Effect of Shielding Gases in Laser Welding of Aluminium Alloys

High reflectivity to laser light, alloying element evaporation during high power laser welding makes aluminium alloys highly susceptibility to weld defects such as porosity, cracking and undercutting. The dynamic behaviour of the keyhole, due to fluctuating plasma above the keyhole and the vaporization ofthe alloying elements with in the keyhole, is the key problem to be solved for the improvement of the weld quality and stabilization of the keyhole dynamics isperhaps the single most important development that can broaden the application of laser welding of aluminium alloys. In laser welding, the shielding gas is commonly used to stabilize the welding process, to improve the welded joint features and to protect the welded seam from oxidation. The chemicalcomposition of the shielding gas is a key factor in achieving the final qualityof the welded joints. Wide range of shielding gases varying from the pure gasesto complex mixtures based on helium, argon, nitrogen and carbon dioxide are commercially available. These gas mixtures should be considered in terms of their suitability during laser welding of aluminium alloys to produce quality welds. The main objective of the present work is to study the effect of the shielding gascomposition during laser welding of aluminium alloys. Aluminium alloy A15754 was welded using 3kW Nd-YAG laser (continuous wave mode). The alloy samples were butt welded with different shielding gases (pure and mixture of gases) so that high quality welds with high joint efficiencies could be produced. It was observed that the chemical composition of the gases influenced the final weld quality and properties. In general, the mixture gases, in correct proportions, enabled better utilisation of the properties of the mixing gases, stabilized the welding process and produced better weld quality compared to the pure shielding gases.

Studies on the Multifaceted Interaction of Atoms and an Electromagnetic Field

In this Thesis the interaction of an electromagnetic field and matter is studied from various aspects in the general framework of cold atoms. Our subjects cover a wide spectrum of phenomena ranging from semiclassical few-level models to fully quantum mechanical interaction with structured reservoirs leading to non-Markovian open quantum system dynamics. Within closed quantum systems, we propose a selective method to manipulate the motional state of atoms in a time-dependent double-well potential and interpret the method in terms of adiabatic processes. Also, we derive a simple wave-packet model, based on distributions of generalized eigenstates, explaining the finite visibility of interference in overlapping continuous-wave atom lasers. In the context of open quantum systems, we develop an unraveling of non-Markovian dynamics in terms of piecewise deterministic quantum jump processes confined in the Hilbert space of the reduced system - the non-Markovian quantum jump method. As examples, we apply it for simple 2- and 3-level systems interacting with a structured reservoir. Also, in the context of ion-cavity QED we study the entanglement generation based on collective Dicke modes in experimentally realistic conditions including photonic losses and an atomic spontaneous decay.

The effect of focal point parameters in fiber laser welding of structural steel

In this thesis the effect of focal point parameters in fiber laser welding of structural steel is studied. The goal is to establish relations between laser power, focal point diameter and focal point position with the resulting quality, weld-bead geometry and hardness of the welds. In the laboratory experiments, AB AH36 shipbuilding steel was welded in an I-butt joint configuration using IPG YLS-10000 continuous wave fiber laser. The quality of the welds produced were evaluated based on standard SFS-EN ISO 13919-1. The weld-bead geometry was defined from the weld cross-sections and Vickers hardness test was used to measure hardness's from the middle of the cross-sections. It was shown that all the studied focal point parameters have an effect on the quality, weld-bead geometry and hardness of the welds produced.

