| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.71 | 194.19 | 19.18 | 104.14 | 13.72 | 50.39 | 7.84 | 339.66 | 0.3849 | -152.1 | -103.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-07 20:00:28 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 | 2.25 | 0.00 | 1.21 | 11.15 | 55.50 | 12.95 | 324.88 | 0.3838 | -941.0 | -744.6 | |
| 0.00 | 0.87 | 0.00 | 0.46 | 11.47 | 55.42 | 12.87 | 325.51 | 0.3872 | -849.0 | -759.5 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 13.47 | 54.71 | 12.16 | 329.73 | 0.4082 | -758.0 | -614.6 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 14.71 | 54.68 | 12.13 | 331.29 | 0.4251 | -445.0 | -430.8 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 14.35 | 54.38 | 11.83 | 331.48 | 0.4178 | -586.0 | -504.2 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 13.35 | 53.67 | 11.12 | 331.76 | 0.3984 | -961.0 | -756.1 | |
| 0.00 | 3.29 | 0.00 | 1.75 | 10.88 | 53.41 | 10.86 | 329.08 | 0.3617 | -757.0 | -667.3 | |
| 4.84 | 6.92 | 2.62 | 3.75 | 14.19 | 53.18 | 10.63 | 333.80 | 0.4069 | -875.9 | -564.7 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 15.86 | 53.11 | 10.56 | 335.70 | 0.4303 | -635.0 | -483.0 | |
| 0.00 | 0.87 | 0.00 | 0.47 | 13.30 | 52.89 | 10.34 | 333.40 | 0.3920 | -729.0 | -686.2 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 14.25 | 52.87 | 10.33 | 334.52 | 0.4056 | -671.0 | -608.5 | |
| 0.00 | 2.85 | 0.00 | 1.54 | 14.18 | 52.62 | 10.07 | 334.99 | 0.4029 | -834.0 | -677.5 | |
| 0.00 | 1.73 | 0.00 | 0.92 | 11.20 | 52.50 | 9.95 | 331.69 | 0.3590 | -928.0 | -710.8 | |
| 12.54 | 33.48 | 6.73 | 17.95 | 13.06 | 52.48 | 9.93 | 334.06 | 0.3857 | -1194.7 | -695.0 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 14.05 | 52.49 | 9.94 | 335.14 | 0.4001 | -858.0 | -736.8 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 11.17 | 52.25 | 9.70 | 332.25 | 0.3566 | -864.0 | -613.2 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 13.82 | 52.29 | 9.75 | 335.33 | 0.3955 | -718.0 | -607.5 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 12.04 | 52.03 | 9.49 | 333.88 | 0.3677 | -912.0 | -723.7 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 12.45 | 52.05 | 9.50 | 334.33 | 0.3738 | -905.0 | -749.8 | |
| 4.84 | 35.21 | 2.60 | 18.93 | 13.47 | 52.03 | 9.48 | 335.54 | 0.3885 | -1054.3 | -768.5 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 13.05 | 51.95 | 9.40 | 335.26 | 0.3819 | -761.0 | -684.1 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 12.26 | 51.86 | 9.31 | 334.56 | 0.3697 | -802.0 | -681.3 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 11.69 | 51.71 | 9.17 | 334.22 | 0.3603 | -961.0 | -815.1 | |
| 1.38 | -20.00 | 0.75 | -20.00 | 14.10 | 51.78 | 9.23 | 336.78 | 0.3962 | -825.6 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.41 | 11.88 | 51.60 | 9.05 | 334.73 | 0.3622 | -605.0 | -466.7 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 14.13 | 51.53 | 8.98 | 337.36 | 0.3950 | -582.0 | -471.2 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 14.57 | 51.05 | 8.50 | 338.87 | 0.3987 | -720.0 | -587.3 | |
