scholarly journals Effect of probing signal on the output signals spectrum of nonlinear spin waves in a cross based on waveguides of iron-yttrium garnet film

2021 ◽  
Vol 29 (5) ◽  
pp. 812-828
Author(s):  
Aleksandr Kozhevnikov ◽  
◽  
Galina Dudko ◽  
Yuri Khivintsev ◽  
Valentin Sakharov ◽  
...  

Subject. A change in the spectrum of spin waves (SW) in a magnetic cross is investigated when two signals pass through it: a pump signal and a probe signal. Objective. Detection of specific features in formation of the spectra of the output signals of SW in the multiport structure based on a yttrium iron garnet (YIG) film in the case of excitation of two magnetostatic surface waves (MSSW) simultaneously by the input antenna, where the first, with power higher than the first-order parametric instability threshold is the pump, and the second one is a probe. Methods. The experiments were performed for a cross structure from YIG film in the form of two orthogonal waveguides with the SW wire antennas placed at the ends of the waveguides, where one of the antennas on the transversely magnetized waveguide was considered as the input. Result. It was found that by choosing the probing signal frequency, one can significantly (by 10 dB) change the relative signal levels for the satellite waves at the output antennas, which are secondary MSSWs with some new frequencies and appear in the output signals spectrum as a result of the thresholdless processes of merging of parametric spin waves generated by MSSW pumping. In this case the secondary MSSWs frequencies can differ at the output antennas located on orthogonal waveguides. Discussion. The discovered effect is associated with the nonreciprocal nature of propagation of both the pumping wave and the waves generated at parametric instability condition in the structure.

JETP Letters ◽  
1996 ◽  
Vol 64 (3) ◽  
pp. 171-176 ◽  
Author(s):  
B. A. Kalinikos ◽  
N. G. Kovshikov ◽  
M. P. Kostylev ◽  
H. Benner

Author(s):  
Seong Hwang ◽  
Seungha Yoon ◽  
Byungro Kim ◽  
Songhee Han ◽  
B K Cho
Keyword(s):  

2020 ◽  
Vol 14 (4) ◽  
pp. 2000011 ◽  
Author(s):  
Morteza Mohseni ◽  
Martin Kewenig ◽  
Roman Verba ◽  
Qi Wang ◽  
Michael Schneider ◽  
...  

2016 ◽  
Vol 7 ◽  
pp. 1-4 ◽  
Author(s):  
Ping Che ◽  
Yan Zhang ◽  
Chuanpu Liu ◽  
Sa Tu ◽  
Zhimin Liao ◽  
...  

2020 ◽  
Vol 14 (4) ◽  
pp. 2070022
Author(s):  
Morteza Mohseni ◽  
Martin Kewenig ◽  
Roman Verba ◽  
Qi Wang ◽  
Michael Schneider ◽  
...  

2019 ◽  
Vol 126 (24) ◽  
pp. 243906
Author(s):  
Jinho Lim ◽  
Wonbae Bang ◽  
Jonathan Trossman ◽  
Dovran Amanov ◽  
C. C. Tsai ◽  
...  

2006 ◽  
Vol 99 (1) ◽  
pp. 013901 ◽  
Author(s):  
Mingzhong Wu ◽  
Boris A. Kalinikos ◽  
Pavol Krivosik ◽  
Carl E. Patton

2020 ◽  
Author(s):  
Kazue Takahashi ◽  
Turc Turc ◽  
Emilia Kilpua ◽  
Naoko Takahashi ◽  
Andrew Dimmock ◽  
...  

<p>Observational studies have demonstrated that ULF waves excited in the ion foreshock are a main source of Pc3-4 ULF waves detected in the magnetosphere. However, quantitative understanding of the propagation of the waves is not easy, because the waves are generated through a kinetic process in the foreshock, pass through the turbulent magnetosheath, and propagate as fast mode waves and couple to shear Alfven waves within the magnetosphere.  Recent advancement of hybrid numerical simulations of foreshock dynamics motivated us to analyze observational data from multiple sources and compare the results with simulation results. We have selected the time interval 1000-1200 UT on 20 July 2016, when the THEMIS, GOES, and Van Allen Probe spacecraft covered the solar wind, foreshock, magnetosheath, and magnetosphere. The EMMA magnetometers (L=1.6-6.5) were located near noon. We found that the spectrum of the magnetic field magnitude (Bt) in the foreshock exhibits a peak near 90 mHz, which agrees with the theoretical prediction assuming an ion beam instability in the foreshock.  A similar Bt spectrum is found in the dayside outer magnetosphere but not in the magnetosheath or in the nightside magnetosphere.  On the ground, a 90 mHz spectral peak was detected in the H component only at L=2-3. The numerical simulation using the VLASIATOR code shows that the foreshock is formed on the prenoon sector but that the effect of the upstream waves in the magnetosphere is most pronounced at noon. The Bt spectrum of the simulated waves in the outer magnetosphere exhibits a peak at 90 mHz, which is consistent with the observation.</p>


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