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The GALPROP Cosmic-ray Propagation and Nonthermal Emissions Framework: Release v57
DOI: 10.3847/1538-4365/ac80f6 Bibcode: 2022ApJS..262...30P

Jóhannesson, G.; Moskalenko, I. V.; Porter, T. A.

The past decade has brought impressive advances in the astrophysics of cosmic rays (CRs) and multiwavelength astronomy, thanks to the new instrumentation launched into space and built on the ground. Modern technologies employed by those instruments provide measurements with unmatched precision, enabling searches for subtle signatures of dark matte…

2022 The Astrophysical Journal Supplement Series
Ulysses 58
Theory of Cosmic Ray Transport in the Heliosphere
DOI: 10.1007/s11214-022-00896-1 Bibcode: 2022SSRv..218...33E

Rankin, J. S.; Potgieter, M. S.; Ruffolo, D. +6 more

Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global challenge in the field of heliophysics, in that such a study, if it were to be performed from first principles, requires the careful modelling of both large scale heliospheric plasma quantities (such as the global structure of the heliosphere, or the heliospheric m…

2022 Space Science Reviews
Ulysses 53
The Structure of the Large-Scale Heliosphere as Seen by Current Models
DOI: 10.1007/s11214-022-00902-6 Bibcode: 2022SSRv..218...36K

Heerikhuisen, Jacob; Fraternale, Federico; Pogorelov, Nikolai +6 more

This review summarizes the current state of research aiming at a description of the global heliosphere using both analytical and numerical modeling efforts, particularly in view of the overall plasma/neutral flow and magnetic field structure, and its relation to energetic neutral atoms. Being part of a larger volume on current heliospheric researc…

2022 Space Science Reviews
SOHO Ulysses 31
Alpha-Proton Differential Flow of the Young Solar Wind: Parker Solar Probe Observations
DOI: 10.3847/2041-8213/ac51e1 Bibcode: 2022ApJ...926L..38M

Bale, S. D.; Allen, R. C.; Raouafi, N. E. +5 more

The velocity of alpha particles relative to protons can vary depending on the solar wind type and distance from the Sun. Measurements from the previous spacecraft provided the alpha-proton differential velocities down to 0.3 au. The Parker Solar Probe (PSP) now enables insights into differential flows of the newly accelerated solar wind closer to …

2022 The Astrophysical Journal
Ulysses 29
Very Local Interstellar Medium Revealed by a Complete Solar Cycle of Interstellar Neutral Helium Observations with IBEX
DOI: 10.3847/1538-4365/ac4bde Bibcode: 2022ApJS..259...42S

McComas, D. J.; Fuselier, S. A.; Galli, A. +8 more

The IBEX-Lo instrument on board the Interstellar Boundary Explorer (IBEX) mission samples interstellar neutral (ISN) helium atoms penetrating the heliosphere from the very local interstellar medium (VLISM). In this study, we analyze the IBEX-Lo ISN helium observations covering a complete solar cycle, from 2009 through 2020 using a comprehensive un…

2022 The Astrophysical Journal Supplement Series
Ulysses 27
Anomalous Cosmic Rays and Heliospheric Energetic Particles
DOI: 10.1007/s11214-022-00890-7 Bibcode: 2022SSRv..218...22G

Fichtner, H.; Leske, R. A.; Hill, M. E. +7 more

We present a review of Anomalous Cosmic Rays (ACRs), including the history of their discovery and recent insights into their acceleration and transport in the heliosphere. We focus on a few selected topics including a discussion of mechanisms of their acceleration, escape from the heliosphere, their effects on the dynamics of the heliosheath, tran…

2022 Space Science Reviews
SOHO Ulysses 26
Recent Developments in Particle Acceleration at Shocks: Theory and Observations
DOI: 10.1007/s11214-022-00892-5 Bibcode: 2022SSRv..218...26P

Giacalone, Joe; Perri, Silvia; Fichtner, Horst +2 more

Energetic particles represent an important component of the plasma in the heliosphere. They range from particles accelerated at impulsive events in the solar corona and at large scale structures in the interplanetary medium, to anomalous cosmic rays accelerated at the boundaries of the heliosphere. In-situ satellite observations, numerical simulat…

2022 Space Science Reviews
Cluster Ulysses 24
Turbulence in the Outer Heliosphere
DOI: 10.1007/s11214-022-00914-2 Bibcode: 2022SSRv..218...50F

Zank, Gary P.; Adhikari, Laxman; Zhao, Lingling +9 more

The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates heliospheric regions with significantly different properties in terms of particle populations, bulk flow and turbulence. Our knowledge of the solar wind turbulence nature and dynamics mostly relies o…

2022 Space Science Reviews
Ulysses 23
A New 3D Solar Wind Speed and Density Model Based on Interplanetary Scintillation
DOI: 10.3847/1538-4365/ac35d7 Bibcode: 2022ApJS..259....2P

Bzowski, M.; Tokumaru, M.; Porowski, C.

The solar wind (SW) is an outflow of the solar coronal plasma, which expands supersonically throughout the heliosphere. SW particles interact by charge exchange with interstellar neutral atoms; on the one hand, they modify the distribution of this gas in interplanetary space, and, on the other hand, they are the seed populations for heliospheric p…

2022 The Astrophysical Journal Supplement Series
Ulysses 22
Mixing Interstellar Clouds Surrounding the Sun
DOI: 10.3847/2041-8213/ac9120 Bibcode: 2022ApJ...937L..32S

Zank, Gary P.; Redfield, Seth; Winslow, Réka M. +9 more

On its journey through the Galaxy, the Sun passes through diverse regions of the interstellar medium. High-resolution spectroscopic measurements of interstellar absorption lines in spectra of nearby stars show absorption components from more than a dozen warm partially ionized clouds within 15 pc of the Sun. The two nearest clouds-the Local Inters…

2022 The Astrophysical Journal
Ulysses 21