Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. The microphysics of collisionless shock waves
 

The microphysics of collisionless shock waves

Journal
REPORTS ON PROGRESS IN PHYSICS  
Date Issued
2016
Author(s)
Marcowith, A.
•
Bret, A.
•
Bykov, A.
•
Dieckman, M. E.
•
O'C Drury, L.
•
Lembège, B.
•
Lemoine, M.
•
MORLINO, GIOVANNI  
•
Murphy, G.
•
Pelletier, G.
•
Plotnikov, I.
•
Reville, B.
•
Riquelme, M.
•
Sironi, L.
•
Stockem Novo, A.
DOI
10.1088/0034-4885/79/4/046901
Abstract
Collisionless shocks, that is shocks mediated by electromagnetic processes, are customary in space physics and in astrophysics. They are to be found in a great variety of objects and environments: magnetospheric and heliospheric shocks, supernova remnants, pulsar winds and their nebulæ, active galactic nuclei, gamma-ray bursts and clusters of galaxies shock waves. Collisionless shock microphysics enters at different stages of shock formation, shock dynamics and particle energization and/or acceleration. It turns out that the shock phenomenon is a multi-scale non-linear problem in time and space. It is complexified by the impact due to high-energy cosmic rays in astrophysical environments. This review adresses the physics of shock formation, shock dynamics and particle acceleration based on a close examination of available multi-wavelength or in situ observations, analytical and numerical developments. A particular emphasis is made on the different instabilities triggered during the shock formation and in association with particle acceleration processes with regards to the properties of the background upstream medium. It appears that among the most important parameters the background magnetic field through the magnetization and its obliquity is the dominant one. The shock velocity that can reach relativistic speeds has also a strong impact over the development of the micro-instabilities and the fate of particle acceleration. Recent developments of laboratory shock experiments has started to bring some new insights in the physics of space plasma and astrophysical shock waves. A special section is dedicated to new laser plasma experiments probing shock physics.
Volume
79
Issue
4
Start page
046901
Uri
http://hdl.handle.net/20.500.12386/28491
Url
https://iopscience.iop.org/article/10.1088/0034-4885/79/4/046901
Issn Identifier
0034-4885
Ads BibCode
2016RPPh...79d6901M
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

1604.00318.pdf

Description
postprint
Size

4.33 MB

Format

Adobe PDF

Checksum (MD5)

e95c83c49daf66c81c5e683176b77424

Loading...
Thumbnail Image
Name

Marcowith_2016_Rep._Prog._Phys._79_046901.pdf

Description
[Administrators only]
Size

4.76 MB

Format

Adobe PDF

Checksum (MD5)

0229c888c326834fc005a4628efae6a8

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback