Results 181 to 190 of about 1,721,894 (339)
A 3-Meter Atmospheric Cherenkov Telescope as a Test Bench for Very High Energy Gamma-Ray Astrophysics Projects [PDF]
T. Yoshikoshi
openalex +1 more source
Enhanced Radiation Exposure of Airline Crew and Passengers During the May 2024 Geomagnetic Storm
Abstract Enhanced radiation at aviation altitudes is a concern for flight crew and passengers. During space weather events, solar flares and coronal mass ejection (CME) driven shocks are sources of energetic particles that can reach Earth's near‐space environment and interact with its magnetic field and atmosphere.
Homayon Aryan +6 more
wiley +1 more source
Underground solution to the long-time solar fusion reaction puzzle. [PDF]
Jiang Y, Liu W.
europepmc +1 more source
Abstract We present a methodology for deriving the horizontal two‐dimensional distribution of low‐energy electron precipitation, specifically the possible lower bound of the differential energy flux of electron precipitation at 100 eV, from a 630‐nm auroral image obtained with a ground‐based all‐sky imager.
K. Yashima +3 more
wiley +1 more source
PROGRAM of the 15-th Nishinomiya-Yukawa Memorial Symposium, Gamma-Ray Bursts and High Energy Astrophysics [PDF]
openalex +1 more source
Abstract A number of mechanisms have been suggested to operate within the terrestrial bow shock to redistribute energy contained in the incoming solar wind flow. The majority of mechanisms involve the generation of turbulence while some are based on particle motion alone.
Simon N. Walker +2 more
wiley +1 more source
Energy calibration of the 2.5 MV Pelletron at the Dalton Cumbrian Facility. [PDF]
Linkowski K +11 more
europepmc +1 more source
Abstract On December 2023, the Juno spacecraft made a flyby of Io above the northern hemisphere at a closest approach (CA) altitude of ∼1,500 km (PJ57). The Juno/Waves and Radio‐occultation measurements showed a surprising large electron density ∼28,000 cm−3 near closest approach.
V. Dols, F. Bagenal
wiley +1 more source
Inverse compton scattering in high energy astrophysics
Jason G. Cullen
openalex +1 more source

