| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.04 | 30.40 | 21.21 | 42.45 | -12.33 | 155.02 | 70.19 | 259.51 | 0.9359 | -10.8 | 58.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-04 15:00:28 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 |
| 8.47 | 12.61 | 12.76 | 18.99 | -12.15 | 156.65 | 71.82 | 259.60 | 0.9458 | 295.7 | 281.4 | |
| 0.00 | 0.60 | 0.00 | 0.89 | -12.08 | 156.21 | 71.38 | 259.71 | 0.9433 | 448.0 | 410.6 | |
| 0.00 | 2.16 | 0.00 | 3.08 | -12.77 | 155.52 | 70.69 | 259.01 | 0.9391 | 281.0 | 235.7 | |
| 0.00 | 0.60 | 0.00 | 0.82 | -10.96 | 154.37 | 69.54 | 261.02 | 0.9328 | -227.0 | -178.7 | |
| 0.00 | 0.95 | 0.00 | 1.29 | -12.87 | 154.40 | 69.57 | 258.96 | 0.9323 | 287.0 | 274.9 | |
| 0.00 | 0.43 | 0.00 | 0.56 | -11.73 | 153.23 | 68.40 | 260.26 | 0.9254 | -484.0 | -438.6 | |
| 0.95 | 11.32 | 1.24 | 14.57 | -12.26 | 153.35 | 68.52 | 259.68 | 0.9260 | -293.9 | -227.9 | |
| 0.00 | 0.69 | 0.00 | 0.89 | -12.07 | 153.16 | 68.34 | 259.89 | 0.9248 | -524.0 | -508.8 | |
| 0.00 | 1.04 | 0.00 | 1.36 | -13.14 | 153.69 | 68.86 | 258.71 | 0.9278 | 210.0 | 204.9 | |
| 5.62 | -7.00 | 7.21 | -7.00 | -12.51 | 153.07 | 68.24 | 259.42 | 0.9240 | -514.0 | 999999 | |
| 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. | |