SDO HMI 2011-07-19 23:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.99 | 343.62 | 41.82 | 191.67 | -22.52 | 136.47 | 1.29 | 182.60 | 0.4620 | -222.7 | -132.0 | |
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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 | 2.09 | 0.00 | 1.17 | -22.13 | 142.12 | 6.95 | 193.93 | 0.4672 | 908.0 | 726.5 | |
| 0.00 | 2.45 | 0.00 | 1.37 | -22.33 | 141.73 | 6.56 | 193.07 | 0.4689 | 926.0 | 810.7 | |
| 0.00 | 2.27 | 0.00 | 1.28 | -22.98 | 141.70 | 6.52 | 192.67 | 0.4785 | 862.0 | 705.8 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -22.60 | 141.51 | 6.34 | 192.51 | 0.4722 | 537.0 | 408.5 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -27.20 | 141.24 | 6.06 | 190.07 | 0.5392 | 515.0 | 492.9 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -23.73 | 140.36 | 5.19 | 189.85 | 0.4858 | 771.0 | 606.7 | |
| 6.71 | 10.34 | 3.75 | 5.78 | -22.42 | 140.15 | 4.97 | 189.95 | 0.4653 | 977.3 | 794.2 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -22.01 | 139.90 | 4.73 | 189.63 | 0.4584 | 958.0 | 717.3 | |
| 0.00 | 2.27 | 0.00 | 1.28 | -23.80 | 139.86 | 4.69 | 188.90 | 0.4855 | 927.0 | 818.2 | |
| 1.72 | 24.58 | 0.96 | 13.71 | -22.25 | 139.74 | 4.57 | 189.23 | 0.4616 | 1019.6 | 861.7 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -23.69 | 139.63 | 4.45 | 188.49 | 0.4834 | 753.0 | 601.7 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -19.84 | 139.41 | 4.24 | 189.48 | 0.4235 | 728.0 | 650.6 | |
| 2.54 | -10.00 | 1.42 | -10.00 | -22.18 | 139.45 | 4.27 | 188.66 | 0.4598 | 1220.8 | 999999 | |
| 0.00 | 10.16 | 0.00 | 5.69 | -22.79 | 139.43 | 4.26 | 188.42 | 0.4692 | 883.0 | 732.4 | |
| 2.90 | -10.00 | 1.62 | -10.00 | -22.31 | 139.25 | 4.08 | 188.23 | 0.4615 | 910.4 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -20.71 | 139.21 | 4.03 | 188.70 | 0.4366 | 740.0 | 526.0 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -20.11 | 139.16 | 3.98 | 188.82 | 0.4271 | 573.0 | 546.6 | |
| 2.45 | 16.42 | 1.36 | 9.11 | -21.76 | 139.10 | 3.93 | 188.11 | 0.4527 | 1060.3 | 904.7 | |
| 0.00 | 3.08 | 0.00 | 1.74 | -23.72 | 139.13 | 3.95 | 187.54 | 0.4828 | 786.0 | 620.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -23.03 | 138.91 | 3.73 | 187.32 | 0.4718 | 699.0 | 579.5 | |
| 0.00 | 4.99 | 0.00 | 2.78 | -22.27 | 138.85 | 3.68 | 187.45 | 0.4601 | 819.0 | 686.1 | |
| 0.00 | 2.45 | 0.00 | 1.38 | -23.38 | 138.88 | 3.71 | 187.18 | 0.4770 | 748.0 | 571.2 | |
| 1.63 | 3.99 | 0.91 | 2.22 | -22.10 | 138.49 | 3.31 | 186.76 | 0.4567 | 774.8 | 653.1 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -21.83 | 138.32 | 3.14 | 186.49 | 0.4521 | 416.0 | 323.2 | |
| 0.00 | 4.72 | 0.00 | 2.64 | -22.72 | 138.27 | 3.09 | 186.16 | 0.4658 | 243.0 | 322.7 | |
| 0.54 | 7.26 | 0.30 | 4.03 | -21.89 | 137.89 | 2.72 | 185.60 | 0.4525 | 650.0 | 508.7 | |
| 0.00 | 1.90 | 0.00 | 1.09 | -24.83 | 137.68 | 2.51 | 184.60 | 0.4973 | 562.0 | 434.4 | |
