True scholar network
Royal Astronomical Society
1365-2966
Monthly
0035-8711
1924
4402077344582
YES
United Kingdom
English
YES
Google Scholar
publishing@ras.ac.uk
Low-mass (M500 < 5 × 1014 M) galaxy clusters have been largely unexplored in radio observations, because of the inadequate sensitivity of existing telescopes. However, the upgraded Giant M...
We present high spatial resolution observations of short -lived transients, ribbon and jets like events above a pore in Ca II H images where fine structure like umbral dots, light bridge and...
Introducing the axial magnetic field (B), velocity ( ), and velocity gradient (dv/dx) retrieved from inversions of Stokes profiles, the role of azimuthal component of the magnetic field in t...
January, 2020
A number of previous papers have developed an ion-proton theory of the pulsar polar cap. The basic equations summarizing this are given here with the results of sets of model step-to-step ca...
November, 2018
It is shown that the ion–proton magnetosphere is unstable in a limited area of the P–P˙ plane against transitions to a self-sustaining inverse Compton scattering mode in which the part...
November, 2018
Salient features of the remarkable band structure seen in the high-frequency interpulse of the Crab pulsar are summarized. It is argued that its source must lie in a current sheet, probably ...
July, 2017
It is shown that the time variability inherent in the ion–proton polar cap leads naturally to the growth of Langmuir modes on narrow bundles of magnetic flux lines and that the observed si...
February, 2017
There is good evidence that electron–positron pair formation is not present in that section of the pulsar open magnetosphere, which is the source of coherent radio emission, but the possib...
July, 2016
Evidence derived with minimal assumptions from existing published observations is presented to show that an ion–proton plasma is the source of radio-frequency emission in millisecond and i...
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