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May 23, 2011
05/11
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Linsky, Jeffrey L.; Diplas, Athanassios; Wood, Brian E.; Brown, Alexander; Ayres, Thomas R.; Savage, Blair D
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We present Goddard High-Resolution Spectrograph observations of the interstellar H I and D I Ly-alpha lines and the Mg II and Fe II resonance lines formed along the lines of sight toward the nearby stars Procyon (3.5 pc, l = 214 deg, b = 13 deg) and Capella (12.5 pc, l = 163 deg, b = 5 deg). New observations of Capella were obtained at orbital phase 0.80, when the radial velocities of the intrinsic Ly-alpha emission lines of each star were nearly reversed from those of the previous observations...
Topics: BOW WAVES, THICKNESS, GAS DYNAMICS, MAGNETOSHEATH, SHOCK WAVES, MAGNETOHYDRODYNAMICS, PREDICTIONS,...
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142
May 23, 2011
05/11
by
Bangalore, A.; Phaengsook, N.; Sankar, L. N
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A 3-D compressible Navier-Stokes solver has been developed and applied to 3-D viscous flow over clean and iced wings. This method uses a third order accurate finite volume scheme with flux difference splitting to model the inviscid fluxes, and second order accurate symmetric differences to model the viscous terms. The effects of turbulence are modeled using a Kappa-epsilon model. In the vicinity of the sold walls the kappa and epsilon values are modeled using Gorski's algebraic model. Sampling...
Topics: ELECTRIC FIELDS, PREDICTIONS, LANGMUIR TURBULENCE, SOLAR PLANETARY INTERACTIONS, SHOCK WAVES,...
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197
May 23, 2011
05/11
by
Nieuwejaar, Nils; Kotz, Davi
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As the I/O needs of parallel scientific applications increase, file systems for multiprocessors are being designed to provide applications with parallel access to multiple disks. Many parallel file systems present applications with a conventional Unix-like interface that allows the application to access multiple disks transparently. The interface conceals the parallelism within the file system, which increases the ease of programmability, but makes it difficult or impossible for sophisticated...
Topics: GEOMAGNETISM, MAGNETIC DISTURBANCES, SOLAR WIND, PERIODIC VARIATIONS, SOLAR PLANETARY INTERACTIONS,...
The international space science community had recognized the importance of space weather more than a decade ago, which resulted in a number of international collaborative activities such as the Climate and Weather of the Sun Earth System (CAWSES) by SCOSTEP and the International Space Weather Initiative (ISWI). The ISWI program is a continuation of the successful International Heliophysical Year (IHY) program. These programs have brought scientists together to tackle the scientific issues...
Topics: NASA Technical Reports Server (NTRS), SPACE WEATHER, SUN, INTERNATIONAL COOPERATION, SOLAR...
416
416
May 23, 2011
05/11
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Breininger, D. R.; Larson, V. L.; Schaub, R.; Duncan, B. W.; Schmalzer, P. A.; Oddy, D. M.; Smith, R. B.; Adrian, F.; Hill, H., Jr
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The Florida Scrub-Jay (Aphelocoma coerulescens) is an indicator of ecosystem integrity of Florida scrub, an endangered ecosystem that requires frequent fire. One of the largest populations of this federally threatened species occurs on John F. Kennedy Space Center/Merritt Island National Wildlife Refuge. Population trends were predicted using population modeling and field data on reproduction and survival of Florida Scrub-Jays collected from 1988 - 1995. Analyses of historical photography...
Topics: AURORAL ZONES, HARMONICS, SOLAR ACTIVITY, SOLAR PLANETARY INTERACTIONS, CYCLOTRON RADIATION,...
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285
May 21, 2011
05/11
by
Bansal, Narottam P
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Tantalum oxide gels in the form of transparent monoliths and powder were prepared from hydrolysis of tantalum pentaethoxide under controlled conditions using different mole ratios of Ta(OC2H5)5:C2H50H:H20:HCl. Alcohol acts as the mutual solvent and HCl as the deflocculating agent. For a fixed alkoxide:water:HCl ratio, time of gel formation increased with the alcohol to alkoxide mole ratio. Thermal evolution of the physical and structural changes in the gel was monitored by differential thermal...
