scholarly journals Kinematic properties of solar coronal mass ejections: Correction for projection effects in spacecraft coronagraph measurements

2008 ◽  
Vol 113 (A1) ◽  
pp. n/a-n/a ◽  
Author(s):  
T. A. Howard ◽  
D. Nandy ◽  
A. C. Koepke
Keyword(s):  
Coronal Mass Ejections ◽  
Kinematic Properties ◽  
Solar Coronal

Solar Radio Emission as a Prediction Technique for Coronal Mass Ejections’ Detection

2017 ◽  
Vol 13 (S335) ◽  
pp. 321-323
Author(s):  
Vladimir M. Fridman ◽  
Olga A. Sheiner
Keyword(s):  
Statistical Analysis ◽  
Radio Emission ◽  
Coronal Mass Ejections ◽  
Solar Radio ◽  
Solar Radio Emission ◽  
Short Term ◽  
Prediction Technique ◽  
Solar Coronal

AbstractIn this report we present a possible scheme of short-term CME detection forecasting developed on the basis of statistical analysis of solar radio emission regularities prior to “isolated” solar Coronal Mass Ejections registered in 1998, 2003, 2009-2013.

The Timing of Flares Associated with the Two Dynamical Types of Solar Coronal Mass Ejections

2002 ◽  
Vol 574 (1) ◽  
pp. L97-L100 ◽  
Author(s):  
M. Zhang ◽  
L. Golub ◽  
E. DeLuca ◽  
J. Burkepile
Keyword(s):  
Coronal Mass Ejections ◽  
Solar Coronal

A Catalogue of Coronal Mass Ejections Observed by the Heliospheric Imagers throughout the STEREO Mission

2020 ◽  
Author(s):  
David Barnes ◽  
Jackie Davies ◽  
Richard Harrison
Keyword(s):  
Solar Wind ◽  
Solar Cycle ◽  
Coronal Mass Ejections ◽  
Angular Separation ◽  
Propagation Direction ◽  
Wide Angle ◽  
Continuous Observation ◽  
Stereo Mission ◽  
Using Data ◽  
Kinematic Properties

<p>Understanding the evolution of the solar wind is fundamental to advancing our knowledge of energy and mass transport in the solar system, rendering it crucial to space weather and its prediction. The advent of truly wide-angle heliospheric imaging has revolutionised the study of Coronal Mass Ejections (CMEs) by enabling their direct and continuous observation out to 1 AU and beyond. A catalogue of CMEs has been compiled using data from the Heliospheric Imagers (HIs) on board the two STEREO spacecraft, which began as part of the FP7 HELCATS project. The mission was launched in 2006 and continues to provide data, therefore spanning 13 years, over which more than two-thousand CMEs have been observed using HI. To these CMEs, we apply geometric models that make use of both single-spacecraft and stereoscopic observations in order to determine their kinematic properties. These include CME speed, acceleration, propagation direction and launch time. The resulting kinematic properties and their statistics are discussed in the context of existing CME catalogues produced from coronagraph observations. This is done with emphasis on how the different models we apply influence our results and how these differences evolve over the solar cycle and as the angular separation of the STEREO spacecraft increases throughout the mission.</p>

scholarly journals Identification of Solar Coronal Mass Ejections in Cosmic Ray Flux Using Flicker Noise Spectroscopy

2015 ◽  
Vol 74 ◽  
pp. 336-339 ◽  
Author(s):  
V.V. Borog ◽  
I.O. Ivanov ◽  
A.V. Kryanev ◽  
S.F. Timashev
Keyword(s):  
Coronal Mass Ejections ◽  
Flicker Noise ◽  
Cosmic Ray ◽  
Noise Spectroscopy ◽  
Cosmic Ray Flux ◽  
Solar Coronal

ARE THE FAINT STRUCTURES AHEAD OF SOLAR CORONAL MASS EJECTIONS REAL SIGNATURES OF DRIVEN SHOCKS?

2014 ◽  
Vol 796 (1) ◽  
pp. L16 ◽  
Author(s):  
Jae-Ok Lee ◽  
Y.-J. Moon ◽  
Jin-Yi Lee ◽  
Kyoung-Sun Lee ◽  
Sujin Kim ◽  
...  
Keyword(s):  
Coronal Mass Ejections ◽  
Solar Coronal
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