Amit Seta

Australian National University

Australia

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Articles (26)

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2025

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2021

Collaborators (17)

Seoyoung Lyla Jung

University of Oxford

UNITED KINGDOM

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Philip Mocz

Princeton University

UNITED STATES

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Marijke Haverkorn

Associate Professor

Radboud University

NETHERLANDS

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Neco Kriel

Australian National University

AUSTRALIA

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Hiep Nguyen

Australian National University

AUSTRALIA

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Joanne Dawson

Macquarie University

AUSTRALIA

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Jeroen Stil

Associate Professor

University of Calgary

CANADA

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Susan Clark

Assistant Professor

Stanford University

UNITED STATES

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N M McClure-Griffiths

Australian National University

AUSTRALIA

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Roland Crocker

Australian National University

AUSTRALIA

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Jo-Anne Brown

Associate Professor

University of Calgary

CANADA

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Christoph Federrath

Australian National University

AUSTRALIA

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Freeke van de Voort

Royal Society University Research Fellow & lecturer (proleptic)

Cardiff University

UNITED KINGDOM

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Elaine Sadler

Professor of Astrophysics

University of Sydney

AUSTRALIA

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Matt L Sampson

Australian National University

AUSTRALIA

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Matthew W Kunz

Princeton University

UNITED STATES

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Yik Ki Ma

Max Planck Institute for Radio Astronomy

GERMANY

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Amit Seta

Research Interests

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Articles (26)

A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity

A comparison of the turbulent dynamo in weakly-collisional and collisional plasmas: from subsonic to supersonic turbulence

Understanding gas mixing in the circumgalactic medium

Magnetic fields in the multiphase interstellar medium of the Milky Way: turbulent kinetic and magnetic energy density relation

Faraday moments of the Southern Twenty-centimeter All-sky Polarization Survey (STAPS)

AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasma

Structure functions with higher-order stencils as a probe to separate small- and large-scale magnetic fields

Multiphase neutral interstellar medium: Analysing simulation with H i 21cm observational data analysis techniques

Turbulence and magnetic fields in star formation

Wide-binary eccentricity distribution in young star clusters: Dependence on the binary separation and mass

Local H i absorption towards the magellanic cloud foreground using ASKAP

The influence of the cloud virial parameter on the initial mass function

Cosmic evolution of the Faraday rotation measure in the intracluster medium of galaxy clusters

Magnetized H i superbubbles in the Small Magellanic Cloud revealed by the POSSUM pilot survey

Detection of magnetic fields in the circumgalactic medium of nearby galaxies using Faraday rotation

Critical magnetic Reynolds number of the turbulent dynamo in collisionless plasmas

Growth or Decay – I: universality of the turbulent dynamo saturation

Correction to: Fundamental scales in the kinematic phase of the turbulent dynamo

Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds

Energy balance and Alfvén Mach numbers in compressible magnetohydrodynamic turbulence with a large-scale magnetic field

Turbulent diffusion of streaming cosmic rays in compressible, partially ionized plasma

The role of the turbulence driving mode for the initial mass function

Turbulent dynamo in the two-phase interstellar medium

Fundamental scales in the kinematic phase of the turbulent dynamo

H i absorption at z ∼ 0.7 against the lobe of the powerful radio galaxy PKS 0409−75

A radio polarization study of magnetic fields in the Small Magellanic Cloud

Collaborators (17)

Seoyoung Lyla Jung

Philip Mocz

Marijke Haverkorn

Neco Kriel

Hiep Nguyen

Joanne Dawson

Jeroen Stil

Susan Clark

N M McClure-Griffiths

Roland Crocker

Jo-Anne Brown

Christoph Federrath

Freeke van de Voort

Elaine Sadler

Matt L Sampson

Matthew W Kunz

Yik Ki Ma

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