SDO HMI 2011-06-15 15:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93.73 | 326.27 | 50.80 | 176.65 | -14.91 | 247.25 | 17.64 | 226.70 | 0.4038 | 212.2 | 199.0 | |
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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 | 0.63 | 0.00 | 0.36 | -17.67 | 251.65 | 22.03 | 228.20 | 0.4813 | 761.0 | 572.3 | |
| 0.00 | 6.34 | 0.00 | 3.49 | -14.54 | 250.47 | 20.85 | 232.19 | 0.4380 | 750.0 | 647.5 | |
| 0.00 | 2.54 | 0.00 | 1.40 | -14.28 | 250.45 | 20.83 | 232.64 | 0.4354 | 733.0 | 636.2 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -15.20 | 250.07 | 20.45 | 230.44 | 0.4391 | 639.0 | 590.8 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -15.10 | 249.96 | 20.34 | 230.47 | 0.4369 | 677.0 | 499.6 | |
| 0.00 | 2.45 | 0.00 | 1.35 | -15.58 | 249.84 | 20.22 | 229.44 | 0.4400 | 650.0 | 538.7 | |
| 22.20 | 35.26 | 12.17 | 19.33 | -14.88 | 249.56 | 19.95 | 230.35 | 0.4300 | 972.1 | 695.0 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -15.51 | 249.22 | 19.61 | 228.72 | 0.4320 | 622.0 | 392.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -13.14 | 248.74 | 19.13 | 232.60 | 0.4033 | 536.0 | 526.8 | |
| 3.17 | 145.37 | 1.73 | 78.84 | -14.62 | 248.84 | 19.22 | 229.82 | 0.4186 | 1089.1 | 651.7 | |
| 1.36 | 4.89 | 0.74 | 2.67 | -15.06 | 248.88 | 19.26 | 229.05 | 0.4235 | 739.7 | 540.7 | |
| 0.00 | 4.17 | 0.00 | 2.28 | -15.38 | 248.91 | 19.29 | 228.51 | 0.4270 | 723.0 | 524.5 | |
| 0.00 | 0.91 | 0.00 | 0.49 | -15.25 | 248.63 | 19.01 | 228.34 | 0.4224 | 981.0 | 805.3 | |
| 23.29 | -10.00 | 12.65 | -10.00 | -14.43 | 248.35 | 18.74 | 229.49 | 0.4109 | 1197.1 | 999999 | |
| 0.00 | 2.45 | 0.00 | 1.32 | -13.17 | 248.25 | 18.63 | 231.83 | 0.3973 | 766.0 | 644.7 | |
| 1.63 | -10.00 | 0.88 | -10.00 | -14.11 | 248.10 | 18.48 | 229.72 | 0.4046 | 1184.1 | 999999 | |
| 2.18 | -10.00 | 1.18 | -10.00 | -15.09 | 247.98 | 18.36 | 227.69 | 0.4131 | -414.7 | 999999 | |
| 2.81 | -10.00 | 1.52 | -10.00 | -14.01 | 247.69 | 18.07 | 229.30 | 0.3987 | 1087.5 | 999999 | |
| 1.54 | -10.00 | 0.83 | -10.00 | -14.36 | 247.55 | 17.94 | 228.42 | 0.4005 | 843.6 | 999999 | |
| 1.18 | -10.00 | 0.64 | -10.00 | -14.17 | 247.54 | 17.92 | 228.76 | 0.3984 | 858.0 | 999999 | |
| 0.00 | 2.36 | 0.00 | 1.28 | -14.96 | 247.57 | 17.95 | 227.30 | 0.4069 | 709.0 | 520.6 | |
| 3.53 | -10.00 | 1.91 | -10.00 | -14.08 | 247.37 | 17.75 | 228.68 | 0.3953 | 1114.8 | 999999 | |
| 0.00 | 1.72 | 0.00 | 0.93 | -15.56 | 247.36 | 17.74 | 225.86 | 0.4108 | 413.0 | 237.9 | |
| 1.27 | -10.00 | 0.68 | -10.00 | -14.14 | 247.14 | 17.52 | 228.21 | 0.3932 | 833.2 | 999999 | |
| 0.00 | 1.81 | 0.00 | 0.98 | -15.69 | 247.21 | 17.59 | 225.39 | 0.4104 | 15.0 | 117.4 | |
| 0.00 | 3.26 | 0.00 | 1.75 | -13.88 | 246.82 | 17.21 | 228.20 | 0.3868 | 995.0 | 781.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -15.12 | 246.76 | 17.14 | 225.72 | 0.3991 | -238.0 | -113.3 | |
