| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.32 | 218.23 | 36.16 | 114.07 | 18.99 | 170.93 | -4.08 | 11.85 | 0.3202 | -118.5 | 95.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-30 07:58:56 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 |
| 7.18 | 80.61 | 3.72 | 41.86 | 18.26 | 174.19 | -0.82 | 2.63 | 0.2981 | -1004.3 | -589.3 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 21.54 | 174.07 | -0.94 | 2.48 | 0.3526 | -733.0 | -555.0 | |
| 25.56 | -1.00 | 13.27 | -1.00 | 18.48 | 173.81 | -1.20 | 3.78 | 0.3021 | -1183.1 | 999999 | |
| 0.00 | 3.59 | 0.00 | 1.87 | 18.63 | 173.28 | -1.73 | 5.40 | 0.3054 | -786.0 | -620.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 19.35 | 173.15 | -1.86 | 5.57 | 0.3175 | 617.0 | 396.8 | |
| 3.59 | 8.80 | 1.87 | 4.58 | 18.76 | 172.94 | -2.07 | 6.42 | 0.3080 | -1010.7 | -655.7 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 20.53 | 172.72 | -2.29 | 6.38 | 0.3377 | -786.0 | -625.8 | |
| 0.00 | 0.34 | 0.00 | 0.18 | 18.23 | 172.72 | -2.29 | 7.29 | 0.2997 | -676.0 | -669.8 | |
| 0.00 | 1.62 | 0.00 | 0.84 | 18.63 | 172.56 | -2.45 | 7.62 | 0.3067 | -486.0 | -424.1 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.91 | 172.56 | -2.45 | 7.50 | 0.3114 | -831.0 | -627.2 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 18.13 | 172.48 | -2.53 | 8.12 | 0.2987 | -644.0 | -496.8 | |
| 8.89 | 10.60 | 4.64 | 5.53 | 18.97 | 171.90 | -3.11 | 9.45 | 0.3140 | -823.9 | -519.9 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.16 | 171.17 | -3.84 | 12.18 | 0.3031 | 1173.0 | 916.3 | |
| 1.03 | 2.74 | 0.53 | 1.42 | 18.32 | 170.91 | -4.10 | 12.84 | 0.3065 | 868.5 | 782.5 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 19.50 | 170.57 | -4.44 | 12.96 | 0.3269 | -877.0 | -707.0 | |
| 0.00 | 2.91 | 0.00 | 1.53 | 19.97 | 170.21 | -4.80 | 13.61 | 0.3358 | -1125.0 | -711.5 | |
| 0.00 | 2.05 | 0.00 | 1.08 | 19.90 | 169.93 | -5.08 | 14.42 | 0.3359 | -889.0 | -727.9 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.06 | 169.92 | -5.09 | 15.13 | 0.3225 | 827.0 | 588.2 | |
| 0.00 | 3.33 | 0.00 | 1.74 | 19.12 | 169.67 | -5.34 | 15.79 | 0.3246 | 714.0 | 623.9 | |
| 0.00 | 0.34 | 0.00 | 0.18 | 18.81 | 169.65 | -5.36 | 16.13 | 0.3197 | 477.0 | 642.2 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 19.12 | 169.39 | -5.62 | 16.58 | 0.3259 | 1111.0 | 840.2 | |
| 0.00 | 1.97 | 0.00 | 1.03 | 18.94 | 169.21 | -5.81 | 17.26 | 0.3238 | 977.0 | 716.4 | |
| 1.45 | 2.82 | 0.76 | 1.48 | 19.25 | 168.91 | -6.10 | 17.77 | 0.3302 | 1029.8 | 834.1 | |
| 0.00 | 1.88 | 0.00 | 0.98 | 18.84 | 168.52 | -6.49 | 19.26 | 0.3259 | 1042.0 | 831.0 | |
| 0.00 | 10.69 | 0.00 | 5.61 | 19.34 | 168.37 | -6.64 | 19.13 | 0.3344 | 1059.0 | 935.7 | |
| 0.00 | 3.85 | 0.00 | 2.04 | 20.65 | 168.12 | -6.89 | 18.45 | 0.3560 | 1011.0 | 803.8 | |
| 2.31 | 14.62 | 1.22 | 7.73 | 20.00 | 168.03 | -6.98 | 19.35 | 0.3464 | 904.3 | 712.8 | |
| 5.81 | 45.56 | 3.05 | 23.94 | 19.28 | 167.90 | -7.11 | 20.44 | 0.3361 | 1232.5 | 653.0 | |
| 6.41 | -28.00 | 3.37 | -28.00 | 19.40 | 167.67 | -7.34 | 20.89 | 0.3393 | 991.9 | 999999 | |
| 2.82 | -27.00 | 1.49 | -27.00 | 20.15 | 167.64 | -7.37 | 20.16 | 0.3509 | 1061.4 | 999999 | |
| 4.27 | -28.00 | 2.24 | -28.00 | 18.97 | 167.66 | -7.35 | 21.42 | 0.3327 | 1152.2 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 20.28 | 167.32 | -7.69 | 20.83 | 0.3547 | 543.0 | 444.4 | |
| 0.00 | 2.05 | 0.00 | 1.09 | 19.99 | 167.04 | -7.97 | 21.81 | 0.3521 | 820.0 | 649.1 | |
| 0.00 | 3.16 | 0.00 | 1.67 | 19.46 | 166.47 | -8.54 | 23.86 | 0.3478 | 981.0 | 801.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 19.21 | 166.32 | -8.69 | 24.53 | 0.3450 | 891.0 | 773.5 | |
| 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. | |