scholarly journals Electron densities inferred from plasma wave spectra obtained by the Waves instrument on Van Allen Probes

2015 ◽  
Vol 120 (2) ◽  
pp. 904-914 ◽  
Author(s):  
W. S. Kurth ◽  
S. De Pascuale ◽  
J. B. Faden ◽  
C. A. Kletzing ◽  
G. B. Hospodarsky ◽  
...  
2009 ◽  
Vol 114 (A5) ◽  
pp. n/a-n/a ◽  
Author(s):  
B. L. Barnhart ◽  
W. S. Kurth ◽  
J. B. Groene ◽  
J. B. Faden ◽  
O. Santolik ◽  
...  

Author(s):  
A. H. Sulaiman ◽  
S. S. Elliott ◽  
W. S. Kurth ◽  
J. B. Faden ◽  
G. B. Hospodarsky ◽  
...  

2016 ◽  
Vol 43 (24) ◽  
pp. 12,348-12,355 ◽  
Author(s):  
X.-J. Zhang ◽  
W. Li ◽  
R. M. Thorne ◽  
V. Angelopoulos ◽  
J. Bortnik ◽  
...  

1983 ◽  
Vol 88 (A12) ◽  
pp. 10123 ◽  
Author(s):  
Ann M. Persoon ◽  
Donald A. Gurnett ◽  
Stanley D. Shawhan

2021 ◽  
Vol 39 (4) ◽  
pp. 613-625
Author(s):  
Geng Wang ◽  
Mingyu Wu ◽  
Guoqiang Wang ◽  
Sudong Xiao ◽  
Irina Zhelavskaya ◽  
...  

Abstract. We investigate the reflection of low-harmonic fast magnetosonic (MS) waves at the local two-ion cutoff frequency (fcutHe+). By comparing the wave signals of the two Van Allen Probes satellites, a distinct boundary where wave energies cannot penetrate inward are found in the time–frequency domain. The boundary is identified as the time series of local fcutHe+. For a certain frequency, there exists a spatial interface formed by fcutHe+, where the incident waves should be reflected. The waves with small incident angles are more likely to penetrate the thin layer where the group velocity reduces significantly and then slow down in a period of several to tens of seconds before the reflection process complete. The cutoff reflection scenario can explain the intense outward waves observed by probe A. These results of MS reflection at fcutHe+ may help to predict the global distribution of MS waves and promote the understanding of wave–particle dynamics in the radiation belt.


1984 ◽  
Vol 11 (10) ◽  
pp. 1050-1053 ◽  
Author(s):  
F. L. Scarf ◽  
F. V. Coroniti ◽  
C. F. Kennel ◽  
E. J. Smith ◽  
J. A. Slavin ◽  
...  
Keyword(s):  

1981 ◽  
Vol 86 (A10) ◽  
pp. 8181-8198 ◽  
Author(s):  
F. L. Scarf ◽  
D. A. Gurnett ◽  
W. S. Kurth
Keyword(s):  

Author(s):  
George B. Hospodarsky ◽  
W. S. Kurth ◽  
C. A. Kletzing ◽  
S. R. Bounds ◽  
O. Santolík ◽  
...  

2004 ◽  
Vol 22 (7) ◽  
pp. 2337-2344 ◽  
Author(s):  
K. Sigsbee ◽  
C. A. Kletzing ◽  
D. A. Gurnett ◽  
J. S. Pickett ◽  
A. Balogh ◽  
...  

Abstract. We present the statistics of Langmuir wave amplitudes in the Earth's foreshock using Cluster Wideband Data (WBD) Plasma Wave Receiver electric field waveforms from spacecraft 2, 3 and 4 on 26 March 2002. The largest amplitude Langmuir waves were observed by Cluster near the boundary between the foreshock and solar wind, in agreement with earlier studies. The characteristics of the waves were similar for all three spacecraft, suggesting that variations in foreshock structure must occur on scales greater than the 50-100km spacecraft separations. The electric field amplitude probability distributions constructed using waveforms from the Cluster WBD Plasma Wave Receiver generally followed the log-normal statistics predicted by stochastic growth theory for the event studied. Comparison with WBD receiver data from 17 February 2002, when spacecraft 4 was set in a special manual gain mode, suggests non-optimal auto-ranging of the instrument may have had some influence on the statistics.


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