SDO HMI 2011-06-03 10:59:10 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.39 | 285.60 | 24.50 | 151.40 | 17.24 | 19.99 | -11.21 | 31.20 | 0.3577 | -455.0 | -300.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-03 10:59:10 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 | 1.27 | 0.00 | 0.67 | 18.82 | 21.38 | -9.83 | 26.13 | 0.3684 | -842.0 | -622.1 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 22.21 | 21.02 | -10.18 | 23.05 | 0.4197 | -613.0 | -480.8 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 18.63 | 21.22 | -9.98 | 26.72 | 0.3667 | -1059.0 | -887.2 | |
| 21.07 | 221.51 | 11.08 | 116.63 | 16.55 | 21.21 | -9.99 | 29.69 | 0.3372 | -1337.0 | -471.5 | |
| 9.49 | -4.00 | 5.02 | -4.00 | 17.32 | 20.98 | -10.23 | 29.11 | 0.3499 | -967.2 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 21.88 | 20.54 | -10.66 | 24.35 | 0.4180 | -609.0 | -463.1 | |
| 10.76 | -4.00 | 5.68 | -4.00 | 16.90 | 20.74 | -10.46 | 30.28 | 0.3460 | -1064.1 | 999999 | |
| 1.90 | -4.00 | 1.00 | -4.00 | 17.22 | 20.56 | -10.64 | 30.22 | 0.3519 | -732.9 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 19.18 | 20.31 | -10.89 | 28.04 | 0.3814 | -752.0 | -607.3 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 19.02 | 20.29 | -10.92 | 28.30 | 0.3793 | -822.0 | -709.0 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 16.14 | 20.27 | -10.93 | 32.61 | 0.3395 | -727.0 | -576.0 | |
| 0.00 | 8.41 | 0.00 | 4.48 | 18.05 | 19.76 | -11.44 | 30.78 | 0.3701 | -664.0 | -693.4 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 17.86 | 19.41 | -11.79 | 31.81 | 0.3704 | -790.0 | -644.8 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 17.73 | 19.23 | -11.97 | 32.41 | 0.3703 | -857.0 | -680.7 | |
| 1.36 | 5.70 | 0.73 | 3.08 | 18.22 | 16.76 | -14.44 | 36.57 | 0.3993 | -833.4 | -721.1 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 18.96 | 15.73 | -15.47 | 37.27 | 0.4183 | 774.0 | 519.6 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 20.03 | 15.15 | -16.05 | 36.66 | 0.4369 | 698.0 | 583.5 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 18.58 | 15.10 | -16.10 | 38.96 | 0.4199 | 1033.0 | 894.0 | |
| 0.00 | 1.81 | 0.00 | 0.99 | 19.09 | 15.01 | -16.19 | 38.30 | 0.4269 | 955.0 | 701.8 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 16.21 | 15.21 | -15.99 | 42.78 | 0.3911 | 878.0 | 574.8 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 17.61 | 15.06 | -16.15 | 40.60 | 0.4090 | 910.0 | 727.1 | |
| 0.00 | 2.08 | 0.00 | 1.12 | 16.37 | 15.10 | -16.10 | 42.68 | 0.3941 | 714.0 | 557.9 | |
| 0.00 | 6.24 | 0.00 | 3.39 | 17.81 | 14.94 | -16.26 | 40.48 | 0.4124 | 1041.0 | 907.7 | |
| 1.81 | 9.76 | 0.99 | 5.34 | 18.61 | 14.83 | -16.37 | 39.36 | 0.4230 | 942.3 | 865.9 | |
| 0.00 | 4.79 | 0.00 | 2.62 | 18.93 | 14.73 | -16.47 | 39.02 | 0.4278 | 915.0 | 771.9 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 19.58 | 14.66 | -16.54 | 38.14 | 0.4361 | 770.0 | 633.0 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 19.87 | 14.53 | -16.67 | 37.92 | 0.4409 | 667.0 | 499.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 23.12 | 13.97 | -17.24 | 34.33 | 0.4851 | 812.0 | 673.5 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 19.84 | 13.99 | -17.21 | 38.82 | 0.4458 | 965.0 | 706.0 | |
| 0.00 | 4.25 | 0.00 | 2.35 | 19.06 | 13.37 | -17.83 | 40.99 | 0.4431 | 655.0 | 600.4 | |
| 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. | |