Lensing from small-scale travelling ionospheric disturbances observed using LOFAR

被引:14
|
作者
Boyde, Ben [1 ]
Wood, Alan [1 ]
Dorrian, Gareth
Fallows, Richard A.
Themens, David [1 ]
Mielich, Jens [2 ]
Elvidge, Sean [1 ]
Mevius, Maaijke
Zucca, Pietro
Dabrowski, Bartosz [3 ]
Krankowski, Andrzej [3 ]
Vocks, Christian [4 ]
Bisi, Mario [5 ]
机构
[1] Univ Birmingham, Sch Engn, Space Environm & Radio Engn, Birmingham B15 2TT, W Midlands, England
[2] Univ Rostock, Leibniz Inst Atmospher Phys, D-18556 Juliusruh, Germany
[3] Univ Warmia & Mazury, Space Radiodiagnost Res Ctr, Ul Romana Prawocheskiego 9, PL-10719 Olsztyn, Poland
[4] Leibniz Inst Astrophys Potsdam, Sternwarte 16, D-14482 Potsdam, Germany
[5] Rutherford Appleton Lab, UKRI STFC, RAL Space, Harwell Campus, Oxford OX11 0QX, Oxon, England
基金
英国科学技术设施理事会; 美国国家科学基金会; 爱尔兰科学基金会;
关键词
Small-scale travelling ionospheric disturbance; phase screen; ionospheric physics; ATMOSPHERIC GRAVITY-WAVES;
D O I
10.1051/swsc/2022030
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observations made using the LOw-Frequency ARray (LOFAR) between 10:15 and 11:48 UT on the 15th of September 2018 over a bandwidth of approximately 25-65 MHz contain discrete pseudo-periodic features of ionospheric origin. These features occur within a period of approximately 10 min and collectively last roughly an hour. They are strongly frequency dependent, broadening significantly in time towards the lower frequencies, and show an overlaid pattern of diffraction fringes. By modelling the ionosphere as a thin phase screen containing a wave-like disturbance, we are able to replicate the observations, suggesting that they are associated with small-scale travelling ionospheric disturbances (TIDs). This modelling indicates that the features observed here require a compact radio source at a low elevation and that the TID or TIDs in question have a wavelength <similar to 30 km. Several features suggest the presence of deviations from an idealised sinusoidal wave form. These results demonstrate LOFAR's capability to identify and characterise small-scale ionospheric structures.
引用
收藏
页数:13
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