scholarly journals In situ statistical observations of Pc1 pearl pulsations and unstructured EMIC waves by the Van Allen Probes

2017 ◽  
Vol 122 (1) ◽  
pp. 105-119 ◽  
Author(s):  
K. W. Paulson ◽  
C. W. Smith ◽  
M. R. Lessard ◽  
R. B. Torbert ◽  
C. A. Kletzing ◽  
...  
Keyword(s):  
2020 ◽  
Vol 125 (4) ◽  
Author(s):  
K. Sigsbee ◽  
C. A. Kletzing ◽  
J. B. Faden ◽  
A. N. Jaynes ◽  
G. D. Reeves ◽  
...  

2014 ◽  
Vol 41 (5) ◽  
pp. 1375-1381 ◽  
Author(s):  
M. E. Usanova ◽  
A. Drozdov ◽  
K. Orlova ◽  
I. R. Mann ◽  
Y. Shprits ◽  
...  

2014 ◽  
Vol 41 (3) ◽  
pp. 785-792 ◽  
Author(s):  
I. R. Mann ◽  
M. E. Usanova ◽  
K. Murphy ◽  
M. T. Robertson ◽  
D. K. Milling ◽  
...  

2016 ◽  
Vol 34 (2) ◽  
pp. 249-257 ◽  
Author(s):  
Ying Xiong ◽  
Zhigang Yuan ◽  
Jingfang Wang

Abstract. In this paper, we report in situ observations by the Cluster spacecraft of energetic ions scattered into the loss cone during the inbound pass from the plasma sheet into the plasmasphere. During the inbound pass of the plasma sheet, Cluster observed the isotropy ratio of energetic ions to gradually decrease from unity and the isotropic boundary extended to lower L value for higher-energy ions, implying that the field line curvature scattering mechanism is responsible for the scattered ions into the loss cone from the plasma sheet. In the outer boundary of a plasmasphere plume, Cluster 3 observed the increase of the isotropy ratio of energetic ions accompanied by enhancements of Pc2 waves with frequencies between the He+ ion gyrofrequency and O+ ion gyrofrequency estimated in the equatorial plane. Those Pc2 waves were left-hand circularly polarized and identified as electromagnetic ion cyclotron (EMIC) waves. Using the observed parameters, the calculations of the pitch angle diffusion coefficients for ring current protons demonstrate that EMIC waves could be responsible for the ions scattering and loss-cone filling. Our observations provide in situ evidence of energetic ion loss in the plasma sheet and the plasmasphere plume. Our results suggest that energetic ions scattering into the loss cone in the central plasma sheet and the outer boundary of the plasmaspheric plume are attributed to the field line curvature scattering mechanism and EMIC wave scattering mechanism, respectively.


2019 ◽  
Vol 46 (11) ◽  
pp. 5662-5669 ◽  
Author(s):  
Y. Miyoshi ◽  
S. Matsuda ◽  
S. Kurita ◽  
K. Nomura ◽  
K. Keika ◽  
...  
Keyword(s):  

2017 ◽  
Vol 122 (7) ◽  
pp. 7387-7395 ◽  
Author(s):  
Xiongdong Yu ◽  
Zhigang Yuan ◽  
Shiyong Huang ◽  
Dedong Wang ◽  
Haimeng Li ◽  
...  
Keyword(s):  

Author(s):  
J.-C. Zhang ◽  
A. A. Saikin ◽  
L. M. Kistler ◽  
C. W. Smith ◽  
H. E. Spence ◽  
...  
Keyword(s):  

2021 ◽  
Author(s):  
Yangfan He ◽  
Hui Wang ◽  
Lühr Hermann ◽  
Kistler Lynn ◽  
Saikin Anthony ◽  
...  

<p>The temporal and spatial evolution of electromagnetic ion cyclotron (EMIC) waves during<br>the magnetic storm of 21–29 June 2015 was investigated using high-resolution magnetic field observations<br>from Swarm constellation in the ionosphere and Van Allen Probes in the magnetosphere. Magnetospheric<br>EMIC waves had a maximum occurrence frequency in the afternoon sector and shifted equatorward during<br>the expansion phase and poleward during the recovery phase. However, ionospheric waves in subauroral<br>regions occurred more frequently in the nighttime than during the day and exhibited less obvious<br>latitudinal movements. During the main phase, dayside EMIC waves occurred in both the ionosphere<br>and magnetosphere in response to the dramatic increase in the solar wind dynamic pressure. Waves were<br>absent in the magnetosphere and ionosphere around the minimum SYM-H. During the early recovery<br>phase, He<sup>+ </sup>band EMIC waves were observed in the ionosphere and magnetosphere. During the late<br>recovery phase, H<sup>+</sup> band EMIC waves emerged in response to enhanced earthward convection during<br>substorms in the premidnight sector. The occurrence of EMIC waves in the noon sector was affected by<br>the intensity of substorm activity. Both ionospheric wave frequency and power were higher in the summer<br>hemisphere than in the winter hemisphere. Waves were confined to an MLT interval of less than 5 hr with a<br>duration of less than 186 min from coordinated observations. The results could provide additional insights<br>into the spatial characteristics and propagation features of EMIC waves during storm periods</p>


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