The Use of High Frequency Solar Radar to Detect Coronal Mass Ejections

Abstract

This report results from a contract tasking Radiophysical Research Institute (NTRFI) as follows: The contractor will investigate techniques of high frequency solar radars and receiving antennas to detect mass motions in the solar corona such as solar mass ejections. Testing will be accomplished and solar data taken using the Sura Radar Facility and the UTR-2 Receiving Antenna as described in the proposal.

Open PDF

Document Details

Document Type
Technical Report
Publication Date
Jan 01, 1998
Accession Number
ADA353482

Entities

People

  • S. V. Polyakov

Organizations

  • Russian Academy of Sciences

Tags

Communities of Interest

  • Energy and Power Technologies
  • Space

DTIC Thesaurus Topics

  • Beam Steering
  • Coronal Mass Ejections
  • Detection
  • Ejection
  • Frequency
  • Frequency Bands
  • Geosynchronous Satellites
  • Modulation
  • Monitoring
  • Radar Cross Sections
  • Radar Signals
  • Radio Waves
  • Scattering
  • Solar Activity
  • Solar Corona
  • Space Weather
  • Wave Propagation

Readers

  • Astronomy and Astrophysics.
  • Radar Systems Engineering.
  • Solar Physics