SDO HMI 2014-03-10 12:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.53 | 229.79 | 24.28 | 115.69 | -10.08 | 358.10 | -9.32 | 107.35 | 0.1699 | 420.0 | 288.9 | |
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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 | 1.39 | 0.00 | 0.69 | -13.70 | 2.14 | -5.28 | 141.75 | 0.1451 | 966.0 | 774.3 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -5.94 | 1.22 | -6.20 | 78.61 | 0.1101 | 845.0 | 677.7 | |
| 0.00 | 2.08 | 0.00 | 1.05 | -14.40 | 0.52 | -6.90 | 137.23 | 0.1723 | 977.0 | 777.6 | |
| 19.50 | 131.93 | 9.75 | 65.96 | -9.97 | 0.09 | -7.33 | 111.29 | 0.1355 | 1347.7 | 472.8 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -5.83 | 0.14 | -7.28 | 79.57 | 0.1288 | 829.0 | 568.5 | |
| 0.00 | 2.69 | 0.00 | 1.34 | -6.10 | 0.10 | -7.32 | 81.67 | 0.1286 | 893.0 | 752.6 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -6.34 | 0.10 | -7.32 | 83.52 | 0.1281 | 870.0 | 735.2 | |
| 20.80 | -4.00 | 10.40 | -4.00 | -9.37 | 359.74 | -7.68 | 106.31 | 0.1381 | 1180.8 | 999999 | |
| 0.00 | 6.41 | 0.00 | 3.21 | -8.67 | 359.18 | -8.25 | 100.64 | 0.1449 | 928.0 | 756.9 | |
| 0.00 | 1.73 | 0.00 | 0.87 | -7.66 | 359.05 | -8.37 | 93.55 | 0.1453 | 873.0 | 739.5 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -8.79 | 358.90 | -8.52 | 101.09 | 0.1499 | 848.0 | 585.3 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -7.92 | 358.83 | -8.59 | 95.26 | 0.1493 | 987.0 | 724.0 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -7.71 | 358.71 | -8.71 | 93.81 | 0.1511 | 908.0 | 763.9 | |
| 0.00 | 2.95 | 0.00 | 1.48 | -9.04 | 358.31 | -9.11 | 102.05 | 0.1606 | 840.0 | 642.6 | |
| 8.23 | 15.34 | 4.13 | 7.70 | -8.56 | 358.14 | -9.28 | 98.93 | 0.1621 | 1081.8 | 663.9 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -9.24 | 357.94 | -9.48 | 102.82 | 0.1675 | 800.0 | 649.6 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -9.42 | 357.88 | -9.55 | 103.78 | 0.1692 | 846.0 | 703.7 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -10.10 | 357.64 | -9.78 | 107.29 | 0.1760 | 804.0 | 671.3 | |
| 0.00 | 1.65 | 0.00 | 0.83 | -8.34 | 357.57 | -9.85 | 97.21 | 0.1714 | 721.0 | 579.9 | |
| 0.00 | 3.99 | 0.00 | 2.00 | -7.95 | 357.52 | -9.90 | 94.92 | 0.1717 | 783.0 | 705.1 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -9.35 | 357.48 | -9.94 | 102.91 | 0.1756 | 787.0 | 557.2 | |
| 0.00 | 1.91 | 0.00 | 0.96 | -8.88 | 357.46 | -9.96 | 100.20 | 0.1744 | -968.0 | -737.8 | |
| 0.00 | 1.39 | 0.00 | 0.70 | -12.39 | 357.34 | -10.08 | 118.30 | 0.1950 | 972.0 | 733.9 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -7.59 | 357.38 | -10.05 | 92.79 | 0.1739 | 762.0 | 553.1 | |
| 0.00 | 2.08 | 0.00 | 1.05 | -9.28 | 356.93 | -10.49 | 101.94 | 0.1845 | -908.0 | -737.4 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -9.67 | 356.86 | -10.57 | 103.91 | 0.1871 | -895.0 | -768.1 | |
