Coronal electron density distributions estimated from CMEs, DH type II radio bursts, and polarized brightness measurements-Reference-Cited by-同舟云学术

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Coronal electron density distributions estimated from CMEs, DH type II radio bursts, and polarized brightness measurements

Published:2016-04 Issue:4 Volume:121 Page:2853-2865
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Lee Jae‐Ok¹,Moon Y.‐J.¹²,Lee Jin‐Yi²,Lee Kyoung‐Sun³,Kim R.‐S.⁴

Affiliation:

1. School of Space ResearchKyung Hee University Yongin South Korea

2. Department of Astronomy and Space ScienceKyung Hee University Yongin South Korea

3. Hinode Science CenterNational Astronomical Observatory of Japan Tokyo Japan

4. Korea Astronomy and Space Science Institute Daejeon South Korea

Funder

Ministry of Education

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA022321

Reference65 articles.

1. SOHOObservations of a Coronal Mass Ejection

2. Solar wind density model from km-wave type III bursts

3. The source region of an interplanetary type II radio burst

4. FIRST COMPLETE DETERMINATION OF PLASMA PHYSICAL PARAMETERS ACROSS A CORONAL MASS EJECTION-DRIVEN SHOCK

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1. Can We Detect Coronal Mass Ejections through Asymmetries of Sun-as-a-star Extreme-ultraviolet Spectral Line Profiles?;The Astrophysical Journal Supplement Series;2022-06-01

2. Interplanetary type II radio bursts and their association with CMEs and flares;Astrophysics and Space Science;2018-05-22

3. Heights of Coronal Mass Ejections and Shocks Inferred from Metric and DH Type II Radio Bursts;Solar Physics;2017-09

4. Variation in Coronal Activity from Solar Cycle 24 Minimum to Maximum Using Three-Dimensional Reconstructions of the Coronal Electron Density from STEREO/COR1;Solar Physics;2017-07-21

5. Investigation on M-class Flare-Associated Coronal Mass Ejections with and Without DH Type II Radio Bursts;Solar Physics;2017-05-24

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