scholarly journals Resolution-dependent subsonic non-thermal line dispersion revealed by ALMA

2021 ◽  
Vol 21 (1) ◽  
pp. 024
Author(s):  
Nan-Nan Yue ◽  
Di Li ◽  
Qi-Zhou Zhang ◽  
Lei Zhu ◽  
Jonathan Henshaw ◽  
...  
Keyword(s):  
2001 ◽  
Vol 28 (1) ◽  
pp. 58-64
Author(s):  
S. McCartan ◽  
T. B. Jones ◽  
C. A. Featherston ◽  
J. A. Brandon

2020 ◽  
Author(s):  
yongchol cha ◽  
hyok choe ◽  
songjin oh ◽  
zinhwa cha ◽  
zhang dong

Abstract Background; The acupuncture meridian is the channel through which Qi & Blood flow, and acupuncture is having many thousands year history for treating various illnesses. However, there was no powerful evidence to prove the existence of meridians until now. Objectives; The purpose of this study is to explain that the meridian-like high thermal line (MLHTL) is the powerful evidence to prove the existence of meridians in human body. Methods; The meridian-like high thermal line inducing and the disease cure effect in the target organs connected along the meridians by the mineral pulse light stimuli, was researched and analyzed. Results; The meridian-like high thermal lines were induced along the classic meridians course at the human body surface, and simultaneously the internal refractory diseases such as nephrotic syndrome and angina pectoris were treated in the target organs connected along the meridians without drug use by the mineral pulse light stimuli. Conclusions; The meridian-like high thermal line is the powerful evidence to prove the existence of meridians in human body. From now on, MPL stimulator (Version 1) can induce MLHTL, and can show the non-drug cure effect in target organ connected along MLHTL.


2018 ◽  
Vol 33 (2) ◽  
pp. 719-727 ◽  
Author(s):  
Leanne Dawson ◽  
Andrew M. Knight
Keyword(s):  

2019 ◽  
Vol 66 (2) ◽  
pp. 1552-1564 ◽  
Author(s):  
Morteza Dabbaghjamanesh ◽  
Abdollah Kavousi-Fard ◽  
Shahab Mehraeen
Keyword(s):  

2015 ◽  
Vol 799 (1) ◽  
pp. L12 ◽  
Author(s):  
B. De Pontieu ◽  
S. McIntosh ◽  
J. Martinez-Sykora ◽  
H. Peter ◽  
T. M. D. Pereira

2010 ◽  
Vol 6 (S273) ◽  
pp. 200-203
Author(s):  
Matteo Cantiello ◽  
Jonathan Braithwaite ◽  
Axel Brandenburg ◽  
Fabio Del Sordo ◽  
Petri Käpylä ◽  
...  

AbstractHot luminous stars show a variety of phenomena in their photospheres and in their winds which still lack clear physical explanations at this time. Among these phenomena are non-thermal line broadening, line profile variability (LPVs), discrete absorption components (DACs), wind clumping and stochastically excited pulsations. Cantiello et al. (2009) argued that a convection zone close to the surface of hot, massive stars, could be responsible for some of these phenomena. This convective zone is caused by a peak in the opacity due to iron recombination and for this reason is referred to as the “iron convection zone” (FeCZ). 3D MHD simulations are used to explore the possible effects of such subsurface convection on the surface properties of hot, massive stars. We argue that turbulence and localized magnetic spots at the surface are the likely consequence of subsurface convection in early type stars.


1983 ◽  
Vol PER-3 (7) ◽  
pp. 18-18
Author(s):  
Stephen D. Foss ◽  
Sheng H. Lin ◽  
Roosevelt A. Fernandes
Keyword(s):  

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