| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.44 | 52.09 | 7.51 | 27.15 | 7.05 | 112.65 | 18.01 | 278.60 | 0.3117 | 92.7 | -174.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-18 02:00:40 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 |
| 0.91 | 10.89 | 0.48 | 5.70 | 6.87 | 113.78 | 19.14 | 277.68 | 0.3299 | -884.4 | -608.8 | |
| 1.45 | 11.98 | 0.76 | 6.28 | 7.63 | 113.75 | 19.11 | 279.99 | 0.3310 | -919.9 | -681.9 | |
| 1.18 | -2.00 | 0.62 | -2.00 | 7.33 | 113.61 | 18.97 | 279.14 | 0.3280 | -1012.9 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 6.79 | 113.20 | 18.56 | 277.62 | 0.3202 | -791.0 | -678.4 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 7.97 | 112.63 | 17.99 | 281.55 | 0.3136 | -690.0 | -506.9 | |
| 0.00 | 2.36 | 0.00 | 1.23 | 7.88 | 112.37 | 17.73 | 281.42 | 0.3091 | -928.0 | -747.6 | |
| 5.90 | 22.14 | 3.06 | 11.48 | 6.77 | 111.84 | 17.20 | 278.00 | 0.2978 | 953.2 | 666.9 | |
| 2.00 | -7.00 | 1.04 | -7.00 | 6.99 | 111.69 | 17.05 | 278.79 | 0.2957 | 859.3 | 999999 | |
| 3.00 | -7.00 | 1.55 | -7.00 | 6.66 | 111.42 | 16.78 | 277.77 | 0.2907 | 1108.0 | 999999 | |
| 0.00 | 2.72 | 0.00 | 1.41 | 7.03 | 111.21 | 16.57 | 279.14 | 0.2879 | 677.0 | 542.2 | |
| 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. | |