| 0.52 | 7.79 | 0.28 | 4.17 | 13.64 | 50.86 | 8.31 | 338.42 | 0.3837 | -916.3 | -279.2 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 14.59 | 50.58 | 8.04 | 339.95 | 0.3965 | -658.0 | -548.0 | |
| 0.00 | 1.64 | 0.00 | 0.88 | 13.53 | 50.51 | 7.97 | 339.14 | 0.3801 | -689.0 | -535.8 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 12.20 | 50.29 | 7.74 | 338.37 | 0.3586 | 863.0 | 725.3 | |
| 0.00 | 2.60 | 0.00 | 1.39 | 13.34 | 50.29 | 7.75 | 339.49 | 0.3759 | 780.0 | 655.3 | |
| 0.00 | 1.82 | 0.00 | 0.96 | 12.45 | 50.14 | 7.59 | 338.99 | 0.3615 | 850.0 | 674.0 | |
| 2.16 | 3.63 | 1.16 | 1.94 | 13.93 | 49.54 | 6.99 | 341.85 | 0.3810 | 928.0 | 692.2 | |
| 0.00 | 2.25 | 0.00 | 1.21 | 14.35 | 49.55 | 7.01 | 342.16 | 0.3874 | 693.0 | 476.0 | |
| 0.00 | 5.45 | 0.00 | 2.91 | 13.49 | 49.43 | 6.89 | 341.73 | 0.3736 | 1090.0 | 888.2 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 13.82 | 48.55 | 6.00 | 344.20 | 0.3746 | 924.0 | 685.4 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 14.69 | 48.45 | 5.90 | 345.06 | 0.3877 | 610.0 | 418.2 | |
| 0.69 | 6.40 | 0.37 | 3.44 | 14.97 | 47.90 | 5.36 | 346.57 | 0.3899 | 872.2 | 571.3 | |
| 0.00 | 1.99 | 0.00 | 1.06 | 14.04 | 47.88 | 5.33 | 346.04 | 0.3752 | 931.0 | 742.7 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 11.88 | 47.80 | 5.25 | 344.69 | 0.3408 | 627.0 | 542.8 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 15.29 | 47.76 | 5.21 | 347.11 | 0.3944 | 495.0 | 368.5 | |
| 0.00 | 0.61 | 0.00 | 0.32 | 14.84 | 47.53 | 4.98 | 347.40 | 0.3865 | 775.0 | 532.7 | |
| 0.35 | 2.51 | 0.18 | 1.34 | 14.26 | 47.21 | 4.66 | 347.87 | 0.3762 | 904.2 | 723.8 | |
| 3.63 | 9.00 | 1.94 | 4.79 | 13.96 | 46.74 | 4.19 | 348.90 | 0.3701 | 1125.9 | 878.8 | |
| 0.00 | 1.90 | 0.00 | 1.01 | 13.64 | 46.58 | 4.03 | 349.15 | 0.3644 | 948.0 | 711.9 | |
| 0.00 | 2.42 | 0.00 | 1.29 | 13.48 | 46.45 | 3.91 | 349.39 | 0.3615 | 827.0 | 652.3 | |
| 1.56 | 17.73 | 0.84 | 9.51 | 15.08 | 46.39 | 3.84 | 350.33 | 0.3869 | 863.9 | 763.2 | |
| 3.20 | -48.00 | 1.71 | -48.00 | 14.86 | 46.36 | 3.81 | 350.31 | 0.3832 | 1117.4 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 15.82 | 46.31 | 3.77 | 350.84 | 0.3985 | 602.0 | 523.5 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 14.31 | 46.16 | 3.61 | 350.56 | 0.3739 | 944.0 | 711.8 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 15.60 | 46.18 | 3.64 | 351.05 | 0.3945 | 740.0 | 498.1 | |
| 0.00 | 3.37 | 0.00 | 1.81 | 15.43 | 46.03 | 3.48 | 351.37 | 0.3916 | 745.0 | 650.6 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 15.14 | 45.96 | 3.41 | 351.42 | 0.3868 | 708.0 | 568.0 | |
| 0.00 | 3.98 | 0.00 | 2.13 | 14.79 | 45.95 | 3.41 | 351.29 | 0.3811 | 816.0 | 785.0 | |
| 0.00 | 1.30 | 0.00 | 0.70 | 15.72 | 45.88 | 3.33 | 351.84 | 0.3958 | 652.0 | 489.3 | |
| 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. | |