From shock to synchrotron: a mini-review on magnetic turbulence in supernova remnants Article Swipe
Magnetic turbulence plays a crucial role in confining charged particles near the shock front of Supernova Remnants, enabling them to reach energies up to hundreds of TeV through a process known as Diffusive Shock Acceleration (DSA). These high-energy electrons spiral along magnetic field lines, emitting X-ray synchrotron radiation. The launch of the Imaging X-ray Polarimetry Explorer (IXPE) has opened a new window into the study of magnetic fields in SNRs through X-ray polarization measurements. For the first time, IXPE allows us to resolve the polarization degree (PD) and angle (PA) in the X-ray band across different areas of SNRs, offering direct insight into the geometry and coherence of magnetic fields on different scales. In this mini-review, I summarize the key observational results on SNRs obtained with IXPE over the past 4 years and discuss their implications for our understanding of magnetic turbulence in synchrotron-emitting regions. I also show how we can combine polarization parameters and standard X-ray spectral/imaging analysis to better constrain the structure and scale of magnetic turbulence immediately downstream of the shock and understand the particle acceleration occurring in SNRs.
Related Topics
Concepts
Physics
Magnetic field
Particle acceleration
Supernova
Turbulence
Polarization (electrochemistry)
Shock (circulatory)
Astrophysics
Synchrotron
Electron
Supernova remnant
Coherence (philosophical gambling strategy)
Polarimetry
Shock wave
Computational physics
Astronomy
Magnetohydrodynamics
Shock waves in astrophysics
Plasma
Acceleration
Fermi acceleration
Synchrotron radiation
Magnetohydrodynamic turbulence
Bow shock (aerodynamics)
Crab Nebula
Pitch angle
Spiral galaxy
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3389/fspas.2025.1717808
- https://public-pages-files-2025.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2025.1717808/pdf
- OA Status
- gold
- References
- 49
- OpenAlex ID
- https://openalex.org/W7104607563
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W7104607563Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.3389/fspas.2025.1717808Digital Object Identifier
- Title
-
From shock to synchrotron: a mini-review on magnetic turbulence in supernova remnantsWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2025Year of publication
- Publication date
-
2025-11-11Full publication date if available
- Authors
-
Emanuele Greco,List of authors in order
- Landing page
-
https://doi.org/10.3389/fspas.2025.1717808Publisher landing page
- PDF URL
-
https://public-pages-files-2025.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2025.1717808/pdfDirect link to full text PDF
- Open access
-
YesWhether a free full text is available
- OA status
-
goldOpen access status per OpenAlex
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-
https://public-pages-files-2025.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2025.1717808/pdfDirect OA link when available
- Concepts
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Physics, Magnetic field, Particle acceleration, Supernova, Turbulence, Polarization (electrochemistry), Shock (circulatory), Astrophysics, Synchrotron, Electron, Supernova remnant, Coherence (philosophical gambling strategy), Polarimetry, Shock wave, Computational physics, Astronomy, Magnetohydrodynamics, Shock waves in astrophysics, Plasma, Acceleration, Fermi acceleration, Synchrotron radiation, Magnetohydrodynamic turbulence, Bow shock (aerodynamics), Crab Nebula, Pitch angle, Spiral galaxyTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
0Total citation count in OpenAlex
- References (count)
-
49Number of works referenced by this work
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| referenced_works | https://openalex.org/W1999903618, https://openalex.org/W2032882333, https://openalex.org/W2063712348, https://openalex.org/W2081160630, https://openalex.org/W3045042879, https://openalex.org/W4400434473, https://openalex.org/W1976316526, https://openalex.org/W2138605662, https://openalex.org/W1966497580, https://openalex.org/W2033871948, https://openalex.org/W2169140569, https://openalex.org/W337816440, https://openalex.org/W4323354972, https://openalex.org/W4396913789, https://openalex.org/W2146989240, https://openalex.org/W4387613889, https://openalex.org/W2109518255, https://openalex.org/W2071877669, https://openalex.org/W2085269085, https://openalex.org/W2963447227, https://openalex.org/W2030370571, https://openalex.org/W2773749868, https://openalex.org/W2050956314, https://openalex.org/W1994673795, https://openalex.org/W3043230089, https://openalex.org/W4410968636, https://openalex.org/W2084477100, https://openalex.org/W1514236604, https://openalex.org/W1521485834, https://openalex.org/W4403823578, https://openalex.org/W2078821620, https://openalex.org/W2078855713, https://openalex.org/W2044304071, https://openalex.org/W1978657060, https://openalex.org/W1985245613, https://openalex.org/W4292702591, https://openalex.org/W4402782218, https://openalex.org/W2086550725, https://openalex.org/W3107235900, https://openalex.org/W2067148460, https://openalex.org/W3104137987, https://openalex.org/W1964293522, https://openalex.org/W4304694332, https://openalex.org/W4224036977, https://openalex.org/W2336202081, https://openalex.org/W1575238798, https://openalex.org/W4387974995, https://openalex.org/W4411454618, https://openalex.org/W2073914801 |
| referenced_works_count | 49 |
| abstract_inverted_index.4 | 130 |
| abstract_inverted_index.I | 116, 145 |
| abstract_inverted_index.a | 3, 28, 59 |
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| abstract_inverted_index.mini-review, | 115 |
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| abstract_inverted_index.measurements. | 73 |
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