Results 71 to 80 of about 79,833 (199)
Study on the UV FEL single‐shot damage threshold of an Au thin film
Single‐shot damage of an 200 nm‐thick Au thin film is experimentally studied with a UV FEL of 121.6 nm wavelength and 2 ps pulse length. The characterized, as well as visually observed, phenomena are analyzed with multiple theoretical approaches.The damage threshold of an Au‐coated flat mirror, one of the reflective optics installed on the FEL‐2 ...
Meiyi Wu +13 more
wiley +1 more source
Pulsar scintillation observations have revealed ubiquitous discrete scintillation screens in the interstellar medium. A major obstacle in identifying the nature of these screens is the uncertainty in their distances, which prevents precise correlation ...
Yuanshang Huang +4 more
doaj +1 more source
Abstract We present broadband ionospheric scintillation observations of highly defined symmetric quasi‐periodic scintillations (QPS: Maruyama, 1991, https://doi.org/10.1029/91rs00357) caused by plasma structures in the mid‐latitude ionosphere using the LOw Frequency ARray (LOFAR: van Haarlem et al., 2013, https://doi.org/10.1051/0004‐6361/201220873 ...
H. Trigg +5 more
wiley +1 more source
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
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
Evaluation of the Scintillation Loss for Optical Communication Systems with Direct Detection [PDF]
In optical communications through the atmosphere, the evaluation of a link feasibility often requires the quantification of the scintillation penalty in terms of power loss. To find how much additional optical power is needed to reach the bit-error-rate (
Perlot, Nicolas
core
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
Interstellar Scintillation Studies of EPTA Pulsars
Liu Y. Interstellar Scintillation Studies of EPTA Pulsars.
Liu, Yulan
openaire +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