| 0.00 | 2.09 | 0.00 | 1.17 | -22.92 | 137.22 | 2.04 | 184.04 | 0.4675 | -223.0 | -93.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -22.58 | 137.14 | 1.97 | 183.95 | 0.4621 | -606.0 | -429.1 | |
| 3.17 | 3.54 | 1.78 | 1.98 | -22.88 | 136.75 | 1.58 | 183.13 | 0.4665 | -480.0 | -420.5 | |
| 1.63 | 204.83 | 0.90 | 114.00 | -21.69 | 136.51 | 1.33 | 182.78 | 0.4476 | -978.3 | -590.5 | |
| 3.36 | -31.00 | 1.87 | -31.00 | -22.64 | 136.45 | 1.28 | 182.56 | 0.4625 | -814.2 | 999999 | |
| 1.54 | -31.00 | 0.86 | -31.00 | -21.92 | 136.25 | 1.07 | 182.22 | 0.4512 | -994.2 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -23.19 | 135.96 | 0.78 | 181.54 | 0.4708 | -530.0 | -489.3 | |
| 11.52 | -31.00 | 6.42 | -31.00 | -22.44 | 135.86 | 0.68 | 181.38 | 0.4590 | -983.7 | 999999 | |
| 1.90 | -31.00 | 1.06 | -31.00 | -22.02 | 135.72 | 0.55 | 181.13 | 0.4525 | -1114.9 | 999999 | |
| 1.27 | -31.00 | 0.71 | -31.00 | -22.23 | 135.49 | 0.32 | 180.65 | 0.4557 | -1157.1 | 999999 | |
| 1.90 | -31.00 | 1.06 | -31.00 | -22.30 | 135.30 | 0.12 | 180.25 | 0.4567 | -1161.2 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -23.26 | 135.10 | -0.08 | 179.85 | 0.4717 | -570.0 | -446.2 | |
| 10.89 | -31.00 | 6.06 | -31.00 | -22.47 | 135.00 | -0.18 | 179.65 | 0.4594 | -1072.0 | 999999 | |
| 0.63 | 3.72 | 0.36 | 2.08 | -23.02 | 134.87 | -0.31 | 179.39 | 0.4679 | -824.1 | -649.0 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -23.30 | 134.83 | -0.34 | 179.33 | 0.4722 | -615.0 | -494.1 | |
| 1.36 | -31.00 | 0.76 | -31.00 | -22.26 | 134.77 | -0.41 | 179.17 | 0.4562 | -987.3 | 999999 | |
| 0.00 | 1.72 | 0.00 | 0.98 | -24.16 | 134.70 | -0.48 | 179.10 | 0.4856 | -1045.0 | -838.3 | |
| 0.00 | 0.63 | 0.00 | 0.36 | -24.06 | 134.56 | -0.61 | 178.84 | 0.4840 | -837.0 | -665.1 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -24.37 | 134.46 | -0.71 | 178.67 | 0.4889 | -631.0 | -565.6 | |
| 16.60 | -31.00 | 9.26 | -31.00 | -22.57 | 134.31 | -0.87 | 178.25 | 0.4612 | -1103.4 | 999999 | |
| 0.73 | -31.00 | 0.40 | -31.00 | -22.44 | 133.95 | -1.23 | 177.51 | 0.4593 | -1043.8 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -24.51 | 133.83 | -1.35 | 177.49 | 0.4913 | -795.0 | -635.3 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -24.66 | 132.48 | -2.69 | 175.03 | 0.4949 | -775.0 | -646.8 | |
| 0.00 | 1.63 | 0.00 | 0.92 | -23.89 | 132.20 | -2.98 | 174.34 | 0.4836 | -868.0 | -656.7 | |
| 0.00 | 2.81 | 0.00 | 1.60 | -24.70 | 131.78 | -3.40 | 173.75 | 0.4965 | -839.0 | -697.5 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -23.82 | 131.73 | -3.44 | 173.45 | 0.4834 | -792.0 | -546.1 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -25.09 | 129.98 | -5.20 | 170.63 | 0.5062 | -435.0 | -337.7 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -23.74 | 129.03 | -6.15 | 168.38 | 0.4886 | 295.0 | 246.0 | |
| 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. | |