| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.34 | 402.71 | 35.71 | 221.72 | -14.83 | 118.48 | 15.20 | 215.34 | 0.4386 | 91.0 | 315.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-10-12 03:59:02 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 |
| 3.77 | 45.62 | 2.09 | 25.36 | -13.92 | 121.16 | 17.88 | 221.44 | 0.4522 | 1033.3 | 346.1 | |
| 1.75 | -1.00 | 0.97 | -1.00 | -14.21 | 121.12 | 17.84 | 220.94 | 0.4551 | 863.3 | 999999 | |
| 1.14 | -1.00 | 0.63 | -1.00 | -14.24 | 120.99 | 17.71 | 220.70 | 0.4541 | 1015.4 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -13.74 | 120.53 | 17.25 | 220.69 | 0.4437 | 422.0 | 400.6 | |
| 0.96 | 2.19 | 0.54 | 1.22 | -14.67 | 120.51 | 17.23 | 219.29 | 0.4543 | 620.9 | 551.9 | |
| 1.49 | 10.42 | 0.82 | 5.78 | -14.41 | 120.42 | 17.14 | 219.53 | 0.4504 | 981.5 | 740.6 | |
| 1.93 | 19.44 | 1.06 | 10.70 | -13.92 | 120.19 | 16.91 | 219.86 | 0.4423 | 933.4 | 711.9 | |
| 1.49 | -7.00 | 0.82 | -7.00 | -13.67 | 120.14 | 16.86 | 220.16 | 0.4388 | 964.2 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -15.79 | 120.31 | 17.03 | 217.41 | 0.4658 | 522.0 | 275.6 | |
| 1.49 | 3.50 | 0.82 | 1.93 | -13.72 | 119.92 | 16.64 | 219.70 | 0.4372 | 934.1 | 820.1 | |
| 2.98 | 209.90 | 1.65 | 116.19 | -14.91 | 119.94 | 16.66 | 218.03 | 0.4517 | 1165.6 | 570.5 | |
| 0.00 | 3.50 | 0.00 | 1.96 | -16.45 | 120.01 | 16.73 | 216.04 | 0.4712 | 540.0 | 443.1 | |
| 0.96 | -11.00 | 0.53 | -11.00 | -14.71 | 119.83 | 16.55 | 218.12 | 0.4482 | 1244.6 | 999999 | |
| 19.00 | -11.00 | 10.53 | -11.00 | -15.06 | 119.66 | 16.39 | 217.35 | 0.4509 | 1184.8 | 999999 | |
| 0.00 | 2.63 | 0.00 | 1.46 | -15.98 | 119.38 | 16.10 | 215.63 | 0.4597 | 748.0 | 597.2 | |
| 0.79 | -11.00 | 0.44 | -11.00 | -15.05 | 119.28 | 16.00 | 216.71 | 0.4471 | 1037.3 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -16.06 | 118.84 | 15.56 | 214.60 | 0.4558 | 672.0 | 447.5 | |
| 0.00 | 1.40 | 0.00 | 0.76 | -14.10 | 117.64 | 14.36 | 215.10 | 0.4201 | 532.0 | 412.2 | |
| 1.66 | 2.28 | 0.91 | 1.24 | -14.81 | 116.47 | 13.20 | 211.92 | 0.4192 | -723.2 | -677.2 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -17.92 | 116.63 | 13.35 | 208.51 | 0.4622 | -737.0 | -524.1 | |
| 1.75 | 7.09 | 0.95 | 3.84 | -14.00 | 116.33 | 13.05 | 212.71 | 0.4073 | -959.2 | -784.6 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -14.29 | 116.32 | 13.04 | 212.29 | 0.4110 | -926.0 | -723.8 | |
| 0.00 | 2.28 | 0.00 | 1.24 | -14.93 | 116.29 | 13.01 | 211.40 | 0.4193 | -830.0 | -677.2 | |
| 0.00 | 2.36 | 0.00 | 1.28 | -14.29 | 116.12 | 12.85 | 211.92 | 0.4093 | -773.0 | -621.1 | |
| 0.00 | 1.93 | 0.00 | 1.05 | -14.92 | 116.07 | 12.79 | 210.97 | 0.4174 | -660.0 | -591.4 | |
| 0.00 | 1.31 | 0.00 | 0.71 | -14.60 | 116.02 | 12.74 | 211.28 | 0.4126 | -919.0 | -761.5 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -14.18 | 115.77 | 12.49 | 211.34 | 0.4049 | -690.0 | -523.4 | |
