Space Weather Using Remote Sensing Data

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

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh22c05j&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH22C-05

Physics

2164 Solar Wind Plasma, 2194 Instruments And Techniques, 7513 Coronal Mass Ejections

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 (e.g. by the SOHO/LASCO coronagraph and Helios photometers) and interplanetary scintillation (IPS) observations. We have refined the program to enable us to analyze time-dependent phenomena, such as the evolution of corotating 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 the three-dimensional analyses in real-time using IPS observations in order to forecast the arrival of CMEs, and we intend to show these analyses at our display. This work is supported by AFRL grant F49620-01-1-0054 and NSF grant ATM-9819947.

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