| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.22 | 127.06 | 14.64 | 68.34 | -15.87 | 249.02 | -1.14 | 177.16 | 0.3915 | 2.2 | -144.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-26 01:00:33 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 | 1.06 | 0.00 | 0.57 | -15.52 | 252.29 | 2.14 | 185.37 | 0.3854 | 664.0 | 490.2 | |
| 0.00 | 5.57 | 0.00 | 2.98 | -15.32 | 252.11 | 1.95 | 184.94 | 0.3819 | 630.0 | 726.4 | |
| 0.00 | 0.80 | 0.00 | 0.42 | -14.57 | 251.70 | 1.54 | 184.05 | 0.3693 | 766.0 | 618.7 | |
| 2.56 | 34.90 | 1.38 | 18.80 | -16.30 | 251.52 | 1.36 | 183.31 | 0.3970 | 891.0 | 719.7 | |
| 8.57 | -4.00 | 4.62 | -4.00 | -16.10 | 251.17 | 1.02 | 182.49 | 0.3935 | 1154.9 | 999999 | |
| 0.53 | 2.39 | 0.29 | 1.29 | -16.82 | 251.05 | 0.89 | 182.12 | 0.4050 | 887.8 | 662.3 | |
| 0.00 | 1.68 | 0.00 | 0.91 | -16.53 | 251.05 | 0.89 | 182.14 | 0.4003 | 700.0 | 532.9 | |
| 2.30 | -4.00 | 1.24 | -4.00 | -16.10 | 250.95 | 0.80 | 181.95 | 0.3934 | 1047.4 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.67 | -17.18 | 250.96 | 0.80 | 181.87 | 0.4107 | 793.0 | 692.6 | |
| 1.15 | -4.00 | 0.62 | -4.00 | -15.74 | 250.89 | 0.73 | 181.83 | 0.3875 | 974.4 | 999999 | |
| 0.00 | 2.47 | 0.00 | 1.35 | -17.51 | 250.55 | 0.39 | 180.90 | 0.4158 | 684.0 | 612.8 | |
| 0.88 | 2.74 | 0.48 | 1.47 | -15.93 | 250.14 | -0.02 | 179.96 | 0.3905 | 895.9 | 655.6 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.67 | 249.95 | -0.20 | 179.49 | 0.3863 | 777.0 | 623.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.48 | 249.92 | -0.23 | 179.41 | 0.3831 | 735.0 | 563.2 | |
| 0.00 | 1.77 | 0.00 | 0.96 | -17.25 | 249.16 | -0.99 | 177.68 | 0.4119 | 414.0 | 323.2 | |
| 0.00 | 3.53 | 0.00 | 1.89 | -15.19 | 248.93 | -1.23 | 176.85 | 0.3789 | -514.0 | -673.8 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -17.35 | 248.91 | -1.25 | 177.11 | 0.4136 | 585.0 | 411.3 | |
| 1.24 | 15.46 | 0.66 | 8.30 | -15.67 | 248.83 | -1.33 | 176.68 | 0.3869 | -918.1 | -799.1 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -15.94 | 248.77 | -1.39 | 176.56 | 0.3912 | -627.0 | -426.2 | |
| 0.88 | -18.00 | 0.47 | -18.00 | -15.64 | 248.67 | -1.48 | 176.29 | 0.3865 | -946.4 | 999999 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -15.45 | 248.46 | -1.70 | 175.71 | 0.3836 | -740.0 | -469.2 | |
| 6.72 | 9.01 | 3.60 | 4.84 | -15.61 | 248.08 | -2.08 | 174.80 | 0.3868 | -992.0 | -662.6 | |
| 0.00 | 1.24 | 0.00 | 0.67 | -15.74 | 247.33 | -2.83 | 172.98 | 0.3902 | -728.0 | -459.6 | |
| 0.00 | 2.12 | 0.00 | 1.15 | -17.02 | 247.15 | -3.01 | 172.96 | 0.4109 | -931.0 | -783.3 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -15.91 | 247.08 | -3.08 | 172.42 | 0.3933 | -811.0 | -620.8 | |
| 0.00 | 1.59 | 0.00 | 0.86 | -15.88 | 246.89 | -3.27 | 171.95 | 0.3932 | -555.0 | -536.0 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -16.04 | 246.67 | -3.49 | 171.47 | 0.3964 | -805.0 | -564.9 | |
| 1.24 | 6.36 | 0.66 | 3.42 | -15.52 | 246.55 | -3.61 | 170.98 | 0.3884 | -1075.6 | -790.1 | |
| 0.00 | 1.86 | 0.00 | 1.00 | -15.85 | 246.51 | -3.64 | 171.03 | 0.3937 | -947.0 | -760.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -15.65 | 246.36 | -3.80 | 170.57 | 0.3910 | -1057.0 | -888.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -15.29 | 246.34 | -3.82 | 170.36 | 0.3853 | -771.0 | -630.1 | |
| 0.00 | 3.89 | 0.00 | 2.10 | -15.88 | 246.14 | -4.02 | 170.13 | 0.3952 | -836.0 | -743.6 | |
| 0.00 | 1.33 | 0.00 | 0.71 | -15.62 | 246.14 | -4.01 | 170.03 | 0.3910 | -617.0 | -491.5 | |
| 1.15 | 13.87 | 0.62 | 7.43 | -15.26 | 245.99 | -4.16 | 169.49 | 0.3858 | -1098.5 | -783.5 | |
| 0.00 | 1.59 | 0.00 | 0.86 | -16.77 | 245.83 | -4.32 | 169.82 | 0.4100 | -696.0 | -550.4 | |
| 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. | |