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Title: Measure the Propagation of a Halo CME and Its Driven Shock with the Observations from a Single Perspective at Earth

Abstract

We present a detailed study of an Earth-directed coronal mass ejection (full-halo CME) event that happened on 2011 February 15, making use of white-light observations by three coronagraphs and radio observations by Wind /WAVES. We applied three different methods to reconstruct the propagation direction and traveling distance of the CME and its driven shock. We measured the kinematics of the CME leading edge from white-light images observed by Solar Terrestrial Relations Observatory ( STEREO ) A and B , tracked the CME-driven shock using the frequency drift observed by Wind /WAVES together with an interplanetary density model, and obtained the equivalent scattering centers of the CME by the polarization ratio (PR) method. For the first time, we applied the PR method to different features distinguished from LASCO/C2 polarimetric observations and calculated their projections onto white-light images observed by STEREO-A and STEREO-B . By combining the graduated cylindrical shell (GCS) forward modeling with the PR method, we proposed a new GCS-PR method to derive 3D parameters of a CME observed from a single perspective at Earth. Comparisons between different methods show a good degree of consistence in the derived 3D results.

Authors:
; ;  [1];  [2];  [3]
  1. Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210008 Nanjing (China)
  2. Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, D-37077 Göttingen (Germany)
  3. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190 (China)
Publication Date:
OSTI Identifier:
22663895
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 835; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; COMPARATIVE EVALUATIONS; CYLINDRICAL CONFIGURATION; DENSITY; DISTANCE; MASS; POLARIZATION; SCATTERING; SIMULATION; SOLAR CORONA; SUN; VISIBLE RADIATION

Citation Formats

Lu, Lei, Feng, Li, Liu, Siming, Inhester, Bernd, and Zhao, Xinhua, E-mail: lfeng@pmo.ac.cn, E-mail: inhester@mps.mpg.de. Measure the Propagation of a Halo CME and Its Driven Shock with the Observations from a Single Perspective at Earth. United States: N. p., 2017. Web. doi:10.3847/1538-4357/835/2/188.
Lu, Lei, Feng, Li, Liu, Siming, Inhester, Bernd, & Zhao, Xinhua, E-mail: lfeng@pmo.ac.cn, E-mail: inhester@mps.mpg.de. Measure the Propagation of a Halo CME and Its Driven Shock with the Observations from a Single Perspective at Earth. United States. doi:10.3847/1538-4357/835/2/188.
Lu, Lei, Feng, Li, Liu, Siming, Inhester, Bernd, and Zhao, Xinhua, E-mail: lfeng@pmo.ac.cn, E-mail: inhester@mps.mpg.de. Wed . "Measure the Propagation of a Halo CME and Its Driven Shock with the Observations from a Single Perspective at Earth". United States. doi:10.3847/1538-4357/835/2/188.
@article{osti_22663895,
title = {Measure the Propagation of a Halo CME and Its Driven Shock with the Observations from a Single Perspective at Earth},
author = {Lu, Lei and Feng, Li and Liu, Siming and Inhester, Bernd and Zhao, Xinhua, E-mail: lfeng@pmo.ac.cn, E-mail: inhester@mps.mpg.de},
abstractNote = {We present a detailed study of an Earth-directed coronal mass ejection (full-halo CME) event that happened on 2011 February 15, making use of white-light observations by three coronagraphs and radio observations by Wind /WAVES. We applied three different methods to reconstruct the propagation direction and traveling distance of the CME and its driven shock. We measured the kinematics of the CME leading edge from white-light images observed by Solar Terrestrial Relations Observatory ( STEREO ) A and B , tracked the CME-driven shock using the frequency drift observed by Wind /WAVES together with an interplanetary density model, and obtained the equivalent scattering centers of the CME by the polarization ratio (PR) method. For the first time, we applied the PR method to different features distinguished from LASCO/C2 polarimetric observations and calculated their projections onto white-light images observed by STEREO-A and STEREO-B . By combining the graduated cylindrical shell (GCS) forward modeling with the PR method, we proposed a new GCS-PR method to derive 3D parameters of a CME observed from a single perspective at Earth. Comparisons between different methods show a good degree of consistence in the derived 3D results.},
doi = {10.3847/1538-4357/835/2/188},
journal = {Astrophysical Journal},
number = 2,
volume = 835,
place = {United States},
year = {Wed Feb 01 00:00:00 EST 2017},
month = {Wed Feb 01 00:00:00 EST 2017}
}