TY - JOUR
T1 - Spatial Extent of Quasiperiodic Emissions Simultaneously Observed by Arase and Van Allen Probes on 29 November 2018
AU - Martinez-Calderon, C.
AU - Němec, F.
AU - Katoh, Y.
AU - Shiokawa, K.
AU - Kletzing, C.
AU - Hospodarsky, G.
AU - Santolik, O.
AU - Kasahara, Y.
AU - Matsuda, S.
AU - Kumamoto, A.
AU - Tsuchiya, F.
AU - Matsuoka, A.
AU - Shoji, M.
AU - Teramoto, M.
AU - Kurita, S.
AU - Miyoshi, Y.
AU - Ozaki, M.
AU - Nishitani, N.
AU - Oinats, A. V.
AU - Kurkin, V. I.
N1 - Funding Information:
This paper analyzed MGF‐L2 v.01.02 data, PWE OFA‐L2 v.02.01 data (including OFA‐Matrix), PWE HFA‐L2 v.01.01 data, PWE HFA‐L3 v.00.02 data, and OBT‐L2 v.02 data. This work was supported by Grants‐in‐Aid for Scientific Research (17F17030) of the Japan Society for the Promotion of Science and by the JSPS International Research Fellowship. Y. K., S. M., Y. M., and K. S. are also supported by Grants‐in‐Aid for Scientific Research (20H01959, 18H03727, 15H05815, 15H05747, 16H06286, 16H06286, 14J02108, and 17K05668) and JSPS Bilateral Open Partnership Joint Research Projects. F. N. was supported by GACR Grant 18‐00844S. O. S. acknowledges support from the Czech Academy of Sciences through the Praemium Academiae award. EMFISIS funding provided by JHU/APL Contract 921647 under NASA's prime Contract NAS501072.
Publisher Copyright:
©2020. American Geophysical Union. All Rights Reserved.
PY - 2020/9/1
Y1 - 2020/9/1
N2 - Recent availability of a considerable amount of satellite and ground-based data has allowed us to analyze rare conjugated events where extremely low and very low frequency waves from the same source region are observed in different locations. Here, we report a quasiperiodic (QP) emission, showing one-to-one correspondence, observed by three satellites in space (Arase and the Van Allen Probes) and a ground station. The main event was on 29 November 2018 from 12:06 to 13:08 UT during geomagnetically quiet times. Using the position of the satellites we estimated the spatial extent of the area where the one-to-one correspondence is observed. We found this to be up to 1.21 Earth's radii by 2.26 hr MLT, in radial and longitudinal directions, respectively. Using simple ray tracing calculations, we discuss the probable source location of these waves. At ∼12:20 UT, changes in the frequency sweep rate of the QP elements are observed at all locations associated with magnetic disturbances. We also discuss temporal changes of the spectral shape of QP observed simultaneously in space and on the ground, suggesting the changes are related to properties of the source mechanisms of the waves. This could be linked to two separate sources or a larger source region with different source intensities (i.e., electron flux). At frequencies below the low hybrid resonance, waves can experience attenuation and/or reflection in the magnetosphere. This could explain the sudden end of the observations at the spacecraft, which are moving away from the area where waves can propagate.
AB - Recent availability of a considerable amount of satellite and ground-based data has allowed us to analyze rare conjugated events where extremely low and very low frequency waves from the same source region are observed in different locations. Here, we report a quasiperiodic (QP) emission, showing one-to-one correspondence, observed by three satellites in space (Arase and the Van Allen Probes) and a ground station. The main event was on 29 November 2018 from 12:06 to 13:08 UT during geomagnetically quiet times. Using the position of the satellites we estimated the spatial extent of the area where the one-to-one correspondence is observed. We found this to be up to 1.21 Earth's radii by 2.26 hr MLT, in radial and longitudinal directions, respectively. Using simple ray tracing calculations, we discuss the probable source location of these waves. At ∼12:20 UT, changes in the frequency sweep rate of the QP elements are observed at all locations associated with magnetic disturbances. We also discuss temporal changes of the spectral shape of QP observed simultaneously in space and on the ground, suggesting the changes are related to properties of the source mechanisms of the waves. This could be linked to two separate sources or a larger source region with different source intensities (i.e., electron flux). At frequencies below the low hybrid resonance, waves can experience attenuation and/or reflection in the magnetosphere. This could explain the sudden end of the observations at the spacecraft, which are moving away from the area where waves can propagate.
KW - ERG
KW - RBSP
KW - VLF/ELF
KW - conjugated events
KW - quasiperiodic emissions
KW - spatial extent
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U2 - 10.1029/2020JA028126
DO - 10.1029/2020JA028126
M3 - Article
AN - SCOPUS:85092603176
SN - 2169-9380
VL - 125
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 9
M1 - e2020JA028126
ER -