activity
19942023
most citedCore and Conal Component Analysis of Pulsar B1933+16 --- Investigation of the Segregated Modes

34 citations · 155 across the 16 of their papers we have counts for

collaborators

16 papers

cond-mat.mtrl-sci2023

On the relative abundances of Cavansite and Pentagonite

Bhalchandra S. Pujari, Sagar Gehlot, Mihir Arjunwadkar +2

Cavansite is a visually stunning blue vanadosilicate mineral with limited occurrences worldwide, whereas Pentagonite is a closely related dimorph with similar physical and chemical…

astro-ph.HE2019★ 31 cited

A Single spark model for PSR J21443933

Dipanjan Mitra, Rahul Basu, George I. Melikidze +1

The partially screened vacuum gap model (PSG) for the inner acceleration region in normal radio pulsars, a variant of the pure vacuum gap model, attempts to account for the observe…

astro-ph.SR2017★ 25 cited

Quantifying weak non-thermal solar radio emission at low radio frequencies

Rohit Sharma, Divya Oberoi, Mihir Arjunwadkar

The recent availability of fine grained high sensitivity data from the new generation low radio frequency instruments such as the Murchison Widefield Array (MWA) have opened up opp…

astro-ph.IM2016

Neutron stars in the light of SKA: Data, statistics, and science

Mihir Arjunwadkar, Akanksha Kashikar, Manjari Bagchi

The Square Kilometre Array (SKA), when it becomes functional, is expected to enrich neutron star (NS) catalogues by at least an order of magnitude over their current state. This in…

astro-ph.HE2016★ 34 cited

Core and Conal Component Analysis of Pulsar B1933+16 --- Investigation of the Segregated Modes

Dipanjan Mitra, Joanna Rankin, Mihir Arjunwadkar

Radio pulsar B1933+16 is brightest core-radiation dominated pulsar in the Arecibo sky, and here we carry out a comprehensive high resolution polarimetric study of its radiation at…

astro-ph.HE2015

Polarized quasiperiodic structures in pulsar radio emission reflect temporal modulations of non-stationary plasma flow

Dipanjan Mitra, Mihir Arjunwadkar, Joanna M. Rankin

Bright single pulses of many radio pulsars show rapid intensity fluctuations (called microstructure) when observed with time resolutions of tens of microseconds. Here, we report an…