Evolution and Impact of Switchbacks Throughout the Heliosphere

Abstract Magnetic switchbacks are large-amplitude fluctuations in the interplanetary magnetic field, and appear frequently in the near-Sun solar wind explored recently by Parker Solar Probe: these new observations have prompted many new studies into their properties and origins. Here, we first review what is known about how switchbacks evolve as they travel away from the Sun: both in terms of their expansion-driven growth and their decay due to various processes like turbulence, reconnection, dispersion, parametric instability, and interaction with interplanetary shocks. We then review the current state of knowledge on how switchbacks impact the physics of the solar wind as a whole: in terms of the turbulent cascade, acceleration and heating of the wind, modification of the open solar flux and scattering of energetic particles. Finally, we suggest future studies to further our understanding of switchback evolution and impacts on the heliosphere.

Authors

Institutions

Publication Details

Journal
Space Science Reviews
Published
2026-07-23
DOI
https://doi.org/10.1007/s11214-026-01311-9
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Evolution and Impact of Switchbacks Throughout the Heliosphere

J. F. Drake, M. Velli, M. I. Desai, L. Sorriso‐Valvo et al.
Space Science Reviews
Solar and Space Plasma Dynamics
article

Evolution and Impact of Switchbacks Throughout the Heliosphere

J. F. Drake, M. Velli, M. I. Desai, L. Sorriso‐Valvo, Gabriel Ho Hin Suen, M. Swisdak, M. J. Owens, T. S. Horbury, Mojtaba Akhavan‐Tafti, A. Larosa, O. V. Agapitov, Jonathan Squire, Lorenzo Matteini, F. Malara, Trevor A. Bowen, Samuel T. Badman, M. S. Madjarska, Nikos Sioulas, Victor Réville, Shirsh Lata Soni, J. L. Verniero, Chen Shi, Anna Tenerani, Alfred Mallet, Nina Bizien, Nicholas Watkins
article en

Abstract

Abstract Magnetic switchbacks are large-amplitude fluctuations in the interplanetary magnetic field, and appear frequently in the near-Sun solar wind explored recently by Parker Solar Probe: these new observations have prompted many new studies into their properties and origins. Here, we first review what is known about how switchbacks evolve as they travel away from the Sun: both in terms of their expansion-driven growth and their decay due to various processes like turbulence, reconnection, dispersion, parametric instability, and interaction with interplanetary shocks. We then review the current state of knowledge on how switchbacks impact the physics of the solar wind as a whole: in terms of the turbulent cascade, acceleration and heating of the wind, modification of the open solar flux and scattering of energetic particles. Finally, we suggest future studies to further our understanding of switchback evolution and impacts on the heliosphere.

Space Science ReviewsVol. 222(5)
Université d'Orléans (FR), Southwest Research Institute (US), Centre National de la Recherche Scientifique (FR), Planetary Science Institute (US), Goddard Space Flight Center (US), Swedish Institute of Space Physics (SE), Université Toulouse III - Paul Sabatier (FR), University of California, Los Angeles (US), Taras Shevchenko National University of Kyiv (UA), Bulgarian Academy of Sciences (BG), University of Michigan (US), Korea Astronomy and Space Science Institute (KR), Space Research and Technology Institute (BG), University of Warwick (GB), Heliophysics (US), Max Planck Institute for Solar System Research (DE), Center for Astrophysics Harvard & Smithsonian (US), Institute for the Science and Technology of Plasmas (IT), Institut de Recherche en Astrophysique et Planétologie (FR), Laboratoire de Physique et Chimie de l’Environnement et de l’Espace (FR), Heliophysics Science Division (US), University College London (GB), University of Calabria (IT), Imperial College London (GB), University of Maryland, College Park (US), University of Reading (GB), University of Otago (NZ), Auburn University (US), The University of Texas at Austin (US), KTH Royal Institute of Technology (SE), London School of Economics and Political Science (GB), University of California, Berkeley (US)
National Science Foundation, National Aeronautics and Space Administration, National Research Foundation, Deutsche Forschungsgemeinschaft, National Research Foundation of Korea, Kungliga Tekniska Högskolan, Vetenskapsrådet, Ministry of Science and ICT, South Korea, Science and Technology Facilities Council, International Space Science Institute
Affordable and clean energy
Openalex Percentile: Top 9%
Solar and Space Plasma Dynamics
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.