SDO HMI 2011-12-07 14:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 160.82 | 912.41 | 97.90 | 556.50 | -22.11 | 107.70 | 28.77 | 229.59 | 0.5868 | 290.1 | 223.1 | |
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back to the solar disc SDO HMI 2011-12-07 14:58:56 UT
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 |
| 14.15 | 64.52 | 8.68 | 39.52 | -17.51 | 110.98 | 32.05 | 239.14 | 0.5917 | 1079.5 | 465.5 | |
| 1.36 | 2.39 | 0.88 | 1.53 | -23.77 | 111.39 | 32.46 | 230.53 | 0.6386 | -665.9 | -498.8 | |
| 0.94 | 644.45 | 0.59 | 398.98 | -23.38 | 109.32 | 30.39 | 229.38 | 0.6140 | 345.5 | 403.0 | |
| 87.28 | -3.00 | 54.28 | -3.00 | -22.84 | 109.07 | 30.14 | 229.91 | 0.6071 | 1244.2 | 999999 | |
| 0.51 | -3.00 | 0.32 | -3.00 | -23.41 | 108.43 | 29.50 | 228.58 | 0.6049 | 684.0 | 999999 | |
| 0.34 | -3.00 | 0.21 | -3.00 | -23.35 | 108.27 | 29.34 | 228.52 | 0.6027 | 694.0 | 999999 | |
| 6.22 | -3.00 | 3.83 | -3.00 | -22.67 | 108.07 | 29.14 | 229.27 | 0.5952 | 1203.3 | 999999 | |
| 1.19 | -3.00 | 0.73 | -3.00 | -22.58 | 107.83 | 28.90 | 229.19 | 0.5918 | 1270.3 | 999999 | |
| 0.00 | 3.84 | 0.00 | 2.40 | -24.51 | 108.30 | 29.37 | 226.99 | 0.6125 | 624.0 | 564.9 | |
| 1.28 | -3.00 | 0.79 | -3.00 | -22.86 | 107.75 | 28.82 | 228.72 | 0.5933 | 809.2 | 999999 | |
| 2.56 | -3.00 | 1.55 | -3.00 | -22.19 | 106.69 | 27.76 | 228.68 | 0.5764 | 688.2 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.76 | -19.97 | 106.03 | 27.10 | 231.30 | 0.5507 | -538.0 | -412.5 | |
| 0.00 | 1.96 | 0.00 | 1.15 | -19.41 | 105.71 | 26.78 | 231.86 | 0.5425 | -639.0 | -408.5 | |
| 0.00 | 0.34 | 0.00 | 0.21 | -22.99 | 106.07 | 27.14 | 226.97 | 0.5767 | -453.0 | -359.5 | |
| 0.00 | 0.85 | 0.00 | 0.53 | -26.38 | 106.66 | 27.73 | 223.09 | 0.6125 | 553.0 | 498.9 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -20.00 | 105.01 | 26.08 | 230.26 | 0.5394 | -622.0 | -520.9 | |
| 0.00 | 0.26 | 0.00 | 0.15 | -21.87 | 105.30 | 26.37 | 227.78 | 0.5587 | -517.0 | -488.0 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -22.03 | 105.01 | 26.08 | 227.26 | 0.5570 | -328.0 | -377.8 | |
| 0.00 | 1.62 | 0.00 | 0.95 | -20.47 | 104.50 | 25.57 | 229.02 | 0.5378 | -837.0 | -546.9 | |
| 1.45 | 14.06 | 0.86 | 8.35 | -22.51 | 104.32 | 25.39 | 225.87 | 0.5541 | -584.1 | -426.3 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -19.72 | 103.82 | 24.88 | 229.46 | 0.5234 | -875.0 | -762.8 | |
| 0.00 | 1.28 | 0.00 | 0.74 | -19.31 | 103.61 | 24.68 | 229.87 | 0.5174 | -777.0 | -624.6 | |
| 2.64 | -20.00 | 1.57 | -20.00 | -22.67 | 104.07 | 25.14 | 225.38 | 0.5529 | -690.5 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.55 | -20.28 | 103.60 | 24.67 | 228.35 | 0.5260 | -866.0 | -718.5 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -22.25 | 103.89 | 24.95 | 225.77 | 0.5471 | -732.0 | -488.5 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -20.44 | 103.52 | 24.59 | 228.03 | 0.5266 | -646.0 | -551.0 | |
