| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.78 | 66.30 | 4.94 | 41.93 | 17.03 | 100.69 | 30.13 | 309.48 | 0.6242 | 94.4 | 112.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-05 17:00:28 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 | 1.04 | 0.00 | 0.68 | 15.24 | 105.02 | 34.47 | 303.47 | 0.6570 | -493.0 | -516.4 | |
| 0.00 | 1.04 | 0.00 | 0.69 | 16.52 | 105.01 | 34.46 | 305.14 | 0.6657 | -422.0 | -329.8 | |
| 0.00 | 1.04 | 0.00 | 0.68 | 15.94 | 104.89 | 34.34 | 304.47 | 0.6603 | -293.0 | -348.6 | |
| 0.00 | 1.30 | 0.00 | 0.85 | 16.53 | 104.68 | 34.13 | 305.41 | 0.6622 | -699.0 | -486.2 | |
| 0.00 | 1.47 | 0.00 | 0.96 | 15.75 | 104.19 | 33.64 | 304.79 | 0.6515 | -642.0 | -512.9 | |
| 0.00 | 0.95 | 0.00 | 0.62 | 17.65 | 103.56 | 33.01 | 307.72 | 0.6586 | -410.0 | -350.0 | |
| 0.00 | 2.68 | 0.00 | 1.73 | 16.85 | 102.73 | 32.18 | 307.39 | 0.6439 | -691.0 | -585.0 | |
| 5.96 | 10.20 | 3.82 | 6.54 | 16.43 | 102.36 | 31.81 | 307.17 | 0.6368 | -872.4 | -711.8 | |
| 0.00 | 1.47 | 0.00 | 0.94 | 16.96 | 102.02 | 31.47 | 308.15 | 0.6373 | -836.0 | -765.4 | |
| 0.00 | 1.30 | 0.00 | 0.84 | 18.23 | 102.02 | 31.46 | 309.76 | 0.6472 | -551.0 | -388.7 | |
| 0.00 | 1.21 | 0.00 | 0.76 | 16.03 | 101.16 | 30.61 | 307.69 | 0.6208 | 516.0 | 352.8 | |
| 0.00 | 0.95 | 0.00 | 0.59 | 15.02 | 100.46 | 29.91 | 306.97 | 0.6051 | 633.0 | 514.4 | |
| 0.00 | 1.81 | 0.00 | 1.15 | 17.03 | 100.62 | 30.07 | 309.49 | 0.6231 | -341.0 | -309.1 | |
| 0.00 | 1.47 | 0.00 | 0.91 | 15.20 | 100.28 | 29.73 | 307.39 | 0.6045 | 656.0 | 592.6 | |
| 0.00 | 1.04 | 0.00 | 0.65 | 15.68 | 100.25 | 29.70 | 308.06 | 0.6081 | 686.0 | 614.8 | |
| 0.00 | 2.94 | 0.00 | 1.93 | 20.82 | 101.14 | 30.59 | 313.67 | 0.6599 | 32.0 | 82.2 | |
| 0.35 | 7.09 | 0.22 | 4.46 | 17.03 | 100.23 | 29.68 | 309.87 | 0.6190 | 642.8 | 274.9 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 14.91 | 99.81 | 29.26 | 307.44 | 0.5970 | 635.0 | 537.8 | |
| 0.00 | 2.68 | 0.00 | 1.64 | 14.58 | 99.62 | 29.07 | 307.16 | 0.5922 | 713.0 | 578.3 | |
| 0.00 | 0.95 | 0.00 | 0.58 | 14.80 | 99.51 | 28.96 | 307.56 | 0.5927 | 439.0 | 408.3 | |
| 0.00 | 2.33 | 0.00 | 1.47 | 17.27 | 99.88 | 29.32 | 310.50 | 0.6173 | -388.0 | -362.2 | |
| 0.43 | 4.84 | 0.27 | 3.01 | 16.60 | 99.47 | 28.92 | 310.01 | 0.6074 | 934.4 | 650.4 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 16.16 | 99.23 | 28.67 | 309.68 | 0.6011 | 747.0 | 619.3 | |
| 0.00 | 1.30 | 0.00 | 0.81 | 18.05 | 99.30 | 28.75 | 312.05 | 0.6181 | 738.0 | 605.4 | |
| 0.00 | 2.68 | 0.00 | 1.69 | 18.68 | 99.34 | 28.79 | 312.79 | 0.6240 | 750.0 | 577.2 | |
| 0.00 | 0.95 | 0.00 | 0.61 | 19.74 | 99.37 | 28.82 | 314.05 | 0.6336 | 434.0 | 383.8 | |
| 0.00 | 0.95 | 0.00 | 0.59 | 17.67 | 98.95 | 28.40 | 311.91 | 0.6112 | 948.0 | 786.0 | |
| 0.00 | 1.81 | 0.00 | 1.14 | 18.13 | 98.99 | 28.44 | 312.45 | 0.6157 | 827.0 | 663.0 | |
| 0.00 | 0.95 | 0.00 | 0.59 | 17.93 | 98.89 | 28.33 | 312.30 | 0.6128 | 838.0 | 666.0 | |
| 0.00 | 0.52 | 0.00 | 0.32 | 17.82 | 97.11 | 26.55 | 313.99 | 0.5938 | 379.0 | 421.3 | |
| 0.00 | 1.04 | 0.00 | 0.66 | 21.66 | 97.38 | 26.83 | 318.29 | 0.6328 | 606.0 | 558.7 | |
| 1.04 | 3.46 | 0.63 | 2.09 | 17.05 | 96.22 | 25.67 | 313.97 | 0.5776 | 934.2 | 726.5 | |
| 0.00 | 1.12 | 0.00 | 0.69 | 18.45 | 96.09 | 25.54 | 315.88 | 0.5898 | -644.0 | -474.4 | |
| 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. | |