Relevant bibliographies by topics / Solar energetic particles

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Solar energetic particles'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 August 2024

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Journal articles on the topic "Solar energetic particles"

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KIRÁLY, PÉTER. "SOLAR ENERGETIC PARTICLES." International Journal of Modern Physics A 20, no. 29 (2005): 6634–41. http://dx.doi.org/10.1142/s0217751x05029678.

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Energetic particles recorded in the Earth environment and in interplanetary space have a multitude of origins, i.e. acceleration and propagation histories. At early days practically all sufficiently energetic particles were considered to have come either from solar flares or from interstellar space. Later on, co-rotating interplanetary shocks, the termination shock of the supersonic solar wind, planetary bow shocks and magnetospheres, and also coronal mass ejections (CME) were recognized as energetic particle sources. It was also recognized that less energetic (suprathermal) particles of solar
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Vilmer, Nicole. "Solar flares and energetic particles." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 370, no. 1970 (2012): 3241–68. http://dx.doi.org/10.1098/rsta.2012.0104.

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Solar flares are now observed at all wavelengths from γ -rays to decametre radio waves. They are commonly associated with efficient production of energetic particles at all energies. These particles play a major role in the active Sun because they contain a large amount of the energy released during flares. Energetic electrons and ions interact with the solar atmosphere and produce high-energy X-rays and γ -rays. Energetic particles can also escape to the corona and interplanetary medium, produce radio emissions (electrons) and may eventually reach the Earth's orbit. I shall review here the av
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Hofer, M. Y., R. G. Marsden, T. R. Sanderson, and C. Tranquille. "From the Sun’s south to the north pole – Ulysses COSPIN/LET composition measurements at solar maximum." Annales Geophysicae 21, no. 6 (2003): 1383–91. http://dx.doi.org/10.5194/angeo-21-1383-2003.

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Abstract. Based on elemental abundance ratios derived from the Ulysses COSPIN/LET measurements, we classified the energetic particle populations during and after the socalled Fast Latitude Scan – the time period during which the Ulysses spacecraft traveled from the highest heliolatitude south to maximum northern latitude, i.e. 27 November 2000 to 13 October 2001 – as being mixed between solar energetic particles (major component) and particles accelerated at stream interaction regions. During the fast latitude scan, the Ulysses spacecraft made the first transit in heliolatitude from pole to po
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Dröge, Wolfgang. "Transport of Solar Energetic Particles." International Astronomical Union Colloquium 142 (1994): 567–76. http://dx.doi.org/10.1017/s0252921100077824.

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AbstractNew developments in the understanding of the interplanetary transport of solar cosmic rays are reviewed. Based on carefully analyzed solar particle events observed on the Helios and ISEE 3 spacecraft, the relation of transport parameters to the structure of the interplanetary magnetic field is discussed. Special emphasis is given to a comparison of particle mean free paths determined from fits to intensity and anisotropy profiles with theoretical predictions derived from magnetic field spectra measured at the time of the solar particle event. Different aspects of the turbulence and wav
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Wang, J. F., and G. Qin. "The Effect of Solar Wind on Charged Particles’ Diffusion Coefficients." Astrophysical Journal 961, no. 1 (2024): 6. http://dx.doi.org/10.3847/1538-4357/ad09b7.

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Abstract The transport of energetic charged particles through magnetized plasmas is ubiquitous in interplanetary space and astrophysics, and the important physical quantities are the parallel and perpendicular diffusion coefficients of energetic charged particles. In this paper, the influence of solar wind on particle transport is investigated. Using the focusing equation, we obtain parallel and perpendicular diffusion coefficients, accounting for the solar wind effect. For different conditions, the relative importance of the solar wind effect to diffusion is investigated. It is shown that, wh
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McKibben, R. B., J. J. Connell, C. Lopate, et al. "Ulysses COSPIN observations of cosmic rays and solar energetic particles from the South Pole to the North Pole of the Sun during solar maximum." Annales Geophysicae 21, no. 6 (2003): 1217–28. http://dx.doi.org/10.5194/angeo-21-1217-2003.

