Isotope Shifts in X-Ray Spectra

Author(s):  
W. H. King
Keyword(s):  
X Ray ◽  
2018 ◽  
Vol 98 (2) ◽  
Author(s):  
I. I. Tupitsyn ◽  
N. A. Zubova ◽  
V. M. Shabaev ◽  
G. Plunien ◽  
Th. Stöhlker

1974 ◽  
Vol 9 (6) ◽  
pp. 2444-2447 ◽  
Author(s):  
Kenneth W. Ford ◽  
George A. Rinker
Keyword(s):  
X Ray ◽  

Pramana ◽  
1983 ◽  
Vol 20 (5) ◽  
pp. 363-373 ◽  
Author(s):  
K V Subba Rao ◽  
A A Kamal
Keyword(s):  
X Ray ◽  

The structure of the resonance line ⋋553.5 nm of Ba ɪ has been studied by means of Doppler-free spectroscopy. Dye laser light was scattered resonantly from an atomic beam containing the natural mixture of isotopes; the spectra were recorded digitally and analysed by computer. The main object was to provide data to reduce uncertainties due to electronic calculations in the extraction of nuclear data from optical measurements. The isotope shifts (MHz), relative to 138 Ba, are 137 Ba, – 214.7 (5); 136 Ba, – 127.5 (13); 135 Ba, – 258.7 (7); 134 Ba, – 142.8 (12). The minus signs indicate that 138 Ba has the lower frequency in each case. These results are combined with muonic X-ray, electronic X-ray and other optical data to extract changes in mean square radius of the nuclear charge distribution. The hyperfine splitting factors 135 A and 135 B were found to be – 97.76 (14) MHz and 32.29 (47) MHz respectively. From an analysis of these and other results for the 6s6p configuration we obtain the quadrupole moment of 135 Ba (uncorrected for quadrupole shielding) to be 0.195 (40) barn (1 barn = 10 -28 m 2 ).


1971 ◽  
Vol 35 (1) ◽  
pp. 33-34 ◽  
Author(s):  
P.L. Lee ◽  
F. Boehm
Keyword(s):  
X Ray ◽  

1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.


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