Topics: AERONOMY, ATMOSPHERIC HEATING, PARTICLE PRECIPITATION, PLANETARY MAGNETOTAILS, ATMOSPHERIC...
I will describe a three-dimensional magnetohydrodynamic model of the solar wind that takes into account turbulent heating of the wind by velocity and magnetic fluctuations as well as a variety of effects produced by interstellar pickup protons. The interstellar pickup protons are treated in the model as one fluid and the protons and electrons are treated together as a second fluid. The model equations include a Reynolds decomposition of the plasma velocity and magnetic field into mean and...
Topics: NASA Technical Reports Server (NTRS), MAGNETOHYDRODYNAMICS, SIMULATION, SOLAR WIND, TURBULENCE...
This document lists the scientific accomplishments of the Orbiter Electron Temperature Probe (OETP) group. The OETP instrument was fabricated in 1976, integrated into the PVO spacecraft in 1977, and placed in orbit about Venus in December 1978. The instrument operated flawlessly for nearly 14 years until PVO was lost as it entered the Venusian atmosphere in October 1992. The OETP group worked closely with other PVO investigators to examine the Venus ionosphere and its interactions with the...
Topics: NASA Technical Reports Server (NTRS), ELECTRON ENERGY, PIONEER VENUS 1 SPACECRAFT, PLANETARY...
Planetary science deals with a wide variety of natural materials in a wide variety of environments. These materials include metals, minerals, ices, gases, plasmas, and organic chemicals. In addition, the newly defined discipline of astrobiology introduces biological materials to planetary science. The environments range from the interiors of planets with megapascal pressures to planetary magnetospheres, encompassing planetary mantles, surfaces, atmospheres, and ionospheres. The interplanetary...
Topics: NASA Technical Reports Server (NTRS), PLANETARY GEOLOGY, ASTROPHYSICS, SOLAR SYSTEM, PLANETARY...
This is the final summary report by Resource Management Associates, Inc., of the first year's work under Contract No. NASW-4011 to the National Aeronautics and Space Administration. The work under this initial phase of the contract relates to the preliminary development of a global, 3-D magnetohydrodynamic computational model to quantitatively describe the detailed continuum field and plasma interaction process of the solar wind with cometary and planetary bodies throughout the solar system....
Topics: NASA Technical Reports Server (NTRS), COMETS, MATHEMATICAL MODELS, SOLAR PLANETARY INTERACTIONS,...
The superrotation of the venusian atmosphere relative to the planet's surface has long been known. Yet the process by which this vigorous circulation is maintained is poorly understood. The purpose of this report is to show that a mechanism by which the solar radiation interacts with the cloudy atmosphere of Venus could be the principle cause of the superrotation. It has been long known that Venus has a high albedo due to the scattering (similar to the reflection process) of solar radiation by...
Topics: NASA Technical Reports Server (NTRS), ATMOSPHERIC CIRCULATION, MOMENTUM TRANSFER, RADIATION...
We often look "through a glass, darkly" at solar system bodies with tenuous atmospheres and direct surface exposure to the local space environment. Space weathering exposure acts via universal space-surface interaction processes to produce a thin patina of outer material covering, potentially obscuring endogenic surface materials of greatest interest for understanding origins and interior evolution. Examples of obscuring exogenic layers are radiation crusts on cometary nuclei and...
Topics: NASA Technical Reports Server (NTRS), SPACE WEATHER, SPACE WEATHERING, SURFACE REACTIONS,...
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343
May 23, 2011
05/11
by
Kondoleon, Anthony S.; Kelleher, William P.; Possel, Peter D
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Magnetic bearings, unlike traditional mechanical bearings, consist of a series of components mated together to form a stabilized system. The correct design of the actuator and sensor will provide a cost effective device with low power requirements. The proper choice of a control system utilizes the variables necessary to control the system in an efficient manner. The specific application will determine the optimum design of the magnetic bearing system including the touch down bearing. Draper...
Topics: PLANETARY IONOSPHERES, MARS ATMOSPHERE, PLANETARY MAGNETIC FIELDS, GAS GIANT PLANETS, NATURAL...