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Abstract. In 2000–2001 Ulysses passed from the south to the north polar regions of the Sun in the inner heliosphere, providing a snapshot of the latitudinal structure of cosmic ray modulation and solar energetic particle populations during a period near solar maximum. Observations from the COSPIN suite of energetic charged particle telescopes show that latitude variations in the cosmic ray intensity in the inner heliosphere are nearly non-existent near solar maximum, whereas small but clear latitude gradients were observed during the similar phase of Ulysses’ orbit near the 1994–95 solar minim
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Vlahos, Loukas, Anastasios Anastasiadis, Athanasios Papaioannou, Athanasios Kouloumvakos, and Heinz Isliker. "Sources of solar energetic particles." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 377, no. 2148 (2019): 20180095. http://dx.doi.org/10.1098/rsta.2018.0095.

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Solar energetic particles are an integral part of the physical processes related with space weather. We present a review for the acceleration mechanisms related to the explosive phenomena (flares and/or coronal mass ejections, CMEs) inside the solar corona. For more than 40 years, the main two-dimensional cartoon representing our understanding of the explosive phenomena inside the solar corona remained almost unchanged. The acceleration mechanisms related to solar flares and CMEs also remained unchanged and were part of the same cartoon. In this review, we revise the standard cartoon and prese
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Dröge, Wolfgang. "Particle Acceleration by Waves and Fields." Highlights of Astronomy 11, no. 2 (1998): 865–68. http://dx.doi.org/10.1017/s1539299600018967.

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The acceleration of electrons and charged nuclei to high energies is a phenomenon occuring at many sites throughout the universe, including the galaxy, pulsars, quasars, and around black holes. In the heliosphere, large solar flares and the often associated coronal mass ejections (CMEs) are the most energetic natural particle accelerators, occasionally accelerating protons to GeV and electrons to tens of MeV energies. The observation of these particles offers the unique opportunity to study fundamental processes in astrophysics. Particles that escape into interplanetary space can be observed i
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Poluianov, S., G. A. Kovaltsov, and I. G. Usoskin. "Solar energetic particles and galactic cosmic rays over millions of years as inferred from data on cosmogenic 26Al in lunar samples." Astronomy & Astrophysics 618 (October 2018): A96. http://dx.doi.org/10.1051/0004-6361/201833561.

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Aims. Lunar soil and rocks are not protected by a magnetic field or an atmosphere and are continuously irradiated by energetic particles that can produce cosmogenic radioisotopes directly inside rocks at different depths depending on the particle’s energy. This allows the mean fluxes of solar and galactic cosmic rays to be assessed on the very long timescales of millions of years. Methods. Here we show that lunar rocks can serve as a very good particle integral spectrometer in the energy range 20–80 MeV. We have developed a new method based on precise modeling, that is applied to measurements
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Droege, Wolfgang. "Transport of solar energetic particles." Astrophysical Journal Supplement Series 90 (February 1994): 567. http://dx.doi.org/10.1086/191876.

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Dissertations / Theses on the topic "Solar energetic particles"

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Sollitt, Luke Stone Edward. "Ionic charge states of solar energetic particles /." Diss., Pasadena, Calif. : California Institute of Technology, 2004. http://resolver.caltech.edu/CaltechETD:etd-09122003-110331.

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Pei, Chunsheng. "Solar Energetic Particle Transport in the Heliosphere." Diss., The University of Arizona, 2007. http://hdl.handle.net/10150/194303.

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The transport of solar energetic particles (SEPs) in the inner heliosphere is a very important issue which can affect our daily life. For example, large SEP events can lead to the failure of power grids, interrupt communications, and may participate in global climate change. The SEPS also can harm humans in space and destroy the instruments on board spacecraft. Studying the transport of SEPs also helps us understand remote regions of space which are not visible to us because there are not enough photons in those places.The interplanetary magnetic field is the medium in which solar energetic pa
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Chollet, Eileen Emily. "Solar-Energetic Particles as a Probe of the Inner Heliosphere." Diss., The University of Arizona, 2008. http://hdl.handle.net/10150/195499.

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In this dissertation, I explore the relationship between solar energetic particles (SEPs) and the interplanetary magnetic field, and I use observations of SEPs to probe the region of space between the Sun and the Earth. After an introduction of major concepts in heliospheric physics, describing some of the history of energetic particles and defining the data sets used in the work, the rest of this dissertation is organized around three major concepts related to energetic particle transport: magnetic field-line length, interplanetary turbulence, and particle scattering and diffusion. In Chapt
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Sun, P., J. R. Jokipii, and J. Giacalone. "PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621389.

