Results 191 to 200 of about 3,434 (238)

Probing the Phase and Mechanism of Captured CO₂ in Supercapacitors by Pore Wetting and NMR Spectroscopy. [PDF]

Chem Mater
Coady Z, Seyffertitz M, Rhodes BJ, Kress T, Turner A, Mapstone G, Xu Z, Paris O, Forse AC.   +8 more
europepmc   +1 more source

Probing boron vacancy defects in hBN via single spin relaxometry. [PDF]

Nat Commun
Melendez AL, Gong R, He G, Wang Y, Wu YC, Poirier T, Randolph S, Ghosh S, Liang L, Jesse S, Li AP, Damron JT, Lawrie BJ, Edgar JH, Vlassiouk IV, Zu C, Zhao H.   +16 more
europepmc   +1 more source

Unraveling the symmetry of Al₅C₃N. [PDF]

Acta Crystallogr B Struct Sci Cryst Eng Mater
Shtender V, Ong CS, Berastegui P, Donzel-Gargand O, Cedervall J, Hervoches C, Beran P, Eriksson O, Jansson U.   +8 more
europepmc   +1 more source

Production of secondary particles from cosmic ray interactions in the earth's atmosphere: Implications for annual effective dose, 14C/12C ratio, and magnetic field effects. [PDF]

PLoS One
Hassanpour M, Rezaie M, Heydarizade Y, Rashed Iqbal Faruque M, Hassanpour M.   +4 more
europepmc   +1 more source

Comparing the Accuracy of Soil Moisture Estimates Derived from Bulk and Energy-Resolved Gamma Radiation Measurements. [PDF]

Sensors (Basel)
Akter S, Huisman JA, Bogena HR.
europepmc   +1 more source

Cyclotron lines in neutron stellar atmospheres

, 1993
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A Neutron Star Atmosphere in the Laboratory with Petawatt Lasers

Astrophysics and Space Science, 2005
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Moon, S. J., Wilks, S. C., Klein, R. I., Remington, B. A., Ryutov, D. D., Mackinnon, A. J., Patel, P. K., Spitkovsky, A.   +7 more
openaire   +2 more sources

fast-neutron flux in the atmosphere

Journal of Geophysical Research, 1963
Neutron flux between one and ten mev from sea level to balloon altitudes, recorded by fast neutron detector insensitive to other ...
R. B. Mendell, S. A. Korff
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Neutron Star Atmospheres

2006
Properties of the thermal radiation emitted by neutron stars (NSs) are determined by thin plasma layers (atmospheres) at their surfaces. The NS atmospheres are very different from those of usual stars due to the immense gravity and huge magnetic fields. Current models of hydrogen NS atmospheres show that the spectra deviate substantially from blackbody
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Some Measurements of Atmospheric Neutrons

Physical Review, 1958
A series or airplane flights carrying neutron counters to an altitude of 700 g cm/sup -2/ was made at 52 20 north geomagnetic latitude in 1955. Enriched and normal BF/sub 3/ counters were covered with Cd, Sn, Pyrex, and limeglass shields. the ratios or the counting rates of the variously shielded counters are compared with the ratios calculated ...
openaire   +1 more source