Results 21 to 30 of about 5,002 (274)
Neutron Star Model Atmospheres [PDF]
AIP Conference Proceedings, 2009 Determination of neutron star (NS) parameters is an important astrophysical problem. The stellar radius depends on the mass and the equation of state (EOS) in the NS core, which is not well known. Therefore, with masses and radii inferred from observations we are able to select between various theories for the EOS.
Valery Suleimanov +8 more
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Modeling Neutron Star Atmospheres
, 2002 10 pages, 13 color figures; to be published in Proceedings of the 270. Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Bad Honnef (Germany), Jan. 21-25, 2002, eds. W. Becker, H.
Zavlin, V., Pavlov, G.
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Yuanzineng kexue jishu, 2022 Based on the test site at the Qinghai Tibet Plateau with an altitude of 4 300 m, atmospheric neutron single event effects of a 65 nm high speed large area static random access memory (SRAM) array were measured in real time.
ZHANG Zhangang;LEI Zhifeng;HUANG Yun;EN Yunfei;ZHANG Yi;TONG Teng;LI Xiaohui;SHI Qian;PENG Chao;HE Yujuan;XIAO Qingzhong;LI Jianke;LU Guoguang
doaj
Observing the neutron component during thunderstorm activity at a mountain CR station
Solar-Terrestrial Physics, 2019 During three summer months in 2015, the Cosmic Ray (CR) station Irkutsk-3000, located at 3000 m above sea level, measured the CR neutron component intensity with the 6NM64 neutron monitor, as well as the atmospheric electric field strength and the level ...
Lukovnikova A.A. +2 more
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Space Weather, 2022 Significant increases to the atmospheric radiation environment are recorded by a network of ground level neutron monitors as ground level enhancements (GLEs).
A. D. P. Hands +5 more
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Atmospheres and spectra of strongly magnetized neutron stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2001 29 pages, 11 figures; corrected factor of 2 in He models: minor changes to figs 4 and 9 as a result; other very minor ...
Ho, Wynn C. G., Lai, Dong
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, 2022 With the loading of Gadolinium in the Super-Kamiokande detector, the overall detection efficiency of neutrons from neutrino-nucleus interaction has greatly increased. Based on semi-tuned atmospheric neutrino event simulation, we estimate how the improved
Seungho Han
core +1 more source
A HYDROGENIC MOLECULAR ATMOSPHERE OF A NEUTRON STAR
Modern Physics Letters A, 2004 A model of a hydrogenic content of atmosphere of the isolated neutron star 1E1207.4-5209 is proposed. It is based on the assumption that the main component in the atmosphere is the exotic molecular ion [Formula: see text] and that there exists a magnetic field in the range of (4±2)×1014 G .
Turbiner, A. V., Vieyra, J. C. Lopez
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Photoionization of Hydrogen in Atmospheres of Magnetic Neutron Stars [PDF]
The Astrophysical Journal, 1997 19 pages including 8 figures, LaTeX (using aas2pp4.sty and epsf.sty). Accepted for publication in ApJ.
Potekhin, A. Y., Pavlov, G. G.
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Unfolding the Neutron Flux Spectrum on the Surface of Mars Using the MSL‐RAD and Odyssey‐HEND Data
Space Weather, 2023 Understanding the long‐term radiation environment at the surface of Mars allows us to estimate the exposure for future robotic and crewed missions. Typically, the radiation environment includes charged particles (i.e., protons and heavier ions) and ...
L. M. Martinez Sierra +10 more
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