pith. sign in

arxiv: 1210.7891 · v1 · pith:3H7LBE7Inew · submitted 2012-10-30 · 🌌 astro-ph.GA · astro-ph.IM

Interstellar scattering - New diagnostics of pulsars and the ISM

classification 🌌 astro-ph.GA astro-ph.IM
keywords fundamentalinterstellaroffersproblemsprospectpulsarscatteringturbulence
0
0 comments X
read the original abstract

Extreme Scattering Events and pulsar secondary spectra have highlighted fundamental problems in our understanding of the dynamics of interstellar turbulence. We describe some of these problems in detail and present the theory behind the technique of speckle imaging, which offers a prospect of revealing fundamental properties of the turbulence. It also offers the prospect of resolving pulsar magnetospheres on ~10 nanoarcsecond scales.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. SPICE: Scintillation Pipeline for Interferometric Candidate Extraction

    astro-ph.IM 2026-06 unverdicted novelty 4.0

    SPICE is an automated pipeline that recovers known pulsars in GMRT data by detecting scintillation signatures in interferometric visibilities.