Thesis (M.S.)--University of Wisconsin--Madison, 1969. / eContent provider-neutral record in process. Description based on print version record. Includes bibliographical references.

Thesis (Ph. D.)--University of Wisconsin--Madison, 1957. / Typescript. Vita. eContent provider-neutral record in process. Description based on print version record. Includes bibliographical references (leaves 289-291).

Typescript, etc.

Typescript, etc.

Ice cream has been defined as » frozen dairy-product, with or without natural flavoring, containing sugar, and a specified amount of butter fat as required by the laws or regulations of the various states and the Federal government. Ordinarily ice cream consists of cream, sugar, flavoring, and some stabilizer which is usually gelatin. These are the principal ingredients, but rich cream may be thinned by the addition of skim milk, or skim-milk powder may be added, to build up the solid s-not- fat and thus improve the body. Ice cream is truly a frozen dairy-product, although other products than cream may enter into its makeup. The different ingredients that enter into an ice cream mix exist in different grades, concentrations and forms. It is desirable, therefore, in order to obtain constructive data, to follow a logical approach which would be to study first, simple isolated portions of the system m that is, the different types of dispersed phases in the dispersion medium taken singly - and then the effects of the combinations of such systems, gradually increasing the complexity.

No description available.

Cheuk Yeuk Pik. / Summary in Chinese. / Thesis (M.B.A.)--Chinese University of Hong Kong. / Bibliography: leaf 49.

The objective of this study was to investigate the potential application of rice bran wax (RBW) organogel to replace solid fat content and create the fat network in ice cream. Ice creams with 10% fat or 15% fat were formulated with RBW organogel as the fat source, and two different emulsifiers were used: polmo, a commercial blend of emulsifiers which contains 80% mono- and diglycerides and 20% polysorbate 80, and Glycerol monooleate (GMO). Candelilla wax (CDW) organogel and carnauba wax (CBW) organogel were also tested for comparison. RBW organogel had the ability to form and sustain structure in 15% fat ice creams when GMO was used as the emulsifier. Transmission electron microscopy revealed that the RBW crystal morphology within the fat droplet, when GMO was used as the emulsifier, was characterized by the growth of crystals at the outer edge of the droplet which increased fat destabilization and network formation. / Nestlé Product Technology Centre, France

Le rayonnement cosmique galactique nucléaire est composé de noyaux de différentes espèces et ses sources sont encore mal identifiées. Cette méconnaissance est en partie due au caractère diffusif de la propagation des noyaux dans les champs magnétiques dont la composante turbulente supprime toute information sur la position des sources. Dans le rayonnement cosmique, on distingue les noyaux pri- maires qui sont principalement créés puis accélérés près de leurs sources des noyaux secondaires, uniquement créés par spallation des primaires plus lourds. La mesure des rapports d'abondance se- condaire sur primaire permet d'étudier les processus de propagation et donc de remonter aux méca- nisme sources du rayonnement cosmique. Cette étude apporte de plus une meilleure compréhension de l'environnement astrophysique galactique. Ce travail nécessite une très bonne connaissance des sections efficaces d'interaction du rayonnement cosmique dans le milieu interstellaire qui régissent la modification des abondances lors de la propagation. La première partie de cette thèse est dédiée à la contrainte des paramètres de propagation du rayonnement cosmique galactique via l'étude des abondances des éléments du quartet (1H,2H,3He,4He). À partir d'une nouvelle estimation des sections efficaces, une analyse statistique a permis de démontrer le potentiel de ces éléments pour contraindre les modèles de propagation du rayonnement cosmique. Ces contraintes restent cependant limitées par la précision statistique des mesures actuelles et justifient la mise en œuvre de nouvelles expériences. La deuxième partie de cette thèse est dédiée à la mesure des abondances avec l'expérience CREAM, une expérience embarquée en ballon. Cette mesure nécessite l'identification des éléments dans le dé- tecteur, le calcul des efficacités des sous-détecteurs, la déconvolution des effets dus aux erreurs sur la mesure de l'énergie ainsi que la prise en compte des effets atmosphériques. Cette analyse des données du 3ième vol de CREAM a permis une estimation des abondances des éléments bore, carbone, azote et oxygène. / The sources of Galactic cosmic-ray (GCR) nuclei are still poorly identified. This is partly due to the diffusive propagation (in turbulent magnetic fields) that erases all directional information about the measured fluxes. The species that are predominantly created and accelerated in the sources are denoted 'primary species'. Those mostly created by spallation of heavier primary species are denoted 'secondary species'. While primary fluxes give access to the source parameters, secondary-to-primary ratios trace propagation processes. Key quantities for such studies are the fragmentation cross sections on the interstellar gas and the measured fluxes and ratios. In the first part of this thesis, we provide new constraints on the Galactic propagation parameters from the quartet elements (1H,2H,3He,4He), relying on a new estimate of their cross sections and an evolved statistical analysis. The derived constraints are competitive with those obtained from the standard B/C ratio analysis. The results are however limited by the precision of current measurements and motivate the development of new experiments. The second part of this thesis is dedicated to the analysis of cosmic-ray fluxes measured with the CREAM balloon-borne experiment. We present the particle identification in the detector, the estimation of efficiencies for each sub-detector, the energy reconstruction, and the atmospheric correction. Applied to the 3rd flight data (CREAM-III), we provide new data points for the boron, carbon, nitrogen and oxygen elements above 100 GeV/n.

Thesis (M.Sc.) -- University of Western Sydney, Hawkesbury, 1997. / Includes bibliographical references (leaves 143-152).