SDO HMI 2014-03-10 05:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.39 | 251.64 | 22.46 | 128.51 | -10.34 | 357.95 | -13.30 | 103.72 | 0.2356 | 336.8 | 278.5 | |
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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 | 1.39 | 0.00 | 0.70 | -14.10 | 2.21 | -9.04 | 128.42 | 0.1954 | 916.0 | 798.0 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -5.50 | 0.57 | -10.68 | 81.29 | 0.1875 | 991.0 | 824.6 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -12.85 | 0.09 | -11.16 | 117.93 | 0.2146 | 724.0 | 511.3 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -5.76 | 0.29 | -10.96 | 82.89 | 0.1915 | 870.0 | 764.1 | |
| 19.59 | 139.40 | 9.90 | 70.44 | -9.98 | 0.02 | -11.23 | 104.66 | 0.1992 | 1372.5 | 479.5 | |
| 15.87 | -5.00 | 8.02 | -5.00 | -9.38 | 359.79 | -11.46 | 101.48 | 0.2009 | 1274.2 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -14.18 | 359.17 | -12.08 | 121.32 | 0.2385 | 823.0 | 690.0 | |
| 0.00 | 1.56 | 0.00 | 0.79 | -8.74 | 359.11 | -12.14 | 97.90 | 0.2109 | 997.0 | 708.4 | |
| 0.00 | 2.25 | 0.00 | 1.14 | -7.87 | 358.83 | -12.42 | 93.70 | 0.2145 | 892.0 | 706.2 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -8.07 | 358.79 | -12.46 | 94.67 | 0.2153 | 1208.0 | 923.3 | |
| 0.00 | 6.42 | 0.00 | 3.26 | -8.87 | 358.58 | -12.67 | 98.26 | 0.2200 | 939.0 | 769.3 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -8.72 | 358.40 | -12.85 | 97.48 | 0.2228 | 949.0 | 825.4 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -8.95 | 358.08 | -13.17 | 98.34 | 0.2285 | 877.0 | 713.7 | |
| 0.00 | 2.25 | 0.00 | 1.15 | -9.15 | 358.01 | -13.24 | 99.20 | 0.2301 | 938.0 | 623.3 | |
| 0.00 | 1.47 | 0.00 | 0.75 | -9.39 | 357.97 | -13.28 | 100.20 | 0.2313 | 880.0 | 722.1 | |
| 7.63 | 24.27 | 3.88 | 12.36 | -8.56 | 357.97 | -13.28 | 96.59 | 0.2297 | 1027.4 | 470.6 | |
| 0.43 | 1.82 | 0.22 | 0.93 | -9.37 | 357.47 | -13.78 | 99.85 | 0.2395 | 860.8 | 719.6 | |
| 0.00 | 1.47 | 0.00 | 0.75 | -8.00 | 357.40 | -13.85 | 94.07 | 0.2387 | 828.0 | 644.2 | |
| 0.00 | 2.51 | 0.00 | 1.29 | -13.33 | 356.96 | -14.29 | 114.58 | 0.2654 | 792.0 | 653.3 | |
| 0.87 | 4.51 | 0.44 | 2.31 | -9.33 | 356.89 | -14.36 | 99.34 | 0.2492 | -1007.4 | -793.8 | |
| 0.00 | 1.30 | 0.00 | 0.67 | -12.06 | 356.59 | -14.66 | 109.58 | 0.2639 | 883.0 | 611.5 | |
| 0.00 | 2.86 | 0.00 | 1.46 | -9.68 | 356.68 | -14.57 | 100.62 | 0.2534 | -1175.0 | -933.2 | |
| 0.00 | 1.13 | 0.00 | 0.58 | -12.65 | 356.18 | -15.07 | 111.20 | 0.2734 | 956.0 | 740.0 | |
| 0.00 | 5.98 | 0.00 | 3.08 | -13.39 | 356.10 | -15.15 | 113.66 | 0.2789 | 411.0 | 790.0 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -12.43 | 356.06 | -15.19 | 110.33 | 0.2740 | 886.0 | 671.7 | |
| 0.00 | 1.65 | 0.00 | 0.85 | -13.89 | 355.84 | -15.41 | 115.00 | 0.2859 | 490.0 | 407.8 | |
| 0.00 | 0.87 | 0.00 | 0.45 | -13.18 | 355.86 | -15.39 | 112.64 | 0.2813 | 947.0 | 867.4 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -13.50 | 355.77 | -15.48 | 113.62 | 0.2845 | 975.0 | 810.7 | |
