| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.88 | 132.93 | 20.13 | 86.60 | 16.32 | 350.51 | -38.89 | 67.87 | 0.6524 | -38.6 | 95.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-30 18:59:11 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 | 2.09 | 0.00 | 1.26 | 19.20 | 357.66 | -31.74 | 59.77 | 0.5771 | -668.0 | -604.0 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 19.22 | 357.20 | -32.20 | 60.05 | 0.5829 | -699.0 | -519.8 | |
| 0.00 | 1.00 | 0.00 | 0.64 | 20.71 | 352.89 | -36.51 | 60.36 | 0.6425 | -700.0 | -558.7 | |
| 0.00 | 1.91 | 0.00 | 1.21 | 18.09 | 352.85 | -36.55 | 64.25 | 0.6307 | -813.0 | -686.9 | |
| 0.00 | 1.54 | 0.00 | 0.97 | 15.79 | 353.13 | -36.27 | 67.64 | 0.6177 | -890.0 | -737.5 | |
| 1.91 | 34.05 | 1.20 | 21.60 | 16.16 | 352.82 | -36.58 | 67.21 | 0.6231 | -904.2 | -602.5 | |
| 0.00 | 1.00 | 0.00 | 0.63 | 14.60 | 352.98 | -36.42 | 69.58 | 0.6153 | -672.0 | -489.2 | |
| 11.62 | -6.00 | 7.40 | -6.00 | 16.18 | 352.30 | -37.10 | 67.41 | 0.6297 | -699.3 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.84 | 19.92 | 351.06 | -38.33 | 62.43 | 0.6601 | -582.0 | -445.4 | |
| 2.91 | 9.81 | 1.86 | 6.30 | 16.41 | 351.80 | -37.60 | 67.26 | 0.6368 | -711.7 | -462.0 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 16.82 | 351.67 | -37.73 | 66.70 | 0.6400 | -457.0 | -371.1 | |
| 0.00 | 4.45 | 0.00 | 2.84 | 15.32 | 351.88 | -37.52 | 68.90 | 0.6318 | -707.0 | -477.3 | |
| 0.00 | 1.27 | 0.00 | 0.82 | 17.51 | 351.38 | -38.02 | 65.80 | 0.6462 | -579.0 | -483.6 | |
| 0.00 | 1.09 | 0.00 | 0.70 | 16.68 | 351.18 | -38.22 | 67.12 | 0.6456 | -441.0 | -277.3 | |
| 0.00 | 0.64 | 0.00 | 0.42 | 18.62 | 350.31 | -39.09 | 64.65 | 0.6635 | -508.0 | -330.9 | |
| 0.00 | 1.09 | 0.00 | 0.72 | 18.46 | 350.27 | -39.13 | 64.89 | 0.6633 | -650.0 | -455.8 | |
| 2.00 | 38.50 | 1.31 | 25.42 | 15.73 | 349.81 | -39.59 | 69.07 | 0.6591 | 998.8 | 610.7 | |
| 2.00 | -17.00 | 1.32 | -17.00 | 15.90 | 349.43 | -39.97 | 68.94 | 0.6642 | 896.6 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.90 | 15.37 | 349.52 | -39.88 | 69.69 | 0.6615 | 685.0 | 633.0 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 15.65 | 349.41 | -39.99 | 69.32 | 0.6637 | 749.0 | 602.2 | |
| 2.09 | -17.00 | 1.39 | -17.00 | 16.04 | 348.90 | -40.50 | 68.92 | 0.6712 | 681.6 | 999999 | |
| 1.09 | -17.00 | 0.73 | -17.00 | 16.26 | 348.80 | -40.60 | 68.64 | 0.6730 | 839.6 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.85 | 15.72 | 348.60 | -40.80 | 69.49 | 0.6738 | 597.0 | 503.6 | |
| 2.81 | 17.61 | 1.91 | 11.91 | 16.93 | 348.08 | -41.32 | 67.94 | 0.6838 | 850.1 | 681.7 | |
| 0.00 | 3.72 | 0.00 | 2.48 | 14.66 | 348.64 | -40.76 | 71.03 | 0.6702 | 596.0 | 598.1 | |
| 0.00 | 1.09 | 0.00 | 0.72 | 14.47 | 348.68 | -40.72 | 71.29 | 0.6691 | 810.0 | 676.8 | |
| 1.09 | -24.00 | 0.74 | -24.00 | 17.09 | 347.95 | -41.45 | 67.76 | 0.6858 | 718.1 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.66 | 13.76 | 348.76 | -40.64 | 72.32 | 0.6663 | 701.0 | 618.5 | |
| 3.36 | -24.00 | 2.27 | -24.00 | 16.55 | 348.05 | -41.35 | 68.49 | 0.6829 | 847.0 | 999999 | |
| 0.00 | 1.54 | 0.00 | 1.06 | 18.11 | 347.36 | -42.04 | 66.54 | 0.6961 | 827.0 | 673.3 | |
| 0.00 | 0.73 | 0.00 | 0.49 | 16.76 | 347.74 | -41.66 | 68.29 | 0.6873 | 584.0 | 451.1 | |
| 0.00 | 1.09 | 0.00 | 0.74 | 16.14 | 347.86 | -41.54 | 69.14 | 0.6839 | 643.0 | 500.1 | |
| 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. | |