Process Synthesis Principles in the Chromatographic Separation of Sugars from Biomass Hydrolysates

2011 ◽  
Vol 34 (2) ◽  
pp. 282-288 ◽  
Author(s):  
P. Saari ◽  
M. Hurme
Keyword(s):  
Chromatographic Separation ◽  
Process Synthesis ◽  
Biomass Hydrolysates ◽  
Separation Of Sugars

Study on Industrial Scale Chromatographic Separation Methods of Galactose from Biomass Hydrolysates

2010 ◽  
Vol 33 (1) ◽  
pp. 137-144 ◽  
Author(s):  
P. Saari ◽  
K. Häkkä ◽  
J. Jumppanen ◽  
H. Heikkilä ◽  
M. Hurme
Keyword(s):  
Chromatographic Separation ◽  
Industrial Scale ◽  
Biomass Hydrolysates

Chromatographic Separation of Sugars with Hydrocellulose

1954 ◽  
Vol 26 (2) ◽  
pp. 264-266 ◽  
Author(s):  
J. D. Geerdes ◽  
B. A. Lewis ◽  
Rex. Montgomery ◽  
Fred. Smith
Keyword(s):  
Chromatographic Separation ◽  
Separation Of Sugars

Chromatographic Separation of Sugars on Charcoal1

1950 ◽  
Vol 72 (2) ◽  
pp. 677-679 ◽  
Author(s):  
Roy L. Whistler ◽  
Donald F. Durso
Keyword(s):  
Chromatographic Separation ◽  
Separation Of Sugars

scholarly journals Chromatographic Separation of Sugars. V. Separation of Some Epimeric Heptonolactones.

1966 ◽  
Vol 20 ◽  
pp. 2081-2085 ◽  
Author(s):  
Ove Kjølberg ◽  
Erik Vellan ◽  
Schneur Rachlin ◽  
Egon Pettersson ◽  
Berndt Sjöberg ◽  
...  
Keyword(s):  
Chromatographic Separation ◽  
Separation Of Sugars

scholarly journals Chromatographic Separation of Sugars. VI. A New Route to the Synthesis of Some Uronic Acids.

1972 ◽  
Vol 26 ◽  
pp. 3245-3250 ◽  
Author(s):  
Ove Kjølberg ◽  
Trygve B. Sverreson ◽  
Leif-Åke Smedman ◽  
J. Songstad ◽  
Åke Pilotti
Keyword(s):  
Chromatographic Separation ◽  
Uronic Acids ◽  
Separation Of Sugars

Distribution of R- and S-Process Elements in the Galactic Halo

1988 ◽  
Vol 132 ◽  
pp. 501-506
Author(s):  
C. Sneden ◽  
C. A. Pilachowski ◽  
K. K. Gilroy ◽  
J. J. Cowan
Keyword(s):  
Heavy Element ◽  
Galactic Halo ◽  
Low Noise ◽  
Heavy Elements ◽  
Process Synthesis ◽  
Element Abundances ◽  
Halo Stars ◽  
Abundance Patterns ◽  
R Process ◽  
Process Elements

Current observational results for the abundances of the very heavy elements (Z>30) in Population II halo stars are reviewed. New high resolution, low noise spectra of many of these extremely metal-poor stars reveal general consistency in their overall abundance patterns. Below Galactic metallicities of [Fe/H] Ã −2, all of the very heavy elements were manufactured almost exclusively in r-process synthesis events. However, there is considerable star-to-star scatter in the overall level of very heavy element abundances, indicating the influence of local supernovas on element production in the very early, unmixed Galactic halo. The s-process appears to contribute substantially to stellar abundances only in stars more metal-rich than [Fe/H] Ã −2.

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