78
78
Jun 26, 2019
06/19
by
Brandt, John C
texts
eye 78
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xii, 199 p.: 25 cm. -
Topic: Solar wind
8
8.0
Jan 17, 2020
01/20
by
Jet Propulsion Laboratory Conference on the Solar Wind (1964 : Pasadena, Calif.)
texts
eye 8
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xxx, 400 pages 24 cm
Topics: Solar wind -- Congresses, 39.54 interplanetary matter, Solar wind, Zonnewind
7
7.0
Jul 19, 2021
07/21
by
Hundhausen, A. J., 1936-
texts
eye 7
favorite 0
comment 0
xii, 238 p. 24 cm
Topics: Solar wind, Sun -- Corona
248
248
May 6, 2010
05/10
by
Spreiter, J. R.; Summers, A. L
texts
eye 248
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Effect of external pressure and oblique incidence of solar wind on terminal shape of geomagnetic field
Topics: GEOMAGNETISM, PRESSURE EFFECTS, SHAPES, SOLAR WIND, GEOMAGNETIC FIELD, PRESSURE, SOLAR WIND
255
255
Jul 11, 2010
07/10
by
Dowson, D.; Hamrock, B. J
texts
eye 255
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The elastic deformation of two ellipsoidal solids in contact and subjected to a Hertzian stress distribution was evaluated numerically as part of a general study of the elastic deformation of such solids in elastohydrodynamic contacts. In the analysis the contact zone is divided into equal rectangular areas and it is assumed that a uniform pressure is applied over each rectangular area. A study was made of the influence on the size of the rectangular area upon accuracy. The results also...
Topics: CONFERENCES, SOLAR WIND, SOLAR PHYSICS
Solar Wind is a Los Angeles based band, whose primary musical focus is instrumental Contemporary Jazz. Other Musical influences such as NAC (New Adult Contemporary), New Age and Fusion, blend to make Solar Wind's sound the essence of Smooth Jazz. Solar Wind is headed by bassist Sean Mason, whose clean, technical style creates a unique approach in this genre. The debut CD, "Grand Tour Alignment", was produced by Sean, and co-produced by guitarist Eric Robson. Mason's electric bass is...
Topic: Solar Wind featuring Sean Mason
34
34
Sep 22, 2020
09/20
by
Meyer-Vernet, Nicole
texts
eye 34
favorite 1
comment 0
1 online resource (xiv, 463 pages) :
Topics: Solar wind -- Mathematics, SCIENCE -- Astronomy
154
154
Oct 29, 2009
10/09
by
NASA/Goddard Space Flight Center Scientific Visualization Studio
movies
eye 154
favorite 1
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This series of animations shows a two-dimensional unstructured mesh particle-magnetohydrodynamic solar wind flow simulation of the interaction of the solar wind with the Earth's magnetosphere. Note: Magnetic field lines superimposed over density for a 2D simulation of the solar wind-magnetosphere interaction. Animator: Liam Krauss (Hughes STX), Andy Acuna (Hughes STX). Scientist: F. Kazeminezhad (NASA/GSFC), Steve Zalesak (NASA/GSFC), Dan Spicer (NASA/GSFC).
Topic: Magnetohydrodynamics, Solar Wind, Space science
Source: http://svs.gsfc.nasa.gov/goto?87
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7.0
texts
eye 7
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295 p. : 28 cm
Topics: Solar wind, Space plasmas, Magnetosphere
273
273
May 6, 2010
05/10
by
Axford, W. I
texts
eye 273
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Magnetic storm energy from viscous interaction between solar wind & earth magnetosphere
Topics: EARTH MAGNETOSPHERE, MAGNETIC PROPERTIES, MAGNETIC STORMS, SOLAR WIND, MAGNETIC STORM,...
377
377
May 6, 2010
05/10
by
Ken Knight, C. E.; Rosenberg, D. L.; Wehner, G. K
texts
eye 377
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comment 0
Simulation of the effect of solar wind bombardment on the lunar surface
Topics: CEMENTATION, LEVELING, LUNAR SURFACE, SIMULATION, SOLAR WIND, SPUTTERING, LUNAR SURFACE,...
225
225
May 6, 2010
05/10
by
Hurley, J
texts
eye 225
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comment 0
Solar wind-geomagnetic field interaction
Topics: GEOMAGNETISM, MAGNETIC PROPERTIES, PENETRATION, SOLAR MAGNETIC FIELD, SOLAR WIND, GEOMAGNETIC...
260
260
Jun 19, 2010
06/10
by
Hirshberg, J
texts
eye 260
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comment 0
No Abstract Available
Topics: M REGION, MAGNETIC STORMS, SOLAR WIND
47
47
Oct 2, 2020
10/20
by
Lockheed Martin
movies
eye 47
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An overview of the Sun's magnetic structures and emissions. Lockheed Martin production #97-33 This NTSC VHS copy is from the personal collection of solar physicist Ted Speiser (1934–2016). It was digitized to Lagarith AVI and transcoded to H.264 MP4 in 2020.
Topics: solar science, solar flares, solar wind
854
854
May 23, 2011
05/11
by
NON
texts
eye 854
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comment 0
Individual papers presented at the conference address the following topics: development of a micro-fiber nickel electrode for nickel-hydrogen cell, high performance nickel electrodes for space power application, bending properties of nickel electrodes for nickel-hydrogen batteries, effect of KOH concentration and anions on the performance of a Ni-H2 battery positive plate, advanced dependent pressure vessel nickel hydrogen spacecraft cell and battery design, electrolyte management...
Topics: POTENTIAL FLOW, HELIOSPHERE, SOLAR WIND, SHOCK WAVES, MAGNETIC FLUX, BOUNDARY CONDITIONS,...
17
17
texts
eye 17
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comment 0
x, 526 p. : 24 cm
Topics: Solar magnetic field, Solar radiation, Solar wind
5
5.0
Sep 10, 2021
09/21
by
Skylab Solar Workshop (1st : 1975-1976 : Boulder, Colo.)
texts
eye 5
favorite 0
comment 0
xii, 454 p. : 24 cm
Topics: Coronal holes (Astronomy) -- Congresses, Solar wind -- Congresses
204
204
Jun 18, 2010
06/10
by
Myers, M. A.; Silva, R. W.; Wolfe, J. H
texts
eye 204
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Solar wind properties observed during flight of IMP-I /Explorer XVIII satellite/
Topics: EXPLORER SATELLITES, EXPLORER 18 SATELLITE, EXPLORER 43 SATELLITE, IMP, SOLAR WIND, EXPLORER XVIII...
280
280
Sep 10, 2010
09/10
by
NASA/JSC
movies
eye 280
favorite 5
comment 0
Weather just does not happen; it is caused. This film describes all three weather scales - the microphysical (tiny particles), middle (front and cells), and global (layers of atmosphere) - that are interrelated in a total system. One of the benefits of the Space Shuttle is the opportunity to test these conditions in zero-g. In addition, the solar wind can be observed and tested from a more advantageous position.
Topics: weather, solar wind, Sapce Shuttle, NASA, JSC
21
21
Dec 5, 2019
12/19
by
Hunter, Nick
texts
eye 21
favorite 0
comment 0
32 pages : 23 cm
Topics: Astronomy, Solar wind -- Juvenile literature, Auroras -- Juvenile literature, Auroras, Magnetic...
10
10.0
Apr 4, 2021
04/21
by
Ken (unknownhand)
data
eye 10
favorite 0
comment 0
Ever play Solar Winds? Well, growing up it was one of my favorite games so I decided to remake what I would think my ship would look like if I could own one. Another cool thing for my desk I guess:). This thing was made with Tinkercad. Edit it online https://tinkercad.com/things/eYuzC7bQf3l
Topics: thingiverse, Vehicles, game, explore, space, stl, solar_wind
3
3.0
Oct 29, 2021
10/21
by
International Astronomical Union. Symposium (142nd : 1989 : Bangalore, India)
texts
eye 3
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comment 0
xi, 540 p. : 25 cm
Topics: Solar wind -- Congresses, Space plasmas -- Congresses, Astrophysics -- Congresses
197
197
May 23, 2011
05/11
by
Nieuwejaar, Nils; Kotz, Davi
texts
eye 197
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comment 0
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,...
121
121
Oct 6, 2020
10/20
by
NOAA
movies
eye 121
favorite 4
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NOAA scientists explain solar disturbances and space weather forecasting techniques. Interviewees include NOAA researchers Gary Heckman, Patrick S. McIntosh, and Ronald D. Zwickl. Sound: narration, interviews, field recording (NOAA offices), and brief analogue synthesizer music. This NTSC VHS dub is from the personal collection of solar physicist Ted Speiser (1934–2016). It was digitized to Lagarith AVI and transcoded to H.264 MP4 in 2020.
Topics: solar wind, solar flares, aurora, solar disturbances, space weather
105
105
Oct 29, 2009
10/09
by
NASA/Goddard Space Flight Center Scientific Visualization Studio
movies
eye 105
favorite 0
comment 0
This series of animations shows a two-dimensional unstructured mesh particle-magnetohydrodynamic solar wind flow simulation of the interaction of the solar wind with the Earth's magnetosphere. Note: Contour lines of the z-component of the magnetic potential for a 2D simulation of the solar wind-magnetosphere interaction. Animator: Liam Krauss (Hughes STX), Andy Acuna (Hughes STX). Scientist: F. Kazeminezhad (NASA/GSFC), Steve Zalesak (NASA/GSFC), Dan Spicer (NASA/GSFC).
Topics: Magnetohydrodynamics, Solar Wind, Space science, What -- CONTOUR, What -- Earth
Source: http://svs.gsfc.nasa.gov/goto?86
401
401
Feb 8, 2011
02/11
by
NASA; Langley Research Center
movies
eye 401
favorite 0
comment 0
What is the Aurora Borealis?
Topics: NASA, KSNN, Solar Wind, Charged Particles, Gas, Television, TV
23
23
Nov 7, 2018
11/18
by
Hartquist, T. W
texts
eye 23
favorite 1
comment 0
1 online resource (x, 167 pages) :
Topics: Solar wind, Astrophysical jets, Stars, New, SCIENCE -- Physics -- Astrophysics
Mendeley Climate Change Library
243
243
Jul 6, 2019
07/19
by
B. M. Jakosky; D. Brain; M. Chaffin; S. Curry; J. Deighan; J. Grebowsky; J. Halekas; F. Leblanc; R. Lillis; J. G. Luhmann; L. Andersson; N. Andre; D. Andrews; D. Baird; D. Baker; J. Bell
texts
eye 243
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Observations of the Mars upper atmosphere made from the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft have been used to determine the loss rates of gas from the upper atmosphere to space for a complete Mars year (16 Nov 2014 – 3 Oct 2016). Loss rates for H and O are sufficient to remove ∼2–3 kg/s to space. By itself, this loss would be significant over the history of the planet. In addition, loss rates would have been greater early in history due to the enhanced solar EUV and...
Topics: Atmosphere, Magnetospheres, Mars, Mars atmosphere, Mars climate, Solar wind
1
1.0
Dec 13, 2021
12/21
by
European Meeting on Solar Physics (8th : 1996 : Chalkidikē, Greece)
texts
eye 1
favorite 0
comment 0
viii, 278 p. : 24 cm
Topics: Solar wind -- Congresses, Solar atmosphere -- Congresses, Heliosphere (Astrophysics) -- Congresses
385
385
Mar 4, 2009
03/09
by
NASA LaRC Office of Education
movies
eye 385
favorite 0
comment 0
What is the Aurora Borealis?
Topics: William Jeffries, Solar Wind, Charged Particles, Gas, Television, TV
Source: http://nasa.ibiblio.org/details.php?videoid=6250&start=100&subject=Science
317
317
Sep 27, 2020
09/20
by
Jim Blinn & Robert Wolff
movies
eye 317
favorite 12
comment 0
A brief video consisting of color computer graphics, with narration summarizing what was known about the magnetic field of Jupiter as of 1983. Includes information about the upcoming Galileo spacecraft's mission to study the magnetosphere in greater detail. Classical music (from Holst's The Planets ) plays in the background. Another description, from the computer science technical report Simulating the Dynamics of the Dancing Lights (U. Waterloo): Blinn and Wolf produced a film in 1983...
Topics: NASA, JPL, Jupiter, magnetosphere, solar wind, Galileo, computer graphics
485
485
Feb 8, 2011
02/11
by
NASA; Langley Research Center
movies
eye 485
favorite 0
comment 0
What is the Aurora Borealis?
Topics: NASA, KSNN, Solar Wind, Charged Particles, Gas, Television, TV
The High Energy Range Spectrometer (HERS) of the Ion Mass Spectrometer on the Giotto spacecraft measured the 3-dimensional distribution of picked-up cometary protons over a distance of approximately 8 million km upstream of the bow shock of Comet Halley. The protons were observed to be elastically scattered out of their original cycloidal trajectories such that they were nonuniformly distributed over a spherical shell in velocity space. The shell radius (relative to its expected radius) and...
Topics: NASA Technical Reports Server (NTRS), BOW WAVES, HALLEY'S COMET, HIGH ENERGY INTERACTIONS, PROTONS,...
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77
movies
eye 77
favorite 3
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This video shows two South American observations of the IRM satellite's release, on 18 July 1985, of barium thermite into the earth's magnetosphere. This was one of several experiments in the AMPTE (Active Magnetospheric Particle Tracer Explorer) program. AMPTE was a trilateral project (USA, UK, and Germany) with the aim of studying the solar wind and initiating the first artificial comet. It consisted of three sub-satellites: CCE, IRM and UKS. From the abstract of the referenced journal...
Topics: AMPTE, IRM, NASA, artificial comet, magnetosphere, solar wind, computer graphics
Studies on Sun-climate connection have been carried out for several decades, and almost all of them focused on the effects of solar total irradiation energy. As the second major terrestrial energy source from outer space, the solar wind energy flux exhibits more significant long-term variations. However, its link to the global climate change is rarely concerned and remains a mystery. As a fundamental and important aspect of the Earth's weather and climate system, tropical cyclone activity has...
Topics: Solar impacts on climate, Solar wind energy flux, Tropical cyclone
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67
movies
eye 67
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comment 0
This video shows the Kitt Peak (Arizona) National Observatory's observation of the IRM satellite's release of barium thermite into the earth's magnetotail, one of several experiments in the AMPTE (Active Magnetospheric Particle Tracer Explorer) program. AMPTE was a trilateral project (USA, UK, and Germany) with the aim of studying the solar wind and initiating the first artificial comet. It consisted of three sub-satellites: CCE, IRM and UKS. From the abstract of the referenced journal...
Topics: AMPTE, IRM, NASA, artificial comet, magnetosphere, solar wind, computer graphics
NASA Grant NAG5-12781 is a study on the "Nature and Variability of Coronal Streamers and their Relationship to the Slow Speed Wind." The two main goals of this study are to identify: 1) Where in the streamer structure does the solar wind originate, and 2) What coronal conditions are responsible for the variability of the slow speed wind. To answer the first question, we examined the mostly closed magnetic field regions in streamer cores to search for evidence of outflow. Preliminary...
Topics: NASA Technical Reports Server (NTRS), SOLAR CORONA, SOLAR WIND VELOCITY, VELOCITY DISTRIBUTION,...
The University of California, San Diego 3D Heliospheric Tomography Model reconstructs the evolution of heliospheric structures, and can make forecasts of solar wind density and velocity up to 72 hours in the future. The latest model version, installed and running in realtime at the Community Coordinated Modeling Center(CCMC), analyzes scintillations of meter wavelength radio point sources recorded by the Solar-Terrestrial Environment Laboratory(STELab) together with realtime measurements of...
Topics: NASA Technical Reports Server (NTRS), SOLAR WIND, THREE DIMENSIONAL MODELS, SOLAR WIND VELOCITY,...
84
84
Nov 2, 2009
11/09
by
NASA/Goddard Space Flight Center Scientific Visualization Studio
image
eye 84
favorite 0
comment 0
The earth's magnetosphere protects the earth from high-energy charged particles coming from the sun. Some charged particles are deflected by the magnetosphere, while others become trapped and produce the aurora. This presentation shows a 3-dimensional model of the magnetosphere. The features that it highlights are flat ribbons representing the paths of charged particles deflected by the magnetosphere, triangular ribbons representing magnetic field lines, and colored surfaces representing...
Topics: Geomagnetic Field, Magnetosphere, Solar Wind, Space science, What -- Earth, What -- Sun
Source: http://svs.gsfc.nasa.gov/goto?3028
215
215
Nov 25, 2009
11/09
by
NASA/Goddard Space Flight Center
movies
eye 215
favorite 2
comment 0
This animation shows a nuetral solar particle's path leaving the Sun, following the magnetic field lines out to the Heliosheath. The solar particle hits a hydrogen atom, stealing it's electron and we follow it until we see it hit one of IBEXs detectors. Note: Solar particle animation Animator: Walt Feimer (HTSI). Scientist: Dave McComas (SwRI). Platforms/Sensors/Data Sets: IBEX.
Topics: HDTV, Heliosphere, Interstellar medium, Neutral Atoms, Solar Wind, IBEX, What -- Sun
Source: http://svs.gsfc.nasa.gov/goto?10332
511
511
Jul 6, 2010
07/10
by
Clark, B. B
texts
eye 511
favorite 0
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Processing techniques were tested for deducing cloud motion vectors from overlapped portions of pairs of pictures made from meteorological satellites. This was accomplished by programming and testing techniques for estimating pattern motion by means of cross correlation analysis with emphasis placed upon identifying and reducing errors resulting from various factors. Techniques were then selected and incorporated into a cloud motion determination program which included a routine which would...
Topics: BOW WAVES, MAGNETIC FIELDS, SHOCK WAVES, EARTH MAGNETOSPHERE, GEOMAGNETISM, SOLAR WIND
Comets emit X-ray via the process of solar wind charge exchange (SWCX). Quantitative measurements of this interaction are important to have insight about the composition of comets. The present work focuses of composition of comets depending on the interaction between both Cometary nucleus and tail with solar wind. The chemical composition of Cometary nuclei was inferred from measurements of neutral and ionized gases from the coma, tail, and dust grains. Data were obtained through space...
Topics: 8p/Tuttle Comet, 103p/Hartley Comet, X-ray Spectra, Solar Wind
Comets emit X-ray via the process of solar wind charge exchange (SWCX). Quantitative measurements of this interaction are important to have insight about the composition of comets. The present work focuses of composition of comets depending on the interaction between both Cometary nucleus and tail with solar wind. The chemical composition of Cometary nuclei was inferred from measurements of neutral and ionized gases from the coma, tail, and dust grains. Data were obtained through space...
Topics: 8p/Tuttle Comet, 103p/Hartley Comet, X-ray Spectra, Solar Wind
161
161
Nov 18, 2009
11/09
by
NASA/Goddard Space Flight Center- Conceptual Image Lab
movies
eye 161
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This animation shows a magnetospheric substorm, during which the reconnection causes energy to be rapidly released along the field lines causing the auroras to brighten. Note: Earth's magnetic field lines including plasma. Animator: Walt Feimer (HTSI).
