| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.13 | 187.88 | 45.92 | 217.59 | -20.47 | 109.92 | -62.36 | 113.28 | 0.9049 | 266.8 | 149.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-30 12:58:56 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 |
| 1.37 | 62.46 | 1.57 | 71.84 | -23.74 | 110.95 | -61.33 | 117.05 | 0.9037 | 500.3 | 240.0 | |
| 11.96 | -1.00 | 13.78 | -1.00 | -23.32 | 110.67 | -61.61 | 116.54 | 0.9048 | 594.6 | 999999 | |
| 0.00 | 1.28 | 0.00 | 1.45 | -22.51 | 110.97 | -61.31 | 115.73 | 0.9014 | 144.0 | 127.0 | |
| 0.00 | 1.20 | 0.00 | 1.44 | -23.15 | 109.28 | -63.00 | 116.04 | 0.9136 | 166.0 | 202.4 | |
| 0.94 | 2.05 | 1.11 | 2.42 | -22.50 | 109.67 | -62.60 | 115.43 | 0.9101 | 331.7 | 321.3 | |
| 0.00 | 4.53 | 0.00 | 5.55 | -22.77 | 108.73 | -63.55 | 115.52 | 0.9165 | 53.0 | 42.1 | |
| 0.00 | 2.14 | 0.00 | 2.59 | -22.19 | 108.93 | -63.35 | 114.94 | 0.9144 | 363.0 | 270.0 | |
| 0.00 | 0.60 | 0.00 | 0.73 | -21.84 | 108.71 | -63.57 | 114.52 | 0.9153 | 141.0 | 94.6 | |
| 14.61 | 79.20 | 15.73 | 85.27 | -16.88 | 111.38 | -60.90 | 109.64 | 0.8897 | 719.9 | 264.5 | |
| 1.71 | 2.73 | 2.32 | 3.70 | -22.88 | 106.11 | -66.16 | 115.13 | 0.9324 | -431.4 | -509.7 | |
| 7.09 | 24.09 | 9.46 | 32.38 | -22.01 | 106.30 | -65.98 | 114.24 | 0.9303 | -525.3 | -164.0 | |
| 0.00 | 0.94 | 0.00 | 1.25 | -21.69 | 106.27 | -66.01 | 113.90 | 0.9301 | -419.0 | -401.2 | |
| 1.45 | 6.66 | 1.95 | 8.97 | -21.41 | 106.13 | -66.15 | 113.57 | 0.9306 | -665.9 | -461.7 | |
| 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. | |