| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.83 | 284.56 | 23.56 | 152.84 | -24.34 | 250.15 | 9.77 | 203.54 | 0.3874 | 713.6 | 335.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2013-01-07 13:58:54 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 | 2.55 | 0.00 | 1.36 | -21.48 | 253.75 | 13.37 | 215.13 | 0.3755 | -827.0 | -698.6 | |
| 43.83 | 265.88 | 23.56 | 142.98 | -24.42 | 250.57 | 10.19 | 204.50 | 0.3902 | 1439.7 | 414.6 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -27.02 | 247.35 | 6.97 | 195.29 | 0.4114 | 701.0 | 482.4 | |
| 0.00 | 0.93 | 0.00 | 0.51 | -28.29 | 245.48 | 5.09 | 190.67 | 0.4243 | -674.0 | -582.3 | |
| 0.00 | 1.53 | 0.00 | 0.80 | -23.14 | 244.43 | 4.05 | 191.07 | 0.3395 | -1049.0 | -924.1 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -25.63 | 244.38 | 3.99 | 189.57 | 0.3793 | -618.0 | -548.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -21.74 | 242.55 | 2.17 | 186.49 | 0.3119 | -846.0 | -648.4 | |
| 0.00 | 1.61 | 0.00 | 0.86 | -25.38 | 241.95 | 1.57 | 183.85 | 0.3707 | -870.0 | -757.2 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -21.90 | 241.72 | 1.34 | 184.00 | 0.3133 | -873.0 | -787.7 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -25.95 | 241.40 | 1.02 | 182.43 | 0.3795 | -871.0 | -661.9 | |
| 0.00 | 3.91 | 0.00 | 2.03 | -21.62 | 241.31 | 0.93 | 182.81 | 0.3082 | -788.0 | -651.2 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -20.94 | 240.71 | 0.33 | 181.03 | 0.2965 | -931.0 | -763.4 | |
| 0.00 | 1.78 | 0.00 | 0.93 | -21.78 | 240.68 | 0.29 | 180.88 | 0.3105 | -899.0 | -738.4 | |
| 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. | |