Beyond certain distance the ICME propagation becomes mostly governed by the interaction of the ICME and the ambient solar wind. Configuration of the interplanetary magnetic field and features of the related ambient solar wind in the ecliptic and meridional plane are different. Therefore, one can expect that the inclination of the CME flux rope axis i.e. tilt, influences the propagation of the ICME itself. In order to study the relation between the tilt parameter and the ICME propagation we investigated isolated Earth-impacting CME-ICME evets in the time period from 2006. to 2014. We determined the CME tilt in the “near-Sun” environment from the 3D reconstruction of the CME, obtained by the Graduated Cylindrical Shell model using coronagraph...
In a case study (June 6-7, 2008) we report on how the internal structure of a coronal mass ejection ...
We study two interplanetary coronal mass ejections (ICMEs) observed at Mercury and at 1 au by spacec...
We present a kinematic study of the evolution of coronal mass ejections (CMEs) in the solar wind. Sp...
Context. The configuration of the interplanetary magnetic field and features of the related ambient ...
Context. The configuration of the interplanetary magnetic field and features of the related ambient ...
The configuration of the interplanetary magnetic field and features of the related ambient solar win...
International audienceAbstract The propagation of interplanetary coronal mass ejections (ICMEs) in t...
International audienceAbstract The propagation of interplanetary coronal mass ejections (ICMEs) in t...
International audienceAbstract The propagation of interplanetary coronal mass ejections (ICMEs) in t...
We study three CME/ICME events (2008 June 1–6, 2009 February 13–18, 2010 April 3–5) tracked from Sun...
Coronal mass ejections (CMEs) are subject to changes in their direction of propagation, tilt, and ot...
This electronic version was submitted by the student author. The certified thesis is available in t...
Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding CMEs and solar...
Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding CMEs and solar...
Interplanetary coronal mass ejections (ICMEs) are a significant feature of the heliospheric environm...
In a case study (June 6-7, 2008) we report on how the internal structure of a coronal mass ejection ...
We study two interplanetary coronal mass ejections (ICMEs) observed at Mercury and at 1 au by spacec...
We present a kinematic study of the evolution of coronal mass ejections (CMEs) in the solar wind. Sp...
Context. The configuration of the interplanetary magnetic field and features of the related ambient ...
Context. The configuration of the interplanetary magnetic field and features of the related ambient ...
The configuration of the interplanetary magnetic field and features of the related ambient solar win...
International audienceAbstract The propagation of interplanetary coronal mass ejections (ICMEs) in t...
International audienceAbstract The propagation of interplanetary coronal mass ejections (ICMEs) in t...
International audienceAbstract The propagation of interplanetary coronal mass ejections (ICMEs) in t...
We study three CME/ICME events (2008 June 1–6, 2009 February 13–18, 2010 April 3–5) tracked from Sun...
Coronal mass ejections (CMEs) are subject to changes in their direction of propagation, tilt, and ot...
This electronic version was submitted by the student author. The certified thesis is available in t...
Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding CMEs and solar...
Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding CMEs and solar...
Interplanetary coronal mass ejections (ICMEs) are a significant feature of the heliospheric environm...
In a case study (June 6-7, 2008) we report on how the internal structure of a coronal mass ejection ...
We study two interplanetary coronal mass ejections (ICMEs) observed at Mercury and at 1 au by spacec...
We present a kinematic study of the evolution of coronal mass ejections (CMEs) in the solar wind. Sp...