scholarly journals Biogas Production and Fundamental Mass Transfer Mechanism in Anaerobic Granular Sludge

2019 ◽  
Vol 11 (16) ◽  
pp. 4443 ◽  
Author(s):  
Afridi ◽  
Jing ◽  
Younas

Anaerobic granules are responsible for organic degradation and biogas production in a reactor. The biogas production is entirely dependent on a mass transfer mechanism, but so far, the fundamental understanding remains poor due to the covered surface of the reactor. The study aimed at investigating the fundamental mass transfer characteristics of single anaerobic granules of different sizes using microscopic imaging and analytical monitoring under single and different organic loadings. The experiment was conducted in a micro reactor and mass transfer was calculated using modified Fick’s law. Scanning electron microscopy was applied to observe biogas production zones in the granule, and a lab-scale microscope equipped with a camera revealed the biogas bubble detachment process in the micro reactor for the first time. In this experiment, the granule size was 1.32, 1.47, and 1.75 mm, but 1.75 mm granules were chosen for further investigation due to their large size. The results revealed that biogas production rates for 1.75 mm granules at initial Chemical Oxygen Demand (COD) 586, 1700, and 6700 mg/L were 0.0108, 0.0236, and 0.1007 m3/kg COD, respectively; whereas the mass transfer rates were calculated as 1.83 × 10−12, 5.30 × 10−12, and 2.08 × 10−11 mg/s. It was concluded that higher organic loading and large granules enhance the mass transfer inside the reactor. Thus, large granules should be preferred in the granule-based reactor to enhance biogas production.

Author(s):  
Dapeng Tan ◽  
Lin Li ◽  
Zichao Yin ◽  
Daifeng Li ◽  
Yinlong Zhu ◽  
...  

2012 ◽  
Vol 21 (1-2) ◽  
Author(s):  
S. Mohamed ◽  
Ph. Podsiadlowski

AbstractDetached, symbiotic binaries are generally assumed to interact via Bondi-Hoyle-Littleton (BHL) wind accretion. However, the accretion rates and outflow geometries that result from this mass-transfer mechanism cannot adequately explain the observations of the nearest and best studied symbiotic binary, Mira, or the formation of some post-AGB binaries, e.g. barium stars. We propose a new mass-transfer mode for Mira-type binaries, which we call ‘wind Roche-lobe overflow’ (WRLOF), and which we demonstrate with 3D hydrodynamic simulations. Importantly, we show that the circumstellar outflows which result from WRLOF tend to be highly aspherical and strongly focused towards the binary orbital plane. Furthermore, the subsequent mass-transfer rates are at least an order of magnitude greater than the analogous BHL values. We discuss the implications of these results for the shaping of bipolar (proto)-planetary nebulae and other related systems.


1994 ◽  
Vol 27 (6) ◽  
pp. 755-759
Author(s):  
Takeshi Kataoka ◽  
Akinori Muto ◽  
Tadaaki Nishiki

Author(s):  
Susanta Kumar Das ◽  
Frank Güell ◽  
Hamza Messaoudi ◽  
Martin Bock ◽  
Ruediger Grunwald

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