SDO HMI 2011-11-14 07:58:58 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 88.44 | 310.48 | 49.26 | 175.54 | 9.66 | 53.81 | 27.91 | 285.22 | 0.4788 | -222.9 | -206.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-14 07:58:58 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 |
| 24.69 | 157.86 | 14.41 | 92.23 | 9.50 | 57.40 | 31.50 | 283.25 | 0.5315 | -1206.8 | -375.3 | |
| 0.00 | 1.46 | 0.00 | 0.84 | 9.94 | 55.70 | 29.79 | 284.67 | 0.5079 | -760.0 | -588.2 | |
| 0.00 | 1.38 | 0.00 | 0.79 | 10.51 | 55.51 | 29.61 | 285.85 | 0.5070 | -767.0 | -597.1 | |
| 1.72 | 2.24 | 0.99 | 1.29 | 11.77 | 55.62 | 29.71 | 288.21 | 0.5129 | -902.5 | -880.2 | |
| 0.00 | 1.89 | 0.00 | 1.09 | 11.90 | 55.32 | 29.42 | 288.60 | 0.5091 | -854.0 | -651.7 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 10.08 | 52.39 | 26.49 | 286.38 | 0.4596 | -723.0 | -518.2 | |
| 22.45 | 44.30 | 12.47 | 24.57 | 9.42 | 52.13 | 26.23 | 285.11 | 0.4535 | -1084.0 | -786.7 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 10.26 | 52.21 | 26.30 | 286.87 | 0.4575 | -646.0 | -535.1 | |
| 3.10 | 3.87 | 1.72 | 2.14 | 9.85 | 51.80 | 25.90 | 286.19 | 0.4500 | -870.0 | -717.7 | |
| 1.29 | -7.00 | 0.71 | -7.00 | 9.22 | 51.72 | 25.81 | 284.86 | 0.4465 | -1107.9 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.24 | 8.81 | 51.42 | 25.51 | 284.09 | 0.4407 | -762.0 | -614.0 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 15.51 | 51.92 | 26.01 | 297.75 | 0.4795 | 776.0 | 585.8 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 12.63 | 50.66 | 24.75 | 292.90 | 0.4454 | 770.0 | 631.8 | |
| 1.63 | 50.15 | 0.89 | 27.17 | 9.27 | 49.57 | 23.66 | 286.06 | 0.4140 | 650.8 | 528.2 | |
| 1.81 | -14.00 | 0.98 | -14.00 | 9.06 | 49.39 | 23.48 | 285.68 | 0.4105 | 733.4 | 999999 | |
| 10.41 | -14.00 | 5.64 | -14.00 | 9.49 | 49.12 | 23.22 | 286.84 | 0.4080 | 938.6 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 10.48 | 49.04 | 23.13 | 289.23 | 0.4109 | -594.0 | -574.6 | |
| 11.10 | -14.00 | 6.00 | -14.00 | 9.19 | 48.87 | 22.97 | 286.28 | 0.4031 | 996.0 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 10.09 | 48.74 | 22.84 | 288.52 | 0.4047 | -848.0 | -691.3 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 9.82 | 48.69 | 22.79 | 287.92 | 0.4028 | -905.0 | -785.8 | |
| 0.00 | 2.24 | 0.00 | 1.22 | 13.79 | 48.68 | 22.77 | 297.02 | 0.4238 | 664.0 | 579.1 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 9.78 | 47.94 | 22.03 | 288.31 | 0.3911 | -964.0 | -715.7 | |
| 0.00 | 3.18 | 0.00 | 1.72 | 13.36 | 47.58 | 21.68 | 297.11 | 0.4054 | 347.0 | 589.8 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 9.11 | 46.86 | 20.95 | 287.37 | 0.3716 | 840.0 | 679.7 | |
| 0.00 | 1.72 | 0.00 | 0.92 | 9.68 | 46.80 | 20.89 | 288.89 | 0.3732 | 644.0 | 585.8 | |
| 6.28 | 16.95 | 3.34 | 9.02 | 9.78 | 46.48 | 20.58 | 289.38 | 0.3688 | 961.5 | 756.0 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 10.43 | 46.53 | 20.62 | 291.04 | 0.3727 | 744.0 | 508.6 | |
| 0.00 | 3.01 | 0.00 | 1.60 | 10.50 | 46.37 | 20.47 | 291.33 | 0.3707 | 822.0 | 653.9 | |
| 3.96 | -26.00 | 2.11 | -26.00 | 10.02 | 46.24 | 20.34 | 290.21 | 0.3663 | 1168.3 | 999999 | |
| 0.00 | 6.19 | 0.00 | 3.29 | 10.56 | 45.96 | 20.05 | 291.87 | 0.3648 | 780.0 | 684.9 | |
| 0.00 | 0.52 | 0.00 | 0.27 | 8.78 | 45.69 | 19.78 | 287.31 | 0.3519 | 794.0 | 678.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 10.39 | 45.69 | 19.78 | 291.65 | 0.3598 | 824.0 | 734.6 | |
| 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. | |