| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.00 | 28.77 | 4.63 | 14.87 | 16.53 | 22.41 | 9.02 | 327.30 | 0.2854 | -56.4 | -143.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-01 23:59:11 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 |
| 1.73 | 3.81 | 0.89 | 1.97 | 13.46 | 26.58 | 13.19 | 309.67 | 0.2896 | 1060.1 | 798.6 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 15.25 | 25.36 | 11.97 | 316.97 | 0.2946 | -887.0 | -717.8 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.40 | 25.15 | 11.76 | 317.85 | 0.2940 | -835.0 | -660.8 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.56 | 24.92 | 11.53 | 321.01 | 0.3059 | -817.0 | -637.9 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 16.70 | 23.67 | 10.28 | 324.41 | 0.2950 | -1022.0 | -817.2 | |
| 0.00 | 4.00 | 0.00 | 2.06 | 15.86 | 22.69 | 9.30 | 325.29 | 0.2743 | -856.0 | -759.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.37 | 21.95 | 8.56 | 328.51 | 0.2745 | -679.0 | -501.5 | |
| 1.73 | 1.91 | 0.89 | 0.98 | 17.38 | 20.99 | 7.60 | 333.21 | 0.2813 | 770.9 | 634.0 | |
| 2.36 | 4.81 | 1.22 | 2.48 | 17.01 | 20.91 | 7.52 | 332.81 | 0.2751 | 967.2 | 725.0 | |
| 3.18 | 3.81 | 1.63 | 1.96 | 16.66 | 20.55 | 7.16 | 333.35 | 0.2672 | 936.5 | 770.0 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 17.48 | 20.51 | 7.12 | 334.83 | 0.2793 | 884.0 | 782.2 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 23.51 | 17.13 | 3.74 | 350.35 | 0.3582 | -837.0 | -632.0 | |
| 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. | |