Inclusion of In-Situ Velocity Measurements into the UCSD Time-Dependent Tomography to Constrain and Better-Forecast Remote-Sensing Observations

• Published in: Solar Physics
• Main Authors: Jackson, B. V., Hick, P. P., Bisi, M. M., Clover, J. M., Buffington, A.
• Format: Article in Journal/Newspaper
• Language: English
• Published: eScholarship, University of California 2010
• Subjects: Physics; Extraterrestrial Physics; Space Sciences; Meteorology/Climatology; Astrophysics and Astroparticles; Radio scintillation; Velocity fields; solar wind; Coronal mass ejections; interplanetary; disturbances; Murchison; EISCAT
• Online Access: http://www.escholarship.org/uc/item/056437md

The University of California, San Diego (UCSD) three-dimensional (3-D) time-dependent tomography program has been used successfully for a decade to reconstruct and forecast coronal mass ejections from interplanetary scintillation observations. More recently, we have extended this tomography techniqu...