Dissemin is shutting down on January 1st, 2025

Published in

American Astronomical Society, Astrophysical Journal Letters, 1(809), p. L12, 2015

DOI: 10.1088/2041-8205/809/1/l12

Links

Tools

Export citation

Search in Google Scholar

Murchison Widefield Array Observations of Anomalous Variability: A Serendipitous Night-time Detection of Interplanetary Scintillation

Journal article published in 2015 by D. L. Kaplan ORCID, Christopher Leigh Williams, S. J. Tingay, P. K. Manoharan ORCID, J. P. Macquart ORCID, P. Hancock ORCID, J. Morgan ORCID, D. A. Mitchell ORCID, R. D. Ekers ORCID, R. B. Wayth ORCID, C. Trott ORCID, T. Murphy ORCID, D. Oberoi ORCID, I. H. Cairns ORCID, Lu Feng and other authors.
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

Full text: Download

Red circle
Preprint: archiving forbidden
Red circle
Postprint: archiving forbidden
Green circle
Published version: archiving allowed
Upload
Policy details
Data provided by SHERPA/RoMEO

Abstract

We present observations of high-amplitude rapid (2 s) variability toward two bright, compact extragalactic radio sources out of several hundred of the brightest radio sources in one of the 30° X 30° Murchison Widefield Array (MWA) Epoch of Reionization fields using the MWA at 155 MHz. After rejecting intrinsic, instrumental, and ionospheric origins we consider the most likely explanation for this variability to be interplanetary scintillation (IPS), likely the result of a large coronal mass ejection propagating from the Sun. This is confirmed by roughly contemporaneous observations with the Ooty Radio Telescope. We see evidence for structure on spatial scales ranging from 10[superscript 6] km. The serendipitous night-time nature of these detections illustrates the new regime that the MWA has opened for IPS studies with sensitive night-time, wide-field, low-frequency observations. This regime complements traditional dedicated strategies for observing IPS and can be utilized in real-time to facilitate dedicated follow-up observations. At the same time, it allows large-scale surveys for compact (arcsec) structures in low-frequency radio sources despite the 2' resolution of the array.