| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.02 | 323.27 | 44.80 | 172.58 | 24.70 | 299.91 | 13.23 | 325.93 | 0.3728 | -57.5 | -1.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-08-31 23:59:08 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 |
| 34.10 | 154.56 | 18.32 | 83.09 | 23.99 | 302.74 | 16.06 | 319.25 | 0.3889 | -1215.3 | -350.1 | |
| 2.42 | 8.50 | 1.29 | 4.54 | 23.83 | 301.69 | 15.01 | 320.77 | 0.3763 | -1091.0 | -835.0 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 23.43 | 301.51 | 14.83 | 320.35 | 0.3696 | -671.0 | -557.8 | |
| 1.97 | -2.00 | 1.05 | -2.00 | 23.84 | 301.49 | 14.81 | 321.14 | 0.3742 | -985.7 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.96 | 24.69 | 301.52 | 14.84 | 322.60 | 0.3849 | -629.0 | -558.0 | |
| 0.00 | 1.52 | 0.00 | 0.81 | 23.56 | 301.29 | 14.61 | 321.00 | 0.3689 | -625.0 | -391.5 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 24.65 | 300.69 | 14.01 | 324.05 | 0.3764 | -751.0 | -549.8 | |
| 3.58 | 11.37 | 1.90 | 6.02 | 23.66 | 299.94 | 13.26 | 323.76 | 0.3568 | -952.0 | -653.5 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 25.22 | 299.83 | 13.15 | 326.62 | 0.3757 | -704.0 | -578.6 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 24.59 | 299.59 | 12.91 | 326.05 | 0.3654 | -828.0 | -626.2 | |
| 1.70 | 2.42 | 0.91 | 1.29 | 25.38 | 299.61 | 12.93 | 327.32 | 0.3759 | -582.6 | -190.6 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 25.13 | 299.48 | 12.80 | 327.17 | 0.3714 | -780.0 | -598.6 | |
| 0.00 | 1.61 | 0.00 | 0.85 | 23.91 | 298.88 | 12.20 | 326.36 | 0.3501 | -1073.0 | -742.9 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 24.49 | 298.39 | 11.71 | 328.36 | 0.3535 | 600.0 | 401.7 | |
| 0.00 | 3.49 | 0.00 | 1.85 | 24.84 | 298.29 | 11.61 | 329.14 | 0.3574 | 856.0 | 718.1 | |
| 1.88 | 2.51 | 0.99 | 1.32 | 24.50 | 297.98 | 11.30 | 329.24 | 0.3502 | 557.8 | 468.1 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 25.90 | 297.98 | 11.30 | 331.38 | 0.3695 | 603.0 | 502.0 | |
| 0.00 | 2.51 | 0.00 | 1.33 | 25.15 | 297.57 | 10.89 | 331.14 | 0.3558 | 765.0 | 640.4 | |
| 1.16 | 5.28 | 0.62 | 2.82 | 26.17 | 297.56 | 10.88 | 332.63 | 0.3700 | 667.0 | 419.1 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 24.74 | 297.29 | 10.61 | 331.13 | 0.3479 | 623.0 | 492.9 | |
| 1.61 | 8.86 | 0.85 | 4.68 | 25.03 | 297.18 | 10.50 | 331.81 | 0.3511 | 771.2 | 717.6 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 25.31 | 297.21 | 10.53 | 332.17 | 0.3553 | 356.0 | 324.9 | |
| 0.00 | 2.33 | 0.00 | 1.24 | 26.11 | 297.24 | 10.56 | 333.21 | 0.3669 | 969.0 | 844.7 | |
| 1.61 | -21.00 | 0.85 | -21.00 | 25.16 | 296.99 | 10.31 | 332.43 | 0.3515 | 786.7 | 999999 | |
| 12.44 | 36.52 | 6.63 | 19.46 | 26.51 | 296.70 | 10.02 | 334.91 | 0.3686 | 960.7 | 300.0 | |
| 3.04 | 63.37 | 1.61 | 33.49 | 25.42 | 296.60 | 9.92 | 333.67 | 0.3524 | 1086.6 | 759.8 | |
| 2.95 | -26.00 | 1.56 | -26.00 | 25.21 | 296.25 | 9.57 | 334.18 | 0.3467 | 872.0 | 999999 | |
| 11.72 | -26.00 | 6.19 | -26.00 | 25.37 | 295.95 | 9.27 | 335.08 | 0.3471 | 1256.1 | 999999 | |
| 0.00 | 1.43 | 0.00 | 0.75 | 24.70 | 295.90 | 9.22 | 334.28 | 0.3370 | 929.0 | 718.9 | |
| 0.89 | -26.00 | 0.47 | -26.00 | 25.57 | 295.73 | 9.05 | 335.86 | 0.3484 | 903.6 | 999999 | |
| 2.95 | -26.00 | 1.56 | -26.00 | 25.92 | 295.76 | 9.08 | 336.24 | 0.3538 | 887.0 | 999999 | |
| 0.00 | 3.49 | 0.00 | 1.85 | 26.21 | 295.75 | 9.07 | 336.63 | 0.3579 | 710.0 | 650.7 | |
| 0.00 | 1.16 | 0.00 | 0.60 | 21.22 | 293.27 | 6.59 | 336.24 | 0.2669 | 773.0 | 572.5 | |
| 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. | |