Nuclear Resonant Absorption of Gamma Rays byCa40

1961 ◽  
Vol 124 (5) ◽  
pp. 1541-1548 ◽  
Author(s):  
A. C. Eckert ◽  
E. F. Shrader
Keyword(s):  
Gamma Rays ◽  
Resonant Absorption

Rocoil-Free Resonant Absorption of 35.5-keV Gamma Rays of Te125

1962 ◽  
Vol 17 (7) ◽  
pp. 1205-1205 ◽  
Author(s):  
Naomoto Shikazono ◽  
Tokio Shôji ◽  
Hidekuni Takekoshi ◽  
Poh-Kun Tseng
Keyword(s):  
Gamma Rays ◽  
Resonant Absorption

Resonant Absorption of Gamma Rays

1957 ◽  
Vol 108 (6) ◽  
pp. 1644-1645 ◽  
Author(s):  
S. S. Hanna ◽  
Luise Meyer-Schützmeister
Keyword(s):  
Gamma Rays ◽  
Resonant Absorption

scholarly journals Emission of gamma rays shifted from resonant absorption by electron-nuclear double transitions in 151 Eu 2+ :CaF 2

1997 ◽  
Vol 37 (3) ◽  
pp. 177-182 ◽  
Author(s):  
S Olariu ◽  
J. J Carroll ◽  
C. B Collins
Keyword(s):  
Gamma Rays ◽  
Resonant Absorption

scholarly journals STUDIES OF NUCLEAR RESONANT ABSORPTION OF GAMMA RAYS. Final Report

1962 ◽  
Author(s):  
J.J. Ezop
Keyword(s):  
Gamma Rays ◽  
Resonant Absorption ◽  
Final Report

On the possible gamma-ray source in Cygnus

1967 ◽  
Vol 31 ◽  
pp. 469-471
Author(s):  
J. G. Duthie ◽  
M. P. Savedoff ◽  
R. Cobb
Keyword(s):  
Gamma Rays ◽  
Gamma Ray ◽  
Right Ascension

A source of gamma rays has been found at right ascension 20h15m, declination +35°, with an uncertainty of 6° in each coordinate. Its flux is (1·5 ± 0·8) x 10-4photons cm-2sec-1at 100 MeV. Possible identifications are reviewed, but no conclusion is reached. The mechanism producing the radiation is also uncertain.

Solar Flare Energetic Neutral Emission Measurements in the Project Coronas-I

1994 ◽  
Vol 144 ◽  
pp. 635-639
Author(s):  
J. Baláž ◽  
A. V. Dmitriev ◽  
M. A. Kovalevskaya ◽  
K. Kudela ◽  
S. N. Kuznetsov ◽  
...  
Keyword(s):  
Solar Flare ◽  
Energy Range ◽  
Gamma Rays ◽  
Pulse Shape ◽  
Gamma Ray ◽  
Pulse Shape Discrimination ◽  
Shape Discrimination ◽  
Solar Neutron ◽  
Low Altitude

AbstractThe experiment SONG (SOlar Neutron and Gamma rays) for the low altitude satellite CORONAS-I is described. The instrument is capable to provide gamma-ray line and continuum detection in the energy range 0.1 – 100 MeV as well as detection of neutrons with energies above 30 MeV. As a by-product, the electrons in the range 11 – 108 MeV will be measured too. The pulse shape discrimination technique (PSD) is used.

Linear Visco-Resistive Computations of Magnetohydrodynamic Waves: I. The Code and Test Cases

1994 ◽  
Vol 144 ◽  
pp. 503-505
Author(s):  
R. Erdélyi ◽  
M. Goossens ◽  
S. Poedts
Keyword(s):  
Resonant Absorption ◽  
Numerical Code ◽  
Mhd Waves ◽  
Test Cases ◽  
Numerical Accuracy ◽  
Element Discretization ◽  
Flux Tubes ◽  
Magnetohydrodynamic Waves ◽  
Viscosity Coefficients ◽  
Magnetic Flux Tubes

AbstractThe stationary state of resonant absorption of linear, MHD waves in cylindrical magnetic flux tubes is studied in viscous, compressible MHD with a numerical code using finite element discretization. The full viscosity tensor with the five viscosity coefficients as given by Braginskii is included in the analysis. Our computations reproduce the absorption rates obtained by Lou in scalar viscous MHD and Goossens and Poedts in resistive MHD, which guarantee the numerical accuracy of the tensorial viscous MHD code.

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