| 0.00 | 1.49 | 0.00 | 0.80 | -14.05 | 115.64 | 12.36 | 211.24 | 0.4020 | -956.0 | -763.6 | |
| 0.00 | 1.66 | 0.00 | 0.91 | -15.40 | 115.72 | 12.44 | 209.69 | 0.4210 | -682.0 | -522.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -14.59 | 115.67 | 12.39 | 210.60 | 0.4097 | -887.0 | -734.5 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -14.27 | 115.62 | 12.34 | 210.91 | 0.4049 | -916.0 | -640.7 | |
| 0.00 | 1.75 | 0.00 | 0.97 | -17.34 | 115.65 | 12.37 | 207.34 | 0.4472 | -892.0 | -646.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -15.26 | 115.52 | 12.24 | 209.45 | 0.4176 | -707.0 | -596.5 | |
| 0.00 | 1.31 | 0.00 | 0.74 | -19.21 | 115.72 | 12.44 | 205.56 | 0.4735 | 883.0 | 732.4 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -17.40 | 115.49 | 12.22 | 206.98 | 0.4469 | -824.0 | -572.3 | |
| 0.00 | 1.49 | 0.00 | 0.81 | -15.22 | 115.17 | 11.89 | 208.80 | 0.4144 | -908.0 | -773.8 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -16.22 | 115.07 | 11.79 | 207.44 | 0.4275 | -760.0 | -569.2 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -15.73 | 114.97 | 11.69 | 207.81 | 0.4200 | -769.0 | -684.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -14.77 | 114.76 | 11.48 | 208.52 | 0.4049 | -888.0 | -683.0 | |
| 3.33 | 12.26 | 1.81 | 6.68 | -15.85 | 114.57 | 11.29 | 206.85 | 0.4188 | -971.3 | -682.7 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -15.08 | 114.33 | 11.06 | 207.25 | 0.4061 | -389.0 | -532.0 | |
| 0.00 | 0.61 | 0.00 | 0.33 | -16.20 | 114.02 | 10.74 | 205.34 | 0.4198 | -698.0 | -457.3 | |
| 0.00 | 1.58 | 0.00 | 0.85 | -14.22 | 113.29 | 10.01 | 205.97 | 0.3864 | -993.0 | -901.3 | |
| 0.00 | 1.84 | 0.00 | 1.00 | -16.06 | 113.37 | 10.10 | 204.15 | 0.4135 | -1039.0 | -753.1 | |
| 0.00 | 4.55 | 0.00 | 2.48 | -16.60 | 113.31 | 10.03 | 203.46 | 0.4210 | -691.0 | -693.9 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -16.34 | 113.20 | 9.92 | 203.49 | 0.4165 | -786.0 | -681.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -16.53 | 113.02 | 9.74 | 202.92 | 0.4182 | -890.0 | -721.5 | |
| 7.71 | 17.34 | 4.10 | 9.21 | -12.97 | 112.70 | 9.42 | 206.11 | 0.3641 | 1045.8 | 874.2 | |
| 1.05 | 15.41 | 0.57 | 8.29 | -15.14 | 112.54 | 9.26 | 203.29 | 0.3948 | -788.2 | -756.1 | |
| 3.50 | -48.00 | 1.86 | -48.00 | -13.06 | 112.36 | 9.09 | 205.19 | 0.3630 | 991.9 | 999999 | |
| 4.12 | -49.00 | 2.21 | -49.00 | -14.88 | 112.37 | 9.10 | 203.18 | 0.3899 | -1038.0 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.33 | -14.87 | 111.78 | 8.50 | 201.82 | 0.3861 | 534.0 | 415.0 | |
| 4.47 | 9.37 | 2.40 | 5.05 | -15.41 | 111.71 | 8.43 | 201.12 | 0.3938 | -931.9 | -829.9 | |
| 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. | |