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234
May 23, 2011
05/11
by
Devasia, Santos
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The research work has advanced the inversion-based guidance theory for: systems with non-hyperbolic internal dynamics; systems with parameter jumps; and systems where a redesign of the output trajectory is desired. A technique to achieve output tracking for nonminimum phase linear systems with non-hyperbolic and near non-hyperbolic internal dynamics was developed. This approach integrated stable inversion techniques, that achieve exact-tracking, with approximation techniques, that modify the...
Topics: INTERPLANETARY MAGNETIC FIELDS, THREE DIMENSIONAL MODELS, MAGNETIC EFFECTS, PLANETARY MAGNETOTAILS,...
A magnetohydrodynamic (MHD) theory is developed for the standoff distance a(s) of the bow shock and the thickness Delta(ms) of the magnetosheath, using the empirical Spreiter et al. relation Delta(ms) = kX and the MHD density ratio X across the shock. The theory includes as special cases the well-known gasdynamic theory and associated phenomenological MHD-like models for Delta(ms) and As. In general, however, MHD effects produce major differences from previous models, especially at low Alfev...
Topics: NASA Technical Reports Server (NTRS), BOW WAVES, MAGNETOSHEATH, SHOCK WAVES, MAGNETOHYDRODYNAMICS,...
A selected set of planetocentric latitudes is used in calculations of the seasonal solar radiation pattern incident on top of the Jovian atmosphere, thereby demonstrating the combined effect of solar distance and declination. Attention is given to hemispheric asymmetries in the Jovian atmosphere's average zonal winds and cloud system morphologies. Marked hemispheric asymmetries are noted in the cloud morphology and in the magnitude and latitudinal position of eastward and westward maxima in the...
Topics: NASA Technical Reports Server (NTRS), INCIDENT RADIATION, JUPITER ATMOSPHERE, SOLAR PLANETARY...
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243
May 23, 2011
05/11
by
NagarajaRao, C. R.; Chen, J
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The post-launch degradation of the visible (channel 1: 0.58- 068 microns) and near-infrared (channel 2: approx. 0.72 - l.l microns) channels of the Advanced Very High Resolution Radiometer (AVHRR) on the NOAA-7, -9, and -11 Polar-orbiting Operational Environmental Satellites (POES) was estimated using the south-eastern part of the Libyan Desert as a radiometrically stable calibration target. The relative annual degradation rates, in per cent, for the two channels are, respectively: 3.6 and 4.3...
Topics: ATMOSPHERIC PHYSICS, COMPLEX SYSTEMS, GALAXIES, PREDICTIONS, RESEARCH FACILITIES, RESEARCH...
In May 1996 the electrical power on Pioneer 10 was no longer adequate to support the Cosmic Ray Telescope Experiment (CRT). In March 1997 ground based operations for the mission were terminated. The 25 years of Pioneer 10 were a remarkable voyage of discovery as it ventured into a vast new unexplored region of space. These observations by the Pioneer experiments led in the development of a new discipline of space science - heliospheric physics. For cosmic ray studies it was an incredible era,...
Topics: NASA Technical Reports Server (NTRS), HELIOSPHERE, PIONEER 10 SPACE PROBE, SOLAR ACTIVITY, SOLAR...
I develop and document a set of procedures which test the quality of predictions of solar wind speed and polarity of the interplanetary magnetic field (IMF) made by coupled models of the ambient solar corona and heliosphere. The Wang-Sheeley-Arge (WSA) model is used to illustrate the application of these validation procedures. I present an algorithm which detects transitions of the solar wind from slow to high speed. I also present an algorithm which processes the measured polarity of the...
Topics: NASA Technical Reports Server (NTRS), ALGORITHMS, INTERPLANETARY MAGNETIC FIELDS, POLARITY, SOLAR...
217
217
May 23, 2011
05/11
by
Mineck, Raymond E.; Hartwich, Peter M
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A test was conducted on a model of the NACA 0012 airfoil section with a solid upper surface or a porous upper surface with a cavity beneath for passive venting. The purposes of the test were to investigate the aerodynamic characteristics of an airfoil with full-chord porosity and to assess the ability of porosity to provide a multipoint or self-adaptive design. The tests were conducted in the Langley 8-Foot Transonic Pressure Tunnel over a Mach number range from 0.50 to 0.82 at chord Reynolds...
