Design of equipment for lunar dust removal

NASA has a long range goal of constructing a fully equipped, manned lunar base on the near side of the moon by the year 2015. During the Apollo Missions, lunar dust coated and fouled equipment surfaces and mechanisms exposed to the lunar environment. In addition, the atmosphere and internal surfaces of the lunar excursion module were contaminated by lunar dust which was brought in on articles passed through the airlock. Consequently, the need exists for device or appliance to remove lunar dust from surfaces of material objects used outside of the proposed lunar habitat. Additionally, several concepts were investigated for preventing the accumulation of lunar dust on mechanisms and finished surfaces. The character of the dust and the lunar environment present unique challenges for the removal of contamination from exposed surfaces. In addition to a study of lunar dust adhesion properties, the project examines the use of various energy domains for removing the dust from exposed surfaces. Also, prevention alternatives are examined for systems exposed to lunar dust. A concept utilizing a pressurized gas is presented for dust removal outside of an atmospherically controlled environment. The concept consists of a small astronaut/robotic compatible device which removes dust from contaminated surfaces by a small burst of gas

Equation of state of a granular gas homogeneously driven by particle rotations

We report an experimental study of a dilute "gas" of magnetic particles subjected to a vertical alternating magnetic field in a 3D container. Due to the torque exerted by the field on the magnetic moment of each particle, a spatially homogeneous and chaotic forcing is reached where only rotational motions are driven. This forcing differs significantly from boundary-driven systems used in most previous experimental studies on non equilibrium dissipative granular gases. Here, no cluster formation occurs, and the equation of state displays strong analogy with the usual gas one apart from a geometric factor. Collision statistics is also measured and shows an exponential tail for the particle velocity distribution. Most of these observations are well explained by a simple model which uncovers out-of-equilibrium systems undergoing uniform "heating".Comment: Europhysics Letters (2013) in pres

Chemical element transport in stellar evolution models

Stellar evolution computations provide the foundation of several methods applied to study the evolutionary properties of stars and stellar populations, both Galactic and extragalactic. The accuracy of the results obtained with these techniques is linked to the accuracy of the stellar models, and in this context the correct treatment of the transport of chemical elements is crucial. Unfortunately, in many respects calculations of the evolution of the chemical abundance profiles in stars are still affected by sometime sizable uncertainties. Here, we review the various mechanisms of element transport included in the current generation of stellar evolution calculations, how they are implemented, the free parameters and uncertainties involved, the impact on the models, and the observational constraints.Comment: 72 pages, 33 figures, invited review paper to be published in Royal Society Open Science Journa

Plasmonic Metamaterials: Physical Background and Some Technological Applications

New technological frontiers appear every year, and few are as intriguing as the field of plasmonic metamaterials (PMMs). These uniquely designed materials use coherent electron oscillations to accomplish an astonishing array of tasks, and they present diverse opportunities in many scientific fields. This paper consists of an explanation of the scientific background of PMMs and some technological applications of these fascinating materials. The physics section addresses the foundational concepts necessary to understand the operation of PMMs, while the technology section addresses various applications, like precise biological and chemical sensors, cloaking devices for several frequency ranges, nanoscale photovoltaics, experimental optical computing components, and superlenses that can surpass the diffraction limit of conventional optics

Dissipation in ferrofluids: Mesoscopic versus hydrodynamic theory

Part of the field dependent dissipation in ferrofluids occurs due to the rotational motion of the ferromagnetic grains relative to the viscous flow of the carrier fluid. The classical theoretical description due to Shliomis uses a mesoscopic treatment of the particle motion to derive a relaxation equation for the non-equilibrium part of the magnetization. Complementary, the hydrodynamic approach of Liu involves only macroscopic quantities and results in dissipative Maxwell equations for the magnetic fields in the ferrofluid. Different stress tensors and constitutive equations lead to deviating theoretical predictions in those situations, where the magnetic relaxation processes cannot be considered instantaneous on the hydrodynamic time scale. We quantify these differences for two situations of experimental relevance namely a resting fluid in an oscillating oblique field and the damping of parametrically excited surface waves. The possibilities of an experimental differentiation between the two theoretical approaches is discussed.Comment: 14 pages, 2 figures, to appear in PR

The Giant Flare of 1998 August 27 from SGR 1900+14: II. Radiative Mechanism and Physical Constraints on the Source

