515 research outputs found
Emission Spectroscopy and Radiometric Measurements in the NASA Ames IHF Arc Jet Facility
Plasma diagnostic measurement campaigns in the NASA Ames Interaction Heating Facility (IHF) have been conducted over the last several years with a view towards characterizing the flow in the arc jet facility by providing data necessary for modeling and simulation. Optical emission spectroscopy has been used in the plenum and in the free jet of the nozzle. Radiation incident over a probe surface has also been measured using radiometry. Plenum measurements have shown distinct radial profiles of temperature over a range of operating conditions. For cases where large amounts of cold air are added radially to the main arc-heated stream, the temperature profiles are higher by as much as 1500 K than the profiles assumed in flow simulations. Optical measurements perpendicular to the flow direction in the free jet showed significant contributions to the molecule emission through inverse pre-dissociation, thus allowing determination of atom number densities from molecular emission. This has been preliminarily demonstrated with the N2 1st Positive System. Despite the use of older rate coefficients, the resulting atom densities are reasonable and surprisingly close to flow predictions
Regularization strategy for the layered inversion of airborne TEM data: application to VTEM data acquired over the basin of Franceville (Gabon)
Airborne transient electromagnetic (TEM) is a cost-effective method to image
the distribution of electrical conductivity in the ground. We consider layered
earth inversion to interpret large data sets of hundreds of kilometre.
Different strategies can be used to solve this inverse problem. This consists
in managing the a priori information to avoid the mathematical instability and
provide the most plausible model of conductivity in depth. In order to obtain
fast and realistic inversion program, we tested three kinds of regularization:
two are based on standard Tikhonov procedure which consist in minimizing not
only the data misfit function but a balanced optimization function with
additional terms constraining the lateral and the vertical smoothness of the
conductivity; another kind of regularization is based on reducing the condition
number of the kernel by changing the layout of layers before minimizing the
data misfit function. Finally, in order to get a more realistic distribution of
conductivity, notably by removing negative conductivity values, we suggest an
additional recursive filter based upon the inversion of the logarithm of the
conductivity. All these methods are tested on synthetic and real data sets.
Synthetic data have been calculated by 2.5D modelling; they are used to
demonstrate that these methods provide equivalent quality in terms of data
misfit and accuracy of the resulting image; the limit essentially comes on
special targets with sharp 2D geometries. The real data case is from
Helicopter-borne TEM data acquired in the basin of Franceville (Gabon) where
borehole conductivity loggings are used to show the good accuracy of the
inverted models in most areas, and some biased depths in areas where strong
lateral changes may occur
The Ames Vertical Gun Range
The Ames Vertical Gun Range (AVGR) is a national facility for conducting laboratory- scale investigations of high-speed impact processes. It provides a set of light-gas, powder, and compressed gas guns capable of accelerating projectiles to speeds up to 7 km s(exp -1). The AVGR has a unique capability to vary the angle between the projectile-launch and gravity vectors between 0 and 90 deg. The target resides in a large chamber (diameter approximately 2.5 m) that can be held at vacuum or filled with an experiment-specific atmosphere. The chamber provides a number of viewing ports and feed-throughs for data, power, and fluids. Impacts are observed via high-speed digital cameras along with investigation-specific instrumentation, such as spectrometers. Use of the range is available via grant proposals through any Planetary Science Research Program element of the NASA Research Opportunities in Space and Earth Sciences (ROSES) calls. Exploratory experiments (one to two days) are additionally possible in order to develop a new proposal
Emission Spectroscopic Measurements with an Optical Probe in the NASA Ames IHF Arc Jet Facility
An optical probe was designed to measure radiation (from inside the arc heater) incident on a test sample immersed in the arc-heated stream. Currently, only crude estimates are available for this incident radiation. Unlike efforts of the past, where the probe line of sight was inclined to the nozzle centerline, the present development focuses on having the probe line of sight coincide with the nozzle centerline. A fiber-coupled spectrometer was used to measure the spectral distribution of incident radiation in the wavelength range of 225 to 900 nm. The radiation heat flux in this wavelength range was determined by integration of measured emission spectral intensity calibrated to incident irradiance from an integrating sphere. Two arc-heater conditions, corresponding to stream bulk enthalpy levels of 12 and 22 MJ/kg, were investigated in the 13-inch diameter nozzle of the Interaction Heating Facility at NASA Ames Research Center. With the probe placed at a distance of 10 inches from the nozzle exit plane, total radiative heat fluxes were measured to be 3.3 and 8.4 W/sq cm for the 12 and 22 MJ/kg conditions, respectively. About 17% of these radiative fluxes were due to bound-bound radiation from atoms and molecules, while the remaining 83% could be attributed to continua (bound-free and/or free-free). A comparison with spectral simulation based on CFD solutions for the arc-heater flow field and with spectroscopic measurements in the plenum region indicates that more than 95% of the measured radiation is generated in the arc region. The total radiative heat flux from the line radiation could increase by a factor of two through contributions from wavelengths outside the measured range, i.e., from the vacuum ultraviolet (wavelengths less than 225 nm) and the infrared (wavelengths greater than 900 nm). An extrapolation of the continuum radiation to these two wavelength regions was not attempted. In the tested configuration, the measured radiative heat flux accounts for only about 1.4% of the nominal heat flux on a flat face model and therefore is considered negligible. In the 6-inch diameter nozzle, on account of shorter path lengths, the radiation heat flux could be significant. Therefore, future tests in the 6-inch nozzle will have radiometers in addition to the optical probe
Alien Registration- Raiche, Marie T. (Lewiston, Androscoggin County)
https://digitalmaine.com/alien_docs/27502/thumbnail.jp
Monitoring Temperature in High Enthalpy Arc-heated Plasma Flows using Tunable Diode Laser Absorption Spectroscopy
A tunable diode laser sensor was designed for in situ monitoring of temperature in the arc heater of the NASA Ames IHF arcjet facility (60 MW). An external cavity diode laser was used to generate light at 777.2 nm and laser absorption used to monitor the population of electronically excited oxygen atoms in an air plasma flow. Under the assumption of thermochemical equilibrium, time-resolved temperature measurements were obtained on four lines-of-sight, which enabled evaluation of the temperature uniformity in the plasma column for different arcjet operating conditions
Alien Registration- Raiche, Paul A. (Lewiston, Androscoggin County)
https://digitalmaine.com/alien_docs/27503/thumbnail.jp
Carbon Atom, Dimer and Trimer Chemistry on Diamond Surfaces from Molecular Dynamics Simulations
Spectroscopic studies of various atmospheres appearing in diamond film synthesis suggest evidence for carbon atoms, dimers, or trimers. Molecular dynamics simulations with the Brenner hydrocarbon potential are being used to investigate the elementary reactions of these species on a hydrogen-terminated diamond (111) surface. In principle these types of simulations can be extended to simulations of growth morphologies, in the 1-2 monolayer regime presently
A Silent Conversation
I’ve always thought that, as human beings, we have a special connection to textile. It’s the first thing we touch when we’re born except the skin of another human being. We are almost always in contact with it, either to protect ourselves from the elements or because of our social constructs that says we need to hide certain parts of our bodies. It seems to be metaphorical to say that it’s a second skin, but that’s literally what it is if you think that we are the only animal to use the skin of another animal to cover our body 2 It is part of our language with all of its metaphors; part of every rituals from birth to death; part of every moment of our lives. So much so that we don’t realize it, we don’t notice it anymore. It’s part of us
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