| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 23.53 | 0.19 | 12.50 | 13.54 | 113.03 | -11.14 | 31.76 | 0.3597 | -766.5 | -647.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-04-30 04:59:07 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 |
| 0.36 | 1.25 | 0.19 | 0.65 | 11.65 | 115.61 | -8.56 | 28.03 | 0.3116 | -1018.5 | -851.0 | |
| 0.00 | 1.16 | 0.00 | 0.60 | 10.60 | 113.99 | -10.18 | 34.17 | 0.3107 | -935.0 | -683.3 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 14.59 | 113.67 | -10.50 | 28.68 | 0.3690 | -899.0 | -762.2 | |
| 0.00 | 1.16 | 0.00 | 0.61 | 10.86 | 113.51 | -10.66 | 34.92 | 0.3187 | -926.0 | -661.8 | |
| 0.00 | 1.78 | 0.00 | 0.95 | 14.88 | 113.15 | -11.02 | 29.47 | 0.3773 | -846.0 | -617.2 | |
| 0.00 | 1.60 | 0.00 | 0.84 | 10.80 | 113.30 | -10.87 | 35.57 | 0.3199 | -922.0 | -662.6 | |
| 0.00 | 1.87 | 0.00 | 0.98 | 10.93 | 113.17 | -11.00 | 35.66 | 0.3229 | -693.0 | -549.5 | |
| 0.00 | 2.67 | 0.00 | 1.42 | 14.12 | 112.84 | -11.33 | 31.22 | 0.3693 | -1133.0 | -918.4 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 14.85 | 112.80 | -11.37 | 30.27 | 0.3797 | -684.0 | -594.2 | |
| 0.00 | 0.71 | 0.00 | 0.40 | 20.10 | 112.46 | -11.71 | 24.86 | 0.4554 | 562.0 | 472.5 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 14.28 | 112.80 | -11.37 | 31.08 | 0.3718 | -906.0 | -733.7 | |
| 0.00 | 2.14 | 0.00 | 1.14 | 14.28 | 112.61 | -11.56 | 31.50 | 0.3735 | -855.0 | -616.5 | |
| 0.00 | 1.69 | 0.00 | 0.91 | 14.54 | 112.53 | -11.64 | 31.30 | 0.3776 | -671.0 | -554.8 | |
| 0.00 | 3.48 | 0.00 | 1.86 | 14.00 | 112.11 | -12.06 | 32.98 | 0.3739 | -757.0 | -668.5 | |
| 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. | |