Academic literature on the topic 'Space and Solar Physics'
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Journal articles on the topic "Space and Solar Physics"
Kuznetsov, V. D., and L. M. Zelenyi. "Space projections on solar-terrestrial physics." Geomagnetism and Aeronomy 49, no. 8 (December 2009): 1137–47. http://dx.doi.org/10.1134/s0016793209080209.
Full textKrimigis, S. M. "Committee on Solar and Space Physics." Eos, Transactions American Geophysical Union 67, no. 33 (1986): 635. http://dx.doi.org/10.1029/eo067i033p00635-01.
Full textSimarski, L. "NRC assesses solar and space physics." Eos, Transactions American Geophysical Union 72, no. 35 (1991): 371. http://dx.doi.org/10.1029/90eo00280.
Full textGómez, Daniel, Luis N. Martín, and Pablo Dmitruk. "Magnetohydrodynamics in solar and space physics." Advances in Space Research 51, no. 10 (May 2013): 1916–23. http://dx.doi.org/10.1016/j.asr.2012.09.016.
Full textGrigoryev, V. M. "A space-borne solar stereoscope experiment in solar physics." Solar Physics 148, no. 2 (December 1993): 389–91. http://dx.doi.org/10.1007/bf00645098.
Full textRutten, Robert J., and Luc Damé. "SIMURIS: High-Resolution Solar Physics." International Astronomical Union Colloquium 141 (1993): 184–87. http://dx.doi.org/10.1017/s0252921100029055.
Full textHill, Frank. "Solar physics with the Virtual Solar Observatory." Proceedings of the International Astronomical Union 2, no. 14 (August 2006): 612. http://dx.doi.org/10.1017/s1743921307012100.
Full textDomingo, V. "Helioseismology from space, the SOHO project." Symposium - International Astronomical Union 123 (1988): 545–48. http://dx.doi.org/10.1017/s007418090015867x.
Full textLanzerotti, L. J. "International Cooperation in Solar and Space Physics." Eos, Transactions American Geophysical Union 66, no. 1 (1985): 1. http://dx.doi.org/10.1029/eo066i001p00001-02.
Full textHarley, Phil. "Space-based solar." Physics World 35, no. 11 (December 1, 2022): 25iii—26i. http://dx.doi.org/10.1088/2058-7058/35/11/25.
Full textDissertations / Theses on the topic "Space and Solar Physics"
Khotyaintsev, Mykola. "Radar Probing of the Sun." Doctoral thesis, Uppsala University, Department of Astronomy and Space Physics, 2006. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-7192.
Full textThis thesis is dedicated to the theory of solar radar experiments. The Sun exhibits a variety of interesting and complicated physical phenomena, examined mainly through analysis of its radiation. Active solar probing by radar provides an alternative possibility to study the Sun. This concept was tested originally in the 1960's by solar radar experiments at El Campo, Texas, but due to an insufficient level of technology at that time the experimental results were of a poor quality and thus difficult to interpret. Recently, the space weather program has stimulated interest in this topic. New experimental proposals require further development of the theory of solar radar experiments to meet the current knowledge about the Sun and the modern level of technology.
Three important elements of solar radar experiments are addressed in this thesis: i) generation of wave turbulence and radiation in the solar corona, ii) propagation of the radar signal to the reflection point, and iii) reflection (scattering) of the incident radar signal from the Sun.
It is believed that the radio emission of solar type II and III bursts occurs due to conversion of Langmuir waves, generated by electron beams, into electromagnetic radiation (plasma emission mechanism). The radar signal propagating through the emission source region can get scattered by the Langmuir turbulence and finally deliver the observer insights of the physics of this turbulence. Such process of scattering is considered in this thesis in the weak turbulence limit by means of the wave-kinetic theory. Scattering frequency shifts, scattering cross-sections, efficiency of scattering (the coefficient of absorption due to scattering), optical depths, and the spectra of the scattered signal are estimated.
Type II solar radio bursts are known to be associated with the electron beams accelerated by interplanetary shocks. From their dynamic spectra the properties of the shocks and regions in the vicinity of the shock are usually inferred by assuming a plasma emission mechanism. In situ observations of the source region of type II burst, presented in this thesis, suggest that an additional emission mechanism may be present. This mechanism is related to energetic particles crossing the shock front, known in electrodynamics as transition radiation.
Plasma density fluctuations are known to scatter radio waves and thus broadening their angular dispersion. In the thesis this process is studied in the solar wind and terrestrial electron and ion foreshocks on the basis of in situ observations of density fluctuations. It is shown that the angular broadening of the radar signal is negligible in this regions.
The results of this thesis can be applied for the preparation of future solar radar experiments and interpretation of experimental data.
Moore, Christopher Samuel. "Atomic Layer Deposition Re ective Coatings for future Astronomical Space Telescopes and the Solar Corona viewed through the MinXSS (Miniature X-ray Solar Spectrometer) CubeSats." Thesis, University of Colorado at Boulder, 2018. http://pqdtopen.proquest.com/#viewpdf?dispub=10680697.
Full textAdvances in technology and instrumentation open new windows for observing astrophysical objects. The first half of my dissertation involves the development of atomic layer deposition (ALD) coatings to create high reflectivity UV mirrors for future satellite astronomical telescopes. Aluminum (Al) has intrinsic reflectance greater than 80% from 90 ? 2,000 nm, but develops a native aluminum oxide (Al2O3) layer upon exposure to air that readily absorbs light below 250 nm. Thus, Al based UV mirrors must be protected by a transmissive overcoat. Traditionally, metal-fluoride overcoats such as MgF2 and LiF are used to mitigate oxidation but with caveats. We utilize a new metal fluoride (AlF3) to protect Al mirrors deposited by ALD. ALD allows for precise thickness control, conformal and near stoichiometric thin films. We prove that depositing ultra-thin (~3 nm) ALD ALF3 to protect Al mirrors after removing the native oxide layer via atomic layer etching (ALE) enhances the reflectance near 90 nm from ~5% to ~30%. X-ray detector technology with high readout rates are necessary for the relatively bright Sun, particularly during large flares. The hot plasma in the solar corona generates X-rays, which yield information on the physical conditions of the plasma. The second half of my dissertation includes detector testing, characterization and solar science with the Miniature X-ray Solar Spectrometer (MinXSS) CubeSats. The MinXSS CubeSats employ Silicon Drift Diode (SDD) detectors called X123, which generate full sun spectrally resolved (~0.15 FWHM at 5.9 keV) measurements of the sparsely measured, 0.5 ? 12 keV range. The absolute radiometric calibration of the MinXSS instrument suite was performed at the National Institute for Standards and Technology (NIST) Synchrotron Ultraviolet Radiation Facility (SURF) and spectral resolution determined from radioactive sources. I used MinXSS along with data from the Geostationary Operational Environmental Satellites (GOES), Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI), Hinode X-ray Telescope (XRT), Hinode Extreme Ultraviolet Imaging Spectrometer (EIS) and Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA) to study the solar corona. This resulted in new insights on the coronal temperature distribution and elemental abundance variations for quiescence, active regions and during solar flares.
Seki, Daikichi. "Space Weather Prediction Using Ground-Based Observations." Doctoral thesis, Kyoto University, 2021. http://hdl.handle.net/2433/263804.
Full text京都大学
新制・課程博士
博士(総合学術)
甲第23343号
総総博第16号
京都大学大学院総合生存学館総合生存学専攻
(主査)教授 山敷 庸亮, 教授 寶 馨, 准教授 浅井 歩
学位規則第4条第1項該当
Doctor of Philosophy
Kyoto University
DFAM
Retinò, Alessandro. "Magnetic Reconnection in Space Plasmas : Cluster Spacecraft Observations." Doctoral thesis, Uppsala University, Department of Astronomy and Space Physics, 2007. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-7891.
Full textMagnetic reconnection is a universal process occurring at boundaries between magnetized plasmas, where changes in the topology of the magnetic field lead to the transport of charged particles across the boundaries and to the conversion of electromagnetic energy into kinetic and thermal energy of the particles. Reconnection occurs in laboratory plasmas, in solar system plasmas and it is considered to play a key role in many other space environments such as magnetized stars and accretion disks around stars and planets under formation. Magnetic reconnection is a multi-scale plasma process where the small spatial and temporal scales are strongly coupled to the large scales. Reconnection is initiated rapidly in small regions by microphysical processes but it affects very large volumes of space for long times. The best laboratory to experimentally study magnetic reconnection at different scales is the near-Earth space, the so-called Geospace, where Cluster spacecraft in situ measurements are available. The European Space Agency Cluster mission is composed of four-spacecraft flying in a formation and this allows, for the first time, simultaneous four-point measurements at different scales, thanks to the changeable spacecraft separation. In this thesis Cluster observations of magnetic reconnection in Geospace are presented both at large and at small scales.