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We use a method developed by Roberts. that optimizes the phase angles of an ensemble of plane waves with amplitudes determined from a Kolmogorov-like power spectrum, to construct magnetic field vector fluctuations having nearly constant magnitude and large variances in its components. This is a representation of the turbulent magnetic field consistent with that observed in the solar wind. Charged-particle pitch-angle diffusion coefficients are determined by integrating the equations of motion for a large number of charged particles moving under the influence of forces from our predefined magne
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Sreeraj, T. "Generation of low frequency waves by energetic particles in space plasmas." Thesis, IIG, 2010. http://localhost:8080/xmlui/handle/123456789/1595.

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Druett, Malcolm. "The effects of energetic particles on radiative transfer and emission from hydrogen in solar flares." Thesis, Northumbria University, 2017. http://nrl.northumbria.ac.uk/36222/.

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There are rapid increases of hard and soft X-rays (HXR, SXR) and ultraviolet (UV) emission with large Doppler blue-shifts associated with plasma up-flows observed at flare onsets accompanied by broadened chromospheric emission with large redshifts. Hα shows red-shifts of 1–4 Å in the impulsive phase of solar flares observed with various past (Ichimoto and Kurokawa, 1984;Wuelser and Marti, 1989) and current (the Swedish Solar Telescope, SST) instruments (Druett et al., 2017). HXR footpoints are observed to be co-temporal and co-spatial with increases in white light (WL) and continuous emission
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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.

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The Sun is the main source of all kind of solar energetic particles in the Solar System, electrons, protons and ions with energies from few keV to several GeV. These particles are released from the solar corona and spread through the interplanetary space, the heliosphere, influenced by the interplanetary magnetic field and arriving to the Earth and interacting with the terrestrial magnetosphere. The effects of SEP interactions with space-based devices, manned missions and the Earth atmosphere are encompassed by what is known as space weather. This thesis describes the work we performed on thi
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Mallik, Procheta Chandra Vasu. "Diagnostics of solar flare energetic particles : neglected hard X-ray processes and neutron astronomy in the inner heliosphere." Thesis, University of Glasgow, 2010. http://theses.gla.ac.uk/1510/.

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For work on my thesis dissertation, we have been studying some energetic processes in solar flares. On our work on hard X-ray (HXR) emission from flares, we have shown that non-thermal recombination emission can compare with the bremsstrahlung HXR flux for certain flare conditions. In this thesis, we show spectral features characteristic of non-thermal recombination HXR emission and suggest how it plays a signicant role in the flare HXR continuum, something that has been ignored in the past. It is important to note that these results could demand a reconsideration of the numbers of accelerated
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Kühl, Patrick [Verfasser]. "Energy Spectra of near relativistic Galactic Cosmic Rays and Solar Energetic Particles - Extending the Measurement Capabilities of EPHIN / Patrick Kühl." Kiel : Universitätsbibliothek Kiel, 2017. http://d-nb.info/1141176114/34.

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Musset, Sophie. "Accélération et propagation des particules énergétiques dans la couronne solaire : de l'analyse des données de l'instrument RHESSI à la préparation de l'exploitation de l'instrument STIX sur Solar Orbiter." Thesis, Paris Sciences et Lettres (ComUE), 2016. http://www.theses.fr/2016PSLEO011/document.

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Le soleil est une étoile active, et les éruptions solaires sont une des manifestations de cette activité. Il est admis que l'énergie disponible pour les éruptions solaires a une origine magnétique, et est transmise au milieu lors de phénomènes de reconnexion magnétique dans la couronne. Une partie de cette énergie permet d'accélérer les particules du milieu (électrons et ions). Cependant, les détails concernant les conditions dans lesquelles les particules sont accélérées et se propagent des régions d'accélération aux sites d'interaction lors des éruptions solaires ne sont pas encore tous comp
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Books on the topic "Solar energetic particles"

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Reames, Donald V. Solar Energetic Particles. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-66402-2.

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Reames, Donald V. Solar Energetic Particles. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-50871-9.

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Lu, Edward Tsang. The evolution of energetic particles and the emitted radiation in solar flaresm. National Aeronautics and Space Administration, 1989.

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W, Urbarz H., and United States. National Aeronautics and Space Administration., eds. A preliminary summary of the observations of the 16 February 1984 solar flare (stip interval XV, 12-21 February 1984). National Aeronautics and Space Administration, 1987.

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Mavromichalaki, Helen. Solar extreme events: Fundamental science and applied aspects. Published for the Committee on Space Research [by] Elsevier, 2009.

