| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.74 | 0.00 | 9.97 | -18.98 | 67.18 | -8.19 | 165.63 | 0.3238 | -344.3 | -287.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-09 16:00:24 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 | 1.10 | 0.00 | 0.56 | -12.81 | 80.99 | 5.62 | 211.81 | 0.1821 | -772.0 | -597.9 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -12.37 | 80.73 | 5.37 | 212.00 | 0.1734 | -866.0 | -602.3 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -13.65 | 80.36 | 5.00 | 206.70 | 0.1894 | -956.0 | -725.0 | |
| 0.00 | 0.76 | 0.00 | 0.38 | -12.94 | 78.71 | 3.35 | 200.06 | 0.1669 | -736.0 | -620.3 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -19.61 | 74.82 | -0.55 | 178.09 | 0.2710 | 772.0 | 654.5 | |
| 0.00 | 2.72 | 0.00 | 1.39 | -17.94 | 74.27 | -1.10 | 175.69 | 0.2432 | 961.0 | 738.6 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -18.91 | 74.17 | -1.20 | 175.62 | 0.2598 | 832.0 | 653.3 | |
| 0.00 | 2.46 | 0.00 | 1.26 | -18.48 | 72.93 | -2.44 | 170.86 | 0.2550 | -1002.0 | -792.7 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -16.51 | 63.21 | -12.15 | 137.28 | 0.2988 | -832.0 | -671.9 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -12.03 | 62.78 | -12.58 | 123.67 | 0.2571 | 836.0 | 674.0 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -24.42 | 54.07 | -21.29 | 136.94 | 0.4862 | -771.0 | -656.4 | |
| 0.00 | 2.21 | 0.00 | 1.25 | -24.16 | 53.63 | -21.73 | 135.98 | 0.4882 | -849.0 | -745.2 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -24.52 | 53.00 | -22.36 | 135.79 | 0.4984 | -729.0 | -621.9 | |
| 0.00 | 0.93 | 0.00 | 0.62 | -28.78 | 40.68 | -34.68 | 130.80 | 0.6612 | -708.0 | -595.1 | |
| 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. | |