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Causes and Consequences of Magnetic Complexity Changes within Interplanetary Coronal Mass Ejections: A Statistical Study
DOI: 10.3847/1538-4357/ac3e60 Bibcode: 2022ApJ...927..102S

Lugaz, Noé; Scolini, Camilla; Winslow, Réka M. +3 more

We present the first statistical analysis of complexity changes affecting the magnetic structure of interplanetary coronal mass ejections (ICMEs), with the aim of answering the questions: How frequently do ICMEs undergo magnetic complexity changes during propagation? What are the causes of such changes? Do the in situ properties of ICMEs differ de…

2022 The Astrophysical Journal
VenusExpress 23
Multi-spacecraft Observations of the Evolution of Interplanetary Coronal Mass Ejections between 0.3 and 2.2 au: Conjunctions with the Juno Spacecraft
DOI: 10.3847/1538-4357/ac731a Bibcode: 2022ApJ...933..127D

Lugaz, Noé; Scolini, Camilla; Winslow, Réka M. +4 more

We present a catalog of 35 interplanetary coronal mass ejections (ICMEs) observed by the Juno spacecraft and at least one other spacecraft during its cruise phase to Jupiter. We identify events observed by MESSENGER, Venus Express, Wind, and STEREO with magnetic features that can be matched unambiguously with those observed by Juno. A multi-spacec…

2022 The Astrophysical Journal
Ulysses VenusExpress 19
Validation and Interpretation of a Three-dimensional Configuration of a Magnetic Cloud Flux Rope
DOI: 10.3847/1538-4357/ac7803 Bibcode: 2022ApJ...934...50H

Qiu, Jiong; Hu, Qiang; Jian, Lan K. +3 more

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 (MFR) identified on the Sun. The MC is characterized by a quasi-three-dimensional (3D) flux rope model based on in situ measurements from the Wind spacecraft. The contents of…

2022 The Astrophysical Journal
SOHO VenusExpress 7
The Solar Wind Parker Spiral Angle Distributions and Variations at 1 au
DOI: 10.3847/1538-4357/ac6bf3 Bibcode: 2022ApJ...931..105C

Xu, Qi; Xu, Xiaojun; Wang, Jing +8 more

Using the data from the Advanced Composition Explorer (ACE) and Wind spacecraft, we statistically studied the Parker spiral angle (PSA) of the solar wind magnetic field from 1998 to 2019 at 1 au. The PSA occurrences over both a Carrington rotation (CR) and a year can be well fitted by a Gaussian distribution. However, large-scale magnetic structur…

2022 The Astrophysical Journal
VenusExpress 6
Galactic Cosmic Rays at Mars and Venus: Temporal Variations from Hours to Decades Measured as the Background Signal of Onboard Microchannel Plates
DOI: 10.3847/1538-4357/ac9a49 Bibcode: 2022ApJ...940..178F

Barabash, Stas; Nilsson, Hans; Holmström, Mats +8 more

A microchannel plate (MCP) is a component widely used for counting particles in space. Using the background counts from MCPs on the Mars Express and Venus Express orbiters-operating over 17 yr and 8 yr, respectively-we investigated the galactic cosmic ray (GCR) characteristics of the inner solar system. The MCP background counts at Mars and Venus,…

2022 The Astrophysical Journal
MEx VenusExpress 5
Multipoint Analysis of the Interaction between a Shock and an ICME-like Structure around 2011 March 22
DOI: 10.3847/2041-8213/ac6879 Bibcode: 2022ApJ...930L..11X

Wang, Yuming; Shen, Chenglong; Xu, Mengjiao +3 more

This work reports on the interaction between a fast forward shock and an interplanetary coronal-mass-ejection-like structure (ICMELS) as observed by in situ observations of radially aligned spacecraft. Around 2011 March 22, the Venus EXpress (VEX) and Solar TErrestrial RElations Observatory-A (STEREO-A) were nearly at the same longitude, providing…

2022 The Astrophysical Journal
VenusExpress 4