296.31 | 0.2948 | -711.0 | -570.4 | |
| 0.00 | 2.98 | 0.00 | 1.53 | 11.63 | 175.33 | 14.97 | 290.82 | 0.2719 | 555.0 | 555.0 | |
| 0.00 | 1.81 | 0.00 | 0.93 | 9.44 | 175.19 | 14.83 | 282.94 | 0.2601 | -972.0 | -832.8 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 9.86 | 174.35 | 13.99 | 285.25 | 0.2479 | 751.0 | 635.1 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 9.59 | 174.30 | 13.94 | 284.20 | 0.2461 | 595.0 | 429.5 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 9.75 | 173.96 | 13.60 | 285.16 | 0.2412 | 839.0 | 762.5 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 9.48 | 173.88 | 13.52 | 284.12 | 0.2389 | 718.0 | 634.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 9.84 | 173.81 | 13.44 | 285.70 | 0.2390 | 815.0 | 697.8 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 8.45 | 173.66 | 13.29 | 279.97 | 0.2320 | 638.0 | 505.5 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 8.54 | 173.50 | 13.14 | 280.48 | 0.2296 | 812.0 | 613.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 9.09 | 173.49 | 13.13 | 282.84 | 0.2311 | 663.0 | 613.1 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 10.25 | 173.51 | 13.14 | 287.67 | 0.2359 | 918.0 | 730.1 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 8.37 | 173.27 | 12.91 | 279.85 | 0.2254 | 774.0 | 644.9 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 9.37 | 173.15 | 12.79 | 284.36 | 0.2265 | 944.0 | 810.8 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 10.23 | 173.12 | 12.76 | 288.03 | 0.2297 | 655.0 | 506.6 | |
| 0.00 | 2.26 | 0.00 | 1.15 | 9.29 | 173.05 | 12.69 | 284.06 | 0.2246 | 992.0 | 827.2 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 9.63 | 172.82 | 12.45 | 285.80 | 0.2220 | 678.0 | 549.0 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 10.39 | 172.78 | 12.42 | 289.14 | 0.2250 | 859.0 | 641.1 | |
| 0.00 | 7.05 | 0.00 | 3.58 | 8.65 | 172.72 | 12.36 | 281.54 | 0.2169 | 981.0 | 764.5 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 8.11 | 172.57 | 12.21 | 279.13 | 0.2130 | 687.0 | 601.7 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 10.45 | 172.56 | 12.20 | 289.71 | 0.2218 | 935.0 | 738.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 8.23 | 172.48 | 12.12 | 279.76 | 0.2118 | 964.0 | 808.8 | |
| 0.00 | 1.90 | 0.00 | 0.96 | 8.39 | 172.46 | 12.10 | 280.50 | 0.2118 | 863.0 | 746.6 | |
| 0.00 | 3.89 | 0.00 | 1.97 | 8.69 | 172.37 | 12.01 | 282.00 | 0.2113 | 994.0 | 863.7 | |
| 0.45 | 4.07 | 0.23 | 2.06 | 8.94 | 172.32 | 11.96 | 283.19 | 0.2111 | 1088.6 | 732.5 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 10.00 | 172.26 | 11.90 | 288.14 | 0.2147 | 1145.0 | 927.7 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 9.74 | 171.87 | 11.51 | 287.43 | 0.2071 | 1100.0 | 853.9 | |
| 0.72 | 2.89 | 0.37 | 1.46 | 9.53 | 171.68 | 11.32 | 286.70 | 0.2030 | 1141.8 | 931.3 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.96 | 171.44 | 11.08 | 289.08 | 0.2012 | 912.0 | 880.9 | |
| 0.00 | 2.62 | 0.00 | 1.32 | 8.66 | 171.27 | 10.91 | 282.85 | 0.1928 | 967.0 | 776.5 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 8.99 | 171.25 | 10.89 | 284.57 | 0.1937 | 870.0 | 697.9 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 9.12 | 171.13 | 10.77 | 285.35 | 0.1922 | 839.0 | 828.7 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 8.83 | 168.35 | 7.99 | 288.10 | 0.1451 | 910.0 | 744.4 | |
| 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. | |