scholarly journals New chorus wave properties near the equator from Van Allen Probes wave observations

2016 ◽  
Vol 43 (10) ◽  
pp. 4725-4735 ◽  
Author(s):  
W. Li ◽  
O. Santolik ◽  
J. Bortnik ◽  
R. M. Thorne ◽  
C. A. Kletzing ◽  
...  
2020 ◽  
Author(s):  
David M. Malaspina ◽  
Allison N Jaynes ◽  
Scot R. Elkington ◽  
Anthony Arthur Chan ◽  
George Blair Hospodarsky ◽  
...  

2019 ◽  
Vol 46 (8) ◽  
pp. 4070-4078 ◽  
Author(s):  
Chao Yue ◽  
Chae‐Woo Jun ◽  
Jacob Bortnik ◽  
Xin An ◽  
Qianli Ma ◽  
...  

2020 ◽  
Author(s):  
David P. Hartley ◽  
Lunjin Chen ◽  
Craig Kletzing ◽  
Richard Horne ◽  
Ondrej Santolik

<p>Correlations between chorus waves and plasmaspheric hiss have been directly observed, leading to the proposition that the two wave modes are causally linked. Ray tracing simulations have confirmed that chorus waves can propagate into the plasmasphere and be a source of plasmaspheric hiss, but only for a specific set of initial conditions, particularly relating to the orientation of the wave vector at the chorus source. In this study, both survey and burst mode observations from the Van Allen Probes EMFISIS Waves instrument are coupled with ray tracing simulations to determine the fraction of chorus wave power that exists with the conditions required to enter the plasmasphere. In general, it is found that only a small fraction (< 2%) of chorus wave power exists with the required wave vector orientation. An exception is found when the chorus source is located close to a plasmaspheric plume. Here, azimuthal density gradients modify the wave propagation to permit a large fraction, up to 94%, of chorus wave power to access the plasmasphere. Therefore plasmaspheric plumes are identified as an important access region if a significant fraction of chorus wave power is to enter the plasmasphere and be a source of plasmaspheric hiss. To provide context, we note that plumes are most commonly observed on the dusk side whereas chorus wave power typically peak on the dawn side. The post-noon sector, where these two statistical distributions overlap, appears to be key for observing correlations between chorus and hiss. As such, particular attention is devoted to this region.</p>


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

2021 ◽  
Author(s):  
Shuai Zhang ◽  
Jonathan Rae ◽  
Clare Watt ◽  
Alexander Degeling ◽  
Anmin Tian ◽  
...  

<p>Whistler mode chorus waves play a vital role in the Earth’s outer radiation belt dynamics through the cyclotron resonant pitch angle diffusion.     Recent numerical studies have shown that the temporal and spatial variability of wave growth parameters have universal importance for the diffusion process, which should be much larger than those in the traditional averaged diffusion model.       In the present study, we analyzed both the temporal and spatial coherence of chorus wave in a statistical method using data from the EMFISIS instrument onboard the Van Allen Probes A&B from November 2012 to July 2019. In total, we find 3,875 chorus wave events to calculate the correlation of wave amplitudes between Van Allen Probes A&B.      The results show that both the spatial and temporal correlation of chorus waves decrease significantly with increasing spacecraft separation and time lag, and the spatial and temporal coherence of chorus wave only last ~433 km and ~12 s. We also find that the spatial coherence of chorus waves is higher at L>6, on the dayside, or with a lower geomagnetic index (AL*), while the temporal coherence of chorus waves does not depend on the L-shell, geomagnetic index (AL*) or magnetic local time (MLT). Our results will increase the accuracy of modeling wave-particle interactions due to chorus waves.</p>


2015 ◽  
Vol 120 (9) ◽  
pp. 7477-7492 ◽  
Author(s):  
A. A. Saikin ◽  
J.‐C. Zhang ◽  
R. C. Allen ◽  
C. W. Smith ◽  
L. M. Kistler ◽  
...  

2014 ◽  
Vol 41 (5) ◽  
pp. 1359-1366 ◽  
Author(s):  
Weichao Tu ◽  
G. S. Cunningham ◽  
Y. Chen ◽  
S. K. Morley ◽  
G. D. Reeves ◽  
...  

2019 ◽  
Vol 46 (5) ◽  
pp. 2337-2346 ◽  
Author(s):  
D. P. Hartley ◽  
C. A. Kletzing ◽  
L. Chen ◽  
R. B. Horne ◽  
O. Santolík

2018 ◽  
Vol 123 (1) ◽  
pp. 297-314 ◽  
Author(s):  
O. V. Agapitov ◽  
D. Mourenas ◽  
A. V. Artemyev ◽  
F. S. Mozer ◽  
G. Hospodarsky ◽  
...  

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

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