Gravitational Interstellar Scintillation
Gravitation could modulate the interstellar scintillation of pulsars in a way that is analogous to refractive interstellar scintillation (RISS). While RISS occurs when a large ionized cloud crosses the pulsar line-of-sight, gravitational interstellar scintillation (GISS) occurs when a compact gravitational deflector lies very near to that line-of-sight.
openaire +2 more sources
Interstellar scintillation studies of pulsars and distribution of scattering plasma in the local interstellar medium [PDF]
Pulsar scintillation measurements from the Ooty Radio Telescope (ORT) are used to investigate the distribution of scattering in the Local Interstellar Medium (LISM; region of ≤ 1 kpc of the Sun), specifically the region in and around the Local ...
Gupta, Yashwant +3 more
core +1 more source
SPICE: Scintillation Pipeline for Interferometric Candidate Extraction
We present Scintillation Pipeline for Interferometric Candidate Extraction (SPICE) an automated CASA-based pipeline developed to identify pulsar candidates in Giant Metrewave Radio Telescope (GMRT) and upgraded GMRT (uGMRT) data through their diffractive
Jitendra Salal +2 more
doaj +1 more source
The Impact of Interstellar Scintillation on Astrometric VLBI [PDF]
IVS 2004 General Meeting ProceedingsWe review the evidence demonstrating the interstellar scintillation (ISS) is the principal mechanism responsible for the intra-day variability (IDV) seen at cm wavelengths in many compact, flat-spectrum extra-galactic ...
Macquart, Jean-Pierre +10 more
core +1 more source
Scintillation Properties of PSR B1133+16 Measured with Very Long Baseline Interferometry
The scintillation of pulsars reveals the small-scale structure of the interstellar medium. A powerful technique for characterizing the scintillating structures (screens) combines analysis of scintillation arcs and very long baseline interferometry (VLBI).
Ashley M. Stock +5 more
doaj +1 more source
Refractive interstellar scintillation in 1741-038
A year of VLA observations of the radio source 1741-038 show that it exhibits pronounced variability at 1.49, 15, and 22 GHz, and somewhat reduced activity at 4.9 GHz. We interpret the unusually strong 1.49 GHz variability as due to refractive interstellar scintillation, and the high-frequency variability as being intrinsic to the source.
R. M. Hjellming, Ramesh Narayan
openaire +1 more source
The interstellar turbulent plasma spectrum in the direction to PSR B1642-03 from multi-frequency observations of interstellar scintillation [PDF]
Multi-frequency observations of interstellar scintillation toward the pulsar PSR B1642-03 were analyzed to estimate the spectrum of interstellar plasma inhomogeneities in the direction of this pulsar. Using data over the frequency range from 103 MHz to 5
W. Sieber +8 more
core +1 more source
Refractive interstellar scintillation of pulsar intensities at 74 MHz [PDF]
Results of daily observations of the flux of nine pulsars made with a large phased-array at 74 MHz from January 24, 1989 for 400 d are presented. Modulation indices and time scales are estimated for the variations.
Gupta, Y., Coles, W. A., Rickett, B. J.
core +2 more sources
Free electrons in the interstellar medium refract and diffract radio waves along multiple paths, resulting in angular and temporal broadening of radio pulses that limits pulsar timing precision.
Abra Geiger +35 more
doaj +1 more source
Precision orbital dynamics from interstellar scintillation arcs for PSR J0437-4715 [PDF]
Intensity scintillations of radio pulsars are known to originate from interference between waves scattered by the electron density irregularities of interstellar plasma, often leading to parabolic arcs in the two-dimensional power spectrum of the ...
Dai, Shi (R20363) +31 more
core +2 more sources

