SDO HMI 2014-12-02 06:00:25 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.21 | 187.92 | 19.50 | 93.48 | 4.42 | 84.84 | 0.98 | 276.55 | 0.0885 | -322.2 | -285.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-12-02 06:00:25 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 | 1.11 | 0.00 | 0.56 | 5.72 | 90.54 | 6.69 | 306.84 | 0.1454 | -823.0 | -593.0 | |
| 0.00 | 1.03 | 0.00 | 0.51 | 3.47 | 89.75 | 5.89 | 294.94 | 0.1134 | -796.0 | -614.7 | |
| 0.00 | 0.77 | 0.00 | 0.39 | 7.68 | 89.67 | 5.81 | 320.28 | 0.1578 | -923.0 | -827.7 | |
| 0.00 | 1.37 | 0.00 | 0.68 | 0.36 | 89.29 | 5.43 | 266.05 | 0.0952 | -798.0 | -613.9 | |
| 0.00 | 1.20 | 0.00 | 0.60 | 7.59 | 89.31 | 5.45 | 321.70 | 0.1527 | -905.0 | -762.7 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 4.56 | 88.56 | 4.71 | 309.21 | 0.1060 | -831.0 | -577.0 | |
| 4.36 | 64.17 | 2.17 | 31.98 | 5.40 | 88.18 | 4.33 | 317.23 | 0.1111 | -1101.5 | -600.0 | |
| 5.55 | -7.00 | 2.77 | -7.00 | 5.60 | 87.92 | 4.06 | 320.27 | 0.1107 | -1288.7 | 999999 | |
| 13.84 | -7.00 | 6.89 | -7.00 | 5.60 | 87.47 | 3.61 | 323.51 | 0.1060 | -1292.0 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 3.18 | 87.40 | 3.54 | 304.59 | 0.0752 | -1089.0 | -880.2 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 3.06 | 87.25 | 3.39 | 304.40 | 0.0719 | -920.0 | -709.4 | |
| 0.00 | 4.70 | 0.00 | 2.33 | 3.35 | 87.16 | 3.30 | 308.41 | 0.0737 | -955.0 | -726.7 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 4.12 | 86.90 | 3.04 | 318.13 | 0.0796 | -948.0 | -808.2 | |
| 0.00 | 0.85 | 0.00 | 0.42 | 3.41 | 86.87 | 3.01 | 311.69 | 0.0704 | -899.0 | -727.4 | |
| 0.00 | 1.54 | 0.00 | 0.76 | 3.95 | 86.84 | 2.98 | 317.16 | 0.0766 | -1113.0 | -919.3 | |
| 0.00 | 1.20 | 0.00 | 0.59 | 3.59 | 86.48 | 2.62 | 317.45 | 0.0678 | -987.0 | -845.0 | |
| 0.00 | 4.19 | 0.00 | 2.08 | 3.92 | 86.33 | 2.47 | 322.14 | 0.0705 | -803.0 | -855.4 | |
| 0.00 | 2.82 | 0.00 | 1.40 | 6.32 | 86.23 | 2.37 | 337.09 | 0.1060 | -782.0 | -572.5 | |
| 0.00 | 1.37 | 0.00 | 0.68 | 5.49 | 85.66 | 1.80 | 339.31 | 0.0889 | -1013.0 | -752.9 | |
| 0.00 | 0.94 | 0.00 | 0.47 | 5.31 | 85.45 | 1.59 | 340.87 | 0.0847 | -987.0 | -711.8 | |
| 0.00 | 3.33 | 0.00 | 1.66 | 5.70 | 85.42 | 1.56 | 342.56 | 0.0910 | -1159.0 | -958.2 | |
| 0.00 | 1.28 | 0.00 | 0.64 | 0.96 | 85.32 | 1.46 | 278.62 | 0.0259 | -1003.0 | -845.5 | |
| 0.00 | 1.20 | 0.00 | 0.59 | 5.25 | 85.27 | 1.41 | 342.67 | 0.0828 | -890.0 | -683.5 | |
| 11.19 | 46.23 | 5.55 | 22.93 | 3.54 | 84.35 | 0.49 | 350.08 | 0.0497 | -1208.7 | -532.7 | |
| 3.50 | -24.00 | 1.74 | -24.00 | 3.86 | 84.20 | 0.34 | 353.76 | 0.0550 | -1106.6 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.59 | 1.38 | 83.99 | 0.13 | 348.37 | 0.0114 | -1010.0 | -836.4 | |