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Mason, G. M. Solar cycle dynamics of solar, magnetospheric, and heliospheric particles, and long-term atmospheric coupling: SAMPEX : progress report for grant NAG 5-2963; period: July 1, 1996 - July 1, 1997. National Aeronautics and Space Administration, 1997.

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Mason, G. M. Solar cycle dynamics of solar, magnetospheric, and heliospheric particles, and long-term atmospheric coupling: SAMPEX : progress report for grant NAG 5-2963; period--July 1, 1995 - July 1, 1996. National Aeronautics and Space Administration, 1996.

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B, Blake J., and United States. National Aeronautics and Space Administration., eds. Solar cycle dynamics of solar, magnetospheric, and heliospheric particles, and long-term atmospheric coupling: SAMPEX : progress report for grant NAG 5-2963; period: July 1, 1996 - July 1, 1997. National Aeronautics and Space Administration, 1997.

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United States. National Aeronautics and Space Administration., ed. [Solar wind composition. National Aeronautics and Space Administration, 1995.

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United States. National Aeronautics and Space Administration., ed. A search for energetic ion directivity in large solar flares: Final technical report. National Aeronautics and Space Administration, 1993.

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Book chapters on the topic "Solar energetic particles"

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Reames, Donald V. "Introducing the Sun and SEPs." In Solar Energetic Particles. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-66402-2_1.

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AbstractThe structure of the Sun, with its energy generation and heating, creates convection and differential rotation of the outer solar plasma. This convection and rotation of the ionized plasma generates the solar magnetic field. This field and its variation spawn all of the solar activity: solar active regions, flares, jets, and coronal mass ejections (CMEs). Solar activity provides the origin and environment for both the impulsive and gradual solar energetic particle (SEP) events. This chapter introduces the background environment and basic properties of SEP events, time durations, abundances, and solar cycle variations.
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Ryan, James M., John A. Lockwood, and Hermann Debrunner. "Solar Energetic Particles." In Space Sciences Series of ISSI. Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-017-1187-6_3.

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Biswas, Sukumar. "Solar Energetic Particles." In Cosmic Perspectives in Space Physics. Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4651-7_6.

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Valtonen, Eino. "Solar Energetic Particles." In The Sun, the Solar Wind, and the Heliosphere. Springer Netherlands, 2010. http://dx.doi.org/10.1007/978-90-481-9787-3_16.

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Reames, Donald V. "Impulsive SEP Events (and Flares)." In Solar Energetic Particles. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-66402-2_4.

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Abstract3He-rich, Fe-rich, and enriched in elements with Z > 50, the abundances of solar energetic particles (SEPs) from the small impulsive SEP events stand out as luminaries in our study. The 3He is enhanced by resonant wave-particle interactions. Element abundances increase 1000-fold as the ~3.6 power of the mass-to-charge ratio A/Q from He to heavy elements like Au or Pb, enhanced during acceleration in islands of magnetic reconnection in solar jets, and probably also in flares. This power-law of enhancement vs. A/Q implies Q determined by a source temperature of 2.5–3.2 MK, typical of jets from solar active regions where these impulsive SEPs occur. However, a few small events are unusual; several have suppressed 4He, and rarely, a few very small events with steep spectra have elements N or S greatly enhanced, perhaps by the same resonant-wave mechanism that enhances 3He. Which mechanism will dominate? The impulsive SEP events we see are associated with narrow CMEs, from solar jets where magnetic reconnection on open field lines gives energetic particles and CMEs direct access to space. Gamma-ray lines tell us that the same acceleration physics may occur in flares.
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Reames, Donald V. "Element Abundances and FIP: SEPs, Corona, and Solar Wind." In Solar Energetic Particles. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-66402-2_8.

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AbstractWe have used abundance measurements to identify the sources and the physical processes of acceleration and transport of SEPs. Here we study energetic particles themselves as samples of the solar corona that is their origin, distinguishing the corona from the photosphere and the SEPs from the solar wind. Theoretically, differences in the first ionization potential “FIP effect” may distinguish closed- and open-field regions at the base of the corona, which may also distinguish SEPs from the solar wind. There is not a single coronal FIP effect, but two patterns, maybe three. Are there variations? What about He?
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Reames, Donald V. "Introduction." In Solar Energetic Particles. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-50871-9_1.

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Reames, Donald V. "History." In Solar Energetic Particles. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-50871-9_2.

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Reames, Donald V. "Distinguishing the Sources." In Solar Energetic Particles. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-50871-9_3.

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Reames, Donald V. "Impulsive SEP Events." In Solar Energetic Particles. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-50871-9_4.

