scholarly journals The Radial Propagation Characteristics of the Injection Front: A Statistical Study Based On BD-IES and Van Allen Probes Observations

Author(s):  
Z. Y. Liu ◽  
Q.-G. Zong ◽  
Y. X. Hao ◽  
Y. Liu ◽  
X.-R. Chen
2017 ◽  
Vol 122 (8) ◽  
pp. 8327-8339 ◽  
Author(s):  
Xiao-Chen Shen ◽  
Mary K. Hudson ◽  
Allison N. Jaynes ◽  
Quanqi Shi ◽  
Anmin Tian ◽  
...  

2016 ◽  
Vol 121 (3) ◽  
pp. 2067-2079 ◽  
Author(s):  
Hao Zheng ◽  
Robert H. Holzworth ◽  
James B. Brundell ◽  
Abram R. Jacobson ◽  
John R. Wygant ◽  
...  

2015 ◽  
Vol 42 (18) ◽  
pp. 7273-7281 ◽  
Author(s):  
C. A. Cattell ◽  
A. W. Breneman ◽  
S. A. Thaller ◽  
J. R. Wygant ◽  
C. A. Kletzing ◽  
...  

2009 ◽  
Vol 114 (A11) ◽  
pp. n/a-n/a ◽  
Author(s):  
Teiji Uozumi ◽  
S. Abe ◽  
K. Kitamura ◽  
T. Tokunaga ◽  
A. Yoshikawa ◽  
...  

2011 ◽  
Vol 38 (20) ◽  
pp. n/a-n/a ◽  
Author(s):  
Oleksiy Agapitov ◽  
Vladimir Krasnoselskikh ◽  
Yuri V. Khotyaintsev ◽  
Guy Rolland

2016 ◽  
Vol 59 (7) ◽  
pp. 1508-1516 ◽  
Author(s):  
QiuGang Zong ◽  
YiXin Hao ◽  
Hong Zou ◽  
SuiYan Fu ◽  
XuZhi Zhou ◽  
...  

2015 ◽  
Vol 120 (6) ◽  
pp. 4748-4762 ◽  
Author(s):  
Lei Dai ◽  
Kazue Takahashi ◽  
Robert Lysak ◽  
Chi Wang ◽  
John R. Wygant ◽  
...  

2018 ◽  
Author(s):  
Shangchun Teng ◽  
Xin Tao ◽  
Wen Li ◽  
Yi Qi ◽  
Xinliang Gao ◽  
...  

Abstract. Spatial distribution and source region size of chorus waves are important parameters in understanding their generation.In this work, we analyze over 3 years of continuous wave burst mode data from Van Allen Probes and build a data set of rising and falling tone chorus. For the L shell range covered by Van Allen Probes data (3.5 ≤ L ≤ 7), statistical results demonstrate that the sector where rising tones are most likely to be observed is the dayside during geomagnetically quiet and moderate times and the dawnside during active times. Moreover, rising tone chorus waves have a higher occurrence rate near the equatorial plane, while the falling tone chorus waves have a higher possibility to be observed at lower L-shell and higher magnetic latitude. By analyzing the direction of Poynting wave vector, we statistically investigate the chorus source region size along a field line, and compare the results with previous theoretical estimates. Our analysis confirms previous conclusions that both rising tone and falling tone chorus waves are generated near the equatorial plane, and shows that previous theoretical estimates roughly agree with the observation within a factor of two. Our results provide important insights into further understanding of chorus generation.


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