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Inter‐Calibrated Measurements of Intense Whistlers by Arase and Van Allen Probes
Author(s) -
Santolík O.,
Miyoshi Y.,
Kolmašová I.,
Matsuda S.,
Hospodarsky G. B.,
Hartley D. P.,
Kasahara Y.,
Kojima H.,
Matsuoka A.,
Shinohara I.,
Kurth W. S.,
Kletzing C. A.
Publication year - 2021
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1029/2021ja029700
Subject(s) - spacecraft , whistler , amplitude , physics , calibration , waveform , polarization (electrochemistry) , ionosphere , space physics , computational physics , magnetic field , remote sensing , aerospace engineering , geophysics , optics , geology , astronomy , chemistry , engineering , quantum mechanics , voltage
Measurements of electromagnetic waves in space plasmas are an important tool for our understanding of physical processes in this environment. Inter‐calibration of data from different spacecraft missions is necessary for combining their measurements in empirical models or case studies. We show results collected during a close conjunction of the Van Allen Probes and Arase spacecraft. The inter‐calibration is based on a fortuitous case of common observations of strong whistlers at frequencies between a few hundred hertz and 10 kHz, which are generated by the same lightning strokes and which propagate along very similar paths to the two spacecraft. Measured amplitudes of the magnetic field fluctuations are the same within ∼14% precision of our analysis, corresponding to 1.2 dB. Currently, archived electric field measurements show twice larger amplitudes on Arase compared to Van Allen Probes but they start to match within ∼33% precision (2.5 dB) once the newest results on the interface of the antennas to the surrounding plasma are included in the calibration procedures. Ray tracing simulations help us to build a consistent scenario of wave propagation to both spacecraft reflected by a successful inter‐calibration of the polarization and propagation parameters obtained from multicomponent measurements. We succeed in linking the spacecraft observations to localizations of lightning return strokes by two different ground‐based networks which independently verify the correctness of the Universal Time tags of waveform measurements by both spacecraft missions, with an uncertainty better than 10 ms.