Thesis (Ph. D.)--Catholic University of America, 1939. / Cover title. From Journal of chemical physics, v. 7, Aug. 1939.

Thesis (Ph. D.)--University of Michigan, 1933. / Cover title. Reprinted from the Physical review, vol. 47, no. 6, March 15, 1935."

Frankfurt (Main), Univ., Diss., 2009

Universiẗat, Diss., 2001--Heidelberg.

Thesis (Ph. D.)--University of Michigan, 1933. / Cover title. Reprinted from the Physical review, vol. 47, no. 6, March 15, 1935."

Universiẗat, Diss., 2001--Stuttgart. / Erscheinungsjahr an der Haupttitelstelle: 2001.

The shape of the Ne.λ6074.3 A° absorption line profile has been investigated using the Zeeman scanning technique. Neon glow discharges at three pressures, 2 Torr, 50 Torr, and 100 Torr, were used as absorbers while a 2 Torr Geissler tube was used as the source. The self-pressure broadening of the observed line was clearly observed and the rate of broadening compares well with theoretical estimates made from the impact theory with a van der Waals interaction assumed. No shift was detected, in contradiction to the theory. This lack of shift, and the rate of pressure broadening observed, were in agreement with the results of Smith (14) regarding the shift and broadening of the Ca.λ6573 A° line by neon. / Science, Faculty of / Physics and Astronomy, Department of / Graduate

Phenology is an integrative science that comprises the study of recurring biological activities or events. In an era of rapidly changing climate, the relationship between the timing of those events and environmental cues such as temperature, snowmelt, water availability, or day length are of particular interest. This article provides an overview of the observer-based plant phenology sampling conducted by the U.S. National Ecological Observatory Network (NEON), the resulting data, and the rationale behind the design. Trained technicians will conduct regular in situ observations of plant phenology at all terrestrial NEON sites for the 30-yr life of the observatory. Standardized and coordinated data across the network of sites can be used to quantify the direction and magnitude of the relationships between phenology and environmental forcings, as well as the degree to which these relationships vary among sites, among species, among phenophases, and through time. Vegetation at NEON sites will also be monitored with tower-based cameras, satellite remote sensing, and annual high-resolution airborne remote sensing. Ground-based measurements can be used to calibrate and improve satellite-derived phenometrics. NEON's phenology monitoring design is complementary to existing phenology research efforts and citizen science initiatives throughout the world and will produce interoperable data. By collocating plant phenology observations with a suite of additional meteorological, biophysical, and ecological measurements (e.g., climate, carbon flux, plant productivity, population dynamics of consumers) at 47 terrestrial sites, the NEON design will enable continental-scale inference about the status, trends, causes, and ecological consequences of phenological change.

