Location of Coronal and IP Type II Burst Source Regions from Radio and White-light Observations

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

[2101] Interplanetary Physics / Coronal Mass Ejections, [2139] Interplanetary Physics / Interplanetary Shocks, [7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7534] Solar Physics, Astrophysics, And Astronomy / Radio Emissions

Scientific paper

We present our preliminary results on the locations of source regions of the type II radio bursts in the metric (m) and dekameter-hectometric (DH) wavelength range. Type II bursts are occasionally observed to consist of two temporally overlapping lanes of metric and DH bursts. It has been suggested that the DH-component could be associated with a CME-driven shock and the m-component with a blast wave or unknown source, or that the DH-component originates from the shock nose and the m-component from the shock flanks. In our study we used time-height measurements of the associated coronal mass ejections (CMEs) to estimate speeds at various position angles (PAs) along the CME front. We also estimated plasma densities at the same PAs in the corona from inversion of polarized brightness (pB) images of SOHO/LASCO coronagraphs. These measurements suggest that both the m and DH-components can be explained reasonably well with a single CME-driven shock as their source.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Location of Coronal and IP Type II Burst Source Regions from Radio and White-light 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 Location of Coronal and IP Type II Burst Source Regions from Radio and White-light Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Location of Coronal and IP Type II Burst Source Regions from Radio and White-light Observations will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-877777

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.