Topics: BOW WAVES, OXYGEN IONS, INTERPLANETARY MAGNETIC FIELDS, SHOCK WAVES, PLANETARY MAGNETOSPHERES,...
Maximum electric fields of Langmuir waves at planetary foreshocks are estimated from the threshold for electrostatic decay, assuming it saturates beam driven growth, and incorporating heliospheric variation of plasma density and temperature. Comparisons with spacecraft observations yields good quantitative agreement. Observations in type 3 radio sources are also in accord with this interpretation. A single mechanism can thus account for the highest fields of beam driven waves in both contexts.
Topics: NASA Technical Reports Server (NTRS), ELECTRIC FIELDS, LANGMUIR TURBULENCE, SOLAR PLANETARY...
The investigations undertaken in this report relate to studies of various solar wind interaction phenomena with Venus, Earth, Mars, Jupiter and Saturn. A computational model is developed for the determination of the detailed plasma and magnetic field properties associated with various planetary obstacles throughout the solar system.
Topics: NASA Technical Reports Server (NTRS), MAGNETIC FIELDS, MAGNETOHYDRODYNAMICS, PLANETARY...
Continuing efforts have been made towards an increased understanding of the solar wind interaction and ionospheric processes at Venus and Mars. This work centered on a systematic development of a new generation of three dimensional magnetohydrodynamic (MHD) numerical code, which models the interaction processes of the solar wind with non-magnetic planets, such as Venus and Mars. We have also worked on a number of different, more specific and discrete studies, as various opportunities arose. We...
Topics: NASA Technical Reports Server (NTRS), SOLAR WIND, THREE DIMENSIONAL MODELS, PLANETARY IONOSPHERES,...
The overall objective of this research program is to better understand the interaction of a magnetized solar wind with the Venus atmosphere through the use of numerical solutions of the time-dependent, 2-D and 3-D magnetohydrodynamic (MHD) equations. Due to the more modest CPU requirements for the 2-D simulations, they were used for studies in which useful information not dependent on the third dimension could be obtained. The 2-D simulations served several purposes in addition to providing...
Topics: NASA Technical Reports Server (NTRS), MAGNETIC EFFECTS, MAGNETOHYDRODYNAMICS, PLANETARY MAGNETIC...
In a previous study, Knudsen et al. suggested that Venus has a weak internal magnetic dipole field of the order of 7 x 10 + 20 G cm(exp -3) that is manifested in the form of magnetic flux tubes threading the ionospheric holes in the Venus nightside ionosphere. They pointed out that any internal field of Venus, dipole or multipole, would be weakened in the subsolar region and concentrated in the antisolar region of the planet by the supersonic transterminator convection of the dayside ionosphere...
Topics: NASA Technical Reports Server (NTRS), INTERPLANETARY MAGNETIC FIELDS, MAGNETIC FIELD RECONNECTION,...
The atmospheres of planetary bodies without significant intrinsic magnetic fields exhibit unique features because they interact with the external plasma flows in their space environment. The plasma interactions also have the potential of altering the evolutionary paths of these atmospheres since the processes (such as ion pickup and sputtering) that lead to loss of constituents have effects unlike those of other escape mechanisms. This ongoing investigation has been concentrating on the...
Topics: NASA Technical Reports Server (NTRS), PLANETARY ATMOSPHERES, PLANETARY MAGNETIC FIELDS, PLASMAS...
Recent observations show an approximately 1.3-year period in the speed of the solar wind detected by the IMP 8 and Voyager 2 spacecraft. A similar period is also seen in the north-south (GSE) component of the magnetic field observed by IMP 8. Since both parameters are commonly used as input to models of geomagnetic activity, the 'ap' index (a measure of geomagnetic disturbance) is examined to look for this periodicity. The Lomb-Scargle periodogram method is used on the ap, plasma, and magnetic...
Topics: NASA Technical Reports Server (NTRS), GEOMAGNETISM, MAGNETIC DISTURBANCES, SOLAR WIND, PERIODIC...
