| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.13 | 0.00 | 10.29 | 5.30 | 25.66 | 7.15 | 328.16 | 0.2448 | -90.0 | -112.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-04-05 23:00:32 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 | 4.75 | 0.00 | 2.43 | 3.55 | 29.18 | 10.67 | 312.42 | 0.2514 | -840.0 | -708.7 | |
| 0.00 | 0.53 | 0.00 | 0.27 | 3.50 | 28.39 | 9.87 | 314.52 | 0.2411 | -717.0 | -631.7 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 3.59 | 28.03 | 9.51 | 315.86 | 0.2378 | -725.0 | -580.8 | |
| 0.00 | 1.58 | 0.00 | 0.80 | 2.11 | 26.68 | 8.16 | 315.60 | 0.2036 | -931.0 | -738.3 | |
| 0.00 | 1.76 | 0.00 | 0.89 | 3.99 | 26.30 | 7.78 | 322.70 | 0.2238 | -797.0 | -675.2 | |
| 0.00 | 1.67 | 0.00 | 0.85 | 4.20 | 26.21 | 7.69 | 323.58 | 0.2258 | -797.0 | -630.9 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 8.12 | 25.05 | 6.53 | 335.57 | 0.2735 | 741.0 | 601.2 | |
| 0.00 | 3.25 | 0.00 | 1.67 | 7.56 | 24.86 | 6.34 | 335.35 | 0.2636 | 793.0 | 655.3 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 7.80 | 24.77 | 6.25 | 336.03 | 0.2668 | 744.0 | 592.1 | |
| 0.00 | 1.58 | 0.00 | 0.81 | 7.25 | 19.01 | 0.49 | 357.93 | 0.2351 | 816.0 | 627.3 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 7.34 | 16.98 | -1.54 | 6.44 | 0.2381 | 723.0 | 635.9 | |
| 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. | |