SDO HMI 2014-07-05 02:00:40 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 |
| 68.93 | 399.08 | 35.07 | 203.52 | 15.12 | 260.72 | -5.96 | 359.70 | 0.2330 | -520.9 | -214.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-05 02:00:40 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 | 1.00 | 0.00 | 0.50 | 12.30 | 266.85 | 0.17 | 358.95 | 0.1572 | 771.0 | 531.7 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 12.79 | 265.13 | -1.55 | 9.08 | 0.1679 | -974.0 | -762.4 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 13.38 | 265.13 | -1.55 | 8.56 | 0.1779 | -997.0 | -778.7 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 13.38 | 264.97 | -1.71 | 9.41 | 0.1783 | -713.0 | -613.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 16.37 | 264.44 | -2.24 | 9.40 | 0.2303 | -812.0 | -603.6 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 12.86 | 264.29 | -2.39 | 13.78 | 0.1718 | -777.0 | -539.6 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 14.62 | 264.11 | -2.57 | 12.45 | 0.2020 | -932.0 | -740.0 | |
| 0.00 | 3.00 | 0.00 | 1.51 | 12.76 | 263.13 | -3.55 | 20.16 | 0.1760 | -902.0 | -801.7 | |
| 1.18 | 4.63 | 0.60 | 2.34 | 14.12 | 262.10 | -4.58 | 22.38 | 0.2042 | -1026.7 | -709.4 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 11.09 | 262.15 | -4.53 | 29.69 | 0.1571 | -815.0 | -646.0 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 14.31 | 262.04 | -4.64 | 22.32 | 0.2075 | -857.0 | -669.7 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 13.16 | 262.03 | -4.65 | 24.74 | 0.1896 | -1082.0 | -912.2 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 12.57 | 262.01 | -4.68 | 26.24 | 0.1807 | -1051.0 | -876.5 | |
| 54.32 | 292.74 | 27.62 | 148.95 | 15.36 | 261.86 | -4.82 | 21.19 | 0.2254 | -1443.5 | -362.7 | |
| 4.45 | -14.00 | 2.26 | -14.00 | 14.71 | 261.62 | -5.06 | 23.31 | 0.2166 | -1125.8 | 999999 | |
| 1.91 | -14.00 | 0.97 | -14.00 | 15.92 | 261.34 | -5.35 | 22.27 | 0.2375 | -779.9 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 12.01 | 261.33 | -5.35 | 31.02 | 0.1779 | -934.0 | -809.2 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 11.98 | 261.11 | -5.57 | 32.13 | 0.1794 | -944.0 | -680.8 | |
| 0.45 | 1.63 | 0.23 | 0.82 | 11.37 | 261.00 | -5.69 | 34.63 | 0.1717 | -1088.8 | -890.3 | |
| 0.00 | 2.36 | 0.00 | 1.21 | 17.36 | 260.37 | -6.31 | 23.34 | 0.2662 | 658.0 | 427.7 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 16.54 | 260.36 | -6.32 | 24.70 | 0.2537 | -468.0 | -206.1 | |
| 0.00 | 3.27 | 0.00 | 1.65 | 12.38 | 260.29 | -6.40 | 34.52 | 0.1929 | -760.0 | -681.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 16.23 | 259.99 | -6.69 | 26.53 | 0.2517 | 695.0 | 522.3 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 14.73 | 259.97 | -6.71 | 29.64 | 0.2295 | -941.0 | -827.5 | |
| 0.00 | 2.45 | 0.00 | 1.25 | 15.67 | 259.72 | -6.96 | 28.54 | 0.2454 | 952.0 | 798.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 15.91 | 259.55 | -7.13 | 28.61 | 0.2504 | 910.0 | 675.1 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 11.97 | 259.51 | -7.17 | 38.91 | 0.1953 | -715.0 | -681.5 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 11.66 | 258.92 | -7.76 | 42.16 | 0.1979 | -743.0 | -609.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.32 | 258.55 | -8.13 | 33.16 | 0.2505 | 634.0 | 462.8 | |
| 3.63 | 7.63 | 1.85 | 3.88 | 13.61 | 258.36 | -8.32 | 38.09 | 0.2291 | -1049.4 | -847.2 | |
| 0.27 | -30.00 | 0.14 | -30.00 | 13.57 | 258.17 | -8.51 | 38.79 | 0.2307 | -815.3 | 999999 | |
| 1.63 | 7.45 | 0.84 | 3.83 | 16.09 | 257.69 | -8.99 | 34.07 | 0.2693 | 970.7 | 752.4 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 13.01 | 257.62 | -9.06 | 42.17 | 0.2296 | -745.0 | -573.6 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 16.31 | 257.42 | -9.26 | 34.37 | 0.2748 | 795.0 | 698.8 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 16.15 | 257.33 | -9.35 | 34.97 | 0.2735 | 1017.0 | 895.0 | |
| 1.09 | 11.99 | 0.56 | 6.18 | 16.18 | 257.07 | -9.61 | 35.63 | 0.2764 | 1089.8 | 845.2 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 15.71 | 256.90 | -9.78 | 37.16 | 0.2719 | 932.0 | 747.2 | |
| 0.00 | 2.63 | 0.00 | 1.36 | 16.71 | 256.69 | -9.99 | 35.52 | 0.2872 | 931.0 | 825.7 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 16.98 | 256.16 | -10.52 | 36.33 | 0.2961 | 798.0 | 595.2 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 14.17 | 255.92 | -10.77 | 43.68 | 0.2634 | 792.0 | 640.8 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 12.82 | 253.58 | -13.10 | 52.95 | 0.2782 | 742.0 | 468.5 | |
| 0.00 | 1.91 | 0.00 | 0.99 | 13.12 | 253.11 | -13.57 | 53.00 | 0.2873 | 856.0 | 724.7 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 17.89 | 252.73 | -13.95 | 42.14 | 0.3435 | -634.0 | -398.2 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 10.35 | 252.99 | -13.69 | 61.89 | 0.2651 | 829.0 | 772.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 14.36 | 252.75 | -13.93 | 50.32 | 0.3044 | 920.0 | 681.4 | |
| 0.00 | 2.00 | 0.00 | 1.06 | 17.47 | 251.81 | -14.88 | 44.79 | 0.3491 | 705.0 | 578.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 10.37 | 252.13 | -14.55 | 63.19 | 0.2781 | 906.0 | 684.4 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 10.48 | 251.07 | -15.61 | 64.36 | 0.2949 | 754.0 | 628.9 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 12.19 | 250.68 | -16.00 | 59.80 | 0.3131 | 708.0 | 553.7 | |
| 0.00 | 2.63 | 0.00 | 1.38 | 12.59 | 250.17 | -16.51 | 59.45 | 0.3235 | 725.0 | 641.4 | |
| 0.00 | 2.00 | 0.00 | 1.05 | 13.42 | 249.95 | -16.73 | 57.54 | 0.3333 | 936.0 | 700.9 | |
| 0.00 | 2.18 | 0.00 | 1.15 | 14.13 | 249.90 | -16.79 | 55.80 | 0.3401 | 651.0 | 476.7 | |
| 0.00 | 3.09 | 0.00 | 1.65 | 17.31 | 249.43 | -17.26 | 49.18 | 0.3758 | 116.0 | 262.6 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 16.87 | 249.00 | -17.68 | 50.78 | 0.3767 | 685.0 | 564.9 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 16.16 | 248.13 | -18.55 | 53.57 | 0.3814 | 679.0 | 535.2 | |
| 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. | |