| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.53 | 0.00 | 10.52 | -13.07 | 253.23 | -39.92 | 113.15 | 0.6811 | 344.0 | 166.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-03 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 |
| 0.00 | 1.18 | 0.00 | 0.75 | -12.88 | 257.69 | -35.47 | 115.13 | 0.6270 | 781.0 | 690.0 | |
| 0.00 | 1.27 | 0.00 | 0.81 | -12.63 | 257.69 | -35.46 | 114.75 | 0.6257 | 946.0 | 769.6 | |
| 0.00 | 0.45 | 0.00 | 0.29 | -12.89 | 257.49 | -35.66 | 115.02 | 0.6294 | 537.0 | 504.2 | |
| 0.00 | 1.45 | 0.00 | 0.92 | -12.35 | 257.50 | -35.65 | 114.23 | 0.6266 | 746.0 | 656.3 | |
| 0.00 | 2.00 | 0.00 | 1.31 | -13.20 | 255.60 | -37.55 | 114.43 | 0.6540 | 683.0 | 582.8 | |
| 0.00 | 1.27 | 0.00 | 0.83 | -13.05 | 255.35 | -37.80 | 114.08 | 0.6563 | 593.0 | 529.5 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -12.46 | 255.18 | -37.97 | 113.14 | 0.6556 | 629.0 | 568.3 | |
| 0.00 | 0.64 | 0.00 | 0.42 | -11.60 | 254.41 | -38.74 | 111.53 | 0.6613 | 539.0 | 411.4 | |
| 0.00 | 1.27 | 0.00 | 0.90 | -15.02 | 250.98 | -42.17 | 114.63 | 0.7156 | 508.0 | 340.4 | |
| 0.00 | 1.27 | 0.00 | 0.91 | -14.23 | 249.84 | -43.31 | 113.08 | 0.7251 | -669.0 | -612.9 | |
| 0.00 | 0.64 | 0.00 | 0.46 | -14.91 | 249.54 | -43.61 | 113.84 | 0.7310 | -557.0 | -529.0 | |
| 0.00 | 2.82 | 0.00 | 2.03 | -14.59 | 249.53 | -43.62 | 113.42 | 0.7299 | -735.0 | -657.8 | |
| 0.00 | 1.00 | 0.00 | 0.71 | -6.09 | 248.24 | -44.91 | 101.58 | 0.7189 | 471.0 | 309.9 | |
| 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. | |