SDO HMI 2011-06-14 13:59:11 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 |
| 48.94 | 136.76 | 25.20 | 70.52 | -15.03 | 246.10 | 2.14 | 187.59 | 0.2801 | 161.0 | -141.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-14 13:59:11 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 | 0.91 | 0.00 | 0.47 | -15.04 | 252.20 | 8.24 | 206.73 | 0.3090 | 619.0 | 595.6 | |
| 8.52 | 12.23 | 4.39 | 6.31 | -14.75 | 248.13 | 4.17 | 194.60 | 0.2802 | 1098.1 | 840.4 | |
| 0.00 | 4.44 | 0.00 | 2.30 | -15.25 | 247.83 | 3.87 | 193.14 | 0.2872 | 719.0 | 633.5 | |
| 6.43 | 46.40 | 3.31 | 23.87 | -14.46 | 247.72 | 3.76 | 193.45 | 0.2739 | 981.7 | 789.3 | |
| 0.00 | 9.15 | 0.00 | 4.73 | -15.32 | 247.42 | 3.46 | 191.75 | 0.2868 | 757.0 | 558.4 | |
| 26.55 | -4.00 | 13.66 | -4.00 | -14.37 | 247.37 | 3.41 | 192.33 | 0.2710 | 1145.7 | 999999 | |
| 0.00 | 1.81 | 0.00 | 0.93 | -14.90 | 246.49 | 2.53 | 188.91 | 0.2772 | 951.0 | 610.5 | |
| 1.36 | 2.81 | 0.70 | 1.44 | -13.83 | 246.45 | 2.49 | 189.41 | 0.2592 | 885.7 | 823.5 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -13.39 | 245.70 | 1.73 | 186.79 | 0.2500 | 612.0 | 421.1 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -13.61 | 245.45 | 1.48 | 185.73 | 0.2532 | -849.0 | -568.2 | |
| 3.81 | 16.13 | 1.97 | 8.33 | -15.60 | 245.02 | 1.06 | 183.57 | 0.2861 | -997.6 | -796.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -15.54 | 244.70 | 0.74 | 182.51 | 0.2848 | -1156.0 | -1037.6 | |
| 2.27 | 3.17 | 1.17 | 1.64 | -15.73 | 244.58 | 0.61 | 182.06 | 0.2879 | -1018.2 | -778.2 | |
| 0.00 | 2.63 | 0.00 | 1.35 | -14.15 | 244.57 | 0.61 | 182.27 | 0.2612 | -1142.0 | -937.8 | |
| 0.00 | 3.72 | 0.00 | 1.92 | -15.16 | 244.42 | 0.45 | 181.58 | 0.2782 | -1191.0 | -947.3 | |
| 0.00 | 5.26 | 0.00 | 2.72 | -15.92 | 244.23 | 0.27 | 180.88 | 0.2909 | -713.0 | -488.7 | |
| 0.00 | 2.08 | 0.00 | 1.07 | -14.87 | 244.19 | 0.23 | 180.83 | 0.2733 | -924.0 | -675.3 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -14.49 | 244.10 | 0.14 | 180.51 | 0.2669 | -935.0 | -670.3 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -18.87 | 243.72 | -0.24 | 179.32 | 0.3400 | 779.0 | 631.3 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -16.01 | 243.56 | -0.40 | 178.68 | 0.2926 | -862.0 | -678.8 | |
| 0.00 | 0.73 | 0.00 | 0.37 | -15.66 | 243.53 | -0.43 | 178.55 | 0.2867 | -748.0 | -623.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -16.24 | 243.40 | -0.56 | 178.19 | 0.2964 | -843.0 | -654.6 | |
| 0.00 | 1.72 | 0.00 | 0.89 | -15.47 | 243.37 | -0.59 | 178.00 | 0.2836 | -1008.0 | -768.6 | |
| 0.00 | 3.44 | 0.00 | 1.78 | -15.76 | 243.34 | -0.62 | 177.92 | 0.2884 | -924.0 | -821.9 | |
| 0.00 | 1.63 | 0.00 | 0.84 | -15.92 | 243.15 | -0.81 | 177.31 | 0.2912 | -1020.0 | -842.6 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -16.08 | 242.87 | -1.10 | 176.40 | 0.2941 | -912.0 | -748.3 | |
| 0.00 | 3.26 | 0.00 | 1.69 | -16.40 | 242.77 | -1.19 | 176.16 | 0.2996 | -996.0 | -773.9 | |
| 0.00 | 2.27 | 0.00 | 1.17 | -15.67 | 242.77 | -1.19 | 176.00 | 0.2873 | -1037.0 | -885.6 | |
| 0.00 | 0.91 | 0.00 | 0.47 | -15.44 | 242.74 | -1.22 | 175.84 | 0.2836 | -882.0 | -739.5 | |
| 0.00 | 0.91 | 0.00 | 0.47 | -17.42 | 242.67 | -1.29 | 176.08 | 0.3167 | -704.0 | -620.2 | |
| 0.00 | 0.45 | 0.00 | 0.23 | -16.05 | 242.39 | -1.57 | 174.84 | 0.2942 | -693.0 | -696.6 | |
| 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. | |