scholarly journals A novel technique to construct the global distribution of whistler mode chorus wave intensity using low-altitude POES electron data

2014 ◽  
Vol 119 (7) ◽  
pp. 5685-5699 ◽  
Author(s):  
Binbin Ni ◽  
Wen Li ◽  
Richard M. Thorne ◽  
Jacob Bortnik ◽  
Janet C. Green ◽  
...  
2020 ◽  
Author(s):  
Yang Zhang ◽  
Binbin Ni ◽  
Xudong Gu ◽  
Yuri Shprits ◽  
Song Fu ◽  
...  

<p><span>Magnetospheric chorus is known to play a significant role in the acceleration and loss of radiation belt electrons. Interactions of chorus waves with radiation belt particles are commonly evaluated using quasi-linear diffusion codes that rely on statistical models, which might not accurately provide the instantaneous global wave distribution from limited in-situ wave measurements. Thus, a novel technique capable of inferring wave amplitudes from POES particle measurements, with an extensive coverage of L-shell and magnetic local time, has been established to obtain event-specific, global dynamic evolutions of chorus waves. This study, using 5 years of POES electron data, further improves the technique, and enables us to subsequently infer the chorus wave amplitudes for all useful data points (removing the electrons which were in the drift loss cone) and to construct the global distribution of lower-band chorus wave intensity. The results obtained from the improved technique reproduce Van Allen Probes in-situ observations of chorus waves reasonably well and reconstruct the major features of the global distribution of chorus waves. We demonstrate that such a data-based, dynamic model can provide near-real-time estimates of chorus wave intensity on a global scale for any time period when POES data are available, which cannot be obtained from in-situ wave measurements by equatorial satellites alone, but is crucial for quantifying the  dynamics of the radiation belt electrons.</span></p>


2020 ◽  
Author(s):  
Frantisek Nemec ◽  
Ondřej Santolík ◽  
Michel Parrot

<p>Frequency-latitude plots of electromagnetic wave intensity in the very low frequency range (VLF, up to about 20 kHz) observed by the low altitude DEMETER spacecraft are analyzed. Apart from electromagnetic waves generated by plasma instabilities in the magnetosphere, a significant portion of the detected wave intensity comes from ground-based lightning activity and VLF military transmitters. These whistler mode waves are observed not only close to source locations, but also close to their geomagnetically conjugated points. There appears to be an upper frequency limit of such emissions, where the wave intensity substantially decreases. Its frequency roughly corresponds to half of the equatorial electron cyclotron frequency at a respective magnetic field line, suggesting a relation to wave ducting in ducts with enhanced density. However, it seems to exhibit a non-negligible longitudinal dependence and it is different during the day than during the night. We use a realistic model of the Earth’s magnetic field to explain the observed variations. We interpret the observations in terms of ducted/unducted wave propagation, and we compare the wave intensities in the source hemisphere with those measured in the hemisphere geomagnetically conjugated.</p>


2013 ◽  
Vol 40 (17) ◽  
pp. 4526-4532 ◽  
Author(s):  
W. Li ◽  
B. Ni ◽  
R. M. Thorne ◽  
J. Bortnik ◽  
J. C. Green ◽  
...  

2020 ◽  
Author(s):  
David M. Malaspina ◽  
Allison N Jaynes ◽  
Scot R. Elkington ◽  
Anthony Arthur Chan ◽  
George Blair Hospodarsky ◽  
...  

2015 ◽  
Vol 120 (4) ◽  
pp. 2819-2837 ◽  
Author(s):  
Jin-Hee Kim ◽  
Dae-Young Lee ◽  
Jung-Hee Cho ◽  
Dae-Kyu Shin ◽  
Kyung-Chan Kim ◽  
...  

2009 ◽  
Vol 36 (9) ◽  
Author(s):  
W. Li ◽  
R. M. Thorne ◽  
V. Angelopoulos ◽  
J. Bortnik ◽  
C. M. Cully ◽  
...  

2020 ◽  
Vol 126 (1) ◽  
Author(s):  
David M. Malaspina ◽  
Allison N. Jaynes ◽  
Scot Elkington ◽  
Anthony Chan ◽  
George Hospodarsky ◽  
...  

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