SDO HMI 2011-10-11 16:59:02 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81.89 | 439.17 | 44.09 | 236.53 | -14.82 | 119.00 | 9.66 | 204.40 | 0.3943 | 362.2 | 248.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-10-11 16:59:02 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 |
| 5.25 | 76.39 | 2.83 | 41.26 | -14.10 | 121.04 | 11.70 | 209.78 | 0.3978 | 1108.8 | 385.5 | |
| 2.54 | -1.00 | 1.37 | -1.00 | -14.39 | 120.84 | 11.50 | 208.99 | 0.4001 | 1000.7 | 999999 | |
| 0.00 | 1.57 | 0.00 | 0.87 | -17.36 | 120.95 | 11.61 | 205.84 | 0.4424 | -862.0 | -683.7 | |
| 2.89 | -1.00 | 1.56 | -1.00 | -14.45 | 120.59 | 11.25 | 208.39 | 0.3990 | 952.2 | 999999 | |
| 0.00 | 5.51 | 0.00 | 2.96 | -13.58 | 120.36 | 11.02 | 208.98 | 0.3851 | 990.0 | 774.2 | |
| 0.00 | 1.22 | 0.00 | 0.66 | -15.11 | 120.43 | 11.09 | 207.26 | 0.4073 | 254.0 | 166.5 | |
| 0.00 | 1.22 | 0.00 | 0.66 | -15.24 | 120.31 | 10.97 | 206.87 | 0.4082 | -150.0 | -124.1 | |
| 0.00 | 2.27 | 0.00 | 1.22 | -13.86 | 120.15 | 10.81 | 208.16 | 0.3875 | 920.0 | 816.5 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -16.24 | 120.27 | 10.93 | 205.68 | 0.4221 | -599.0 | -411.6 | |
| 0.00 | 5.16 | 0.00 | 2.81 | -15.69 | 120.15 | 10.81 | 206.02 | 0.4134 | 27.0 | 152.0 | |
| 4.90 | 247.70 | 2.63 | 133.52 | -13.98 | 119.84 | 10.50 | 207.33 | 0.3869 | 1086.2 | 520.7 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -13.60 | 119.82 | 10.49 | 207.77 | 0.3813 | 703.0 | 525.8 | |
| 0.00 | 4.20 | 0.00 | 2.28 | -15.81 | 119.78 | 10.44 | 205.10 | 0.4125 | 240.0 | 210.4 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -13.18 | 119.59 | 10.25 | 207.76 | 0.3736 | 801.0 | 636.7 | |
| 49.70 | -11.00 | 26.83 | -11.00 | -14.97 | 119.61 | 10.27 | 205.66 | 0.3993 | 1224.5 | 999999 | |
| 0.00 | 1.75 | 0.00 | 0.95 | -16.48 | 119.53 | 10.19 | 203.89 | 0.4206 | 701.0 | 556.1 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -16.87 | 119.26 | 9.92 | 202.96 | 0.4245 | 767.0 | 637.4 | |
| 1.31 | -11.00 | 0.71 | -11.00 | -14.99 | 119.14 | 9.80 | 204.60 | 0.3965 | 996.1 | 999999 | |
| 0.00 | 1.75 | 0.00 | 0.93 | -13.17 | 119.03 | 9.69 | 206.46 | 0.3693 | 903.0 | 819.4 | |
| 0.87 | -11.00 | 0.47 | -11.00 | -14.93 | 119.01 | 9.67 | 204.39 | 0.3946 | 958.9 | 999999 | |
| 3.06 | -11.00 | 1.65 | -11.00 | -14.79 | 118.78 | 9.44 | 204.03 | 0.3912 | 1132.5 | 999999 | |
| 0.00 | 1.57 | 0.00 | 0.84 | -13.54 | 118.51 | 9.17 | 204.80 | 0.3711 | 946.0 | 715.1 | |
| 0.00 | 2.19 | 0.00 | 1.17 | -14.52 | 117.92 | 8.59 | 202.34 | 0.3818 | 37.0 | 21.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -16.29 | 117.78 | 8.44 | 200.32 | 0.4073 | 766.0 | 559.4 | |
