Physics
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..823j&link_type=abstract
In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2
Physics
1
Heliosphere: Structures
Scientific paper
The Air Force/NASA Solar Mass Ejection Imager (SMEI) launched January 6, 2003 is now recording whole sky data on each 100-minute orbit. Precise photometric images of the heliosphere around Earth are expected from these data. To optimize the information available from this and similar instruments, we are developing a tomographic technique for analyzing remote sensing observations of the heliosphere using both interplanetary scintillation (IPS) and Thomson scattering data. The technique provides a three-dimensional reconstruction of heliospheric velocities and densities. We have refined our tomography program to analyze time-dependent phenomena such as evolving corotating heliospheric structures and more discrete events such as coronal mass ejections (CMEs).
Buffington Andrew
Hick Pierre P.
Jackson Bernard V.
No associations
LandOfFree
Time-dependent tomography of heliospheric structures using IPS and Thomson scattering observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Time-dependent tomography of heliospheric structures using IPS and Thomson scattering observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Time-dependent tomography of heliospheric structures using IPS and Thomson scattering observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1153024