This study presents noble gas compositions (He, Ne, Ar, Kr, and Xe) of lavas from several Hawaiian volcanoes. Lavas from the Hawaii Scientific Drilling Project (HSDP) core, surface samples from Mauna Kea, Mauna Loa, Kilauea, Hualalai, Kohala and Haleakala as well as lavas from a deep well on the summit of Kilauea were investigated. Noble gases, especially helium, are used as tracers for mantle reservoirs, based on the assumption that high 3He/4He ratios (>8 RA) represent material from the deep and supposedly less degassed mantle, whereas lower ratios (~ 8 RA) are thought to represent the upper mantle. Shield stage Mauna Kea, Kohala and Kilauea lavas yielded MORB-like to moderately high 3He/4He ratios, while 3He/4He ratios in post-shield stage Haleakala lavas are MORB-like. Few samples show 20Ne/22Ne and 21Ne/22Ne ratios different from the atmospheric values, however, Mauna Kea and Kilauea lavas with excess in mantle Ne agree well with the Loihi-Kilauea line in a neon three-isotope plot, whereas one Kohala sample plots on the MORB correlation line. The values in the 4He/40Ar* (40Ar* denotes radiogenic Ar) versus 4He diagram imply open system fractionation of He from Ar, with a deficiency in 4He. Calculated 4He/40Ar*, 3He/22Nes (22NeS denotes solar Ne) and 4He/21Ne ratios for the sample suite are lower than the respective production and primordial ratios, supporting the observation of a fractionation of He from the heavier noble gases, with a depletion of He with respect to Ne and Ar. The depletion of He is interpreted to be partly due to solubility controlled gas loss during magma ascent. However, the preferential He loss suggests that He is more incompatible than Ne and Ar during magmatic processes. In a binary mixing model, the isotopic He and Ne pattern are best explained by a mixture of a MORB-like end-member with a plume like or primordial end-member with a fractionation in 3He/22Ne, represented by a curve parameter r of 15 (r=(³He/²²Ne)MORB/(³He/²²Ne)PLUME or PRIMORDIAL). Whether the high 3He/4He ratios in Hawaiian lavas are indicative of a primitive component within the Hawaiian plume or are rather a product of the crystal-melt- partitioning behavior during partial melting remains to be resolved. / Ozeaninselbasalte (OIBs), die durch Intraplatten-Vulkane gebildet werden wie z.B. Hawaii, sind geochemisch oft durch variable Isotopensignaturen charakterisiert, die verschiedene Mantelquellen widerspiegeln. Diese Variationen können über kurze Distanzen auf lokalem Maßstab auftreten. Im Rahmen dieser Arbeit wurden Edelgasisotopenzusammensetzungen (He, Ne, Ar, Kr, Xe) verschiedener hawaiianischer Vulkane ermittelt. Bohrkernproben vom Hawaii Scientific Drilling Project (HSDP), Oberflächenproben von den Vulkanen Mauna Kea, Mauna Loa, Kilauea, Hualalai, Kohala und Haleakala, sowie Proben aus einer Bohrung am Gipfel des Kilauea wurden untersucht. Edelgase, insbesondere Helium, dienen als geochemische Tracer. Dies ist auf der Annahme begründet, dass hohe 3He/4He Verhältnisse (> 8 RA) (RA ist das atmosphärische 3He/4He Verhältnis) Material aus dem tiefen Erdmantel repräsentieren, während niedrigere 3He/4He Verhältnisse (~ 8 RA) dem oberen Erdmantel entsprechen. Mauna Kea, Kohala und Kilauea Laven erreichten 3He/4He Verhältnisse zwischen 8 und 18 RA, während Haleakala Laven 3He/4He Verhältnisse von ~ 8 RA nicht überschreiten. Nur wenige Proben zeigten 20Ne/22Ne und 21Ne/22Ne Verhältnisse unterschiedlich vom Luftwert, was auf eine Herkunft aus dem tiefen Erdmantel schließen lässt. Edelgasisotopenwerte weisen auf eine Fraktionierung von He und Ar hin, mit einem Defizit an He. Berechnete 4He/40Ar*, 3He/22Nes (22NeS ist solares Ne) and 4He/21Ne Verhältnisse für die Proben sind niedriger als die entsprechenden Produktions- und primordialen Verhältnisse. Dies unterstützt die Beobachtung einer Fraktionierung von He gegenüber den schwereren Edelgasen, mit einer Verarmung von He gegenüber Ne und Ar. Ein beitragender Faktor bei der He Verarmung ist der löslichkeitskontrollierte Gasverlust während des Magmenaufstiegs. Der bevorzugte Verlust von He lässt jedoch auch darauf schließen, dass He sich bei magmatischen Prozessen inkompatibler verhält als Ne und Ar. Inwiefern die hohen 3He/4He Verhältnisse in hawaiianischen Laven ihren Ursprung in primitiven Komponenten innerhalb des hawaiianischen Plumes haben oder vielmehr in dem Verteilungsverhalten zwischen Mineralphase und Schmelze begründet sind, bleibt zu klären.

[I examensarbetet ingår utställningen "Cavatina":] Cavatina är ett känt musikstycke för gitarr, urspringligen filmusik till filmen "the deer hunter" komponerat av Stanley Myers. I videoinstallationen framförs stycket på klassisk gitarr med chansoperationer, med hjälp av tre tärningar som bestämmer hur strängarna ska stämmas om. Allteftersom stycket spelas förändras musikens karaktär. Teknik: Video Mått/längd på film/video: 19 min.