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12篇 您的检索式:作者名="John P Wolf"
    题名 作者 年代 出处 被引量
1Consistent infinitesimal finite element cell method: three- dimensional vector wave equation显示文摘Wolf John P Song Chongmin 1996International Journal for Numerical Methods in Engineering1996,39,13:1
2The scaled boundary finite element method - a primer derivation- s显示文摘John P Wolf Chongmin Song 2000Computers & Structures2000,78,:1
3The scaled boundary finite-element method - a primer solution procedures显示文摘Chongmin Song John P Wolf 2000Computers & Structures2000,78,:1
4Consistent Infinitesimal Finite-element Cell Method: Three-dimensional Vector Wave Equation显示文摘Song Chongmin Wolf John P 1996International Journal for Numerical Methods in Engineering1996,39,13:1
5The scaled boundary finite element method-a primer derivations显示文摘John P Wolf Chongmin Song 2000Com- puters & Structures2000,78,:1
6The scaled boundary finite-element method-a primer solution procedures 显示文摘Chongmin Song John P Wolf 2000Computers & Structures2000,78,:1
7Spring-Dashpot-Mass Model for Foundation Vibrations显示文摘John P Wolf 1997EESD1997,26,:1
8Recursive evaluation of interaction forces of unbounded soil in the time domain 显示文摘John P Wolf Masato Motosaka 1989Earthquake Engineering and Structure Dynamic1989,18,3:1
9Realtime CORBA 显示文摘WOLFE V F JOHN R KORTMANN P 2000IEEE Transaction on Parallell and Distributed System2000,,11:1
10Consistent infinitesimal finite dement cell method: three-dimensional vector wave equation显示文摘Wolf John P Song Chongmi 1996International Journal for Numerical Methods in Engineering1996,39,13:1
11Demonstrated brain insulin resistance in Alzheimer’s disease patients is associated with IGF-1 resistance, IRS-1 dysregulation, and cognitive decline显示文摘Talbot Konrad Wang Hoau-Yan Kazi Hala Han Li-Ying Bakshi Kalindi P Stucky Andres Fuino Robert L Kawaguchi Krista R Samoyedny Andrew J Wilson Robert S Arvanitakis Zoe Schneider Julie A Wolf Bryan A Bennett David A Trojanowski John Q Arnold 2012EN2012,,4:1
12Deriving the coronal hole electron temperature: electron density dependent ionization / recombination considerations显示文摘Comparison of appropriate theoretically derived line ratios with observational data can yield estimates of a plasma’s physical parameters,such as electron density or temperature.The usual practice in the calculation of the line ratio is the assumption of excitation by electrons/protons followed by radiative decay.Furthermore,it is normal to use the so-called coronal approximation,i.e.one only considers ionization and recombination to and from the ground-state.A more accurate treatment is to include ionization/recombination to and from metastable levels.Here,we apply this to two lines from adjacent ionization stages,Mg IX 368  and Mg X 625 ,which has been shown to be a very useful temperature diagnostic.At densities typical of coronal hole conditions,the difference between the electron temperature derived assuming the zero density limit compared with the electron density dependent ionization/recombination is small.This,however,is not the case for flares where the electron density is orders of magnitude larger.The derived temperature for the coronal hole at solar maximum is around 1.04MK compared to just below 0.82MK at solar minimum.John Gerard Doyle Steven Chapman Paul Bryans David Pérez-Suárez Avninda Singh Hugh Summers Daniel Wolf Savin 2010Research in Astronomy and Astrophysics2010,10,1:0
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