論文

査読有り
2017年12月

Wire Probe Antenna (WPT) and Electric Field Detector (EFD) of Plasma Wave Experiment (PWE) aboard the Arase satellite: specifications and initial evaluation results

EARTH PLANETS AND SPACE
  • Yasumasa Kasaba
  • Keigo Ishisaka
  • Yoshiya Kasahara
  • Tomohiko Imachi
  • Satoshi Yagitani
  • Hirotsugu Kojima
  • Shoya Matsuda
  • Masafumi Shoji
  • Satoshi Kurita
  • Tomoaki Hori
  • Atsuki Shinbori
  • Mariko Teramoto
  • Yoshizumi Miyoshi
  • Tomoko Nakagawa
  • Naoko Takahashi
  • Yukitoshi Nishimura
  • Ayako Matsuoka
  • Atsushi Kumamoto
  • Fuminori Tsuchiya
  • Reiko Nomura
  • 全て表示

69
174
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1186/s40623-017-0760-x
出版者・発行元
SPRINGER HEIDELBERG

This paper summarizes the specifications and initial evaluation results of Wire Probe Antenna (WPT) and Electric Field Detector (EFD), the key components for the electric field measurement of the Plasma Wave Experiment (PWE) aboard the Arase (ERG) satellite. WPT consists of two pairs of dipole antennas with similar to 31-m tip-to-tip length. Each antenna element has a spherical probe (60 mm diameter) at each end of the wire (15 m length). They are extended orthogonally in the spin plane of the spacecraft, which is roughly perpendicular to the Sun and enables to measure the electric field in the frequency range of DC to 10 MHz. This system is almost identical to the WPT of Plasma Wave Investigation aboard the BepiColombo Mercury Magnetospheric Orbiter, except for the material of the spherical probe (ERG: Al alloy, MMO: Ti alloy). EFD is a part of the EWO (EFD/WFC/OFA) receiver and measures the 2-ch electric field at a sampling rate of 512 Hz (dynamic range: +/- 200 mV/m) and the 4-ch spacecraft potential at a sampling rate of 128 Hz (dynamic range: +/- 100 V and +/- 3 V/m), with the bias control capability of WPT. The electric field waveform provides (1) fundamental information about the plasma dynamics and accelerations and (2) the characteristics of MHD and ion waves in various magnetospheric statuses with the magnetic field measured by MGF and PWE-MSC. The spacecraft potential provides information on thermal electron plasma variations and structure combined with the electron density obtained from the upper hybrid resonance frequency provided by PWE-HFA. EFD has two data modes. The continuous (medium-mode) data are provided as (1) 2-ch waveforms at 64 Hz (in apoapsis mode, L > 4) or 256 Hz (in periapsis mode, L < 4), (2) 1-ch spectrum within 1-232 Hz with 1-s resolution, and (3) 4-ch spacecraft potential at 8 Hz. The burst (high-mode) data are intermittently obtained as (4) 2-ch waveforms at 512 Hz and (5) 4-ch spacecraft potential at 128 Hz and downloaded with the WFC-E/B datasets after the selection. This paper also shows the initial evaluation results in the initial observation phase.

リンク情報
DOI
https://doi.org/10.1186/s40623-017-0760-x
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000418945500001&DestApp=WOS_CPL
ID情報
  • DOI : 10.1186/s40623-017-0760-x
  • ISSN : 1880-5981
  • Web of Science ID : WOS:000418945500001

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