In order to bridge the gap between heliospheric and solar observations of coronal mass
ejections (CMEs), one of the key steps is to improve the understanding of their …

One strong magnetic cloud (MC) with a magnetic field magnitude reaching∼ 40 nT at 1 au
during 2012 June 16–17 is examined in association with a preexisting magnetic flux rope …

We present the first analysis of internal coronal mass ejection (CME) structure observed very
close to the Sun by the Wide-field Imager for Solar PRobe (WISPR) instrument on board the …

Context. The active galactic nucleus within M87, a giant elliptical galaxy, is responsible for
one of the closest kiloparsec-scale relativistic jets to Earth. It is thus a perfect target for …

Coronal mass ejections (CMEs) represent one type of the major eruption from the Sun. Their
interplanetary counterparts, the interplanetary CMEs (ICMEs), are the direct manifestations …

Increasingly one interplanetary coronal mass ejection (ICME) structure can propagate
across more than one spacecraft in the solar wind. This usually happens when two or more …

We report, in detail, an optimization approach for fitting a three-dimensional (3D) magnetic
cloud (MC) model to in situ spacecraft measurements. The model, dubbed the Freidberg …

Magnetic flux rope, a type of magnetic field structure in space plasmas, has been studied for
decades through both observational and theoretical means. We provide a brief report on our …

Magnetic flux ropes are a type of space plasma structures, exhibiting a set of observational
signatures based on in-situ spacecraft measurements. In the solar wind, they are found to …