| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 110.54 | 382.78 | 60.56 | 210.60 | 9.03 | 99.52 | -22.46 | 60.30 | 0.4356 | 75.2 | 184.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-06 03:00:24 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 |
| 13.60 | 24.05 | 7.25 | 12.82 | 8.67 | 104.03 | -17.95 | 55.49 | 0.3714 | -1140.4 | -557.3 | |
| 0.00 | 2.12 | 0.00 | 1.14 | 8.79 | 103.68 | -18.30 | 55.72 | 0.3772 | -769.0 | -675.1 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 8.07 | 103.68 | -18.30 | 57.35 | 0.3708 | -1038.0 | -854.3 | |
| 0.00 | 2.12 | 0.00 | 1.13 | 8.26 | 103.55 | -18.43 | 57.12 | 0.3743 | -968.0 | -795.9 | |
| 12.49 | 19.97 | 6.69 | 10.70 | 8.77 | 103.21 | -18.77 | 56.44 | 0.3834 | -1130.2 | -646.3 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 10.45 | 102.92 | -19.06 | 53.30 | 0.4023 | -741.0 | -573.8 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 9.42 | 102.92 | -19.06 | 55.45 | 0.3929 | -743.0 | -613.1 | |
| 4.42 | 6.54 | 2.38 | 3.52 | 9.15 | 102.68 | -19.30 | 56.35 | 0.3937 | -976.0 | -662.4 | |
| 2.46 | 22.35 | 1.32 | 11.97 | 7.61 | 102.69 | -19.28 | 59.74 | 0.3807 | -1184.2 | -789.0 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 8.64 | 102.55 | -19.43 | 57.63 | 0.3911 | -831.0 | -650.7 | |
| 0.00 | 2.63 | 0.00 | 1.42 | 8.52 | 102.49 | -19.49 | 57.97 | 0.3909 | -797.0 | -682.7 | |
| 2.63 | -9.00 | 1.41 | -9.00 | 7.77 | 102.47 | -19.51 | 59.68 | 0.3851 | -1076.9 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 9.43 | 102.06 | -19.92 | 56.57 | 0.4045 | -784.0 | -672.5 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 8.87 | 101.62 | -20.36 | 58.33 | 0.4057 | -721.0 | -593.8 | |
| 0.00 | 1.70 | 0.00 | 0.92 | 9.45 | 101.39 | -20.59 | 57.39 | 0.4136 | -833.0 | -554.0 | |
| 5.44 | 8.67 | 2.97 | 4.73 | 9.70 | 100.99 | -20.99 | 57.37 | 0.4210 | -882.3 | -574.3 | |
| 0.85 | 3.91 | 0.46 | 2.12 | 8.08 | 100.86 | -21.12 | 60.94 | 0.4098 | -851.0 | -752.8 | |
| 0.00 | 2.55 | 0.00 | 1.38 | 7.51 | 100.73 | -21.25 | 62.32 | 0.4075 | -732.0 | -594.7 | |
| 0.00 | 1.87 | 0.00 | 1.03 | 9.87 | 100.34 | -21.64 | 57.82 | 0.4311 | -144.0 | 12.7 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 9.57 | 100.33 | -21.65 | 58.45 | 0.4288 | -578.0 | -370.5 | |
| 0.00 | 1.10 | 0.00 | 0.60 | 7.70 | 100.40 | -21.58 | 62.27 | 0.4135 | -671.0 | -534.2 | |
| 0.00 | 2.38 | 0.00 | 1.31 | 9.42 | 100.01 | -21.97 | 59.10 | 0.4319 | 184.0 | 197.1 | |
| 2.21 | 3.65 | 1.21 | 2.00 | 7.93 | 99.43 | -22.55 | 62.80 | 0.4289 | -850.9 | -534.7 | |
| 1.95 | 6.97 | 1.07 | 3.83 | 8.62 | 99.39 | -22.59 | 61.41 | 0.4344 | 1173.5 | 777.7 | |
| 4.25 | 258.83 | 2.35 | 143.79 | 9.84 | 99.11 | -22.87 | 59.27 | 0.4473 | 1074.1 | 454.5 | |
| 1.10 | -24.00 | 0.61 | -24.00 | 8.66 | 99.19 | -22.79 | 61.54 | 0.4374 | 1007.8 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.79 | 8.06 | 99.16 | -22.82 | 62.81 | 0.4335 | -494.0 | -324.1 | |
| 1.61 | -25.00 | 0.89 | -25.00 | 9.79 | 98.89 | -23.09 | 59.62 | 0.4499 | 861.9 | 999999 | |
| 3.48 | -25.00 | 1.93 | -25.00 | 9.53 | 98.42 | -23.56 | 60.62 | 0.4544 | 812.1 | 999999 | |
| 31.53 | -25.00 | 17.47 | -25.00 | 8.98 | 98.39 | -23.59 | 61.72 | 0.4508 | 1202.7 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.82 | 12.38 | 97.65 | -24.33 | 56.16 | 0.4866 | 346.0 | 288.2 | |
| 22.52 | -25.00 | 12.55 | -25.00 | 9.33 | 97.81 | -24.17 | 61.61 | 0.4612 | 1163.6 | 999999 | |
| 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. | |