Search Publications

Dayside Transient Phenomena and Their Impact on the Magnetosphere and Ionosphere
DOI: 10.1007/s11214-021-00865-0 Bibcode: 2022SSRv..218...40Z

Zong, Qiugang; Lin, Yu; Kallio, Esa +17 more

Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux transfer events, and surface waves, are frequently observed upstream from the bow shock, in the magnetosheath, and at the magnetopause. They play a significant role in the solar wind-magnetosphere-ionosphere coupling. Foreshock transient phenomena, associat…

2022 Space Science Reviews
Cluster 73
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
Particles and Photons as Drivers for Particle Release from the Surfaces of the Moon and Mercury
DOI: 10.1007/s11214-022-00875-6 Bibcode: 2022SSRv..218...10W

Wurz, P.; Lammer, H.; Galli, A. +13 more

The Moon and Mercury are airless bodies, thus they are directly exposed to the ambient plasma (ions and electrons), to photons mostly from the Sun from infrared range all the way to X-rays, and to meteoroid fluxes. Direct exposure to these exogenic sources has important consequences for the formation and evolution of planetary surfaces, including …

2022 Space Science Reviews
SOHO 32
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
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
The Structure of the Global Heliosphere as Seen by In-Situ Ions from the Voyagers and Remotely Sensed ENAs from Cassini
DOI: 10.1007/s11214-022-00889-0 Bibcode: 2022SSRv..218...21D

Krimigis, Stamatios M.; Mitchell, Donald G.; Hilchenbach, Martin +5 more

The exploration of interplanetary space and our solar bubble, the heliosphere, has made a big leap over the past two decades, due to the path-breaking observations of the two Voyager spacecraft, launched more than 44 years ago. Their in-situ particle and fields measurements were complemented by remote observations of 5.2 to 55 keV Energetic Neutra…

2022 Space Science Reviews
Cassini SOHO 23
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
In Situ Observations of Interstellar Pickup Ions from 1 au to the Outer Heliosphere
DOI: 10.1007/s11214-022-00895-2 Bibcode: 2022SSRv..218...28Z

McComas, D. J.; Möbius, E.; Pogorelov, N. V. +5 more

Interstellar pickup ions are an ubiquitous and thermodynamically important component of the solar wind plasma in the heliosphere. These PUIs are born from the ionization of the interstellar neutral gas, consisting of hydrogen, helium, and trace amounts of heavier elements, in the solar wind as the heliosphere moves through the local interstellar m…

2022 Space Science Reviews
Ulysses 21
Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium
DOI: 10.1007/s11214-022-00912-4 Bibcode: 2022SSRv..218...42R

Heber, Bernd; Zhang, Ming; Potgieter, Marius S. +7 more

We review recent observations and modeling developments on the subject of galactic cosmic rays through the heliosphere and in the Very Local Interstellar Medium, emphasizing knowledge that has accumulated over the past decade. We begin by highlighting key measurements of cosmic-ray spectra by Voyager, PAMELA, and AMS and discuss advances in global…

2022 Space Science Reviews
Ulysses 20