Disclaimer: The following material is being kept online for archival purposes.
Although accurate at the time of publication, it is no longer being updated. The page may contain broken links or outdated information, and parts may not function in current web browsers.
CME observations using IPS imaging technique
Abrupt increases in solar wind density fluctuations have been detected
from 327MHz interplanetary scintillation (IPS) imaging observations of
the solar wind. These IPS events are considered as transient phenomena
caused by CME in the IP medium. From comaprison with in situ measurements
of solar wind at 1 AU, the IPS events are found to be closely associated
with density enhancements, particularly those leading a jump in solar wind
Authors: Tokumaru, N., M. Kojima, and K. Fujiki
Organization: STE Lab., Nagoya Univ.
Address: 3-13 Honohara, Toyokawa
Aichi 442-8507, Japan
Above is background material for archival reference only.