315
315
May 27, 2011
05/11
by
Howes, Walton L
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Similarity relations for frequency pass band, as well as overall, time average pressure fluctuations outside a jet are derived and tested using experimental data. Similarity of the pressure fields was found for different jet velocities. Nozzle contour dissimilarity and differing jet temperatures were found to limit seriously the application of the similarity relations, especially near the jet nozzle.
Topics: SOLAR WIND, CONTROLLED FUSION, ELECTRONS, HEATING, MORPHOLOGY, PLASMA INTERACTIONS, PLASMA PHYSICS,...
Voyager spacecraft radio, interplanetary plasma, and interplanetary magnetic field data are used to show that large amplitude fluctuations in the power generated by the Saturn kilometric radio emission are best correlated with solar wind ram pressure variation. In all, thirteen solar wind quantities previously found important in driving terrestrial magnetospheric substorms and other auroral processes were examined for evidence of correlations with the Saturn radio emission. The results are...
Topics: NASA Technical Reports Server (NTRS), KILOMETRIC WAVES, PLANETARY RADIATION, RADIO EMISSION, SATURN...
This report by the Committee on Solar and Space Physics and the Committee on Solar-Terrestrial Research recommends the major directions for scientific research in space physics for the coming decade. As a field of science, space physics has passed through the stage of simply looking to see what is out beyond Earth's atmosphere. It has become a 'hard' science, focusing on understanding the fundamental interactions between charged particles, electromagnetic fields, and gases in the natural...
Topics: NASA Technical Reports Server (NTRS), ATMOSPHERIC PHYSICS, ELECTROMAGNETIC FIELDS, HELIOSPHERE,...
This investigation concentrated on the question of how atmosphere escape, related to both photochemistry and the Mars solar wind interaction, may have affected the evolution of Mars' atmosphere over time. The principal investigator and postdoctoral researcher adopted the premise that contemporary escape processes have dominated the losses to space over the past 3.5 billion years, but that the associated loss rates have been modified by solar evolution. A model was constructed for the...
Topics: NASA Technical Reports Server (NTRS), MARS ATMOSPHERE, PHOTOCHEMICAL REACTIONS, PLANETARY...
A detailed study of the magnetic field data from both Voyagers 1 and 2 has revealed several interesting properties of the near and distant Jovian magnetotail. During the first encounter, as Voyager 1 passed between 80 and 140 R sub J from Jupiter in the near tail, the spacecraft was almost entirely in the northerm lobe magnetic field. The frequency spectrum of magnetic fluctuation in this region cannot be characterized by a power law and does not appear to be turbulent. The distant tail spectra...
Topics: NASA Technical Reports Server (NTRS), GEOMAGNETIC TAIL, JUPITER (PLANET), PLANETARY MAGNETIC...
This is the final report summarizing the work done during the last three years under NASA Grant NAG5-8946. Our efforts centered on a systematic development of a new generation of three dimensional magneto-hydrodynamic (MHD) numerical code, which models the interaction processes of the solar wind or fast flowing magnetospheric plasma with 'non-magnetic' solar system bodies (e.g. Venus, Mars, Europa, Titan). We have also worked on a number of different, more specific and discrete studies, as...
Topics: NASA Technical Reports Server (NTRS), SOLAR WIND, MAGNETOHYDRODYNAMICS, MODELS, PLANETARY...
Progress is reported in the development of a global, 3-D magnetohydrodynamic computational model to quantitatively describe the detailed continuum field and plasma interaction process of the solar wind with cometary and planetary magneto/ionopause shapes. Activities described include enhancements to the present Level 1 model, development of the 3-D gas dynamic flow field solvers for the Level 2 model, and continued development of the 3-D frozen magnetic field solver for the Level 2 model.
Topics: NASA Technical Reports Server (NTRS), COMETARY ATMOSPHERES, COMPUTATIONAL ASTROPHYSICS,...
During the years 2000-2011 the radio instruments onboard Cassini, Wind and STEREO spacecraft have Recorded a large amount of the Jovian decametric radio emission (DAM). In this paper we report on the analysis of the new type of Jovian periodic radio bursts recently revealed in the decametric frequency range. These bursts, which are non-Io component of DAM, are characterized by a strong periodic reoccurrence over several Jovian days with a period approx. = 1:5% longer than the rotation rate of...