| 0.00 | 1.88 | 0.00 | 0.94 | 9.12 | 83.79 | -0.07 | 0.46 | 0.1464 | -882.0 | -659.2 | |
| 0.00 | 0.77 | 0.00 | 0.38 | -0.33 | 82.90 | -0.96 | 138.13 | 0.0253 | -750.0 | -616.6 | |
| 0.00 | 1.37 | 0.00 | 0.68 | 3.72 | 82.28 | -1.58 | 27.98 | 0.0590 | 935.0 | 640.2 | |
| 0.00 | 4.02 | 0.00 | 1.99 | 3.04 | 81.48 | -2.38 | 46.03 | 0.0580 | 915.0 | 821.9 | |
| 0.00 | 3.25 | 0.00 | 1.61 | 2.18 | 81.24 | -2.62 | 61.20 | 0.0523 | 1103.0 | 873.0 | |
| 0.00 | 1.20 | 0.00 | 0.59 | 1.62 | 81.21 | -2.65 | 71.67 | 0.0489 | 894.0 | 658.9 | |
| 0.00 | 2.14 | 0.00 | 1.06 | 4.04 | 81.00 | -2.86 | 40.82 | 0.0765 | 894.0 | 687.8 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 4.49 | 80.02 | -3.84 | 45.61 | 0.0939 | 730.0 | 550.1 | |
| 0.00 | 1.03 | 0.00 | 0.51 | 4.13 | 79.90 | -3.96 | 49.32 | 0.0912 | 1004.0 | 805.1 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 2.83 | 79.64 | -4.22 | 63.60 | 0.0824 | 991.0 | 805.4 | |
| 0.00 | 1.11 | 0.00 | 0.55 | 4.10 | 79.64 | -4.22 | 51.40 | 0.0944 | 948.0 | 664.5 | |
| 0.00 | 1.11 | 0.00 | 0.55 | 0.97 | 79.29 | -4.57 | 87.13 | 0.0802 | 1015.0 | 797.0 | |
| 0.00 | 2.31 | 0.00 | 1.15 | 2.89 | 79.02 | -4.84 | 66.01 | 0.0927 | 933.0 | 743.8 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 4.69 | 78.83 | -5.03 | 51.71 | 0.1118 | 931.0 | 782.4 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -0.27 | 78.69 | -5.17 | 101.09 | 0.0922 | 841.0 | 730.1 | |
| 0.00 | 1.11 | 0.00 | 0.55 | 2.68 | 78.69 | -5.17 | 69.35 | 0.0966 | 910.0 | 643.5 | |
| 0.77 | 1.71 | 0.38 | 0.85 | 4.61 | 78.59 | -5.27 | 53.61 | 0.1142 | 1175.6 | 1009.0 | |
| 0.00 | 1.11 | 0.00 | 0.55 | 4.87 | 78.20 | -5.66 | 53.72 | 0.1224 | 1052.0 | 892.1 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 3.75 | 77.41 | -6.45 | 64.91 | 0.1244 | 1046.0 | 898.0 | |
| 0.00 | 0.94 | 0.00 | 0.47 | 3.13 | 77.41 | -6.45 | 69.61 | 0.1202 | 729.0 | 671.5 | |
| 0.00 | 1.71 | 0.00 | 0.85 | 4.16 | 76.84 | -7.02 | 63.90 | 0.1364 | 851.0 | 739.8 | |
| 0.00 | 0.51 | 0.00 | 0.26 | 5.49 | 76.38 | -7.48 | 57.39 | 0.1546 | 473.0 | 513.5 | |
| 0.00 | 0.77 | 0.00 | 0.38 | 3.63 | 76.15 | -7.71 | 69.33 | 0.1437 | 902.0 | 722.2 | |
| 0.00 | 2.39 | 0.00 | 1.20 | 5.49 | 76.08 | -7.78 | 58.39 | 0.1590 | 927.0 | 577.8 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 6.21 | 75.59 | -8.27 | 56.31 | 0.1727 | 831.0 | 694.7 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 1.79 | 74.94 | -8.92 | 83.18 | 0.1568 | 784.0 | 666.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 5.04 | 71.29 | -12.57 | 70.84 | 0.2306 | 752.0 | 605.8 | |
| 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. | |