Use of Interplanetary Radio Scintillation Power Spectra in Predicting Geomagnetic Disturbances.

Abstract

An investigation of the feasibility of using interplanetary scintillations (IPS) of cosmic radio sources for prediction of geomagnetic disturbances has been carried out based on observations taken May-December 1974 and May-August 1976. The 1974 observations were taken with the University of Iowa COCOA-Cross array at 34.3 MHz located at Clark Lake Radio Observatory near Borrego Springs, California and synoptic data on 33 sources were reduced to yield scintillation index (band-pass integrated IPS power) for each source. In 1976, COCOA-Cross observations at 34.3 MHz were supplemented by 38 MHz observations from the University of Maryland TPT array, also at Clark Lake, and the high time resolution data were reduced to obtain IPS power spectra from 0.1 to 3 Hz. From detailed analyses of both data sets, we conclude that IPS prediction of the onset of geomagnetic disturbances may be feasible with a lead time of about one day. (Author)

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Document Details

Document Type
Technical Report
Publication Date
Oct 31, 1977
Accession Number
ADA050172

Entities

People

  • B. L. Gotwols
  • D. G. Mitchell
  • E. C. Roelof
  • S. D. Shawhan
  • W. M. Cronyn

Organizations

  • Johns Hopkins University

Tags

Communities of Interest

  • Energy and Power Technologies
  • Space

DTIC Thesaurus Topics

  • Air Force
  • Confidence Limits
  • Data Analysis
  • Data Sets
  • Databases
  • Electrons
  • Frequency
  • Grids
  • Information Science
  • Lead Time
  • Magnetic Disturbances
  • Observation
  • Observatories
  • Physics Laboratories
  • Power Spectra
  • Scattering
  • Wind Velocity

Fields of Study

  • Physics

Readers

  • Archaeological Resource Survey
  • Radio communications and signal processing.
  • Solar Physics