Topics: NASA Technical Reports Server (NTRS), RADIO BURSTS, RADIO EMISSION, JUPITER (PLANET), IO, PLANETARY...
The primary objective of this research program is to improve our understanding of the physical processes occurring in the interaction of the solar wind with Venus. This will be accomplished through the use of numerical solutions of the two- and three-dimensional magnetohydrodynamic (MHD) equations and through comparisons of the computed results with available observations. A large portion of this effort involves the study of processes due to the presence of the magnetic field and the effects of...
Topics: NASA Technical Reports Server (NTRS), INTERPLANETARY MAGNETIC FIELDS, VENUS (PLANET),...
Global mean temperatures near 273 K on early Mars are difficult to explain in the context of standards solar evolution models. Even assuming maximum CO2 greenhouse warming, the required flux is approximately 15 percent too low. Here we consider two astrophysical models that could increase the flux by this amount. The first model is a nonstandard solar model in which the early Sun had a mass somewhat greater than today's mass (1.02-1.06 solar mass). The second model is based on a standard...
Topics: NASA Technical Reports Server (NTRS), MARS ENVIRONMENT, PLANETARY TEMPERATURE, SOLAR FLUX, SOLAR...
Atmospheric observations reported on include recent measurements of thermospherical composition, gas temperatures, auroral emissions, ion-neutral collisional coupling, electric fields, and plasma convection. Theoretical studies reported on include model calculations of thermospherical general circulation, thermospheric tides, thermospheric tidal coupling to the lower atmosphere, interactions between thermospheic chemistry and dynamics and thermosphere-ionosphere coupling processes. The...
Topics: NASA Technical Reports Server (NTRS), ATMOSPHERIC COMPOSITION, AURORAL ZONES, CONVECTIVE FLOW,...
The Pioneer Venus Orbiter (PVO) mission has played a key role in establishing the nature of the solar wind interaction with Venus. Although earlier probes had determined that Venus presented an obstacle much smaller than the size of earth's magnetosphere to the solar wind, they did not carry out in situ measurements pertaining to solar wind interaction studies at low enough altitudes to determine why. They also did not provide datasets of sufficient duration to study the variability of the...
Topics: NASA Technical Reports Server (NTRS), PLANETARY MAGNETIC FIELDS, PLANETARY MAGNETOSPHERES, PLASMA...
Analysis and interpretation of data from the Orbiter Retarding Potential Analyzer (ORPA) onboard the Pioneer Venus Orbiter is reported. By comparing ORPA data to proton data from the Orbiter Plasma Analyzer (OPA), it was found that the ORPA suprathermal electron densities taken outside the Venusian ionopause represent solar wind electron densities, thus allowing the high resolution study of Venus bow shocks using both magnetic field and solar wind electron data. A preliminary analysis of 366...
Topics: NASA Technical Reports Server (NTRS), BOW WAVES, PLANETARY MAGNETOSPHERES, PIONEER VENUS 1...
It has long been recognized that solar wind bombardment onto exposed surfaces in the solar system will produce an energetic component to the exospheres about those bodies. Laboratory experiments have shown that there is no increase in the sputtering yield caused by highly charged heavy ions for metallic and for semiconducting surfaces, but the sputter yield can be noticeably increased in the case of a good insulating surface. Recently measurements of the solar wind composition have become...
Topics: NASA Technical Reports Server (NTRS), ENERGETIC PARTICLES, SOLAR WIND, SPUTTERING, SOLAR PLANETARY...
In this paper the response of the heliospheric termination shock to an incident interplanetary shock is examined. This paper is an extension of a recent study by Barnes (1993), which treated the analogous problem for an incident contact discontinuity. The termination shock is treated as a strong gas-dynamic shock. The post-interaction configuration consists of a moving termination shock, a postshock contact discontinuity, and either a shock or rarefaction wave propagating the disturbance signal...
Topics: NASA Technical Reports Server (NTRS), SHOCK WAVES, HELIOSPHERE, ELASTIC WAVES, SHOCK DISCONTINUITY,...