Inverkan av indirekt rekombination på fotoinducerad absorption

I organiska halvledare påverkas mängden laddningsbärare kraftigt av indirekt rekombination, det vill säga processen då fria laddningsbärare försvinner genom att kombineras med orörliga laddningsbärare av motsatt laddning. De orörliga laddningsbärarna uppstår när laddningsbärare fastnar i fällor, som är energitillstånd med låg energi och densitet. Utöver indirekt rekombination sker även direkt rekombination mellan fria laddningsbärare. Då man tillverkar solceller av organiska halvledare påverkas effektiviteten av energidistributionen och rekombinationsprocesserna i materialen. Utveckling av olika metoder för undersökning av dessa egenskaper är således till nytta i jakten på bättre solcellsmaterial. Målet med detta arbete var att vidareutveckla dataanalysen för cwPA-mätningar(från engelska continuous-wave Photoinduced Absorption) för att ur resultaten få information om indirekt rekombination och fälldistributioner. I cwPA-mätningar studerar man fotoinducerad absorption, det vill säga förändringen i absorption hos ett prov då densiteten av fotogenererade laddningsbärare varierar. Laddningsbärarna genereras av ett pumpljus vars intensitet ges av en fyrkantsvåg som växlar mellan 0 och I med vinkelfrekvensen omega. Resultaten fås i form av i-fas-signal (PAI), som har samma frekvens och fas som pumpljuset, och kvadratur (PAQ), som har samma frekvens som pumpljuset men är fasförskjuten 90 grader. Fördelen med denna mätning är förutom känsligheten att den är kontaktlös, vilket gör att den visar egenskaperna hos det undersökta materialet utan att påverkas av elektriska kontakter. För att undersöka inverkan av indirekt rekombination på cwPA-mätningar simulerades mätresultat genom att använda numeriska beräkningar. Grunden för simuleringarna var att lösa differentialekvationer för densiteter av laddningsbärare i olika tillstånd. Beräkningarna använde en modell med transporttillstånd och fällor placerade så att energidistributionen var symmetrisk för elektroner och hål. Modellen antog att laddningsbärare inte kunde röra sig direkt mellan fällor utan endast via transporttillstånd. Från simuleringarna erhölls användbara samband mellan fotoinducerad absorption och olika fälldistributioner. Särskilt påverkade distributionerna i-fas-signalen för hög intensitet på pumpljuset och kvadraturen för låg frekvens på fyrkantsvågen. För en exponentiell fälldistribution hittades samband mellan mätresultat och distributionens karakteristiska energi (Ech) i förhållande till temperaturen (T). Dessa är för hög intensitet PAI~I^(1+Ech/kT) och för låg frekvens PAQ~omega^(kT/Ech). Resultaten visade att man kan skilja på en exponentiell fälldistribution, en gaussisk fälldistribution och ett system som domineras av direkt rekombination genom att göra cwPA-mätningar vid olika temperaturer.

Studies of Solar Activity with Emphasis on Quasi-Periodic Oscillations

In this thesis mainly long quasi-periodic solar oscillations in various solar atmospheric structures are discussed, based on data obtained at several wavelengths, focussing, however, mainly on radio frequencies. Sunspot (Articles II and III) and quiet Sun area (QSA) (Article I) oscillations are investigated along with quasi-periodic pulsations (QPP) in a flaring event with wide-range radio spectra (Article IV). Various oscillation periods are detected; 3–15, 35–70 and 90 minutes (QSA), 10-60 and 80-130 minutes (in sunspots at various radio frequencies), 3-5, 10-23, 220-240, 340 and 470 minutes (in sunspots at photosphere) and 8-12 and 15-17 seconds (in a solar flare at radio frequencies). Some of the oscillation periods are detected for the first time, while some of them have been confirmed earlier by other research groups. Solar oscillations can provide more information on the nature of various solar structures. This thesis presents the physical mechanisms of some solar structure oscillations. Two different theoretical approaches are chosen; magnetohydrodynamics (MHD) and the shallow sunspot model. These two theories can explain a wide range of solar oscillations from a few seconds up to some hours. Various wave modes in loop structures cause solar oscillations (<45 minutes) both in sunspots and quiet Sun areas. Periods lasting more than 45 minutes in the sunspots (and a fraction of the shorter periods) are related to sunspot oscillations as a whole. Sometimes similar oscillation periods are detected both in sunspot area variations and respectively in magnetic field strength changes. This result supports a concept that these oscillations are related to sunspot oscillations as a whole. In addition, a theory behind QPPs at radio frequencies in solar flares is presented. The thesis also covers solar instrumentation and data sources. Additionally, the data processing methods are presented. As the majority of the investigations in this thesis focus on radio frequencies, also the most typical radio emission mechanisms are presented. The main structures of the Sun, which are related to solar oscillations, are also presented. Two separate projects are included in this thesis. Solar cyclicity is studied using the extensively large solar radio map archieve from Metsähovi Radio Observatory (MRO) at 37 GHz, between 1978 and 2011 (Article V) covering two full solar cycles. Also, some new solar instrumentation (Article VI) was developed during this thesis.