scholarly journals Monitoring thermal field, humidity field and energy balance over heterogeneous surfaces in the typical valley-city

2020 ◽  
Vol 30 (12) ◽  
pp. 2015-2032
Author(s):  
Guodong Li ◽  
Junhua Zhang ◽  
Parham A. Mirzaei ◽  
Shengyan Ding ◽  
Yapeng Ding ◽  
...  
Author(s):  
Lubica Bednarova ◽  
Lukáš Tóth ◽  
Tomáš Brestovič ◽  
Natália Jasminská ◽  
Marián Lázár ◽  
...  

The present article deals with the material and energy balance of a fuel cell during hydrogen supply from a metal hydride tank. It describes potential utilisation of heat from a fuel cell for heating a tank in order to achieve the required kinetics of the process. The concluding part hereof contains a numerical calculation of the thermal field of the designed tank during the fuel cell operation.


2013 ◽  
Vol 33 (12) ◽  
pp. 3792-3804
Author(s):  
李国栋 LI Guodong ◽  
张俊华 ZHANG Junhua ◽  
王乃昂 WANG Naiang ◽  
彭剑峰 PENG Jianfeng ◽  
程弘毅 CHENG Hongyi

2014 ◽  
Vol 50 (S1) ◽  
pp. 553-565 ◽  
Author(s):  
Soojin Kim ◽  
Young-Hee Lee ◽  
Kyu Rang Kim ◽  
Young-San Park

1994 ◽  
Vol 144 ◽  
pp. 315-321 ◽  
Author(s):  
M. G. Rovira ◽  
J. M. Fontenla ◽  
J.-C. Vial ◽  
P. Gouttebroze

AbstractWe have improved previous model calculations of the prominence-corona transition region including the effect of the ambipolar diffusion in the statistical equilibrium and energy balance equations. We show its influence on the different parameters that characterize the resulting prominence theoretical structure. We take into account the effect of the partial frequency redistribution (PRD) in the line profiles and total intensities calculations.


1977 ◽  
Vol 36 ◽  
pp. 143-180 ◽  
Author(s):  
J.O. Stenflo

It is well-known that solar activity is basically caused by the Interaction of magnetic fields with convection and solar rotation, resulting in a great variety of dynamic phenomena, like flares, surges, sunspots, prominences, etc. Many conferences have been devoted to solar activity, including the role of magnetic fields. Similar attention has not been paid to the role of magnetic fields for the overall dynamics and energy balance of the solar atmosphere, related to the general problem of chromospheric and coronal heating. To penetrate this problem we have to focus our attention more on the physical conditions in the ‘quiet’ regions than on the conspicuous phenomena in active regions.


1989 ◽  
Vol 50 (C8) ◽  
pp. C8-9-C8-14
Author(s):  
H. J. KREUSER ◽  
L. C. WANG

Author(s):  
B Otto ◽  
H Rochlitz ◽  
M Möhlig ◽  
L Burget ◽  
J Kampe ◽  
...  
Keyword(s):  

2005 ◽  
Vol 43 (10) ◽  
Author(s):  
B Otto ◽  
F Lippl ◽  
P Pfluger ◽  
J Spranger ◽  
U Cuntz ◽  
...  
Keyword(s):  

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