Filament Eruptions and the Solar Radio F10.7 Flux

Abstract

Objective 1: Determine whether the presence of, or changes in, an H filament can be used to infer properties of a flare-CME. This studied whether the actual presence of a filament can be used to assist in predicting future flare-CME events. It searched for a correlation between the physical properties of the filament (e.g., length, shape), changes in these properties prior to a flare-CME event, and measures of event strength (e.g., CME speed, CME kinetic energy, presence of a Moreton wave). Objective 2: Create high spatial resolution images of the Sun at 10.7cm.

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Document Details

Document Type
Technical Report
Publication Date
Aug 01, 2018
Accession Number
AD1057169

Entities

People

  • R. T. James McAteer

Organizations

  • New Mexico State University

Tags

Communities of Interest

  • Energy and Power Technologies
  • Space

DTIC Thesaurus Topics

  • Air Force
  • Air Force Research Laboratories
  • Bremsstrahlung
  • Coronal Mass Ejections
  • Department Of Defense
  • Environment
  • Military Research
  • New Mexico
  • Physical Properties
  • Scientific Research
  • Solar Activity
  • Solar Flares
  • Solar Radiation
  • Space Sciences
  • Space Weather
  • Students
  • Sun

Fields of Study

  • Physics

Readers

  • Computational Modeling and Simulation
  • Solar Physics

Technology Areas

  • AI & ML
  • AI & ML - Bayesian Inference