Abstract Flares originate from the impulsive release of magnetic energy in the solar atmosphere. The rise in X‐ray flux enhances ionization/electron content in the upper atmosphere, modifying the photochemical and dynamical processes that govern the ionosphere‐thermosphere behavior.
Komal, Duggirala Pallamraju
wiley +1 more source
Reading signatures of supermassive binary black holes in pulsar timing array observations. [PDF]
Goncharov B +12 more
europepmc +1 more source
Reduced gas accretion onto galaxies due to effects of external giant radio lobes. [PDF]
Qiu Y, Cen R.
europepmc +1 more source
Formation time-scales for stellar bars in diverse galactic discs. [PDF]
Frosst M, Obreschkow D, Ludlow A.
europepmc +1 more source
Content-based image retrieval using COSFIRE descriptors with application to radio astronomy [PDF]
Steven Ndung’u +3 more
openalex +1 more source
Square Kilometre Array Enhancement: A Convex Programming Approach to Optimize SKA-Low Stations in the Case of Perturbed Vogel Layout. [PDF]
Battaglia GM +4 more
europepmc +1 more source
Orientational Structure and Electro-Optical Properties of Chiral Nematic Droplets with Conical Anchoring. [PDF]
Feizer KA +3 more
europepmc +1 more source
Experiences of commercial supercomputing in radio astronomy data processing
I.J. Kemp +3 more
openalex +1 more source
Multiple outflows and delayed ejections revealed by early imaging of novae. [PDF]
Aydi E +41 more
europepmc +1 more source

