| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.83 | 198.29 | 24.33 | 130.66 | 15.63 | 233.40 | 39.18 | 292.61 | 0.6614 | -955.9 | -355.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-28 20:58:56 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 |
| 0.00 | 1.28 | 0.00 | 0.88 | 18.25 | 235.59 | 41.37 | 295.38 | 0.6971 | -509.0 | -434.8 | |
| 3.50 | 3.76 | 2.39 | 2.57 | 17.63 | 235.25 | 41.03 | 294.68 | 0.6909 | -540.8 | -468.3 | |
| 0.00 | 1.37 | 0.00 | 0.93 | 17.82 | 234.93 | 40.71 | 295.08 | 0.6879 | -661.0 | -611.6 | |
| 0.43 | 189.15 | 0.28 | 124.49 | 14.89 | 233.40 | 39.18 | 291.54 | 0.6587 | -858.8 | -348.8 | |
| 25.30 | -4.00 | 16.66 | -4.00 | 15.41 | 233.44 | 39.22 | 292.28 | 0.6610 | -1122.1 | 999999 | |
| 1.79 | -4.00 | 1.18 | -4.00 | 15.72 | 233.03 | 38.81 | 292.90 | 0.6573 | -1033.9 | 999999 | |
| 2.82 | -4.00 | 1.86 | -4.00 | 16.33 | 233.18 | 38.95 | 293.73 | 0.6614 | -762.2 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.83 | 13.48 | 232.49 | 38.26 | 289.79 | 0.6424 | -723.0 | -546.1 | |
| 2.99 | -4.00 | 1.96 | -4.00 | 16.09 | 232.92 | 38.70 | 293.49 | 0.6574 | -868.6 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 19.19 | 232.08 | 37.86 | 298.35 | 0.6609 | -717.0 | -589.9 | |
| 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. | |