A Study of Interacting Plasma Phenomena Using the Tomographic 3-Dimensional Reconstruction Techniques Developed for the Solar Mass Ejection Imager (SMEI)

Details A Study of Interacting Plasma Phenomena Using the Tomographic 3-Dimensional Reconstruction Techniques Developed for the Solar Mass Ejection Imager (SMEI) A Study of Interacting Plasma Phenomena Using the Tomographic 3-Dimensional Reconstruction Techniques Developed for the Solar Mass Ejection Imager (SMEI)

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh11d..04j&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH11D-04

Other

2102 Corotating Streams, 2111 Ejecta, Driver Gases, And Magnetic Clouds, 2164 Solar Wind Plasma, 7513 Coronal Mass Ejections, 7894 Instruments And Techniques

Scientific paper

We are developing tomographic techniques for analyzing remote sensing observations of heliospheric density and velocity structure as observed in Thomson scattering (e.g. using the Helios photometer data) for eventual use with Solar Mass Ejection Imager (SMEI) observations. We have refined the tomography program to enable us to analyze time-dependent phenomena, such as the evolution of corotating heliospheric structures and more discrete events such as coronal mass ejections. Both types of phenomena are discerned in our data, and are reconstructed in three dimensions. We use our tomography technique to study the interaction of these phenomena as they move outward from the Sun for several events that have been studied by multiple spacecraft in-situ observations and other techniques. This work is supported by NASA grant NAG5-8504 and AFOSR grant F49620-01-1-0054. >http://casswww.ucsd.edu/solar/crew/bjackson /index.html

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