On the Rates of Coronal Mass Ejections: Remote Solar and In Situ Observations

2006 ◽  
Vol 647 (1) ◽  
pp. 648-653 ◽  
Author(s):  
Pete Riley ◽  
C. Schatzman ◽  
H. V. Cane ◽  
I. G. Richardson ◽  
N. Gopalswamy
Keyword(s):  
Coronal Mass Ejections ◽  
In Situ Observations

Linking Remote-Sensing and In Situ Observations of Coronal Mass Ejections Using STEREO

Solar Physics ◽  
2011 ◽  
Vol 270 (2) ◽  
pp. 561-573 ◽  
Author(s):  
L. Rodriguez ◽  
M. Mierla ◽  
A. N. Zhukov ◽  
M. West ◽  
E. Kilpua
Keyword(s):  
Remote Sensing ◽  
Coronal Mass Ejections ◽  
In Situ Observations

scholarly journals Properties of the Sheath Regions of Coronal Mass Ejections with or without Shocks from STEREO in situ Observations near 1 au

2020 ◽  
Vol 904 (2) ◽  
pp. 177
Author(s):  
Tarik M. Salman ◽  
Noé Lugaz ◽  
Charles J. Farrugia ◽  
Reka M. Winslow ◽  
Lan K. Jian ◽  
...  
Keyword(s):  
Coronal Mass Ejections ◽  
In Situ Observations

scholarly journals INTERACTIONS BETWEEN CORONAL MASS EJECTIONS VIEWED IN COORDINATED IMAGING AND IN SITU OBSERVATIONS

2012 ◽  
Vol 746 (2) ◽  
pp. L15 ◽  
Author(s):  
Ying D. Liu ◽  
Janet G. Luhmann ◽  
Christian Möstl ◽  
Juan C. Martinez-Oliveros ◽  
Stuart D. Bale ◽  
...  
Keyword(s):  
Coronal Mass Ejections ◽  
In Situ Observations

Using In-Situ Juno Observations to Understand the Evolution of Interplanetary Coronal Mass Ejections Within 1 AU and Beyond

2020 ◽  
Author(s):  
Emma Davies ◽  
Robert Forsyth ◽  
Simon Good
Keyword(s):  
Coronal Mass Ejections ◽  
Flux Rope ◽  
General Shape ◽  
Interplanetary Coronal Mass Ejections ◽  
Sheath Region ◽  
In Situ Observations ◽  
Phase Data ◽  
Radial Evolution ◽  
Inner Heliosphere

<p>Understanding the evolution of interplanetary coronal mass ejections (ICMEs) as they propagate through the heliosphere is essential in forecasting space weather severity. Much of our knowledge of ICMEs has been gained using in-situ measurements from single spacecraft, although the increasing number of missions in the inner heliosphere has led to an increase in multi-spacecraft studies improving our understanding of the global structure of ICMEs. Whilst most such recent studies have focused on the inner heliosphere within 1 AU, Juno cruise phase data provides a new opportunity to study ICME evolution over greater distances. We present analysis of ICMEs observed in-situ both by Juno and at least one other spacecraft within 1 AU to investigate their evolution as they propagate through the heliosphere. Investigation of the sheath region and timing considerations between spacecraft allows for the general shape of the shock front to be reconstructed. Combining in-situ observations and results of flux rope fitting techniques determines the global picture of the ICME as it propagates. However, effects on in-situ observations due to radial evolution and due to the longitudinal separation between multi-spacecraft remain hard to separate. We note the importance of the interplanetary environment in which the ICME propagates and the need for caution in radial alignment studies.  </p>

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