| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83.02 | 440.74 | 44.59 | 235.58 | 15.09 | 232.27 | -17.44 | 50.65 | 0.3731 | -488.3 | -250.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-24 15:58:57 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 | 1.28 | 0.00 | 0.67 | 15.00 | 236.75 | -12.96 | 43.27 | 0.3175 | -943.0 | -686.0 | |
| 7.70 | 26.71 | 4.02 | 13.93 | 13.48 | 235.43 | -14.28 | 49.57 | 0.3165 | -1160.2 | -601.4 | |
| 1.54 | 1.63 | 0.81 | 0.85 | 13.26 | 234.78 | -14.93 | 51.32 | 0.3226 | -967.1 | -681.0 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 17.58 | 234.13 | -15.57 | 43.04 | 0.3766 | -846.0 | -629.4 | |
| 47.76 | 289.24 | 25.20 | 152.62 | 14.89 | 234.29 | -15.42 | 48.33 | 0.3454 | -1415.3 | -414.6 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 12.72 | 234.34 | -15.36 | 53.47 | 0.3231 | -1018.0 | -803.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.27 | 233.42 | -16.28 | 44.88 | 0.3812 | -847.0 | -694.7 | |
| 0.00 | 3.25 | 0.00 | 1.73 | 14.94 | 232.47 | -17.24 | 51.27 | 0.3687 | -907.0 | -714.4 | |
| 0.00 | 3.85 | 0.00 | 2.05 | 13.96 | 231.90 | -17.80 | 54.30 | 0.3669 | -342.0 | -592.1 | |
| 0.00 | 0.34 | 0.00 | 0.18 | 12.06 | 232.05 | -17.66 | 58.67 | 0.3489 | 792.0 | 746.8 | |
| 0.00 | 1.88 | 0.00 | 1.02 | 18.18 | 231.34 | -18.36 | 46.46 | 0.4147 | -843.0 | -668.9 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 17.19 | 231.42 | -18.29 | 48.22 | 0.4038 | -985.0 | -741.4 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 17.41 | 231.36 | -18.34 | 47.88 | 0.4066 | -755.0 | -614.0 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 17.34 | 231.17 | -18.53 | 48.28 | 0.4082 | -696.0 | -530.8 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 16.85 | 230.96 | -18.74 | 49.55 | 0.4059 | -789.0 | -611.1 | |
| 0.00 | 6.76 | 0.00 | 3.65 | 15.99 | 231.01 | -18.69 | 51.19 | 0.3970 | -909.0 | -835.8 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 15.47 | 231.00 | -18.71 | 52.29 | 0.3924 | -739.0 | -590.9 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 16.77 | 228.64 | -21.07 | 52.81 | 0.4339 | -808.0 | -620.0 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 16.89 | 228.36 | -21.35 | 52.92 | 0.4385 | -627.0 | -391.5 | |
| 0.00 | 2.57 | 0.00 | 1.43 | 17.37 | 227.56 | -22.14 | 52.95 | 0.4526 | -817.0 | -655.9 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 17.91 | 226.82 | -22.89 | 52.81 | 0.4665 | -694.0 | -540.0 | |
| 0.00 | 1.37 | 0.00 | 0.76 | 15.83 | 226.72 | -22.99 | 56.82 | 0.4508 | 1050.0 | 907.8 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 12.19 | 226.90 | -22.80 | 64.13 | 0.4228 | 683.0 | 467.2 | |
| 0.00 | 2.40 | 0.00 | 1.34 | 17.02 | 226.30 | -23.41 | 55.01 | 0.4656 | 893.0 | 863.0 | |
| 7.36 | 22.26 | 4.10 | 12.36 | 15.61 | 226.11 | -23.60 | 57.87 | 0.4572 | 968.6 | 448.8 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 16.77 | 225.79 | -23.91 | 56.01 | 0.4701 | 789.0 | 623.3 | |
| 0.00 | 2.05 | 0.00 | 1.15 | 16.70 | 225.56 | -24.14 | 56.36 | 0.4725 | 831.0 | 759.8 | |
| 7.28 | 59.58 | 4.07 | 33.37 | 15.94 | 225.63 | -24.08 | 57.72 | 0.4659 | 1205.1 | 633.2 | |
| 2.31 | -28.00 | 1.30 | -28.00 | 16.45 | 225.43 | -24.28 | 56.95 | 0.4724 | 821.6 | 999999 | |
| 0.60 | -28.00 | 0.34 | -28.00 | 16.06 | 225.41 | -24.29 | 57.71 | 0.4697 | 875.3 | 999999 | |
| 4.19 | -28.00 | 2.35 | -28.00 | 15.78 | 225.28 | -24.43 | 58.36 | 0.4694 | 881.1 | 999999 | |
| 2.48 | -28.00 | 1.39 | -28.00 | 16.12 | 225.20 | -24.51 | 57.80 | 0.4728 | 753.8 | 999999 | |
| 1.80 | -28.00 | 1.01 | -28.00 | 15.54 | 225.28 | -24.43 | 58.83 | 0.4677 | 696.4 | 999999 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 14.59 | 225.36 | -24.35 | 60.57 | 0.4600 | 723.0 | 505.9 | |
| 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. | |