| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.12 | 21.30 | 1.13 | 11.39 | 16.54 | 27.01 | 6.54 | 343.04 | 0.3772 | -67.1 | -137.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-13 20:00:24 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 | 1.02 | 0.00 | 0.54 | 14.97 | 29.78 | 9.30 | 334.74 | 0.3675 | -835.0 | -667.0 | |
| 1.44 | 3.57 | 0.77 | 1.91 | 15.85 | 29.76 | 9.28 | 335.81 | 0.3802 | -1037.2 | -871.5 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.00 | 29.39 | 8.92 | 336.82 | 0.3801 | -825.0 | -607.9 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 14.93 | 29.01 | 8.53 | 336.55 | 0.3617 | -886.0 | -756.4 | |
| 0.00 | 1.10 | 0.00 | 0.59 | 16.25 | 28.50 | 8.03 | 339.15 | 0.3783 | -851.0 | -642.1 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 17.70 | 28.38 | 7.90 | 340.78 | 0.3996 | -689.0 | -578.4 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 16.68 | 27.93 | 7.46 | 340.91 | 0.3818 | -568.0 | -546.8 | |
| 0.00 | 1.61 | 0.00 | 0.85 | 15.44 | 26.38 | 5.90 | 343.72 | 0.3549 | -1034.0 | -705.0 | |
| 0.00 | 1.10 | 0.00 | 0.60 | 20.22 | 26.07 | 5.59 | 347.61 | 0.4282 | 792.0 | 600.8 | |
| 0.68 | 1.87 | 0.36 | 1.00 | 17.43 | 25.63 | 5.16 | 347.01 | 0.3831 | 950.0 | 715.3 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 16.03 | 25.50 | 5.02 | 346.44 | 0.3606 | 1003.0 | 765.6 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 18.09 | 24.32 | 3.84 | 350.55 | 0.3894 | 699.0 | 438.1 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 17.00 | 22.56 | 2.09 | 354.55 | 0.3683 | 871.0 | 707.7 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 15.99 | 22.06 | 1.58 | 355.64 | 0.3511 | 882.0 | 638.5 | |
| 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. | |