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P. A. Kamini

Researcher at Raman Research Institute

Publications -  12
Citations -  978

P. A. Kamini is an academic researcher from Raman Research Institute. The author has contributed to research in topics: Murchison Widefield Array & Telescope. The author has an hindex of 6, co-authored 10 publications receiving 943 citations.

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The Murchison Widefield Array: Design Overview

TL;DR: The Murchison Widefield Array is a dipole-based aperture array synthesis telescope designed to operate in the 80-300 MHz frequency range, capable of a wide range of science investigations but initially focused on three key science projects: detection and characterization of three-dimensional brightness temperature fluctuations in the 21 cm line of neutral hydrogen during the epoch of reionization.
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First spectroscopic imaging observations of the sun at low radio frequencies with the murchison widefield array prototype

Divya Oberoi, +73 more
TL;DR: In this paper, the first spectroscopic images of solar radio transients from the prototype for the Murchison Widefield Array, observed on 2010 March 27, were presented, covering the instantaneous frequency band 170.9- 201.6 MHz.
Journal ArticleDOI

Interferometric Imaging with the 32 Element Murchison Wide-Field Array

TL;DR: The Murchison Wide-Field Array (MWA) is a low-frequency radio telescope, currently under construction, intended to search for the spectral signature of the epoch of reionization (EOR) and to probe the structure of the solar corona as mentioned in this paper.
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A digital-receiver for the Murchison Widefield Array

Thiagaraj Prabu, +63 more
TL;DR: An FPGA-based digital-receiver has been developed for a low-frequency imaging radio interferometer, the Murchison Widefield Array (MWA), and the design, implementation, current status, and plans for future enhancements are presented.