Results 1 to 10 of about 3,259 (256)
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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Model Atmospheres for Low-Field Neutron Stars [PDF]
The Astrophysical Journal, 1996 We compute model atmospheres and emergent spectra for low field (B<10^10 G) neutron stars, using new opacity and equation of state data from the OPAL project. These computations, incorporating improved treatments of flux transport and convective stability, provide spectra for hydrogen, solar abundance and iron atmospheres.
Rajagopal, Mohan, Romani, Roger
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A neutron star with a carbon atmosphere in the Cassiopeia A supernova remnant [PDF]
Nature, 2009 The surface of hot neutron stars is covered by a thin atmosphere. If there is accretion after neutron star formation, the atmosphere could be composed of light elements (H or He); if no accretion takes place or if thermonuclear reactions occur after accretion, heavy elements (for example, Fe) are expected.
Ho, Wynn C. G., Heinke, Craig O.
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Applied System InnovationThis research investigates atmospheric neutron-induced single event effects (SEEs) on advanced artificial intelligence (AI) chips during natural environment operation.
Weitao Yang +4 more
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Model Atmospheres for X-ray Bursting Neutron Stars [PDF]
Symposium - International Astronomical Union, 1986 Self consistent neutron star atmospheric models have been constructed which include the effects of Comptonization, free-free and bound-free absorption. It has been demonstrated that for parameters relevant to x-ray bursting neutron stars the atmosphere does not radiate like a blackbody during any phase of an x-ray burst.
R. A. London, W. M. Howard, R. E. Taam
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Yuanzineng kexue jishuAs the core of high-voltage direct-current transmission technology, the DC converter valve and its key power device thyristor face a high risk of failure caused by atmospheric neutron when operating in high-altitude areas. The atmospheric neutron failure
PENG Chao1, ZHOU Yang2, CHEN Zhongyuan2, LEI Zhifeng1, MA Teng1, ZHANG Zhangang1, ZHANG Hong1, HE Yujuan1
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Atmospheric Effects on Neutron Star Parameter Constraints with NICER
The Astrophysical Journal, 2023 We present an analysis of the effects of uncertainties in the atmosphere models on the radius, mass, and other neutron star parameter constraints for the NICER observations of rotation-powered millisecond pulsars.
Tuomo Salmi +9 more
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Influence of Solar Wind on Secondary Cosmic Rays and Atmospheric Electricity
Frontiers in Earth Science, 2021 A relationship between the heliospheric magnetic field, atmospheric electric field, lightning activity, and secondary cosmic rays measured on the high mount of Lomnický Štít (2,634 m a.s.l.), Slovakia, during the declining phase of the solar cycle 24 is ...
Jaroslav Chum +7 more
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