| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 135.93 | 625.49 | 71.16 | 328.16 | 7.96 | 128.95 | -17.52 | 66.55 | 0.3250 | 29.6 | 29.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-02 11:58:56 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 |
| 0.00 | 1.37 | 0.00 | 0.70 | 8.33 | 134.97 | -11.50 | 56.14 | 0.2386 | 784.0 | 538.1 | |
| 15.28 | 184.19 | 7.79 | 94.00 | 6.81 | 134.07 | -12.40 | 63.55 | 0.2392 | -1379.5 | -427.6 | |
| 16.65 | -2.00 | 8.50 | -2.00 | 7.14 | 133.82 | -12.65 | 62.79 | 0.2455 | -1225.4 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.65 | 3.76 | 133.56 | -12.91 | 76.64 | 0.2303 | -796.0 | -644.1 | |
| 1.54 | -2.00 | 0.79 | -2.00 | 7.20 | 133.27 | -13.20 | 63.55 | 0.2543 | -835.1 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 8.69 | 133.00 | -13.47 | 58.96 | 0.2699 | 840.0 | 666.2 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 8.24 | 132.86 | -13.61 | 60.67 | 0.2683 | -696.0 | -506.1 | |
| 0.00 | 1.88 | 0.00 | 0.96 | 7.70 | 132.73 | -13.74 | 62.69 | 0.2661 | -620.0 | -497.1 | |
| 0.00 | 1.20 | 0.00 | 0.61 | 8.18 | 132.68 | -13.79 | 61.18 | 0.2705 | -775.0 | -622.4 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 7.37 | 132.49 | -13.98 | 64.19 | 0.2673 | -722.0 | -433.5 | |
| 4.44 | 34.24 | 2.28 | 17.61 | 6.99 | 132.41 | -14.06 | 65.64 | 0.2658 | -1090.9 | -828.1 | |
| 0.00 | 5.81 | 0.00 | 2.98 | 6.27 | 132.22 | -14.25 | 68.42 | 0.2643 | -765.0 | -776.7 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 4.29 | 132.11 | -14.35 | 75.87 | 0.2561 | -813.0 | -744.3 | |
| 20.92 | -11.00 | 10.76 | -11.00 | 7.05 | 132.01 | -14.46 | 66.02 | 0.2724 | -1014.3 | 999999 | |
| 0.00 | 2.73 | 0.00 | 1.41 | 6.60 | 131.97 | -14.50 | 67.62 | 0.2703 | -887.0 | -690.4 | |
| 0.00 | 0.85 | 0.00 | 0.44 | 4.17 | 131.84 | -14.63 | 76.56 | 0.2601 | -701.0 | -523.7 | |
| 2.39 | 3.59 | 1.23 | 1.85 | 7.34 | 131.51 | -14.96 | 65.75 | 0.2821 | -950.5 | -776.2 | |
| 0.00 | 7.51 | 0.00 | 3.89 | 7.43 | 131.11 | -15.36 | 66.01 | 0.2888 | -706.0 | -603.3 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 6.74 | 131.04 | -15.43 | 68.33 | 0.2857 | -824.0 | -588.0 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 6.92 | 131.00 | -15.47 | 67.79 | 0.2873 | -790.0 | -630.6 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 7.28 | 130.65 | -15.82 | 67.09 | 0.2949 | -700.0 | -623.1 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 5.02 | 130.44 | -16.03 | 74.73 | 0.2865 | -1049.0 | -842.4 | |
| 0.00 | 3.33 | 0.00 | 1.73 | 7.19 | 130.22 | -16.25 | 67.90 | 0.3010 | -881.0 | -597.4 | |
| 4.44 | 19.13 | 2.33 | 10.04 | 10.68 | 129.77 | -16.70 | 58.49 | 0.3326 | -1037.5 | -793.2 | |
| 0.85 | -24.00 | 0.45 | -24.00 | 10.35 | 129.48 | -16.99 | 59.78 | 0.3342 | -859.4 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 8.53 | 129.57 | -16.90 | 64.69 | 0.3194 | -704.0 | -627.9 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 7.27 | 129.41 | -17.06 | 68.56 | 0.3141 | -850.0 | -592.0 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 7.48 | 129.18 | -17.29 | 68.19 | 0.3188 | -660.0 | -475.4 | |
