Microquasar V4641 Sgr and Its Deep Investigation with LACT as a Super-PeVatron of Cosmic Rays. [PDF]
Cao Z, Khangulyan D, Liu J, Liu R.
europepmc +1 more source
Laboratory astrophysics experiments studying hydrodynamic and magnetically-driven plasma jets [PDF]
F. Suzuki-Vidal +18 more
openalex +1 more source
The Chinese Radio Telescope Array for Interplanetary Scintillation Monitoring
Abstract Solar flares, coronal mass ejections (CMEs) and enegertic particles, etc., are the driving sources that may cause catastrophic space weathers. It is desirable to obtain information of solar eruptions like flares and CMEs, etc., propagating from the Sun to the near‐Earth space.
Yihua Yan +10 more
wiley +1 more source
A fast, accurate and oscillation-free spectral collocation solver for high-dimensional transport problems. [PDF]
Cavallini N +3 more
europepmc +1 more source
Charge exchange processes involving highly charged ions and targets of interest in astrophysics and fusion plasmas [PDF]
S. Otranto
openalex +1 more source
Global Ionospheric Slab Thickness Prediction Model Using XGBoost and Ensemble Learning
Abstract The ionospheric equivalent slab thickness is a key parameter for understanding the plasma distribution in the ionosphere, with direct relevance to satellite navigation, communication, and skywave over‐the‐horizon radar. However, traditional prediction methods often suffer from regional biases, limiting their global applicability.
C. Han +8 more
wiley +1 more source
Correlation between active regions' spectra at high radio frequencies and solar flare occurrences. [PDF]
Mulas S +33 more
europepmc +1 more source
Basis of plasma astrophysics in stability of the triple star system
Ayan Kumar Makar
openalex +1 more source
Laser-Plasma and Self-Absorption Measurements with Applications to Analysis of Atomic and Molecular Stellar Astrophysics Spectra [PDF]
Christian G. Parigger +2 more
openalex +1 more source
Freshly Generated Super Sunrise Plasma Bubbles During the Geomagnetic Storm on November 5–6, 2023
Abstract During the geomagnetic storm on November 5–6, 2023, freshly generated super sunrise equatorial plasma bubbles (EPBs) and associated irregularities over the 80°–140°E sector were observed combining ground‐based and space observations from GNSS, ionosondes, HF Doppler records, and several satellite missions (COSMIC2, Swarm, and DMSP).
Ke Li +7 more
wiley +1 more source