| 0.00 | 1.40 | 0.00 | 0.75 | -13.82 | 117.65 | 8.31 | 202.42 | 0.3695 | 774.0 | 631.6 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -14.03 | 117.06 | 7.73 | 200.78 | 0.3693 | -388.0 | -249.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -14.89 | 116.94 | 7.60 | 199.65 | 0.3816 | -713.0 | -523.7 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -14.47 | 116.74 | 7.40 | 199.55 | 0.3742 | -718.0 | -520.7 | |
| 0.00 | 3.32 | 0.00 | 1.78 | -14.66 | 116.68 | 7.34 | 199.24 | 0.3768 | -815.0 | -707.4 | |
| 0.00 | 6.91 | 0.00 | 3.70 | -15.08 | 116.38 | 7.04 | 198.16 | 0.3816 | -855.0 | -810.3 | |
| 1.22 | 1.75 | 0.65 | 0.93 | -14.43 | 116.27 | 6.93 | 198.43 | 0.3711 | -860.5 | -859.5 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -15.33 | 116.30 | 6.96 | 197.74 | 0.3851 | -654.0 | -508.3 | |
| 0.00 | 11.02 | 0.00 | 5.87 | -14.27 | 116.02 | 6.68 | 197.94 | 0.3673 | -1025.0 | -864.6 | |
| 0.00 | 1.22 | 0.00 | 0.66 | -15.39 | 115.93 | 6.59 | 196.80 | 0.3842 | -856.0 | -669.8 | |
| 0.00 | 4.37 | 0.00 | 2.32 | -14.04 | 115.73 | 6.39 | 197.41 | 0.3624 | -1023.0 | -827.8 | |
| 3.15 | 7.17 | 1.67 | 3.81 | -13.91 | 115.51 | 6.17 | 196.95 | 0.3593 | -1169.5 | -835.4 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -15.51 | 115.52 | 6.18 | 195.74 | 0.3843 | -654.0 | -550.5 | |
| 0.00 | 2.19 | 0.00 | 1.17 | -14.58 | 115.46 | 6.13 | 196.30 | 0.3695 | -870.0 | -714.8 | |
| 0.00 | 1.92 | 0.00 | 1.06 | -19.20 | 115.43 | 6.09 | 193.19 | 0.4408 | 839.0 | 532.2 | |
| 0.00 | 1.92 | 0.00 | 1.02 | -13.69 | 115.19 | 5.85 | 196.32 | 0.3543 | -893.0 | -791.9 | |
| 1.66 | 8.92 | 0.89 | 4.79 | -15.99 | 114.63 | 5.29 | 193.26 | 0.3881 | -1037.1 | -764.6 | |
| 0.00 | 2.71 | 0.00 | 1.46 | -16.28 | 114.64 | 5.30 | 193.10 | 0.3927 | -824.0 | -683.4 | |
| 0.00 | 1.84 | 0.00 | 0.98 | -15.54 | 114.53 | 5.19 | 193.29 | 0.3806 | -841.0 | -617.0 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -15.27 | 114.18 | 4.84 | 192.58 | 0.3752 | -950.0 | -797.3 | |
| 0.00 | 2.10 | 0.00 | 1.16 | -19.29 | 114.25 | 4.91 | 190.67 | 0.4383 | -707.0 | -644.3 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -18.30 | 114.13 | 4.79 | 190.86 | 0.4225 | -757.0 | -650.9 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -15.85 | 113.69 | 4.35 | 191.04 | 0.3827 | -733.0 | -514.1 | |
| 0.00 | 2.80 | 0.00 | 1.50 | -16.07 | 113.48 | 4.14 | 190.40 | 0.3857 | -800.0 | -593.7 | |
| 5.34 | 7.09 | 2.83 | 3.75 | -14.24 | 113.23 | 3.89 | 190.69 | 0.3556 | -1062.5 | -780.4 | |
| 0.00 | 1.66 | 0.00 | 0.89 | -16.10 | 113.17 | 3.83 | 189.62 | 0.3853 | -919.0 | -763.5 | |
| 0.00 | 2.27 | 0.00 | 1.22 | -16.26 | 112.86 | 3.52 | 188.79 | 0.3870 | -856.0 | -730.3 | |
| 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. | |