TWRS phase 1 infrastructure project (W-519) characterization

Abstract

environmental samples collected for the TWRS (W-519) Infrastructure Characterization effort in and around the 200 East Area. w Soil, Augering, Characterization, Samples, W-519, This document provides a detailed description of the TRADEMARK DISCLAIMER. Reference herein to any specific comnercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recmndation, or favoring by the united States Government or any agency thereof or its contractors or subcontractors.

Biodegradation of Aliphatic Homopolyesters and Aliphatic−Aromatic Copolyesters by Anaerobic Microorganisms

“…Obviously, glucose suppresses the PHB depolymerizing enzyme secretion, probably by catabolite repression. 40,42 It is known for clostridia that easily degradable substrates might mask abilities for biosynthesis and biodegradation and hence extracellular enzymes of polymeric substrates. 40,42 It is assumed that the presence of glucose as a growth substrate results in what is known as inducer (3-hydroxybutyrate) expulsion as has been observed for other clostridia.…”

“…40,42 It is known for clostridia that easily degradable substrates might mask abilities for biosynthesis and biodegradation and hence extracellular enzymes of polymeric substrates. 40,42 It is assumed that the presence of glucose as a growth substrate results in what is known as inducer (3-hydroxybutyrate) expulsion as has been observed for other clostridia. 42,43 Accordingly, the PHB depolymerizing enzyme is not induced and PHB is not degraded.…”

“…40,42 It is assumed that the presence of glucose as a growth substrate results in what is known as inducer (3-hydroxybutyrate) expulsion as has been observed for other clostridia. 42,43 Accordingly, the PHB depolymerizing enzyme is not induced and PHB is not degraded.…”

Astro Particle Physics from Space

“…Often, however, simpler apparatus were used, based on calorimeters, emulsion chambers or Cerenkov detectors: in these cases only partial information were obtained. Until recently the most sophisticated CR spectrometers were flown on balloons operating between 30 and 35 km of height (BESS [3], MASS [4], CAPRICE [5], IMAX [6]) but in 1998 a large magnetic spectrometer, AMS [7], has been operated in space, providing for the first time a very precise measurement on the composition of primary CR before their entrance in the atmosphere. Fig.…”