| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.00 | 0.00 | 11.91 | 13.93 | 260.19 | 27.11 | 290.21 | 0.4709 | 242.4 | 150.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-03 20:00:39 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 | 1.99 | 0.00 | 1.24 | 13.97 | 270.12 | 37.04 | 285.27 | 0.6082 | -729.0 | -510.7 | |
| 0.00 | 1.45 | 0.00 | 0.89 | 16.14 | 268.55 | 35.48 | 289.30 | 0.5929 | -575.0 | -464.8 | |
| 0.00 | 1.99 | 0.00 | 1.22 | 16.43 | 268.38 | 35.30 | 289.84 | 0.5915 | -572.0 | -505.3 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 17.01 | 267.42 | 34.34 | 291.18 | 0.5807 | 587.0 | 418.4 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 16.39 | 266.30 | 33.22 | 290.58 | 0.5636 | -641.0 | -509.2 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 16.56 | 266.10 | 33.03 | 290.95 | 0.5615 | -594.0 | -482.3 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -1.55 | 261.18 | 28.11 | 255.88 | 0.4876 | 542.0 | 434.9 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 9.47 | 260.98 | 27.90 | 279.01 | 0.4693 | 639.0 | 436.7 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 12.23 | 260.32 | 27.24 | 285.07 | 0.4651 | 432.0 | 341.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 9.82 | 258.80 | 25.72 | 280.27 | 0.4364 | 887.0 | 739.6 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 8.52 | 251.52 | 18.44 | 279.07 | 0.3182 | 851.0 | 667.8 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.63 | 250.04 | 16.96 | 306.61 | 0.3479 | 871.0 | 716.9 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 17.21 | 249.76 | 16.69 | 305.98 | 0.3404 | 792.0 | 595.9 | |
| 0.00 | 3.80 | 0.00 | 1.97 | 14.88 | 247.80 | 14.72 | 302.81 | 0.2935 | 904.0 | 705.5 | |
| 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. | |