| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.38 | 290.59 | 23.82 | 159.86 | 16.41 | 169.40 | -23.14 | 60.29 | 0.4357 | -837.7 | -380.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-15 15:59:11 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 | 1.27 | 0.00 | 0.69 | 20.00 | 173.12 | -19.42 | 48.74 | 0.4174 | -827.0 | -675.1 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 19.09 | 171.79 | -20.75 | 52.25 | 0.4252 | -779.0 | -601.0 | |
| 43.38 | 277.26 | 23.82 | 152.25 | 16.29 | 169.56 | -22.98 | 60.39 | 0.4327 | -1217.5 | -411.2 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 17.34 | 168.91 | -23.63 | 58.88 | 0.4488 | 53.0 | 40.9 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 18.52 | 168.46 | -24.08 | 57.00 | 0.4632 | -692.0 | -546.8 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 22.20 | 165.09 | -27.46 | 53.61 | 0.5323 | 811.0 | 657.9 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 16.94 | 165.08 | -27.47 | 62.85 | 0.4978 | 707.0 | 551.1 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 23.19 | 163.78 | -28.76 | 53.14 | 0.5550 | 833.0 | 605.6 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 14.33 | 162.00 | -30.54 | 69.53 | 0.5275 | 714.0 | 611.3 | |
| 0.00 | 2.27 | 0.00 | 1.34 | 17.05 | 161.32 | -31.22 | 65.05 | 0.5486 | 688.0 | 467.8 | |
| 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. | |