(ABBREVIATED) The extraordinary 1998 August 27 giant flare places strong constraints on the physical properties of its source, SGR 1900+14. We make detailed comparisons of the published data with the magnetar model. The giant flare evolved through three stages, whose radiative mechanisms we address in turn. A triggering mechanism is proposed, whereby a helical distortion of the core magnetic field induces large-scale fracturing in the crust and a twisting deformation of the crust and exterior magnetic field. The envelope of the pulsating tail of the August 27 flare can be accurately fit, after ~40 s, by the contracting surface of a relativistically hot, but inhomogeneous, trapped fireball. We quantify the effects of direct neutrino-pair emission, thereby deducing a lower bound ~ 10^{32} G-cm^3 to the magnetic moment of the confining field. The radiative flux during the intermediate ~40 s of the burst appears to exceed the trapped fireball fit. The spectrum and lightcurve of this smooth tail are consistent with heating in an extended pair corona, possibly powered by continuing seismic activity in the star. We consider in detail the critical luminosity, below which a stable balance can be maintained between heating and radiative cooling in a confined, magnetized pair plasma; but above which the confined plasma runs away to local thermodynamic equilibrium. In the later pulsating tail, the best fit temperature equilibrates at a value which agrees well with the regulating effect of photon splitting. The remarkable four-peaked substructure within each 5.16-s pulse provides strong evidence for the presence of higher magnetic multipoles in SGR 1900+14. The corresponding collimation of the X-ray flux is related to radiative transport in a super-QED magnetic field.Comment: 11 July 2001, accepted for publication in the Astrophysical Journa

A centrifugal microfluidic platform for capturing, assaying and manipulation of beads and biological cells

Microfluidics is deemed a field with great opportunities, especially for applications in medical diagnostics. The vision is to miniaturize processes typically performed in a central clinical lab into small, simple to use devices - so called lab-on-a-chip (LOC) systems. A wide variety of concepts for liquid actuation have been developed, including pressure driven flow, electro-osmotic actuation or capillary driven methods. This work is based on the centrifugal platform (lab-on-a-disc). Fluid actuation is performed by the forces induced due to the rotation of the disc, thus eliminating the need for external pumps since only a spindle motor is necessary to rotate the disc and propel the liquids inside of the micro structures. Lab-on-a-disc systems are especially promising for point-of-care applications involving particles or cells due to the centrifugal force present in a rotating system. Capturing, assaying and identification of biological cells and microparticles are important operations for lab-on-a-disc platforms, and the focus of this work is to provide novel building blocks towards an integrated system for cell and particle based assays. As a main outcome of my work, a novel particle capturing and manipulation scheme on a centrifugal microfluidic platform has been developed. To capture particles (biological cells or micro-beads) I designed an array of V-shaped micro cups and characterized it. Particles sediment under stagnant flow conditions into the array where they are then mechanically trapped in spatially well-defined locations. Due to the absence of flow during the capturing process, i.e. particle sedimentation is driven by the artificial gravity field on the centrifugal platform, the capture efficiency of this approach is close to 100% which is notably higher than values reported for typical pressure driven systems. After capturing the particles, the surrounding medium can easily be exchanged to expose them to various conditions such as staining solutions or washing buffers, and thus perform assays on the captured particles. By scale matching the size of the capturing elements to the size of the particles, sharply peaked single occupancy can be achieved. Since all particles are arrayed in the same focal plane in spatially well defined locations, operations such as counting or fluorescent detection can be performed easily. The application of this platform to perform multiplexed bead-based immunoassays as well as the discrimination of various cell types based on intra cellular and membrane based markers using fluorescently tagged antibodies is demonstrated. Additionally, methods to manipulate captured particles either in batch mode or on an individual particle level have been developed and characterized. Batch release of captured particles is performed by a novel magnetic actuator which is solely controlled by the rotation frequency of the disc. Furthermore, the application of this actuator to rapidly mix liquids is shown. Manipulation of individual particles is performed using an optical tweezers setup which has been developed as part of this work. Additionally, this optical module also provides fluorescence detection capabilities. This is the first time that optical tweezers have been combined with a centrifugal microfluidic system. This work presents the core technology for an integrated centrifugal platform to perform cell and particle based assays for fundamental research as well as for point-of- care applications. The key outputs of my specific work are: 1. Design, fabrication and characterization of a novel particle capturing scheme on a centrifugal microfluidic platform (V-cups) with very high capture efficiency (close to 100%) and sharply peaked single occupancy (up to 99.7% single occupancy). 2. A novel rotation frequency controlled magnetic actuator for releasing captured particles as well as for rapidly mixing liquids has been developed, manufactured and characterized. 3. The V-cup platform has successfully been employed to capture cells and perform multi-step antibody staining assays for cell discrimination. 4. An optical tweezers setup has been built and integrated into a centrifugal teststand, and successful manipulation of individual particles trapped in the V-cup array is demonstrated