Magnetic clouds (MCs) are objects in expansion during their travel through the heliosphere. In situ observations indicate that their front travel faster than their back, showing a clear empirical signature of expansion. With the aim of quantifying the expansion rate of MCs in the inner heliosphere (0.3 to 1 AU), we present here a statistical study of events observed by the spacecraft Helios 1 and 2, during their complete period of operations. From the analysis of the profile of the MC magnetic field components in its local frame, which is obtained from a rotation of the observed magnetic field vectors to a system of reference oriented as the main axis of the flux rope, we revise a list of events identified in previous works and redefine imp...
It has been observed that a magnetic cloud (MC) can affect the propagation conditions of solar energ...
Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are import...
Context. Magnetic clouds (MCs) are large-scale interplanetary transient structures in the heliospher...
International audienceContext. Observations of magnetic clouds (MCs) are consistent with the presenc...
Context. A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejec...
Context. Significant quantities of magnetized plasma are transported from the Sun to the interstella...
The interplanetary evolution of 11 magnetic clouds (MCs) recorded by at least two radially aligned s...
Context. A magnetic cloud (MC) is a magnetic flux rope in the solar wind (SW), which, at 1 AU, is ob...
Context. A magnetic cloud (MC) is a magnetic flux rope in the solar wind (SW), Which, at 1 AU, is o...
Plasma and magnetic field data from the Helios 1/2 spacecraft have been used to investigate the str...
The conservation of magnetic flux in systems of very low dissipation, as the interplanetary medium, ...
Magnetic clouds (MCs) transport the magnetic flux and helicity released by the Sun. They are general...
This Letter exploits joint observations of the same interplanetary coronal mass ejection by widely s...
Aims. Magnetic clouds are large interplanetary flux ropes that propagate in the solar wind from the ...
It has been observed that a magnetic cloud (MC) can affect the propagation conditions of solar energ...
Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are import...
Context. Magnetic clouds (MCs) are large-scale interplanetary transient structures in the heliospher...
International audienceContext. Observations of magnetic clouds (MCs) are consistent with the presenc...
Context. A large amount of magnetized plasma is frequently ejected from the Sun as coronal mass ejec...
Context. Significant quantities of magnetized plasma are transported from the Sun to the interstella...
The interplanetary evolution of 11 magnetic clouds (MCs) recorded by at least two radially aligned s...
Context. A magnetic cloud (MC) is a magnetic flux rope in the solar wind (SW), which, at 1 AU, is ob...
Context. A magnetic cloud (MC) is a magnetic flux rope in the solar wind (SW), Which, at 1 AU, is o...
Plasma and magnetic field data from the Helios 1/2 spacecraft have been used to investigate the str...
The conservation of magnetic flux in systems of very low dissipation, as the interplanetary medium, ...
Magnetic clouds (MCs) transport the magnetic flux and helicity released by the Sun. They are general...
This Letter exploits joint observations of the same interplanetary coronal mass ejection by widely s...
Aims. Magnetic clouds are large interplanetary flux ropes that propagate in the solar wind from the ...
It has been observed that a magnetic cloud (MC) can affect the propagation conditions of solar energ...
Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are import...
Context. Magnetic clouds (MCs) are large-scale interplanetary transient structures in the heliospher...