Report of the Ad Hoc Committee on fusion plasma research facilities

1976 ◽  
Author(s):  
Not Given Author
1994 ◽  
Vol 37 (5) ◽  
Author(s):  
A. M. DzIewonski

The origins of the Federation of Digital Seismograph Networks (FDSN) can be traced to the summer of 1984. At that time, GEOSCOPE - the French global network of broadband instruments - was already well under way, and in the United States, the Incorporated Research Institutions for Seismology (IRIS) had just published its Science Plan for Global Seismographic Network (GSN). There was clearly an opportunity and the need to involve scientists from other countries in planning for the future of global seismology. An ad hoc meeting of some ten West European seismologists had been arranged in August during the annual meeting of the European Geophysical Society in Louvain. This may be considered to signify the beginning of widescale international cooperation, even though this particular group eventually became the nucleus of ORFEUS (Observatories and Research Facilities for EUropean Seismology). Rather than taking an active role in deployment of new stations, it chose to focus on the issue of providing the service for data collection and exchange, with an important mission of developing the requisite software.


2005 ◽  
Vol 81 (11) ◽  
pp. 849-862
Author(s):  
Yutaka KAMADA ◽  
Michiya SHIMADA ◽  
Yukitoshi MIURA ◽  
Yuichi OGAWA

2013 ◽  
Vol 64 (2) ◽  
pp. 298-302
Author(s):  
B. Berlinger ◽  
A. Brooks ◽  
H. Feder ◽  
J. Gumbas ◽  
T. Franckowiak ◽  
...  

2018 ◽  
Vol 96 (8) ◽  
pp. 871-877
Author(s):  
Arun Goyal ◽  
Indu Khatri ◽  
Narendra Singh ◽  
Sunny Aggarwal ◽  
A.K. Singh ◽  
...  

We report an extensive and elaborate theoretical study of atomic data for Cs XXV by using multi-configuration Dirac–Fock method and calculated energy levels for the lowest 110 fine structure levels. We have presented the radiative data for electric and magnetic dipole (E1, M1) and quadrupole (E2, M2) transitions among lowest 110 levels. We have made comparisons of our calculated excitation energies with theoretically calculated and experimentally observed energy levels. We have studied the effect of correlation by introducing more configurations in our calculations. We have also computed energy levels by performing similar relativistic distorted wave calculations using Flexible Atomic Code. Additionally, we have also provided new atomic data for Cs XXV and identified extreme ultraviolet and soft X-ray spectral lines with gA spectra for E1 and M2 transitions, which are not published elsewhere in the literature. We believe that our results may be beneficial in fusion plasma research and applications.


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