| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 116.19 | 429.47 | 62.42 | 231.00 | 16.57 | 48.57 | 10.29 | 333.80 | 0.3887 | -291.5 | -114.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-05-06 16:59:07 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 | 2.15 | 0.00 | 1.19 | 18.41 | 53.92 | 15.65 | 325.55 | 0.4542 | 775.0 | 622.8 | |
| 10.99 | 281.54 | 5.93 | 151.97 | 16.06 | 50.89 | 12.62 | 327.96 | 0.3974 | -1102.5 | -384.8 | |
| 1.70 | -2.00 | 0.92 | -2.00 | 16.41 | 50.89 | 12.61 | 328.46 | 0.4021 | -859.6 | 999999 | |
| 2.59 | -2.00 | 1.40 | -2.00 | 16.58 | 50.90 | 12.62 | 328.66 | 0.4043 | -761.2 | 999999 | |
| 1.34 | -2.00 | 0.72 | -2.00 | 16.57 | 50.70 | 12.43 | 329.05 | 0.4027 | -858.7 | 999999 | |
| 0.98 | -2.00 | 0.53 | -2.00 | 16.67 | 50.58 | 12.30 | 329.42 | 0.4030 | -877.5 | 999999 | |
| 33.34 | -2.00 | 17.96 | -2.00 | 16.21 | 50.39 | 12.11 | 329.20 | 0.3953 | -1269.6 | 999999 | |
| 7.87 | -2.00 | 4.25 | -2.00 | 16.79 | 50.36 | 12.09 | 330.03 | 0.4029 | -924.6 | 999999 | |
| 0.54 | -2.00 | 0.29 | -2.00 | 15.60 | 49.87 | 11.59 | 329.45 | 0.3825 | -1232.2 | 999999 | |
| 8.49 | -2.00 | 4.56 | -2.00 | 16.14 | 49.81 | 11.53 | 330.33 | 0.3895 | -1106.9 | 999999 | |
| 2.06 | -2.00 | 1.11 | -2.00 | 16.56 | 49.44 | 11.17 | 331.63 | 0.3925 | -639.4 | 999999 | |
| 4.29 | 5.99 | 2.29 | 3.20 | 15.62 | 48.88 | 10.60 | 331.66 | 0.3749 | -1020.9 | -752.4 | |
| 0.00 | 1.88 | 0.00 | 1.02 | 18.94 | 48.30 | 10.02 | 336.74 | 0.4186 | -837.0 | -670.7 | |
| 0.00 | 1.34 | 0.00 | 0.72 | 15.93 | 47.97 | 9.69 | 334.13 | 0.3726 | -870.0 | -688.9 | |
| 9.47 | 12.42 | 5.16 | 6.77 | 19.14 | 47.89 | 9.61 | 337.78 | 0.4188 | -918.0 | -761.6 | |
| 0.00 | 2.23 | 0.00 | 1.22 | 19.03 | 47.49 | 9.22 | 338.51 | 0.4150 | -878.0 | -768.2 | |
| 0.00 | 1.70 | 0.00 | 0.91 | 16.40 | 46.84 | 8.57 | 337.30 | 0.3720 | 777.0 | 509.5 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 16.77 | 45.55 | 7.28 | 340.79 | 0.3702 | -652.0 | -552.2 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 17.74 | 45.24 | 6.96 | 342.39 | 0.3835 | 648.0 | 484.7 | |
| 0.00 | 2.15 | 0.00 | 1.15 | 17.29 | 45.06 | 6.79 | 342.44 | 0.3756 | 669.0 | 450.5 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 17.64 | 45.04 | 6.77 | 342.78 | 0.3810 | 736.0 | 609.8 | |
| 0.00 | 1.34 | 0.00 | 0.72 | 17.48 | 44.85 | 6.57 | 343.12 | 0.3775 | 821.0 | 686.8 | |
| 0.00 | 0.72 | 0.00 | 0.38 | 17.38 | 44.62 | 6.34 | 343.59 | 0.3749 | 790.0 | 637.1 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 17.67 | 44.60 | 6.32 | 343.87 | 0.3794 | 910.0 | 777.5 | |
| 0.00 | 1.43 | 0.00 | 0.77 | 17.90 | 44.48 | 6.20 | 344.33 | 0.3823 | 806.0 | 676.6 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 17.51 | 44.47 | 6.19 | 344.07 | 0.3762 | 824.0 | 580.9 | |
| 24.22 | 98.76 | 12.89 | 52.54 | 16.99 | 44.35 | 6.08 | 343.94 | 0.3676 | 1070.2 | 579.0 | |
| 1.61 | -27.00 | 0.85 | -27.00 | 16.28 | 44.23 | 5.96 | 343.67 | 0.3560 | 1077.3 | 999999 | |
| 6.70 | -27.00 | 3.56 | -27.00 | 16.50 | 44.08 | 5.81 | 344.24 | 0.3588 | 1151.4 | 999999 | |
| 0.00 | 4.38 | 0.00 | 2.32 | 16.37 | 43.73 | 5.46 | 345.06 | 0.3552 | 1035.0 | 816.0 | |
| 0.00 | 1.52 | 0.00 | 0.81 | 17.27 | 42.93 | 4.66 | 347.74 | 0.3664 | 903.0 | 761.2 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 18.24 | 42.80 | 4.52 | 348.63 | 0.3814 | 748.0 | 673.2 | |
| 0.00 | 2.06 | 0.00 | 1.11 | 19.29 | 41.89 | 3.62 | 351.30 | 0.3955 | 884.0 | 600.9 | |
| 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. | |