| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.52 | 13.04 | 0.33 | 8.54 | -23.78 | 9.79 | -30.98 | 133.84 | 0.6553 | 489.0 | 448.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-08 05:00:28 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 |
| 0.00 | 1.21 | 0.00 | 0.78 | -24.75 | 12.48 | -28.28 | 137.44 | 0.6385 | 668.0 | 600.7 | |
| 0.52 | 1.73 | 0.33 | 1.12 | -23.38 | 10.47 | -30.29 | 133.95 | 0.6454 | -827.8 | -644.9 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -24.85 | 9.55 | -31.22 | 134.90 | 0.6662 | 722.0 | 546.2 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -21.33 | 10.37 | -30.39 | 131.31 | 0.6296 | 678.0 | 534.2 | |
| 0.00 | 0.35 | 0.00 | 0.23 | -24.99 | 9.39 | -31.37 | 134.93 | 0.6688 | 650.0 | 559.5 | |
| 0.00 | 1.47 | 0.00 | 0.94 | -22.10 | 10.01 | -30.76 | 131.96 | 0.6395 | 702.0 | 542.3 | |
| 0.00 | 1.12 | 0.00 | 0.75 | -24.76 | 9.23 | -31.54 | 134.52 | 0.6685 | 712.0 | 622.8 | |
| 0.00 | 0.86 | 0.00 | 0.58 | -24.80 | 8.87 | -31.90 | 134.27 | 0.6722 | 478.0 | 403.7 | |
| 0.00 | 0.95 | 0.00 | 0.61 | -22.12 | 9.59 | -31.17 | 131.62 | 0.6438 | 616.0 | 532.8 | |
| 0.00 | 1.12 | 0.00 | 0.75 | -24.60 | 8.93 | -31.84 | 134.08 | 0.6700 | 668.0 | 541.2 | |
| 0.00 | 2.24 | 0.00 | 1.49 | -24.34 | 8.81 | -31.95 | 133.67 | 0.6690 | 747.0 | 635.0 | |
| 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. | |