At large temporal (a few hours) and spatial (several thousands km) scales, both fluid and kinetic evidence of reconnection is provided. The evidence consist of ions accelerated and transmitted across the Earth’s magnetopause. The observations show that component reconnection occurs at the magnetopause and that reconnection is continuous in time.
The microphysics of reconnection is investigated at smaller temporal (a few ion gyroperiods) and spatial (a few ion gyroradii) scales. Two regions are important for the microphysics: the X-region, around the X-line, where reconnection is initiated and the separatrix region, away from the X-line, where most of the energy conversion occurs. Observations of a separatrix region at the magnetopause are shown and the microphysics is described in detail. The separatrix region is shown to be highly structured and dynamic even away from the X-line.
Finally the discovery of magnetic reconnection in turbulent plasma is presented by showing, for the first time, in situ evidence of reconnection in a thin current sheet found in the turbulent plasma downstream of the quasi-parallel Earth’s bow shock. It is shown that turbulent reconnection is fast and that electromagnetic energy is converted into heating and acceleration of particles in turbulent plasma. It is also shown that reconnecting current sheets are abundant in turbulent plasma and that reconnection can be an efficient energy dissipation mechanism.
Rosenqvist, Lisa. "Energy Transfer and Conversion in the Magnetosphere-Ionosphere System." Doctoral thesis, Uppsala University, Department of Astronomy and Space Physics, 2008. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-8716.
Full textMagnetized planets, such as Earth, are strongly influenced by the solar wind. The Sun is very dynamic, releasing varying amounts of energy, resulting in a fluctuating energy and momentum exchange between the solar wind and planetary magnetospheres. The efficiency of this coupling is thought to be controlled by magnetic reconnection occurring at the boundary between solar wind and planetary magnetic fields. One of the main tasks in space physics research is to increase the understanding of this coupling between the Sun and other solar system bodies. Perhaps the most important aspect regards the transfer of energy from the solar wind to the terrestrial magnetosphere as this is the main source for driving plasma processes in the magnetosphere-ionosphere system. This may also have a direct practical influence on our life here on Earth as it is responsible for Space Weather effects. In this thesis I investigate both the global scale of the varying solar-terrestrial coupling and local phenomena in more detail. I use mainly the European Space Agency Cluster mission which provide unprecedented three-dimensional observations via its formation of four identical spacecraft. The Cluster data are complimented with observations from a broad range of instruments both onboard spacecraft and from groundbased magnetometers and radars.
A period of very strong solar driving in late October 2003 is investigated. We show that some of the strongest substorms in the history of magnetic recordings were triggered by pressure pulses impacting a quasi-stable magnetosphere. We make for the first time direct estimates of the local energy flow into the magnetotail using Cluster measurements. Observational estimates suggest a good energy balance between the magnetosphere-ionosphere system while empirical proxies seem to suffer from over/under estimations during such extreme conditions.
Another period of extreme interplanetary conditions give rise to accelerated flows along the magnetopause which could account for an enhanced energy coupling between the solar wind and the magnetosphere. We discuss whether such conditions could explain the simultaneous observation of a large auroral spiral across the polar cap.
Contrary to extreme conditions the energy conversion across the dayside magnetopause has been estimated during an extended period of steady interplanetary conditions. A new method to determine the rate at which reconnection occurs is described that utilizes the magnitude of the local energy conversion from Cluster. The observations show a varying reconnection rate which support the previous interpretation that reconnection is continuous but its rate is modulated.
Finally, we compare local energy estimates from Cluster with a global magnetohydrodynamic simulation. The results show that the observations are reliably reproduced by the model and may be used to validate and scale global magnetohydrodynamic models.
Pacheco, Mateo Daniel. "Analysis and modelling of the solar energetic particle radiation environment in the inner heliosphere in preparation for Solar Orbiter." Doctoral thesis, Universitat de Barcelona, 2019. http://hdl.handle.net/10803/667033.
Full textEl Sol és la principal font de partícules que podem trobar al medi interplanetari del sistema solar, i els esdeveniments solars de partícules energètiques són la principal font de radiació dins de l'heliosfera. L'estudi i predicció d'aquest tipus d'esdeveniments i les seves causes i conseqüències ha esdevingut una àrea d'especial interès per la seva importància enfront dels perills que suposa aquesta radiació per a les telecomunicacions i la salut durant missions espacials tripulades. En aquesta tesi exposem el treball que hem desenvolupat en aquest camp, dividit en 3 àmbits diferents: i) estudi observacional d'esdeveniments de partícules fent servir dades observacionals de missions espacials com STEREO i Helios, i eines com SEPEM; ii) desenvolupament d'eines i modalització d'instruments de partícules per fer-los servir conjuntament amb els models preexistents per la simulació d'esdeveniments; iii) simulació d'esdeveniments de partícules mitjançant models de transport, tant adaptant eines prèviament desenvolupades pel nostre grup, com SEPInversion, com nou programari capaç de realitzar inversions totals, es a dir, tenint en compte la resposta angular i energètica dels instruments. Les eines desenvolupades ens han permès estudiar les condicions de radiació a l'heliosfera interior com no s'havia fet fins ara. Els resultats obtinguts així com aquestes eines seran molt útils per a l'estudi i interpretació de les dades científiques provinents de les futures missions espacials com Parker Solar Probe o Solar Orbiter. A més a més, les eines desenvolupades ens permetran fer un ús efectiu d'aquestes dades tan aviat com estiguin disponibles.
Cimaroli, Alexander J. "Development of Deposition and Characterization Systems for Thin Film Solar Cells." University of Toledo / OhioLINK, 2016. http://rave.ohiolink.edu/etdc/view?acc_num=toledo1481295690696407.
Full textPerna, Davide. "Physical properties of asteroid targets of the Rosetta space mission, and of minor bodies of the outer Solar System." Observatoire de Paris (1667-....), 2010. https://hal.science/tel-02094984.
Full textThe minor bodies of the Solar System are the remnants of the primordial planetesimal population, their investigation can hence improve our knowledge about the environment conditions in the solar nebula, and the thermal and physical processes that took place in the early phases of the Solar System. During my Phd, I focused on the physical characterization of the asteroids (2867) Steins and (21) Lutetia, targets of the Esa-Rosetta space mission, and of the minor bodies of the outer Solar System (Centaurs et Trans-Neptunian Objects, TNOS). I performed visible photometric and spectroscopic observations of Steins and Lutetia using the Telescopio Nazionale Galileo, from the reduction, and the analysis, and the interpretation of the obtained data, I improved the physical knowledge of both the objects prior to the Rosetta fly-by. In this thesis I also present the results I obtained as part of large programme performed at the European Southern Observatory on Centaurs and the Trans-Neptunian Objects. I contributed to the interpretation of the obtained spectra using radiative transfer models. On the basis of the obtained photometric colors, I derived the taxonomic classification of the observed objects, and I performed a statistical analysis using also the whole available literature looking for correlations between taxonomy and dynamics. From the interpretation of the light curves I gathered information about the rotation, shape and density of the objects under analysis, and I investigated the density statistics of the small bodies of the outer Solar System combining these new results with literature data
Jaklovsky, Simon. "Drag based forecast for CME arrival." Thesis, Uppsala universitet, Institutionen för fysik och astronomi, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-415153.
Full textHåkansson, Marcus. "Back-tracing of water ions at comet 67P/Churyumov–Gerasimenko." Thesis, Luleå tekniska universitet, Rymdteknik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-67050.
Full textBooks on the topic "Space and Solar Physics"
H, Waite J., Burch J. L. 1942-, Moore R. L. 1942-, AGU Books Board, and Yosemite Conference on Outstanding Problems in Solar System Plasma Physics: Theory and Instrumentation (1988 : Yosemite National Park, Calif.), eds. Solar system plasma physics. Washington, DC: American Geophysical Union, 1989.
Find full textSchunk, R. W. Solar-terrestrial physics: A space age birth. Logan, Utah: Faculty Association, 1986.
Find full textInc, ebrary. Solar and space physics and its role in space exploration. Washington, DC: National Academies Press, 2004.
Find full textGeorge, Fisher, and SpringerLink (Online service), eds. Solar Flare Magnetic Fields and Plasmas. New York, NY: Springer US, 2012.
Find full textGombosi, Tamas I. Physics of the Space Environment. Cambridge: Cambridge University Press, 1998.
Find full textGombosi, Tamás I. Physics of the space environment. Cambridge: Cambridge University Press, 1998.
Find full textKoskinen, Hannu E. J. Physics of space storms: From the solar surface to the Earth. Berlin: Springer, 2011.
Find full textPaolo, Farinella, ed. Physics of the earth and the solar system: Dynamics and evolution, space navigation, space-time structure. Dordrecht, The Netherlands: Kluwer Academic Publishers, 1990.
Find full textPaolo, Farinella, and Vokrouhlický David, eds. Physics of the solar system: Dynamics and evolution, space physics, and spacetime structure. Dordrecht: Kluwer Academic Publishers, 2003.
Find full textNational Research Council (U.S.). Committee on Solar and Space Physics. An implementation plan for priorities in solar-system space physics. Washington, D.C: National Academy Press, 1985.
Find full textBook chapters on the topic "Space and Solar Physics"
Kallenrode, May-Britt. "Solar-Terrestrial Relationships." In Space Physics, 375–403. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-662-09959-9_10.
Full textKallenrode, May-Britt. "Solar—Terrestrial Relationships." In Space Physics, 303–20. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04443-8_10.
Full textKallenrode, May-Britt. "Solar—Terrestrial Relationships." In Space Physics, 293–311. Berlin, Heidelberg: Springer Berlin Heidelberg, 1998. http://dx.doi.org/10.1007/978-3-662-03653-2_13.
Full textKallenrode, May-Britt. "Sun and Solar Wind: Plasmas in the Heliosphere." In Space Physics, 135–211. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-662-09959-9_6.
Full textKallenrode, May-Britt. "Sun and Solar Wind: Plasmas in the Heliosphere." In Space Physics, 103–58. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04443-8_6.
Full textKallenrode, May-Britt. "Sun and Solar Wind: Plasmas in the Heliosphere." In Space Physics, 143–86. Berlin, Heidelberg: Springer Berlin Heidelberg, 1998. http://dx.doi.org/10.1007/978-3-662-03653-2_8.
Full textBiswas, Sukumar. "Solar Energetic Particles." In Cosmic Perspectives in Space Physics, 233–82. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4651-7_6.
Full textMcilwain, Carl E. "Test Particle Measurements in Space Plasmas." In Solar System Plasma Physics, 89–93. Washington, D. C.: American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm054p0089.
Full textHasegawa, Akira, and Tetsuya Sato. "Stationary Solar Plasma System." In Physics and Chemistry in Space, 109–70. Berlin, Heidelberg: Springer Berlin Heidelberg, 1989. http://dx.doi.org/10.1007/978-3-642-74185-2_3.
Full textGosling, J. T. "The solar flare myth in solar-terrestrial physics." In Solar System Plasmas in Space and Time, 65–69. Washington, D. C.: American Geophysical Union, 1994. http://dx.doi.org/10.1029/gm084p0065.
Full textConference papers on the topic "Space and Solar Physics"
Parker, E. N. "Space physics before the space age." In The solar wind nine conference. AIP, 1999. http://dx.doi.org/10.1063/1.58782.
Full textManeva, Y. G., J. A. Araneda, E. Marsch, and Ivan Zhelyazkov. "Parametrically Unstable Alfvén-cyclotron Waves and Wave—Particle Interactions in the Solar Corona and Solar Wind." In SPACE PLASMA PHYSICS: School of Space Plasma Physics. AIP, 2009. http://dx.doi.org/10.1063/1.3137931.
Full textRuderman, M. S., and Ivan Zhelyazkov. "Theory of Transverse Oscillations of Solar Coronal Loops." In SPACE PLASMA PHYSICS: School of Space Plasma Physics. AIP, 2009. http://dx.doi.org/10.1063/1.3137928.
Full textPirvutoiu, C., D. Vladoiu, G. Maris, and Ivan Zhelyazkov. "On the Relationship between Solar Wind Characteristics and Geomagnetic Activity." In SPACE PLASMA PHYSICS: School of Space Plasma Physics. AIP, 2009. http://dx.doi.org/10.1063/1.3137935.
Full textFilippov, B., S. Koutchmy, O. Martsenyuk, and Y. Platov. "Solar eruptive phenomena." In SPACE PLASMA PHYSICS: Proceedings of the 4th School and Workshop on Space Plasma Physics. AIP, 2013. http://dx.doi.org/10.1063/1.4818861.
Full textZaqarashvili, T. V., and Ivan Zhelyazkov. "Spectral Line Non-thermal Broadening and MHD Waves in the Solar Corona." In SPACE PLASMA PHYSICS: School of Space Plasma Physics. AIP, 2009. http://dx.doi.org/10.1063/1.3137929.
Full textCliver, E. W. "Solar flare gamma-ray emission and energetic particles in space." In High energy solar physics. AIP, 1996. http://dx.doi.org/10.1063/1.50980.
Full textSmart, D. F., and M. A. Shea. "High energy particles in interplanetary space on 11 June 1991." In High energy solar physics. AIP, 1996. http://dx.doi.org/10.1063/1.50946.
Full textShopov, Y. Y., A. Varonov, and D. A. Stoykova. "RGB color photometry of the solar corona from total solar eclipses." In SPACE PLASMA PHYSICS: Proceedings of the 5th School and Workshop on Space Plasma Physics. AIP Publishing LLC, 2016. http://dx.doi.org/10.1063/1.4942577.
Full textRossolenko, S., E. Antonova, I. Kirpichev, Yu Yermolaev, and Ivan Zhelyazkov. "Interaction of Solar Wind with Earth’s Magnetosphere and Formation of Magnetospheric Boundary Layers." In SPACE PLASMA PHYSICS: School of Space Plasma Physics. AIP, 2009. http://dx.doi.org/10.1063/1.3137933.
Full textReports on the topic "Space and Solar Physics"
BARKHATOV, NIKOLAY, and SERGEY REVUNOV. A software-computational neural network tool for predicting the electromagnetic state of the polar magnetosphere, taking into account the process that simulates its slow loading by the kinetic energy of the solar wind. SIB-Expertise, December 2021. http://dx.doi.org/10.12731/er0519.07122021.
Full textBowles, T. J., S. J. Brice, E. I. Esch, M. M. Fowler, A. Goldschmidt, A. Hime, F. McGirt, et al. Solar Neutrino Physics. Office of Scientific and Technical Information (OSTI), July 1999. http://dx.doi.org/10.2172/759169.
Full textGarretson, Peter. Solar Power in Space? Fort Belvoir, VA: Defense Technical Information Center, January 2012. http://dx.doi.org/10.21236/ada567884.
Full textAlbert, Andrea. High-energy Particle Physics -- In Space! Office of Scientific and Technical Information (OSTI), September 2018. http://dx.doi.org/10.2172/1469489.
Full textArif, Humayun, Hugo Barbosa, Christophe Bardet, Michel Baroud, Alberto Behar, Keith Berrier, Phillipe Berthe, et al. Space Solar Power Program. Final report. Office of Scientific and Technical Information (OSTI), August 1992. http://dx.doi.org/10.2172/6591719.
Full textHarvey, John, and Robert Howard. Solar Magnetic Drivers of Space Weather. Fort Belvoir, VA: Defense Technical Information Center, September 1997. http://dx.doi.org/10.21236/ada634656.
Full textHammer, David A. Plasma Physics Applications to Intense Radiation Sources, Pulsed Power and Space Physics. Fort Belvoir, VA: Defense Technical Information Center, September 1990. http://dx.doi.org/10.21236/ada226666.
Full textRubenchik, A., J. Parker, R. Beach, and R. Yamamoto. Solar Power Beaming: From Space to Earth. Office of Scientific and Technical Information (OSTI), April 2009. http://dx.doi.org/10.2172/952766.
Full textBirn, J. Solar terrestrial coupling through space plasma processes. Office of Scientific and Technical Information (OSTI), December 2000. http://dx.doi.org/10.2172/768901.
Full textPal, P. B. Particle physics confronts the solar neutrino problem. Office of Scientific and Technical Information (OSTI), June 1991. http://dx.doi.org/10.2172/10144522.
Full text