| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.94 | 293.19 | 33.56 | 159.87 | 9.61 | 54.42 | 23.58 | 287.33 | 0.4137 | -431.1 | -252.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-13 22:58:58 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 |
| 30.01 | 177.77 | 16.70 | 98.95 | 9.45 | 57.33 | 26.49 | 284.91 | 0.4573 | -1218.6 | -400.3 | |
| 0.00 | 1.89 | 0.00 | 1.04 | 6.03 | 57.00 | 26.16 | 277.49 | 0.4441 | -730.0 | -569.5 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 9.66 | 56.05 | 25.21 | 285.99 | 0.4386 | -932.0 | -702.3 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 11.81 | 56.10 | 25.27 | 290.66 | 0.4484 | -798.0 | -538.9 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 11.79 | 55.97 | 25.13 | 290.69 | 0.4463 | -734.0 | -426.5 | |
| 3.53 | 5.59 | 1.94 | 3.08 | 11.52 | 55.68 | 24.84 | 290.32 | 0.4407 | -942.9 | -634.0 | |
| 0.00 | 1.55 | 0.00 | 0.85 | 11.62 | 55.25 | 24.41 | 290.82 | 0.4350 | -751.0 | -600.8 | |
| 1.38 | 25.03 | 0.73 | 13.31 | 9.63 | 51.56 | 20.72 | 288.71 | 0.3700 | -819.8 | -762.8 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 10.58 | 51.60 | 20.76 | 291.15 | 0.3752 | -438.0 | -356.0 | |
| 0.00 | 1.89 | 0.00 | 1.01 | 9.03 | 51.43 | 20.59 | 287.25 | 0.3653 | -553.0 | -514.2 | |
| 2.58 | -8.00 | 1.37 | -8.00 | 9.78 | 51.38 | 20.54 | 289.25 | 0.3679 | -926.3 | 999999 | |
| 7.40 | -8.00 | 3.93 | -8.00 | 9.45 | 51.33 | 20.49 | 288.43 | 0.3655 | -1096.3 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.69 | 10.08 | 51.34 | 20.50 | 290.07 | 0.3686 | -707.0 | -564.3 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 9.91 | 51.13 | 20.29 | 289.78 | 0.3647 | -892.0 | -740.6 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 9.61 | 50.95 | 20.11 | 289.14 | 0.3605 | -916.0 | -787.5 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 9.94 | 50.88 | 20.04 | 290.08 | 0.3609 | -828.0 | -682.6 | |
| 0.00 | 1.29 | 0.00 | 0.68 | 9.06 | 49.83 | 19.00 | 288.55 | 0.3406 | 446.0 | 333.5 | |
| 0.00 | 2.24 | 0.00 | 1.18 | 9.27 | 49.62 | 18.79 | 289.33 | 0.3383 | 616.0 | 396.0 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 9.10 | 49.36 | 18.52 | 289.06 | 0.3333 | -507.0 | -381.4 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 8.93 | 49.10 | 18.26 | 288.78 | 0.3284 | 517.0 | 438.6 | |
| 3.53 | 20.64 | 1.85 | 10.81 | 9.38 | 48.84 | 18.00 | 290.34 | 0.3266 | 908.1 | 581.1 | |
| 4.82 | -21.00 | 2.52 | -21.00 | 9.11 | 48.73 | 17.89 | 289.66 | 0.3235 | 1080.5 | 999999 | |
| 2.32 | 6.45 | 1.22 | 3.38 | 10.31 | 48.70 | 17.86 | 293.15 | 0.3297 | -953.0 | -898.7 | |
| 0.00 | 2.58 | 0.00 | 1.35 | 9.63 | 47.97 | 17.13 | 291.97 | 0.3145 | -927.0 | -718.1 | |
| 0.00 | 2.32 | 0.00 | 1.21 | 11.16 | 47.42 | 16.58 | 297.14 | 0.3161 | 698.0 | 583.0 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 8.78 | 46.67 | 15.84 | 290.74 | 0.2897 | 790.0 | 619.1 | |
| 2.41 | 24.51 | 1.25 | 12.70 | 10.13 | 46.55 | 15.71 | 295.20 | 0.2959 | 835.8 | 810.9 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 10.49 | 46.54 | 15.70 | 296.32 | 0.2982 | 809.0 | 676.6 | |
| 3.96 | -27.00 | 2.05 | -27.00 | 9.83 | 46.44 | 15.60 | 294.41 | 0.2923 | 1091.3 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 10.07 | 46.14 | 15.30 | 295.58 | 0.2894 | 840.0 | 602.8 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 13.32 | 45.57 | 14.73 | 306.08 | 0.3075 | 792.0 | 563.3 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 10.65 | 45.23 | 14.39 | 298.78 | 0.2800 | 807.0 | 639.8 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 12.40 | 45.07 | 14.24 | 304.36 | 0.2923 | 849.0 | 680.6 | |
| 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. | |