| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.20 | 0.00 | 7.55 | 10.82 | 179.85 | 19.57 | 285.61 | 0.3477 | -305.9 | -209.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-05 14:00:36 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 | 1.79 | 0.00 | 0.99 | 10.85 | 186.91 | 26.64 | 279.84 | 0.4487 | -800.0 | -685.0 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 11.47 | 186.84 | 26.56 | 281.22 | 0.4486 | -770.0 | -576.5 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 11.25 | 186.37 | 26.09 | 280.85 | 0.4410 | -686.0 | -472.1 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 10.67 | 186.31 | 26.04 | 279.56 | 0.4392 | -741.0 | -608.5 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 11.92 | 186.40 | 26.13 | 282.35 | 0.4429 | -763.0 | -657.1 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 11.65 | 186.20 | 25.93 | 281.81 | 0.4393 | -662.0 | -523.7 | |
| 0.00 | 1.34 | 0.00 | 0.74 | 11.58 | 185.95 | 25.68 | 281.71 | 0.4353 | -798.0 | -640.9 | |
| 0.00 | 1.88 | 0.00 | 0.95 | 10.15 | 172.80 | 12.52 | 284.18 | 0.2211 | 796.0 | 624.8 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 9.98 | 172.47 | 12.20 | 283.71 | 0.2152 | 869.0 | 597.2 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 3.03 | 170.88 | 10.60 | 248.87 | 0.1978 | -699.0 | -522.0 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 16.47 | 161.03 | 0.75 | 355.51 | 0.1619 | 889.0 | 744.9 | |
| 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. | |