| 0.00 | 2.86 | 0.00 | 1.48 | -12.90 | 355.69 | -15.56 | 111.51 | 0.2824 | 778.0 | 799.8 | |
| 0.00 | 1.47 | 0.00 | 0.77 | -14.84 | 354.46 | -16.79 | 116.19 | 0.3126 | -954.0 | -775.5 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -15.30 | 354.07 | -17.18 | 117.08 | 0.3215 | -848.0 | -681.6 | |
| 0.00 | 1.56 | 0.00 | 0.82 | -15.21 | 353.23 | -18.02 | 115.85 | 0.3332 | -788.0 | -662.7 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -17.10 | 352.89 | -18.36 | 120.50 | 0.3510 | -882.0 | -748.1 | |
| 0.00 | 1.56 | 0.00 | 0.83 | -17.25 | 352.71 | -18.54 | 120.65 | 0.3546 | -818.0 | -695.1 | |
| 0.00 | 1.39 | 0.00 | 0.74 | -17.33 | 352.57 | -18.69 | 120.69 | 0.3572 | -621.0 | -580.9 | |
| 0.00 | 1.73 | 0.00 | 0.91 | -14.08 | 352.84 | -18.41 | 112.27 | 0.3324 | -737.0 | -621.3 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -16.97 | 352.57 | -18.68 | 119.78 | 0.3545 | -915.0 | -756.2 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -8.30 | 353.10 | -18.15 | 94.56 | 0.3106 | -925.0 | -739.6 | |
| 0.00 | 1.82 | 0.00 | 0.96 | -14.07 | 352.52 | -18.73 | 111.93 | 0.3372 | -833.0 | -694.7 | |
| 0.00 | 2.51 | 0.00 | 1.32 | -13.83 | 352.51 | -18.74 | 111.24 | 0.3362 | -971.0 | -738.9 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -8.70 | 352.73 | -18.52 | 95.79 | 0.3170 | -691.0 | -565.6 | |
| 0.00 | 2.95 | 0.00 | 1.56 | -14.37 | 351.84 | -19.41 | 112.16 | 0.3491 | -914.0 | -744.3 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -4.24 | 352.21 | -19.04 | 82.02 | 0.3299 | -710.0 | -524.9 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -12.63 | 351.15 | -20.10 | 106.83 | 0.3519 | -880.0 | -756.6 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -16.62 | 349.46 | -21.79 | 115.75 | 0.3966 | -807.0 | -663.2 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -12.01 | 349.83 | -21.42 | 104.38 | 0.3703 | -776.0 | -635.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -16.73 | 349.11 | -22.14 | 115.70 | 0.4023 | -705.0 | -495.9 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -10.11 | 349.62 | -21.63 | 99.21 | 0.3692 | -856.0 | -683.9 | |
| 0.00 | 1.73 | 0.00 | 0.92 | -9.51 | 349.60 | -21.65 | 97.58 | 0.3687 | -789.0 | -646.8 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -13.15 | 349.30 | -21.95 | 107.08 | 0.3824 | -806.0 | -617.7 | |
| 0.00 | 2.25 | 0.00 | 1.21 | -12.91 | 349.33 | -21.92 | 106.48 | 0.3812 | -887.0 | -686.4 | |
| 0.00 | 1.39 | 0.00 | 0.74 | -9.81 | 349.55 | -21.70 | 98.37 | 0.3699 | -875.0 | -727.2 | |
| 0.00 | 2.17 | 0.00 | 1.16 | -10.41 | 349.50 | -21.75 | 99.96 | 0.3716 | -754.0 | -662.0 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -18.61 | 347.29 | -23.96 | 118.32 | 0.4391 | -677.0 | -568.8 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -13.25 | 346.53 | -24.72 | 105.90 | 0.4251 | -670.0 | -510.7 | |
| 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. | |