Exploring the Galactic plasma with pulsars in the SKA Era

The ionised media that permeate the Milky Way have been active topics of research since the discovery of pulsars in 1967. In fact, pulsars allow one to study several aspects of said plasma, such as their column density, turbulence, scattering measures, and discrete, intervening structures in between the neutron star and the observer, and aspects of the magnetic field throughout. Such sources of information allow us to characterise the electron distribution in the terrestrial ionosphere, the Solar Wind, and our Galaxy and the impact on other experiments involving pulsars such as Pulsar Timing Arrays. In this article, we review the state-of-the-art of plasma research using pulsars, the aspects that should be taken into consideration for optimal plasma studies, and we provide future perspectives on improvements to those enabled by the SKA.

Authors

Institutions

Publication Details

Journal
The Open Journal of Astrophysics
Published
2025-12-19
DOI
https://doi.org/10.33232/001c.154250
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Exploring the Galactic plasma with pulsars in the SKA Era

C. Tiburzi, L. Levin, Daniel J. Reardon, N. D. R. Bhat et al.
The Open Journal of Astrophysics
Pulsars and Gravitational Waves Research
article

Exploring the Galactic plasma with pulsars in the SKA Era

C. Tiburzi, L. Levin, Daniel J. Reardon, N. D. R. Bhat, J. R. Dawson, Michael T. Lam, G. Shaifullah, N. K. Porayko, M. A. Walker, Marisa Geyer, W. C. Jing, M. J. Keith, S. C. Susarla, Stella Koch Ocker, Adam T. Deller, F. Iraci, M. Mevius
article en

Abstract

The ionised media that permeate the Milky Way have been active topics of research since the discovery of pulsars in 1967. In fact, pulsars allow one to study several aspects of said plasma, such as their column density, turbulence, scattering measures, and discrete, intervening structures in between the neutron star and the observer, and aspects of the magnetic field throughout. Such sources of information allow us to characterise the electron distribution in the terrestrial ionosphere, the Solar Wind, and our Galaxy and the impact on other experiments involving pulsars such as Pulsar Timing Arrays. In this article, we review the state-of-the-art of plasma research using pulsars, the aspects that should be taken into consideration for optimal plasma studies, and we provide future perspectives on improvements to those enabled by the SKA.

The Open Journal of AstrophysicsVol. 8 Supplement(1)
California Institute of Technology (US), University of Cape Town (ZA), University of Cagliari (IT), Ollscoil na Gaillimhe – University of Galway (IE), Lomonosov Moscow State University (RU), Italian Aerospace Research Centre (IT), Manly Hospital (AU), University of Manchester (GB), Astronomical Institute of the Slovak Academy of Sciences (SK), National Astronomical Observatories (CN), Swinburne University of Technology (AU), University of Milano-Bicocca (IT), Search for Extraterrestrial Intelligence (US), National Institute for Astrophysics (IT), Netherlands Institute for Radio Astronomy (NL), Macquarie University (AU)
Openalex Percentile: Top 72%
Pulsars and Gravitational Waves Research
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.