| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.79 | 387.23 | 35.59 | 200.93 | 9.70 | 55.49 | -16.00 | 67.42 | 0.2950 | -410.2 | -329.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-10 20:58:58 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 | 1.21 | 0.00 | 0.61 | 6.91 | 60.49 | -11.00 | 71.76 | 0.2004 | -745.0 | -433.1 | |
| 0.00 | 1.38 | 0.00 | 0.70 | 7.29 | 58.13 | -13.37 | 73.09 | 0.2408 | -1008.0 | -821.9 | |
| 46.07 | 289.58 | 23.70 | 149.10 | 9.42 | 56.88 | -14.62 | 66.75 | 0.2722 | -1443.4 | -460.5 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 11.03 | 56.55 | -14.95 | 61.94 | 0.2882 | -702.0 | -516.2 | |
| 2.41 | -3.00 | 1.25 | -3.00 | 9.77 | 56.17 | -15.32 | 66.51 | 0.2852 | -798.2 | 999999 | |
| 0.00 | 2.15 | 0.00 | 1.12 | 10.84 | 55.93 | -15.56 | 63.42 | 0.2960 | -872.0 | -686.3 | |
| 1.55 | -3.00 | 0.80 | -3.00 | 9.79 | 55.80 | -15.70 | 66.90 | 0.2912 | -557.0 | 999999 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 11.46 | 55.39 | -16.10 | 62.30 | 0.3084 | -947.0 | -750.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 11.13 | 55.32 | -16.18 | 63.38 | 0.3071 | -835.0 | -683.7 | |
| 0.00 | 0.34 | 0.00 | 0.18 | 9.13 | 55.33 | -16.17 | 69.58 | 0.2946 | -454.0 | -464.8 | |
| 2.32 | 19.37 | 1.21 | 10.06 | 9.15 | 54.70 | -16.79 | 70.17 | 0.3046 | -826.7 | -121.0 | |
| 9.90 | 14.72 | 5.16 | 7.67 | 8.51 | 54.20 | -17.30 | 72.63 | 0.3095 | 942.8 | 351.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 12.18 | 53.57 | -17.92 | 62.64 | 0.3402 | 855.0 | 730.6 | |
| 1.46 | 3.01 | 0.77 | 1.59 | 10.02 | 51.99 | -19.50 | 70.12 | 0.3512 | -999.9 | -887.9 | |
| 2.84 | 3.10 | 1.50 | 1.64 | 9.81 | 51.72 | -19.78 | 70.93 | 0.3544 | -954.8 | -971.3 | |
| 0.00 | 6.37 | 0.00 | 3.39 | 9.80 | 51.04 | -20.45 | 71.49 | 0.3647 | -955.0 | -829.8 | |
| 1.38 | 1.72 | 0.74 | 0.92 | 11.31 | 50.58 | -20.91 | 67.96 | 0.3793 | 940.4 | 932.8 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 13.92 | 50.32 | -21.17 | 61.95 | 0.3989 | 909.0 | 699.6 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 12.63 | 50.38 | -21.12 | 64.93 | 0.3898 | 922.0 | 660.6 | |
| 0.00 | 6.20 | 0.00 | 3.35 | 13.65 | 50.19 | -21.31 | 62.72 | 0.3990 | 505.0 | 664.5 | |
| 0.00 | 3.62 | 0.00 | 1.94 | 11.04 | 50.25 | -21.25 | 68.93 | 0.3829 | 830.0 | 776.7 | |
| 0.00 | 1.38 | 0.00 | 0.74 | 12.29 | 49.92 | -21.58 | 66.16 | 0.3946 | 756.0 | 531.1 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 10.85 | 49.87 | -21.62 | 69.69 | 0.3876 | 158.0 | 124.5 | |
| 0.00 | 6.72 | 0.00 | 3.60 | 10.34 | 49.81 | -21.68 | 71.01 | 0.3861 | -431.0 | -580.8 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 11.23 | 49.38 | -22.11 | 69.14 | 0.3968 | 869.0 | 598.9 | |
| 0.86 | 3.62 | 0.46 | 1.95 | 10.96 | 49.34 | -22.15 | 69.83 | 0.3961 | 697.7 | 538.8 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 12.86 | 47.39 | -24.11 | 66.92 | 0.4347 | 698.0 | 552.2 | |
| 0.00 | 1.55 | 0.00 | 0.85 | 12.53 | 47.09 | -24.41 | 67.88 | 0.4373 | 844.0 | 559.8 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 11.63 | 45.90 | -25.59 | 70.60 | 0.4505 | 826.0 | 648.5 | |
| 0.00 | 1.21 | 0.00 | 0.67 | 12.61 | 45.50 | -26.00 | 68.78 | 0.4608 | 732.0 | 624.1 | |
| 0.00 | 1.21 | 0.00 | 0.67 | 12.15 | 45.38 | -26.12 | 69.81 | 0.4605 | 866.0 | 688.4 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 12.54 | 45.30 | -26.19 | 69.04 | 0.4633 | 593.0 | 469.2 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 11.85 | 45.21 | -26.29 | 70.55 | 0.4616 | 845.0 | 723.0 | |
| 0.00 | 2.84 | 0.00 | 1.59 | 12.06 | 45.12 | -26.38 | 70.16 | 0.4638 | 585.0 | 586.4 | |
| 0.00 | 0.69 | 0.00 | 0.39 | 11.83 | 44.39 | -27.10 | 71.05 | 0.4734 | 552.0 | 539.9 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 11.91 | 44.08 | -27.42 | 71.05 | 0.4784 | 795.0 | 636.4 | |
| 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. | |