| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.13 | 260.87 | 36.03 | 136.01 | 18.95 | 171.17 | -1.66 | 4.73 | 0.3140 | -82.5 | -62.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-30 11:58:56 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 |
| 0.00 | 1.20 | 0.00 | 0.62 | 19.29 | 175.00 | 2.17 | 353.49 | 0.3174 | -835.0 | -593.6 | |
| 2.82 | 116.98 | 1.46 | 60.76 | 18.30 | 174.24 | 1.41 | 355.50 | 0.2997 | -1072.9 | -568.8 | |
| 19.23 | -2.00 | 9.99 | -2.00 | 18.49 | 173.93 | 1.10 | 356.52 | 0.3024 | -1297.4 | 999999 | |
| 2.65 | -2.00 | 1.38 | -2.00 | 18.61 | 173.31 | 0.48 | 358.49 | 0.3041 | -1037.0 | 999999 | |
| 3.08 | -2.00 | 1.60 | -2.00 | 18.89 | 173.15 | 0.33 | 359.00 | 0.3087 | -914.4 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.21 | 172.78 | -0.05 | 0.16 | 0.2972 | -893.0 | -702.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 18.95 | 172.75 | -0.08 | 0.25 | 0.3097 | -889.0 | -613.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 18.61 | 172.65 | -0.17 | 0.54 | 0.3040 | -881.0 | -687.7 | |
| 0.00 | 1.79 | 0.00 | 0.93 | 19.04 | 172.56 | -0.27 | 0.82 | 0.3112 | -891.0 | -686.3 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.49 | 172.09 | -0.73 | 2.32 | 0.3021 | -666.0 | -476.8 | |
| 7.26 | 10.42 | 3.78 | 5.43 | 18.92 | 172.06 | -0.77 | 2.36 | 0.3094 | -833.2 | -334.5 | |
| 0.00 | 2.82 | 0.00 | 1.47 | 18.76 | 171.31 | -1.52 | 4.69 | 0.3076 | 271.0 | 61.2 | |
| 4.61 | 6.67 | 2.39 | 3.46 | 18.27 | 171.10 | -1.73 | 5.51 | 0.2996 | 983.2 | 736.0 | |
| 0.00 | 3.25 | 0.00 | 1.69 | 18.98 | 171.09 | -1.74 | 5.30 | 0.3115 | -839.0 | -742.5 | |
| 0.00 | 1.79 | 0.00 | 0.93 | 18.92 | 170.87 | -1.96 | 5.99 | 0.3108 | -801.0 | -598.8 | |
| 1.45 | 1.62 | 0.75 | 0.84 | 18.27 | 170.82 | -2.01 | 6.40 | 0.3001 | 832.9 | 608.5 | |
| 0.00 | 3.25 | 0.00 | 1.70 | 19.45 | 170.77 | -2.06 | 6.10 | 0.3198 | -725.0 | -717.3 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 19.98 | 170.32 | -2.50 | 7.19 | 0.3293 | -1014.0 | -781.5 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 20.04 | 169.85 | -2.98 | 8.50 | 0.3314 | -861.0 | -733.5 | |
| 3.67 | 5.98 | 1.92 | 3.12 | 19.23 | 169.65 | -3.18 | 9.51 | 0.3187 | 918.4 | 801.2 | |
| 0.00 | 3.33 | 0.00 | 1.74 | 18.83 | 169.62 | -3.20 | 9.80 | 0.3121 | 1102.0 | 866.3 | |
| 0.00 | 6.49 | 0.00 | 3.39 | 19.01 | 169.34 | -3.49 | 10.54 | 0.3160 | 1268.0 | 1004.0 | |
| 0.00 | 5.21 | 0.00 | 2.73 | 19.29 | 168.92 | -3.90 | 11.57 | 0.3219 | 751.0 | 646.0 | |
| 0.00 | 1.97 | 0.00 | 1.03 | 18.82 | 168.53 | -4.30 | 13.05 | 0.3157 | 783.0 | 693.9 | |
| 0.00 | 2.39 | 0.00 | 1.26 | 20.76 | 168.19 | -4.64 | 12.60 | 0.3481 | 1007.0 | 780.6 | |
| 2.22 | 4.19 | 1.17 | 2.20 | 20.01 | 167.93 | -4.90 | 13.84 | 0.3371 | 941.0 | 709.7 | |
| 15.81 | 48.54 | 8.28 | 25.40 | 19.38 | 167.73 | -5.10 | 14.89 | 0.3279 | 1035.8 | 703.3 | |
| 1.20 | 12.82 | 0.63 | 6.75 | 20.32 | 167.66 | -5.16 | 14.30 | 0.3431 | 802.6 | 648.4 | |
| 5.13 | -27.00 | 2.68 | -27.00 | 19.01 | 167.58 | -5.25 | 15.61 | 0.3226 | 1051.8 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.98 | 167.17 | -5.65 | 16.79 | 0.3240 | 113.0 | 122.9 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 19.91 | 166.95 | -5.88 | 16.53 | 0.3398 | 740.0 | 643.4 | |
| 0.00 | 5.21 | 0.00 | 2.74 | 19.35 | 166.44 | -6.39 | 18.44 | 0.3335 | 792.0 | 698.8 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.41 | 166.28 | -6.55 | 18.80 | 0.3353 | 595.0 | 498.0 | |
| 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. | |