| 0.00 | 1.91 | 0.00 | 0.97 | -13.38 | 356.12 | -11.30 | 119.91 | 0.2210 | 952.0 | 838.4 | |
| 0.00 | 1.73 | 0.00 | 0.88 | -13.59 | 356.01 | -11.41 | 120.51 | 0.2242 | 1055.0 | 777.8 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -12.96 | 356.04 | -11.38 | 118.04 | 0.2188 | 1045.0 | 908.3 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -12.18 | 356.08 | -11.34 | 114.82 | 0.2128 | 726.0 | 529.2 | |
| 0.00 | 1.04 | 0.00 | 0.53 | -14.03 | 355.74 | -11.68 | 121.65 | 0.2318 | 1028.0 | 806.8 | |
| 0.00 | 1.47 | 0.00 | 0.75 | -13.82 | 355.50 | -11.92 | 120.35 | 0.2335 | 799.0 | 643.5 | |
| 0.00 | 0.87 | 0.00 | 0.44 | -14.87 | 354.62 | -12.80 | 122.45 | 0.2549 | -936.0 | -620.8 | |
| 0.00 | 1.13 | 0.00 | 0.58 | -16.79 | 354.14 | -13.28 | 127.61 | 0.2788 | -924.0 | -697.2 | |
| 0.00 | 2.34 | 0.00 | 1.20 | -14.66 | 353.59 | -13.83 | 119.91 | 0.2680 | -931.0 | -793.0 | |
| 0.00 | 2.51 | 0.00 | 1.31 | -17.32 | 352.63 | -14.80 | 126.32 | 0.3040 | -834.0 | -697.7 | |
| 0.00 | 1.91 | 0.00 | 0.97 | -7.69 | 353.13 | -14.29 | 92.80 | 0.2460 | -926.0 | -794.1 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -17.10 | 352.55 | -14.87 | 125.59 | 0.3031 | -892.0 | -733.2 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -8.60 | 352.75 | -14.67 | 96.39 | 0.2531 | -903.0 | -730.5 | |
| 0.00 | 1.13 | 0.00 | 0.58 | -10.23 | 352.59 | -14.83 | 102.67 | 0.2594 | -963.0 | -750.8 | |
| 0.00 | 1.99 | 0.00 | 1.03 | -14.37 | 352.12 | -15.30 | 116.74 | 0.2876 | -777.0 | -682.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -14.06 | 350.86 | -16.56 | 114.18 | 0.3044 | -750.0 | -588.9 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -16.92 | 349.87 | -17.55 | 121.10 | 0.3384 | -763.0 | -568.7 | |
| 0.00 | 0.87 | 0.00 | 0.45 | -12.63 | 350.23 | -17.19 | 109.07 | 0.3065 | -772.0 | -669.8 | |
| 0.00 | 2.95 | 0.00 | 1.54 | -13.36 | 349.67 | -17.76 | 110.80 | 0.3188 | -870.0 | -790.0 | |
| 0.00 | 1.65 | 0.00 | 0.86 | -9.74 | 349.84 | -17.58 | 99.50 | 0.3032 | -848.0 | -593.1 | |
| 0.00 | 2.08 | 0.00 | 1.09 | -13.26 | 349.48 | -17.94 | 110.34 | 0.3212 | -646.0 | -617.8 | |
| 0.00 | 1.39 | 0.00 | 0.72 | -12.93 | 349.44 | -17.98 | 109.31 | 0.3202 | -913.0 | -745.4 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -9.58 | 349.50 | -17.92 | 98.85 | 0.3084 | -751.0 | -579.5 | |
| 0.00 | 1.47 | 0.00 | 0.77 | -9.79 | 349.43 | -17.99 | 99.48 | 0.3100 | -818.0 | -613.8 | |
| 0.00 | 1.91 | 0.00 | 0.99 | -10.17 | 349.31 | -18.11 | 100.66 | 0.3128 | -844.0 | -709.3 | |
| 0.00 | 1.47 | 0.00 | 0.77 | -11.77 | 348.95 | -18.47 | 105.44 | 0.3232 | -852.0 | -694.1 | |
| 0.00 | 0.87 | 0.00 | 0.45 | -12.81 | 348.81 | -18.62 | 108.45 | 0.3296 | -702.0 | -608.4 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -18.45 | 347.36 | -20.06 | 121.83 | 0.3847 | -728.0 | -581.5 | |
| 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. | |