| 0.00 | 4.35 | 0.00 | 2.28 | 7.42 | 128.68 | -17.79 | 68.90 | 0.3262 | -736.0 | -740.7 | |
| 1.02 | 3.67 | 0.54 | 1.94 | 9.78 | 128.31 | -18.16 | 62.83 | 0.3467 | -716.1 | -571.4 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 9.00 | 128.36 | -18.11 | 64.84 | 0.3408 | 924.0 | 802.7 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 7.21 | 128.41 | -18.06 | 69.78 | 0.3293 | -853.0 | -726.2 | |
| 8.28 | 11.70 | 4.37 | 6.17 | 8.31 | 127.82 | -18.65 | 67.30 | 0.3445 | 1125.3 | 854.9 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 6.76 | 127.64 | -18.83 | 71.77 | 0.3389 | -710.0 | -573.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 8.61 | 127.49 | -18.98 | 66.84 | 0.3513 | 1141.0 | 949.3 | |
| 5.81 | 8.11 | 3.08 | 4.30 | 8.99 | 127.25 | -19.22 | 66.08 | 0.3573 | 1088.0 | 688.9 | |
| 0.85 | 7.43 | 0.45 | 3.95 | 9.35 | 127.07 | -19.40 | 65.35 | 0.3622 | 906.1 | 831.6 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 6.85 | 126.72 | -19.75 | 72.29 | 0.3537 | -845.0 | -620.5 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 11.06 | 126.03 | -20.44 | 62.31 | 0.3887 | 800.0 | 576.4 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 10.21 | 125.80 | -20.67 | 64.54 | 0.3864 | 899.0 | 700.3 | |
| 51.58 | 279.23 | 27.56 | 149.15 | 8.45 | 125.72 | -20.75 | 68.94 | 0.3772 | 1267.1 | 421.4 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 10.09 | 125.52 | -20.95 | 65.11 | 0.3897 | 887.0 | 722.2 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 11.05 | 125.42 | -21.05 | 62.97 | 0.3974 | 807.0 | 697.5 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 10.54 | 125.39 | -21.08 | 64.18 | 0.3944 | 844.0 | 786.2 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 10.27 | 125.41 | -21.06 | 64.79 | 0.3924 | 950.0 | 837.7 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 10.54 | 125.20 | -21.27 | 64.37 | 0.3972 | 747.0 | 625.7 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 9.94 | 125.24 | -21.23 | 65.74 | 0.3929 | 870.0 | 640.6 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 8.77 | 123.32 | -23.15 | 70.10 | 0.4151 | 806.0 | 672.4 | |
| 1.88 | 2.48 | 1.03 | 1.35 | 9.51 | 122.87 | -23.60 | 68.75 | 0.4254 | 777.5 | 826.9 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 9.42 | 122.45 | -24.02 | 69.27 | 0.4312 | 743.0 | 576.7 | |
| 0.00 | 3.07 | 0.00 | 1.68 | 7.57 | 122.28 | -24.19 | 73.54 | 0.4253 | 768.0 | 665.6 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 13.20 | 121.31 | -25.16 | 62.34 | 0.4693 | 691.0 | 473.4 | |
| 0.00 | 2.31 | 0.00 | 1.28 | 5.99 | 120.36 | -26.11 | 78.04 | 0.4492 | 743.0 | 713.4 | |
| 0.00 | 2.39 | 0.00 | 1.33 | 6.10 | 120.19 | -26.28 | 77.85 | 0.4522 | 772.0 | 614.7 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 12.89 | 118.87 | -27.60 | 64.87 | 0.5009 | 581.0 | 472.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |