SDO HMI 2014-09-17 18:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.19 | 102.45 | 1.59 | 51.62 | 13.06 | 352.34 | -7.28 | 45.20 | 0.1657 | -331.4 | -424.1 | |
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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 | 1.42 | 0.00 | 0.71 | 13.05 | 358.50 | -1.11 | 10.45 | 0.1047 | -1012.0 | -909.6 | |
| 0.00 | 2.48 | 0.00 | 1.24 | 12.80 | 357.79 | -1.82 | 17.49 | 0.1036 | -946.0 | -738.5 | |
| 0.00 | 0.44 | 0.00 | 0.22 | 12.17 | 357.58 | -2.03 | 21.66 | 0.0944 | -422.0 | -531.0 | |
| 0.00 | 2.13 | 0.00 | 1.06 | 11.38 | 356.82 | -2.80 | 33.00 | 0.0882 | -1040.0 | -800.8 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 12.44 | 356.78 | -2.84 | 27.70 | 0.1045 | -1052.0 | -891.7 | |
| 0.00 | 4.97 | 0.00 | 2.47 | 11.80 | 356.69 | -2.92 | 31.64 | 0.0956 | -793.0 | -814.7 | |
| 0.00 | 2.48 | 0.00 | 1.24 | 12.68 | 356.62 | -2.99 | 27.90 | 0.1094 | -994.0 | -787.2 | |
| 0.00 | 1.86 | 0.00 | 0.93 | 11.56 | 356.35 | -3.26 | 35.95 | 0.0954 | -813.0 | -713.8 | |
| 0.53 | 4.08 | 0.26 | 2.03 | 11.13 | 356.05 | -3.56 | 41.27 | 0.0929 | -1120.7 | -986.7 | |
| 0.00 | 0.27 | 0.00 | 0.13 | 11.44 | 356.05 | -3.57 | 39.21 | 0.0969 | -874.0 | -882.3 | |
| 0.44 | 6.21 | 0.22 | 3.10 | 12.34 | 355.88 | -3.73 | 35.09 | 0.1111 | -1076.0 | -980.5 | |
| 0.00 | 2.84 | 0.00 | 1.42 | 13.52 | 355.40 | -4.21 | 32.76 | 0.1326 | -1124.0 | -880.3 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 11.61 | 355.40 | -4.22 | 42.75 | 0.1066 | -1113.0 | -905.4 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 10.86 | 355.26 | -4.36 | 49.05 | 0.0993 | -1137.0 | -890.1 | |
| 0.00 | 2.84 | 0.00 | 1.41 | 11.52 | 355.18 | -4.43 | 44.76 | 0.1080 | -999.0 | -943.5 | |
| 0.00 | 2.13 | 0.00 | 1.06 | 11.25 | 355.10 | -4.52 | 47.18 | 0.1058 | -903.0 | -780.6 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 10.37 | 355.02 | -4.60 | 54.44 | 0.0974 | -1046.0 | -882.8 | |
| 0.00 | 3.19 | 0.00 | 1.59 | 11.73 | 354.97 | -4.65 | 44.76 | 0.1132 | -985.0 | -875.5 | |
| 2.22 | 6.39 | 1.11 | 3.19 | 12.30 | 354.93 | -4.69 | 41.59 | 0.1209 | -1148.5 | -911.0 | |
| 0.00 | 2.84 | 0.00 | 1.42 | 13.88 | 354.90 | -4.72 | 34.24 | 0.1426 | -982.0 | -882.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 13.91 | 354.71 | -4.90 | 35.15 | 0.1448 | -888.0 | -744.4 | |
| 0.00 | 2.31 | 0.00 | 1.15 | 13.63 | 354.56 | -5.05 | 37.12 | 0.1425 | -976.0 | -778.1 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 11.48 | 354.57 | -5.05 | 48.66 | 0.1153 | -750.0 | -576.2 | |
| 0.00 | 2.31 | 0.00 | 1.15 | 12.24 | 354.40 | -5.21 | 44.95 | 0.1263 | -701.0 | -605.4 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 11.97 | 354.31 | -5.30 | 47.02 | 0.1241 | -1030.0 | -832.5 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 10.85 | 354.30 | -5.31 | 54.53 | 0.1122 | -877.0 | -736.9 | |
| 0.00 | 2.31 | 0.00 | 1.15 | 10.48 | 354.12 | -5.49 | 58.14 | 0.1113 | -923.0 | -777.6 | |
| 0.00 | 1.60 | 0.00 | 0.81 | 16.16 | 352.67 | -6.94 | 36.42 | 0.1964 | -993.0 | -691.3 | |
| 0.00 | 1.60 | 0.00 | 0.80 | 14.42 | 351.92 | -7.70 | 45.53 | 0.1827 | -1111.0 | -902.4 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 14.66 | 351.72 | -7.90 | 45.29 | 0.1879 | -865.0 | -693.4 | |
| 0.00 | 1.51 | 0.00 | 0.76 | 14.45 | 351.69 | -7.92 | 46.21 | 0.1857 | -943.0 | -724.8 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 14.72 | 351.56 | -8.06 | 45.62 | 0.1905 | -943.0 | -837.7 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 11.75 | 351.53 | -8.08 | 59.49 | 0.1606 | -649.0 | -544.7 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 14.90 | 351.36 | -8.25 | 45.60 | 0.1950 | -638.0 | -585.7 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 15.38 | 351.25 | -8.36 | 44.20 | 0.2021 | -925.0 | -748.8 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 14.50 | 351.16 | -8.46 | 47.83 | 0.1930 | -841.0 | -697.0 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 15.68 | 350.80 | -8.82 | 44.64 | 0.2110 | -847.0 | -677.4 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 8.46 | 349.91 | -9.70 | 81.66 | 0.1692 | 960.0 | 694.2 | |
| 0.00 | 0.89 | 0.00 | 0.46 | 20.94 | 348.36 | -11.25 | 37.15 | 0.3030 | 689.0 | 562.0 | |
| 0.00 | 1.51 | 0.00 | 0.77 | 11.90 | 347.02 | -12.60 | 68.18 | 0.2309 | 1036.0 | 813.8 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 13.73 | 346.71 | -12.91 | 61.57 | 0.2479 | 965.0 | 910.1 | |
| 0.00 | 0.80 | 0.00 | 0.41 | 12.81 | 346.06 | -13.56 | 66.00 | 0.2514 | 769.0 | 680.7 | |
| 0.00 | 1.51 | 0.00 | 0.78 | 14.52 | 345.51 | -14.11 | 60.82 | 0.2714 | 835.0 | 670.4 | |
| 0.00 | 0.89 | 0.00 | 0.46 | 18.88 | 345.05 | -14.57 | 48.99 | 0.3167 | 716.0 | 566.5 | |
| 0.00 | 1.77 | 0.00 | 0.91 | 13.54 | 345.28 | -14.33 | 64.48 | 0.2679 | 863.0 | 748.2 | |
| 0.00 | 2.04 | 0.00 | 1.05 | 14.05 | 344.93 | -14.69 | 63.27 | 0.2766 | 1120.0 | 957.3 | |
| 0.00 | 1.33 | 0.00 | 0.69 | 14.17 | 344.76 | -14.85 | 63.12 | 0.2799 | 997.0 | 870.8 | |
| 0.00 | 0.44 | 0.00 | 0.23 | 14.53 | 344.74 | -14.88 | 61.98 | 0.2828 | 867.0 | 663.0 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 13.89 | 344.71 | -14.90 | 64.09 | 0.2787 | 934.0 | 807.5 | |
| 0.00 | 1.86 | 0.00 | 0.96 | 15.00 | 344.35 | -15.27 | 61.05 | 0.2919 | 718.0 | 584.5 | |
| 0.00 | 1.42 | 0.00 | 0.73 | 14.82 | 344.23 | -15.38 | 61.79 | 0.2923 | 950.0 | 772.8 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 15.02 | 343.77 | -15.85 | 61.84 | 0.3005 | 907.0 | 718.3 | |
| 0.00 | 2.48 | 0.00 | 1.29 | 14.83 | 343.58 | -16.03 | 62.65 | 0.3019 | 827.0 | 646.6 | |
| 0.00 | 1.33 | 0.00 | 0.71 | 16.62 | 339.97 | -19.64 | 62.00 | 0.3664 | 749.0 | 539.4 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 15.76 | 339.86 | -19.75 | 64.30 | 0.3626 | 723.0 | 566.8 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 20.85 | 336.40 | -23.21 | 56.26 | 0.4448 | 758.0 | 589.9 | |
| 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. | |