Add to ORKGSorry, the full text of this article is not available here. Please click on the alternative location to access it.In the previous paper of this series, Deshpande & Rankin reported results regarding the sub-pulse drift phenomenon in pulsar B0943+10 at 430 and 111MHz. This study has led to the identification of a stable system of sub-beams circulating around the magnetic axis of this star. Here, we present a single-pulse analysis of our observations of this pulsar at 35MHz. The fluctuation properties seen at this low frequency, as well as our independent estimates of the number of sub-beams required and their circulation time, agree remarkably well with the reported behaviour at higher frequencies. We use the `cartographic' transform mapping ...
Aims. The usefulness and versatility of the PSRSALSA open-source pulsar data-analysis project is dem...
PSR B0818-41 is one of the few pulsars that show multiple drift regions having well-defined phase re...
Open Access.“Sub-pulse drifting”, one of the rich phenomena exhibited by many pulsars, have been sug...
Restricted Access.In the previous paper of this series, Deshpande & Rankin reported results regardin...
In the previous paper of this series, Deshpande & Rankin reported results regarding the sub-pulse dr...
Sorry, the full text of this article is not available here. Please click on the alternative location...
Restricted AccessThe `drifting' sub-pulses exhibited by some radio pulsars have fascinated both obse...
Recent results regarding subpulse drift in pulsar B0943 + 10 have led to the identification of a sta...
The ``drifting'' subpulses exhibited by some radio pulsars have fascinated both observers and theori...
The beautiful sequences of drifting subpulses observed in some radio pulsars have been regarded as a...
We use broadband sensitive LOFAR observations in the 25–80 MHz frequency range to study the single-p...
Pulsar B0943+10 is well known for its “B” (burst) mode, characterized by accurately drifting subpuls...
Aims. We aim to expand our understanding of radio wave emission and propagation in the pulsar magnet...
Contains fulltext : 36190.pdf (publisher's version ) (Open Access)This thesis cons...
This paper reports new observations of pulsars B0943+10 and B1822−09 carried out with the Arecibo Ob...
Aims. The usefulness and versatility of the PSRSALSA open-source pulsar data-analysis project is dem...
PSR B0818-41 is one of the few pulsars that show multiple drift regions having well-defined phase re...
Open Access.“Sub-pulse drifting”, one of the rich phenomena exhibited by many pulsars, have been sug...
Restricted Access.In the previous paper of this series, Deshpande & Rankin reported results regardin...
In the previous paper of this series, Deshpande & Rankin reported results regarding the sub-pulse dr...
Sorry, the full text of this article is not available here. Please click on the alternative location...
Restricted AccessThe `drifting' sub-pulses exhibited by some radio pulsars have fascinated both obse...
Recent results regarding subpulse drift in pulsar B0943 + 10 have led to the identification of a sta...
The ``drifting'' subpulses exhibited by some radio pulsars have fascinated both observers and theori...
The beautiful sequences of drifting subpulses observed in some radio pulsars have been regarded as a...
We use broadband sensitive LOFAR observations in the 25–80 MHz frequency range to study the single-p...
Pulsar B0943+10 is well known for its “B” (burst) mode, characterized by accurately drifting subpuls...
Aims. We aim to expand our understanding of radio wave emission and propagation in the pulsar magnet...
Contains fulltext : 36190.pdf (publisher's version ) (Open Access)This thesis cons...
This paper reports new observations of pulsars B0943+10 and B1822−09 carried out with the Arecibo Ob...
Aims. The usefulness and versatility of the PSRSALSA open-source pulsar data-analysis project is dem...
PSR B0818-41 is one of the few pulsars that show multiple drift regions having well-defined phase re...
Open Access.“Sub-pulse drifting”, one of the rich phenomena exhibited by many pulsars, have been sug...