Topics: Aurora, HDTV, Magnetic Reconnection, Solar Wind, Space Weather, THEMIS, What -- THEMIS
Source: http://svs.gsfc.nasa.gov/goto?10104
A brief review is given of recent developments in the observation of the solar wind by the method of interplanetary scintillation. The emphasis is on observations of the velocity structure, the electron density and the effect of propagating disturbances in the interplanetary medium as detected principally by intensity and phase scintillation and by spectral broadening.
Topics: NASA Technical Reports Server (NTRS), INTERPLANETARY MEDIUM, SCINTILLATION, SOLAR WIND, ELECTRON...
Measurements from the HELIOS solar probes indicated that apart from solar activity related disturbances there exist two states of the solar wind which might result from basic differences in the acceleration process: the fast solar wind (v 600 kms(-)1) emanating from magnetically open regions in the solar corona and the "slow" solar wind (v 400 kms(-)1) correlated with the more active regions and its mainly closed magnetic structures. In a comprehensive study using all HELIOS data...
Topics: NASA Technical Reports Server (NTRS), HELIOS 1, HELIOS 2, HELIOSPHERE, SOLAR CYCLES, SOLAR WIND,...
The solar transition region is in a dynamic state characterized by impulsively upflowing plasma and continually downflowing plasma. Using numerical simulations, the conjecture that the areas of downflowing plasma are simply the base regions of coronal loops in which the heating rate is gradually decreasing and the areas of upflowing plasma are the base regions of coronal loops in which the heating rate is gradually increasing is examined. The calculations suggest that gradually reducing or...
Topics: NASA Technical Reports Server (NTRS), CORONAL LOOPS, HIGH TEMPERATURE PLASMAS, MAGNETOHYDRODYNAMIC...
311
311
May 23, 2011
05/11
by
Ding, Z.; Anghaie, S
texts
eye 311
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A unique numerical method has been developed to model the dynamic processes of bulk evaporation and condensation processes, associated with internal heat generation and natural convection under different gravity levels. The internal energy formulation, for the bulk liquid-vapor phase change problems in an encapsulated container, was employed. The equations, governing the conservation of mass, momentum and energy for both phases involved in phase change, were solved. The thermal performance of a...
Topics: MARS ATMOSPHERE, SOLAR WIND, SOFTWARE DEVELOPMENT TOOLS, MARS (PLANET), SOLAR WIND VELOCITY,...
289
289
May 31, 2011
05/11
by
Harvey, G. A.; Lash, T. J.; Kinard, W. H.; Bull, K.; deGeest, F
texts
eye 289
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The Materials International Space Station Experiment (MISSE) is scheduled to be deployed during the summer of 2001. This experiment is a cooperative endeavor by NASA-LaRC, NASA-GRC, NASA MSFC, NASA-JSC, the Materials Laboratory at the Air Force Research Laboratory, and the Boeing Phantom Works. The objective of the experiment is to evaluate performance, stability, and long term survivability of materials and components planned for use by NASA and DOD on future LEO, synchronous orbit, and...
Topics: IONS, PLASMA PHYSICS, POLAR CAPS, SPACE PLASMAS, SOLAR WIND, WIND VELOCITY
89
89
Nov 18, 2009
11/09
by
NASA/Goddard Space Flight Center, Conceptual Image Lab
movies
eye 89
favorite 0
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THEMIS (Time History of Events and Microscale Interactions durind Substorms) answers fundamental outstanding questions regarding the magnetospheric substorm instability, a dominant mechanism of transport and explosive release of solar wind energy within Geospace. THEMIS will elucidate which magnetotail process is responsible for substorm onset at the region where substorm auroras map (~10Re): (i) a local disruption of the plasma sheet current or (ii) that current's interaction with the rapid...
Topics: Aurora, HDTV, Magnetic Reconnection, Solar Wind, THEMIS, What -- THEMIS, Where -- California
Source: http://svs.gsfc.nasa.gov/goto?10103
