Geomagnetic Disturbances

Abstract

The changing magnetic field of the Sun interacts with the Earth s magnetosphere to cause geomagnetic activity. Our goal is to understand the processes that determine the inputs to the terrestrial system and generate magnetospheric disturbances. How does solar activity originate? How is it expressed in the corona and interplanetary medium? Can we forecast the quantities that determine how the terrestrial environment ultimately responds? Our aim is to understand the solar causes of geomagnetic disturbances and to build tools that can, from photospheric observations, forecast the conditions that result in space weather disturbances.

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Document Details

Document Type
Technical Report
Publication Date
Sep 30, 2003
Accession Number
ADA629098

Entities

People

  • Philip Scherrer
  • Xuepu Zhao

Organizations

  • Stanford University

Tags

Communities of Interest

  • Autonomy

DTIC Thesaurus Topics

  • Coronal Mass Ejections
  • Department Of Defense
  • Electronic Mail
  • Environment
  • Magnetic Disturbances
  • Magnetic Fields
  • Magnetic Flux
  • Magnetosphere
  • Observation
  • Observatories
  • Solar Activity
  • Solar Observatories
  • Solar Physics
  • Solar Wind
  • Space Weather
  • Sun
  • Websites

Fields of Study

  • Environmental science

Readers

  • Atmospheric Science / Meteorology, specifically Wind Wave Turbulence.
  • Ocean-Atmosphere Mesoscale Modeling, Data Assimilation, and Flux Boundary Layers
  • Solar Physics

Technology Areas

  • Space