| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.58 | 51.49 | 0.83 | 27.54 | -13.34 | 161.93 | 7.43 | 200.19 | 0.3697 | 142.9 | 49.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-03 07:00:33 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 | 0.63 | -22.11 | 173.39 | 18.90 | 212.29 | 0.5639 | 695.0 | 611.1 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -17.66 | 170.80 | 16.31 | 213.35 | 0.4887 | 612.0 | 528.3 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -6.27 | 167.47 | 12.98 | 225.41 | 0.3148 | 788.0 | 592.2 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -9.12 | 167.53 | 13.03 | 219.70 | 0.3501 | 846.0 | 635.7 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -10.34 | 167.57 | 13.08 | 217.64 | 0.3661 | 841.0 | 618.6 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -9.92 | 167.31 | 12.81 | 217.78 | 0.3581 | 865.0 | 678.8 | |
| 0.00 | 1.94 | 0.00 | 1.05 | -13.88 | 166.20 | 11.70 | 209.52 | 0.4014 | 765.0 | 612.0 | |
| 0.00 | 1.76 | 0.00 | 0.93 | -9.51 | 165.77 | 11.27 | 214.99 | 0.3377 | 887.0 | 688.9 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -10.38 | 165.58 | 11.08 | 213.10 | 0.3479 | 839.0 | 663.1 | |
| 0.00 | 2.55 | 0.00 | 1.34 | -9.50 | 165.24 | 10.75 | 213.72 | 0.3327 | 695.0 | 590.7 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -22.78 | 165.59 | 11.09 | 199.95 | 0.5221 | 685.0 | 591.4 | |
| 0.00 | 1.85 | 0.00 | 1.02 | -17.34 | 164.41 | 9.92 | 202.13 | 0.4383 | 34.0 | 92.2 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -23.31 | 164.57 | 10.07 | 197.91 | 0.5245 | 613.0 | 541.9 | |
| 0.70 | 3.35 | 0.37 | 1.75 | -10.34 | 163.59 | 9.10 | 208.21 | 0.3306 | -945.6 | -748.0 | |
| 0.00 | 1.41 | 0.00 | 0.74 | -10.17 | 163.10 | 8.60 | 207.12 | 0.3244 | -738.0 | -389.3 | |
| 0.00 | 1.67 | 0.00 | 0.94 | -20.77 | 162.73 | 8.24 | 196.28 | 0.4799 | 592.0 | 406.7 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -12.07 | 161.60 | 7.11 | 200.75 | 0.3430 | 792.0 | 576.1 | |
| 0.00 | 2.55 | 0.00 | 1.34 | -11.49 | 161.22 | 6.72 | 200.31 | 0.3320 | 897.0 | 807.7 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -11.36 | 161.09 | 6.60 | 200.10 | 0.3293 | 1128.0 | 828.0 | |
| 0.88 | 2.46 | 0.46 | 1.29 | -11.46 | 159.22 | 4.72 | 194.60 | 0.3217 | -881.6 | -675.9 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -14.27 | 159.21 | 4.71 | 192.60 | 0.3664 | -920.0 | -651.6 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -11.18 | 159.09 | 4.60 | 194.44 | 0.3165 | 670.0 | 480.3 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -12.32 | 159.05 | 4.55 | 193.46 | 0.3347 | -953.0 | -795.5 | |
| 0.00 | 2.55 | 0.00 | 1.34 | -11.56 | 159.00 | 4.51 | 193.89 | 0.3223 | -932.0 | -703.3 | |
| 0.00 | 2.11 | 0.00 | 1.12 | -13.94 | 158.33 | 3.84 | 190.49 | 0.3583 | -978.0 | -822.1 | |
| 0.00 | 1.94 | 0.00 | 1.02 | -13.61 | 158.17 | 3.68 | 190.23 | 0.3526 | -930.0 | -749.3 | |
| 0.00 | 0.62 | 0.00 | 0.32 | -12.85 | 158.16 | 3.67 | 190.61 | 0.3402 | -897.0 | -728.7 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -22.65 | 157.80 | 3.31 | 186.22 | 0.4935 | 577.0 | 472.2 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -14.89 | 157.32 | 2.83 | 187.41 | 0.3711 | -909.0 | -706.6 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -19.86 | 157.14 | 2.64 | 185.56 | 0.4495 | 762.0 | 580.6 | |
| 0.00 | 4.58 | 0.00 | 2.42 | -13.54 | 156.78 | 2.29 | 186.42 | 0.3481 | -794.0 | -722.8 | |
| 0.00 | 1.58 | 0.00 | 0.82 | -9.14 | 154.38 | -0.11 | 179.58 | 0.2728 | 741.0 | 570.4 | |
| 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. | |