| 3.99 | 13.14 | 2.16 | 7.12 | -15.91 | 246.59 | 16.98 | 224.00 | 0.4059 | -708.8 | -463.0 | |
| 4.08 | 5.08 | 2.20 | 2.73 | -15.21 | 246.34 | 16.72 | 224.85 | 0.3953 | -668.0 | -103.0 | |
| 3.81 | -28.00 | 2.06 | -28.00 | -16.07 | 246.28 | 16.66 | 223.20 | 0.4042 | -816.9 | 999999 | |
| 0.00 | 1.81 | 0.00 | 0.98 | -15.94 | 245.97 | 16.35 | 222.90 | 0.3993 | -869.0 | -703.8 | |
| 0.00 | 1.72 | 0.00 | 0.93 | -15.74 | 245.82 | 16.20 | 222.99 | 0.3955 | -735.0 | -618.4 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -15.55 | 245.77 | 16.15 | 223.26 | 0.3928 | -700.0 | -479.9 | |
| 0.00 | 0.63 | 0.00 | 0.34 | -13.37 | 245.45 | 15.83 | 226.91 | 0.3649 | 637.0 | 438.6 | |
| 1.99 | 4.35 | 1.07 | 2.33 | -15.52 | 245.21 | 15.59 | 222.33 | 0.3863 | -868.6 | -713.5 | |
| 5.26 | 8.34 | 2.80 | 4.44 | -14.00 | 244.97 | 15.35 | 224.78 | 0.3662 | -910.7 | -785.6 | |
| 0.00 | 1.63 | 0.00 | 0.87 | -15.01 | 245.01 | 15.39 | 222.90 | 0.3782 | -1052.0 | -844.8 | |
| 0.82 | 12.05 | 0.44 | 6.48 | -15.90 | 245.04 | 15.43 | 221.35 | 0.3889 | -1041.6 | -795.7 | |
| 2.27 | 9.43 | 1.21 | 5.04 | -15.33 | 244.61 | 14.99 | 221.58 | 0.3775 | -946.8 | -799.7 | |
| 0.00 | 3.53 | 0.00 | 1.88 | -14.28 | 244.27 | 14.65 | 222.93 | 0.3616 | -791.0 | -729.1 | |
| 5.08 | 9.06 | 2.72 | 4.86 | -16.06 | 244.30 | 14.68 | 219.70 | 0.3829 | -917.6 | -824.2 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -15.42 | 244.06 | 14.44 | 220.37 | 0.3727 | -793.0 | -686.7 | |
| 0.00 | 1.90 | 0.00 | 1.01 | -14.37 | 243.92 | 14.30 | 222.06 | 0.3588 | -1075.0 | -905.5 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -17.98 | 243.96 | 14.34 | 215.92 | 0.4033 | 888.0 | 681.5 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -15.86 | 243.76 | 14.15 | 219.01 | 0.3751 | -978.0 | -801.2 | |
| 0.00 | 1.90 | 0.00 | 1.02 | -16.05 | 243.61 | 14.00 | 218.39 | 0.3759 | -1063.0 | -729.6 | |
| 0.00 | 1.45 | 0.00 | 0.78 | -16.24 | 243.56 | 13.95 | 217.96 | 0.3777 | -839.0 | -700.8 | |
| 0.00 | 6.07 | 0.00 | 3.24 | -15.99 | 243.32 | 13.70 | 217.91 | 0.3721 | -928.0 | -858.2 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -16.53 | 243.32 | 13.70 | 217.01 | 0.3790 | -670.0 | -544.7 | |
| 0.00 | 4.35 | 0.00 | 2.32 | -16.18 | 243.07 | 13.45 | 217.09 | 0.3720 | -844.0 | -766.6 | |
| 0.00 | 4.08 | 0.00 | 2.17 | -15.67 | 242.84 | 13.22 | 217.50 | 0.3633 | -987.0 | -615.2 | |
| 2.27 | 5.35 | 1.21 | 2.85 | -16.02 | 242.83 | 13.21 | 216.88 | 0.3676 | -1009.5 | -880.3 | |
| 0.00 | 2.27 | 0.00 | 1.21 | -17.52 | 241.82 | 12.21 | 212.39 | 0.3780 | -867.0 | -733.4 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -20.10 | 239.97 | 10.35 | 205.09 | 0.3995 | -890.0 | -677.7 | |
| 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. | |