| 0.00 | 0.94 | 0.00 | 0.55 | -22.67 | 103.79 | 24.86 | 225.08 | 0.5500 | -754.0 | -620.5 | |
| 0.00 | 2.05 | 0.00 | 1.20 | -21.17 | 103.51 | 24.58 | 226.93 | 0.5331 | -704.0 | -625.6 | |
| 0.00 | 1.88 | 0.00 | 1.10 | -21.29 | 103.32 | 24.39 | 226.54 | 0.5322 | -885.0 | -744.1 | |
| 3.15 | 8.95 | 1.88 | 5.34 | -23.76 | 103.76 | 24.83 | 223.54 | 0.5600 | -665.7 | -567.2 | |
| 0.00 | 1.62 | 0.00 | 0.96 | -22.86 | 103.54 | 24.61 | 224.55 | 0.5493 | -638.0 | -586.6 | |
| 0.00 | 2.47 | 0.00 | 1.42 | -19.72 | 102.88 | 23.95 | 228.44 | 0.5128 | -741.0 | -656.9 | |
| 2.64 | 3.32 | 1.54 | 1.94 | -21.52 | 102.95 | 24.01 | 225.80 | 0.5303 | -810.4 | -625.0 | |
| 0.00 | 2.64 | 0.00 | 1.54 | -21.55 | 102.64 | 23.71 | 225.40 | 0.5273 | -530.0 | -607.4 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -21.96 | 102.68 | 23.74 | 224.85 | 0.5317 | -686.0 | -612.6 | |
| 0.00 | 0.85 | 0.00 | 0.51 | -23.99 | 102.88 | 23.95 | 222.28 | 0.5535 | -613.0 | -471.7 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -22.82 | 102.52 | 23.59 | 223.45 | 0.5385 | -792.0 | -681.9 | |
| 2.13 | 123.76 | 1.23 | 71.04 | -21.32 | 102.19 | 23.25 | 225.21 | 0.5203 | -657.0 | -549.8 | |
| 1.36 | -38.00 | 0.78 | -38.00 | -19.97 | 101.93 | 23.00 | 226.96 | 0.5045 | -947.0 | 999999 | |
| 24.46 | -38.00 | 14.06 | -38.00 | -20.50 | 101.88 | 22.95 | 226.08 | 0.5091 | -1146.4 | 999999 | |
| 5.11 | -38.00 | 2.95 | -38.00 | -21.13 | 101.98 | 23.05 | 225.25 | 0.5163 | -840.6 | 999999 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -23.31 | 102.29 | 23.36 | 222.52 | 0.5410 | -545.0 | -432.1 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -23.66 | 102.11 | 23.18 | 221.84 | 0.5427 | -743.0 | -545.6 | |
| 2.05 | -38.00 | 1.17 | -38.00 | -20.22 | 101.42 | 22.49 | 225.97 | 0.5014 | -1067.0 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -23.50 | 101.80 | 22.87 | 221.69 | 0.5381 | -691.0 | -545.8 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -23.08 | 101.73 | 22.80 | 222.17 | 0.5331 | -789.0 | -642.5 | |
| 0.00 | 4.26 | 0.00 | 2.43 | -20.28 | 100.89 | 21.96 | 225.22 | 0.4962 | -998.0 | -832.8 | |
| 0.00 | 1.62 | 0.00 | 0.92 | -20.37 | 100.56 | 21.63 | 224.67 | 0.4936 | -681.0 | -561.5 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -20.50 | 100.35 | 21.41 | 224.20 | 0.4926 | -833.0 | -762.1 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -22.34 | 99.06 | 20.13 | 219.83 | 0.4989 | -634.0 | -532.5 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -21.92 | 98.52 | 19.59 | 219.68 | 0.4891 | -740.0 | -526.0 | |
| 0.00 | 2.56 | 0.00 | 1.45 | -22.08 | 98.38 | 19.44 | 219.26 | 0.4895 | -828.0 | -642.1 | |
| 0.00 | 1.79 | 0.00 | 0.98 | -18.52 | 97.13 | 18.19 | 222.85 | 0.4372 | -708.0 | -615.0 | |
| 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. | |