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Conference papers on the topic "Solar energetic particles"

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Cane, H. V., I. G. Richardson, and G. Wibberenz. "Energetic particles and solar wind disturbances." In Proceedings of the eigth international solar wind conference: Solar wind eight. AIP, 1996. http://dx.doi.org/10.1063/1.51494.

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Ruffolo, D. "INTERACTING AND ESCAPING SOLAR ENERGETIC PARTICLES." In 25th International Cosmic Ray Conference. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789814529044_0007.

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Tsvetkov, Tsvetan, Rositsa Miteva, and Nikola Petrov. "Filaments related to solar energetic particles." In 10th Jubilee International Conference of the Balkan Physical Union. Author(s), 2019. http://dx.doi.org/10.1063/1.5091227.

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Reames, Donald V. "Solar energetic particles and space weather." In Space technology and applications international forum - 2001. AIP, 2001. http://dx.doi.org/10.1063/1.1358070.

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Cliver, Edward W. "Solar energetic particles: Acceleration and transport." In The 26th international cosmic ray conference (ICRC). AIP, 2000. http://dx.doi.org/10.1063/1.1291471.

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Stone, E. C. "Solar abundances as derived from solar energetic particles." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.37986.

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Reames, Donald V. "Energetic particles from solar flares and coronal mass ejections." In High energy solar physics. AIP, 1996. http://dx.doi.org/10.1063/1.50970.

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Rozhkova, D. V., L. K. Kashapova, and I. N. Myagkova. "MODELING OF TIME PROFILES OF EVENTS IN SOLAR ENERGETIC PARTICLES." In All-Russia Conference on Solar and Solar-Terrestrial Physics. The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo, 2023. http://dx.doi.org/10.31725/0552-5829-2023-281-284.

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Cohen, C. M. S. "The isotopic composition of solar energetic particles." In Acceleration and transport of energetic particles observed in the heliosphere (ACE-2000 symposium). AIP, 2000. http://dx.doi.org/10.1063/1.1324281.

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von Rosenvinge, Tycho, Ian Richardson, H. V. Cane, et al. "The Longitudinal Distribution of Solar Energetic Particles." In The 34th International Cosmic Ray Conference. Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0104.

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Reports on the topic "Solar energetic particles"

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Velinov, Peter I. Y., and Lachezar Mateev. Anisotropic Penetration of Solar Energetic Particles in the Earth Environment. "Prof. Marin Drinov" Publishing House of Bulgarian Academy of Sciences, 2018. http://dx.doi.org/10.7546/crabs.2018.03.11.

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Kahler, Stephen W. Renewal: New Aspects of Acceleration and Transport of Solar Energetic Particles (SEPs) from the Sun to the Earth. Defense Technical Information Center, 2014. http://dx.doi.org/10.21236/ada619635.

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Kahler, S. W. Coronal Mass Ejections and Solar Energetic Particle Events,. Defense Technical Information Center, 1996. http://dx.doi.org/10.21236/ada319321.

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Nitta, N. V., E. W. Cliver, A. J. Tylka, and P. Smit. Source Regions of Major Solar Energetic Particle Events. Defense Technical Information Center, 2003. http://dx.doi.org/10.21236/ada423842.

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Guo, Fan. Understanding Energetic Particle Dynamics in Solar and Heliospheric Science. Office of Scientific and Technical Information (OSTI), 2017. http://dx.doi.org/10.2172/1373515.

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Kahler, S. W. Solar Fast Wind Regions as Sources of Gradual 20 MeV Solar Energetic Particle Events. Defense Technical Information Center, 2003. http://dx.doi.org/10.21236/ada423046.

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Makela, Pertti, Nat Gopalswamy, Hong Xie, Sachiko Akiyama, Seiji Yashiro, and Neeharika Takur. On the Properties of Solar Energetic Particle Events Associated with Metric Type II Radio Bursts. Balkan, Black sea and Caspian sea Regional Network for Space Weather Studies, 2020. http://dx.doi.org/10.31401/sungeo.2019.02.04.

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Gopalswamy, Nat, Pertti Mäkelä, Hong Xie, Sachiko Akiyama, Seiji Yashiro, and Neeharika Takur. On the Properties of Solar Energetic Particle Events Associated with Metric Type II Radio Bursts. Balkan, Black sea and Caspian sea Regional Network for Space Weather Studies, 2020. http://dx.doi.org/10.31401/sungeo.2020.02.04.

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