| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.02 | 107.53 | 18.71 | 72.38 | -4.83 | 84.25 | -41.68 | 101.95 | 0.6794 | 266.5 | 224.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-01 18:00:28 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 | 1.56 | 0.00 | 1.00 | -7.62 | 88.13 | -37.81 | 107.48 | 0.6393 | 292.0 | 282.4 | |
| 1.47 | 4.33 | 0.96 | 2.82 | -6.02 | 86.63 | -39.30 | 104.49 | 0.6530 | 749.2 | 576.0 | |
| 0.00 | 0.87 | 0.00 | 0.57 | -5.29 | 86.15 | -39.79 | 103.23 | 0.6569 | -544.0 | -413.7 | |
| 0.00 | 1.64 | 0.00 | 1.08 | -4.91 | 86.02 | -39.91 | 102.61 | 0.6574 | -762.0 | -527.7 | |
| 0.00 | 1.38 | 0.00 | 0.92 | -6.64 | 85.83 | -40.10 | 105.10 | 0.6651 | -581.0 | -519.9 | |
| 0.00 | 1.38 | 0.00 | 0.91 | -4.26 | 85.76 | -40.18 | 101.56 | 0.6591 | 535.0 | 323.9 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -5.71 | 85.57 | -40.37 | 103.65 | 0.6656 | -349.0 | -348.7 | |
| 0.00 | 2.08 | 0.00 | 1.38 | -5.99 | 85.50 | -40.44 | 104.03 | 0.6672 | -643.0 | -557.6 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -5.08 | 85.58 | -40.36 | 102.72 | 0.6636 | -527.0 | -461.7 | |
| 0.00 | 3.63 | 0.00 | 2.41 | -5.61 | 85.30 | -40.64 | 103.41 | 0.6686 | -481.0 | -345.5 | |
| 0.69 | 1.90 | 0.46 | 1.26 | -5.28 | 85.25 | -40.69 | 102.91 | 0.6684 | -892.1 | -691.3 | |
| 4.76 | 8.74 | 3.18 | 5.84 | -5.68 | 84.94 | -41.00 | 103.40 | 0.6735 | 652.5 | 390.2 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -5.29 | 84.97 | -40.97 | 102.84 | 0.6719 | 282.0 | 409.7 | |
| 11.94 | 44.64 | 7.97 | 29.75 | -4.25 | 84.73 | -41.21 | 101.24 | 0.6722 | 1073.0 | 567.0 | |
| 2.34 | 4.33 | 1.56 | 2.89 | -4.73 | 84.66 | -41.28 | 101.93 | 0.6744 | 730.1 | 514.0 | |
| 3.37 | -14.00 | 2.25 | -14.00 | -4.05 | 84.58 | -41.35 | 100.90 | 0.6735 | 843.3 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.75 | -4.89 | 84.52 | -41.41 | 102.12 | 0.6764 | 584.0 | 502.5 | |
| 1.21 | -14.00 | 0.81 | -14.00 | -4.27 | 84.37 | -41.57 | 101.16 | 0.6768 | 596.9 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.93 | -3.43 | 84.26 | -41.68 | 99.92 | 0.6761 | 571.0 | 467.0 | |
| 1.12 | 2.68 | 0.76 | 1.80 | -3.91 | 84.19 | -41.74 | 100.60 | 0.6781 | 692.3 | 555.7 | |
| 0.00 | 2.60 | 0.00 | 1.75 | -4.88 | 84.04 | -41.89 | 101.96 | 0.6824 | 719.0 | 548.7 | |
| 1.12 | 4.07 | 0.76 | 2.74 | -3.68 | 84.01 | -41.93 | 100.22 | 0.6799 | 658.0 | 558.2 | |
| 0.00 | 1.30 | 0.00 | 0.88 | -5.13 | 83.90 | -42.03 | 102.28 | 0.6848 | 216.0 | 239.1 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -5.09 | 83.50 | -42.44 | 102.10 | 0.6897 | 438.0 | 343.2 | |
| 0.00 | 1.73 | 0.00 | 1.18 | -4.68 | 83.41 | -42.52 | 101.48 | 0.6898 | 602.0 | 502.5 | |
| 0.00 | 3.63 | 0.00 | 2.48 | -4.50 | 83.26 | -42.67 | 101.19 | 0.6912 | 564.0 | 367.4 | |
| 0.00 | 1.56 | 0.00 | 1.09 | -4.87 | 81.96 | -43.98 | 101.35 | 0.7080 | -445.0 | -469.3 | |
| 0.00 | 1.04 | 0.00 | 0.73 | -5.13 | 81.68 | -44.25 | 101.63 | 0.7119 | -558.0 | -533.4 | |
| 0.00 | 2.16 | 0.00 | 1.60 | -6.26 | 79.12 | -46.81 | 102.46 | 0.7446 | -682.0 | -501.3 | |
| 0.00 | 2.16 | 0.00 | 1.61 | -6.50 | 78.65 | -47.29 | 102.65 | 0.7505 | -730.0 | -603.1 | |
| 0.00 | 1.38 | 0.00 | 1.03 | -6.26 | 78.55 | -47.39 | 102.31 | 0.7511 | -672.0 | -478.3 | |
| 0.00 | 0.61 | 0.00 | 0.45 | -5.71 | 78.21 | -47.72 | 101.50 | 0.7537 | -401.0 | -420.6 | |
| 0.00 | 1.12 | 0.00 | 0.85 | -5.48 | 77.97 | -47.97 | 101.14 | 0.7559 | -370.0 | -353.4 | |
| 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. | |