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An application of thermogravimetry to quantitative studies ... - Springer link.springer.com/article/10.1007/BF01905171Private View Thermogravimetry is a fast, accurate and highly sensitive method for the quantitative determination of halloysite, kaolinite and gibbsite in ∼10 mg altered feldspar grains from lateritic saprolite materials. A wide range in composition occurs between grains, and is evidence of the existence of various geochemical microenvironments within lateritic saprolite. Variations in dehydroxylation ...
Diffusion of antioxidants in sheets and plates of isotactic ... - Springer link.springer.com/article/10.1007/BF01904450Private View The diffusion of the phenolic antioxidant 1, 3, 5-tris (3,5-ditert. butyl-4-hydroxybenzyl)mesitylene (IRGANOX 1330) in compressed sheets of isotactic polypropylene (iPP) was investigated over the temperature range from 80°C to 120°C by isothermal differential-thermal-analysis (DTA).The measurements showed a clear relation between oxidation induction time and oxidation maximum time, (both ...
The collisions of two plasma streams - Springer link.springer.com/article/10.1007/BF01557098Private View The mutual interaction of two colliding plasma streams is investigated by means of the perturbation method. The disordered random motions of electrons are taken into account. It is shown that electron oscillations occur only when certain conditions as to the density and relative velocity of the colliding streams are fulfilled. The order of magnitude of the thickness of the shock generated by ...
UBL · Международная логистика и импорт товаров в Россию ubl.com.ruPrivate View Отправ л яя запрос, вы сог л ашаетесь на обработку персона л ьных данных в соответствии с федера л ьным законом „О персона л ьных данных“ от 27.07.2006 №152-ФЗ. UBL не предостав л яет третьим л ицам персона л ьные данные л иц ...
Considerations about telescopes for infra red astronomy - Springer link.springer.com/article/10.1007/BF02743514Private View The choice of a telescope which may be used for groundbased infra-red observations is discussed. A number of facts suggests that two types of telescopes may be used: a smallF number, low-opticaltolerance telescope in the near infra-red (up to 3.5 fjt.m) and in far infrared (beyond 300 (xm); a largeF number, high-optical-requirement telescope in the intermediate infra-red. The efficiency of ...