Geomagnetic Disturbances

Abstract

Interactions of the changing magnetic field of the Sun with the Earth's magnetosphere cause geomagnetic activity. We seek to understand the physical processes that affect the inputs to the terrestrial system and generate geomagnetospheric disturbances. The goal is to understand how solar activity originates, how it is expressed in the corona and interplanetary medium, and how it ultimately affects the terrestrial environment. We are working to develop tools that can, from photospheric observations, reliably forecast the solar events and solar wind conditions that cause the geomagnetic disturbances that impact human activities on and near the Earth.

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Document Details

Document Type
Technical Report
Publication Date
Sep 30, 1998
Accession Number
ADA537680

Entities

People

  • J. T. Hoeksema
  • Philip Scherrer

Organizations

  • Stanford University

Tags

Communities of Interest

  • Materials and Manufacturing Processes

DTIC Thesaurus Topics

  • Coronal Mass Ejections
  • Cycles
  • Electronic Mail
  • Filaments
  • Magnetic Disturbances
  • Magnetic Fields
  • Observation
  • Observatories
  • Software Prototyping
  • Solar Activity
  • Solar Corona
  • Solar Cycle
  • Solar Observatories
  • Solar Wind
  • Sun
  • Websites
  • Wind

Fields of Study

  • Environmental science
  • Physics

Readers

  • Oncology
  • Solar Physics
  • Space/Atmospheric Physics.