We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim of the present study is to provide a link between the different aspects of this phenomenon, starting with information on the origins of the MCs at the Sun and following by the analysis of in-situ observations at 1 AU and at Ulysses. The candidate source regions were identified in SOHO/EIT and SOHO/MDI observations. They were correlated with H-α images that were obtained from ground-based observatories. Hints on the internal magnetic field configuration of the associated coronal mass ejections are obtained from LASCO C2 images. In interplanetary space, magnetic and plasma moments of the distribution function of plasma species (ACE/Uly...
Coronal mass ejections (CMEs) are large-scale explosions on the Sun that expel plasma and magnetic ...
Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are import...
In-situ measurements of interplanetary coronal mass ejections (ICMEs) display a wide range of proper...
We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim ...
We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim o...
We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim o...
Abstract. We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The ...
Magnetic Clouds (MCs) are the interplanetary manifestation of Coronal Mass Ejections. These huge ast...
Plasma and magnetic field data from the Helios 1/2 spacecraft have been used to investigate the str...
This Letter exploits joint observations of the same interplanetary coronal mass ejection by widely s...
Context. A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejec...
Using Advanced Composition Explorer (ACE) in situ data we identify and describe an interplanetary ma...
Magnetic clouds are the interplanetary manifestation of coronal mass ejections, which are transient ...
This study identifies the solar origins of magnetic clouds that are observed at 1 AU and predic...
Coronal mass ejections (CMEs) are large-scale explosions on the Sun that expel plasma and magnetic ...
Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are import...
In-situ measurements of interplanetary coronal mass ejections (ICMEs) display a wide range of proper...
We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim ...
We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim o...
We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim o...
Abstract. We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The ...
Magnetic Clouds (MCs) are the interplanetary manifestation of Coronal Mass Ejections. These huge ast...
Plasma and magnetic field data from the Helios 1/2 spacecraft have been used to investigate the str...
This Letter exploits joint observations of the same interplanetary coronal mass ejection by widely s...
Context. A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejec...
Using Advanced Composition Explorer (ACE) in situ data we identify and describe an interplanetary ma...
Magnetic clouds are the interplanetary manifestation of coronal mass ejections, which are transient ...
This study identifies the solar origins of magnetic clouds that are observed at 1 AU and predic...
Coronal mass ejections (CMEs) are large-scale explosions on the Sun that expel plasma and magnetic ...
Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are import...
In-situ measurements of interplanetary coronal mass ejections (ICMEs) display a wide range of proper...