| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.37 | 341.32 | 39.10 | 179.50 | 19.39 | 123.51 | 5.05 | 345.85 | 0.3372 | 283.1 | 157.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-04 14:58:56 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 |
| 1.11 | 15.01 | 0.59 | 8.00 | 20.07 | 127.77 | 9.30 | 335.65 | 0.3697 | -839.4 | -740.2 | |
| 2.56 | -1.00 | 1.36 | -1.00 | 20.23 | 127.74 | 9.28 | 335.89 | 0.3719 | -920.0 | 999999 | |
| 2.64 | 15.27 | 1.41 | 8.11 | 19.94 | 127.25 | 8.78 | 336.70 | 0.3645 | -1159.9 | -753.7 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 19.66 | 126.85 | 8.39 | 337.32 | 0.3578 | -843.0 | -724.5 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 21.08 | 126.58 | 8.11 | 339.48 | 0.3773 | -561.0 | -454.0 | |
| 1.19 | 23.12 | 0.63 | 12.23 | 19.54 | 126.47 | 8.00 | 338.12 | 0.3535 | -1059.8 | -825.8 | |
| 0.00 | 2.56 | 0.00 | 1.36 | 20.35 | 126.41 | 7.95 | 339.13 | 0.3655 | -945.0 | -782.5 | |
| 0.00 | 2.05 | 0.00 | 1.09 | 20.64 | 126.36 | 7.90 | 339.54 | 0.3695 | -930.0 | -620.5 | |
| 2.99 | 4.01 | 1.58 | 2.13 | 20.01 | 126.30 | 7.83 | 339.04 | 0.3596 | -1023.2 | -856.5 | |
| 0.00 | 10.07 | 0.00 | 5.37 | 20.95 | 126.25 | 7.79 | 340.11 | 0.3736 | -1072.0 | -818.2 | |
| 6.82 | -6.00 | 3.61 | -6.00 | 19.66 | 126.12 | 7.66 | 339.10 | 0.3533 | -1057.0 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 20.20 | 126.09 | 7.62 | 339.75 | 0.3612 | -816.0 | -622.0 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 21.02 | 125.94 | 7.47 | 340.92 | 0.3729 | -679.0 | -509.8 | |
| 1.19 | 3.16 | 0.63 | 1.67 | 19.60 | 125.52 | 7.05 | 340.55 | 0.3490 | -954.2 | -778.7 | |
| 0.00 | 3.33 | 0.00 | 1.75 | 18.92 | 125.40 | 6.93 | 340.15 | 0.3377 | -1028.0 | -881.2 | |
| 0.00 | 2.30 | 0.00 | 1.22 | 19.85 | 125.44 | 6.97 | 341.01 | 0.3524 | -775.0 | -500.9 | |
| 0.00 | 1.71 | 0.00 | 0.90 | 18.76 | 125.36 | 6.89 | 340.09 | 0.3351 | -857.0 | -646.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 19.04 | 125.24 | 6.78 | 340.68 | 0.3388 | -627.0 | -510.6 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 19.67 | 124.99 | 6.52 | 341.98 | 0.3471 | -429.0 | -363.0 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 19.63 | 124.13 | 5.67 | 344.17 | 0.3426 | 965.0 | 743.1 | |
| 0.43 | 1.36 | 0.22 | 0.72 | 19.23 | 124.06 | 5.59 | 344.03 | 0.3358 | 857.2 | 763.4 | |
| 1.36 | 2.47 | 0.73 | 1.32 | 21.33 | 123.97 | 5.51 | 345.90 | 0.3686 | 904.5 | 728.3 | |
| 2.22 | 3.07 | 1.16 | 1.61 | 18.76 | 123.88 | 5.42 | 344.09 | 0.3276 | 895.3 | 780.7 | |
| 1.79 | 237.50 | 0.94 | 124.41 | 19.57 | 123.09 | 4.63 | 346.92 | 0.3373 | 996.4 | 485.0 | |
| 2.39 | -24.00 | 1.26 | -24.00 | 19.60 | 122.94 | 4.47 | 347.37 | 0.3372 | 854.1 | 999999 | |
| 5.20 | -24.00 | 2.73 | -24.00 | 19.48 | 122.71 | 4.25 | 347.89 | 0.3344 | 1009.1 | 999999 | |
| 1.79 | -24.00 | 0.94 | -24.00 | 19.20 | 122.64 | 4.18 | 347.90 | 0.3297 | 972.9 | 999999 | |
| 33.44 | -24.00 | 17.50 | -24.00 | 18.92 | 122.29 | 3.83 | 348.71 | 0.3239 | 1237.3 | 999999 | |
| 1.02 | -24.00 | 0.54 | -24.00 | 19.39 | 121.99 | 3.52 | 349.86 | 0.3306 | 821.9 | 999999 | |
| 0.00 | 2.30 | 0.00 | 1.23 | 21.68 | 122.04 | 3.58 | 350.89 | 0.3679 | 743.0 | 619.4 | |
| 2.22 | -24.00 | 1.16 | -24.00 | 19.57 | 121.93 | 3.46 | 350.12 | 0.3335 | 873.3 | 999999 | |
| 1.79 | -24.00 | 0.94 | -24.00 | 19.73 | 121.78 | 3.31 | 350.64 | 0.3356 | 816.1 | 999999 | |
| 2.22 | 2.82 | 1.17 | 1.49 | 20.99 | 121.65 | 3.18 | 351.59 | 0.3557 | 810.3 | 647.3 | |
| 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. | |