A three-dimensional code for a rapidly rotating magnetosphere in which the MHD equations and the Maxwell equations were solved by using the two step Lax Endroff scheme, was developed. Preliminary results were presented at the Fall AGU meeting in San Francisco. The basic simulation model to study the solar wind interactions was adapted to other bodies in addition to Jupiter. Because of the recent comet flybys, a comet was chosen as the first model. The aim was to model the formation of the...
Topics: NASA Technical Reports Server (NTRS), ASTRONOMICAL MODELS, BOW WAVES, COMETARY MAGNETOSPHERES,...
The Cold War's end opened an opportunity for greater cooperation in planetary exploration for the United States and Russia. Two study groups were formed, Mars Together and FIRE and ICE. The Mars Together team developed a concept for a flight in 1998 that merged one U.S. Mars Surveyor 98 mission with the former Russian Mars 96 mission to further understanding of the Mars surface and atmosphere. The FIRE and ICE team developed concepts for a dual-spacecraft mission to the solar corona and for a...
Topics: NASA Technical Reports Server (NTRS), INTERNATIONAL COOPERATION, MARS (PLANET), MARS EXPLORATION,...
The quadrennium 1975-1978 was a period of great advance for solar-wind studies, a period that combined exploration of new regions with increased maturity in established fields of study. The Helios, Pioneer, and Voyager spacecraft have been exploring the inner and outer regions of the solar wind. There has been a rebirth of the study of possible relations between solar variability and Earth's climate and weather, stimulated largely by Eddy's investigation of the Maunder Minimum; the solar wind...
Topics: NASA Technical Reports Server (NTRS), SOLAR WIND, CLIMATE, WEATHER, CORONAL HOLES, INTERPLANETARY...
Long latitude distributions of atmospheric neutral hydrogen were derived at Venus for the period 1979 to 1980. In-situ measurements of H+, O+, O, and CO2 obtained from the ion and neutral mass spectrometers on the Pioneer Venus orbiter are combined with the appropriate chemical equilibrium relationship to determine the abundance of neutral hydrogen which is very difficult to measure directly. The measurements are all obtained below 165 km on the nightside and below 200 km on the dayside, based...
Topics: NASA Technical Reports Server (NTRS), ATMOSPHERIC COMPOSITION, ATMOSPHERIC DENSITY, MAGNETIC...
A suborbital experiment was designed to study the photochemistry of the mesosphere by observing simultaneously the airglow emissions with in-situ minor species number density profiles. The experiment was very successful and some preliminary results have already been reported in various scientific meetings. Two scientific papers are currently in the process of final preparation for submission for publication. In this final project report, we will first give a background description of the...
Topics: NASA Technical Reports Server (NTRS), ATMOSPHERIC COMPOSITION, ATMOSPHERIC DENSITY, ATMOSPHERIC...
Our understanding of planetary ionospheres made some progress during the last four years. Most of this progress was due to new and/or improved theoretical models, although some new data were also obtained by direct and remote sensing observations. The very basic processes such as ionization, chemical transformations and diffusive as well as convective transports are analogous in all ionospheres; the major differences are the result of factors such as different neutral atmospheres, intrinsic...
Topics: NASA Technical Reports Server (NTRS), PLANETARY IONOSPHERES, COMETARY ATMOSPHERES, SPACE PLASMAS,...
Solar wind plasma parameters and the Interplanetary Magnetic Field (IMF) observed by the WIND spacecraft upstream of the bow shock were used as input to magnetohydrodynamic (MHD) simulations of two substorm events. The power deposited into the ionosphere due to electron precipitation was calculated both from VIS observations and from the simulations.
Topics: NASA Technical Reports Server (NTRS), MAGNETOHYDRODYNAMICS, PLASMAS (PHYSICS), COMPUTERIZED...
Pioneer 10 Plasma Analyzer experiment flight data during the Jupiter flyby are presented. The observations show that the interaction of Jupiter's magnetic field with the solar wind is similar in many ways to that at earth, but the scale size is over 100 times larger. Jupiter is found to have a detached standing bow shock wave of high Alfven Mach number. Jupiter has a prominent magnetopause which deflects the magnetosheath plasma and excludes its direct entry into the Jovian magnetosphere. The...
Topics: NASA Technical Reports Server (NTRS), JUPITER (PLANET), PIONEER 10 SPACE PROBE, PLANETARY...
