Acceleration and Deceleration of CMEs Associated with Long Wavelength Radio Bursts

Details Acceleration and Deceleration of CMEs Associated with Long Wavelength Radio Bursts Acceleration and Deceleration of CMEs Associated with Long Wavelength Radio Bursts

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh31c07g&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH31C-07

Physics

7513 Coronal Mass Ejections, 7531 Prominence Eruptions, 7534 Radio Emissions, 7851 Shock Waves

Scientific paper

Type II radio bursts in the Decameter-Hectometric (DH) wavelengths indicate powerful MHD shocks leaving the inner corona. Almost all of these bursts are associated with massive and faster-than-average coronal mass ejections (CMEs). A particularly interesting characteristic of these DH CMEs is that they are predominantly decelerating in the coronagraph field of view. In the past, it was thought that there are mainly constant speed and accelerating CMEs. We discuss the possible explanations for the CME deceleration in the near-Sun interplanetary medium. Research supported by NASA, NSF and Air Force Office of Scientific Research

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