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Application of prassadco to the solar orbiter data of the low frequency receiver

  • O. Santolík
  • , J. Souček
  • , V. Fiala
  • , J. Chum
  • , T. Chust
  • , M. Maksimovic
  • Charles University
  • of Sciences
  • (CNRS/UVSQ/UPMC)
  • Sorbonne Univ.

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Low frequency (0-10 kHz) waves will be recorded by the planned Low Frequency Receiver (LFR) of the Radio and Plasma Wave (RPW) experiment for the Solar Orbiter mission. Interesting solar wind waves, as the ionacoustic and whistler-mode waves appear in this low frequency range. A sophisticated on board data processing and data reduction software can significantly increase the scientific content of these data at a given telemetry bandwidth. On-board spectral analysis will allow us to obtain spectral matrices of three magnetic and three electric components from search coils and electric antennas, respectively. From these matrices we plan to identify the basic wave properties: wave mode, polarization and wave vector direction. We plan to implement analysis techniques which are routinely used for the CLUSTER and DEMETER data (PRASSADCO routines for propagation analysis).

Original languageEnglish
Title of host publicationProceedings of the Second Solar Orbiter Workshop
EditionSP-641
Publication statusPublished - 1 Oct 2006
Externally publishedYes
Event2nd Solar Orbiter Workshop - Athens, Greece
Duration: 16 Oct 200620 Oct 2006

Publication series

NameEuropean Space Agency, (Special Publication) ESA SP
NumberSP-641
ISSN (Print)0379-6566

Conference

Conference2nd Solar Orbiter Workshop
Country/TerritoryGreece
CityAthens
Period16/10/0620/10/06

Keywords

  • Ion acoustic mode
  • Waves in plasmas
  • Whistler mode

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