Space Weather Using Remote Sensing Data

Details Space Weather Using Remote Sensing Data Space Weather Using Remote Sensing Data

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh31a0698j&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH31A-0698

Physics

2102 Corotating Streams, 2111 Ejecta, Driver Gases, And Magnetic Clouds, 2164 Solar Wind Plasma, 7513 Coronal Mass Ejections, 7899 General Or Miscellaneous

Scientific paper

We are developing tomographic techniques for analyzing remote sensing observations of the coronal and heliospheric density and velocity structure as observed in Thomson scattering and also using interplanetary scintillation (IPS) observations. We have refined our program to enable us to analyze time-dependent phenomena, such as the evolution of co-rotating heliospheric structures and rapidly evolving events such as coronal mass ejections, as observed e.g. with the future Solar Mass Ejection Imager (SMEI) experiment. We currently provide heliospheric three-dimensional reconstructions in real-time using IPS observations from STELab, Nagoya University, Japan in order to forecast the arrival at Earth of CMEs. We compare these reconstructions modeled at Earth with ACE in-situ spacecraft data and show these analyses along with a goodness-of-fit criterion designed to certify the reconstructions and refine our technique. This work is supported by AFOSR contract F49620-01-1-0054 and NASA contract NAG5-8504. index.html

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