61![Title: From X-ray observations of solar flare energetic electrons, to new models of particle acceleration and transport Speaker: Eduard Kontar (Glasgow University) Abstract: Recent hard X-ray observations of solar flares Title: From X-ray observations of solar flare energetic electrons, to new models of particle acceleration and transport Speaker: Eduard Kontar (Glasgow University) Abstract: Recent hard X-ray observations of solar flares](https://www.pdfsearch.io/img/deb92bc77153b35c480837c047e9a348.jpg) | Add to Reading ListSource URL: www.mssl.ucl.ac.uk- Date: 2009-11-06 09:40:19
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62![J. Fluid Mech.(2002), vol. 000, pp.1-24. ã 2002 Cambridge University Press DOI: S0022112001007145 Printed in the United Kingdom Slip velocity and lift J. Fluid Mech.(2002), vol. 000, pp.1-24. ã 2002 Cambridge University Press DOI: S0022112001007145 Printed in the United Kingdom Slip velocity and lift](https://www.pdfsearch.io/img/5111a555fa219f46e15ff52c40f5ec73.jpg) | Add to Reading ListSource URL: www.aem.umn.eduLanguage: English - Date: 2001-12-20 10:09:29
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63![Magnetic field amplification and electron acceleration to near-energy equipartition with ions by a mildly relativistic quasi-parallel plasma protoshock Magnetic field amplification and electron acceleration to near-energy equipartition with ions by a mildly relativistic quasi-parallel plasma protoshock](https://www.pdfsearch.io/img/808fc16e84ee27b5175c86d2e5604533.jpg) | Add to Reading ListSource URL: www.aanda.orgLanguage: English |
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64![Solar Energetic Particle Acceleration at a CME-Driven Coronal/Interplanetary Shock Solar Energetic Particle Acceleration at a CME-Driven Coronal/Interplanetary Shock](https://www.pdfsearch.io/img/236c92958c50a72363032d140a23f165.jpg) | Add to Reading ListSource URL: www.vsp.ucar.edu- Date: 2010-12-14 17:06:01
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65![DIFFUSIVE SCATTERING AND WAVE-PARTICLE COUPLING IN FRONT OF THE EARTH’S QUASI-PARALLEL BOW SHOCK A. Kis2 , M. Scholer1 , B. Klecker1 , E. A. Lucek3 , I. Dandouras4 , I. Lemperger2 , V. Wesztergom2 1 Max-Planck-Institut DIFFUSIVE SCATTERING AND WAVE-PARTICLE COUPLING IN FRONT OF THE EARTH’S QUASI-PARALLEL BOW SHOCK A. Kis2 , M. Scholer1 , B. Klecker1 , E. A. Lucek3 , I. Dandouras4 , I. Lemperger2 , V. Wesztergom2 1 Max-Planck-Institut](https://www.pdfsearch.io/img/e4e23af2f4a35ae8ba16993e668516d4.jpg) | Add to Reading ListSource URL: physics.bgu.ac.ilLanguage: English - Date: 2014-01-24 14:15:09
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66![PARTICLE ACCELERATION BY CASCADING ALFVEN WAVE TURBULENCE David Eichler Department of Physics, Ben-Gurion University of the Negev Particle acceleration by cascading Alfven wave turbulence was suggested (Eichler, 1979) as PARTICLE ACCELERATION BY CASCADING ALFVEN WAVE TURBULENCE David Eichler Department of Physics, Ben-Gurion University of the Negev Particle acceleration by cascading Alfven wave turbulence was suggested (Eichler, 1979) as](https://www.pdfsearch.io/img/ecfdc910d6fa468fd1b8de5e4389f8a5.jpg) | Add to Reading ListSource URL: physics.bgu.ac.ilLanguage: English - Date: 2014-01-24 14:14:59
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67![Microsoft Word - interaction-rayonnement-matiere-en.doc Microsoft Word - interaction-rayonnement-matiere-en.doc](https://www.pdfsearch.io/img/b8062d9652a627f299076415e4091845.jpg) | Add to Reading ListSource URL: www-hpc.cea.frLanguage: English - Date: 2010-01-08 05:32:42
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68![Particle acceleration in shocks driven by Coronal Mass Ejections (CMEs) is usually considered to be the most important mechanism in the genesis of large solar energetic particle (SEP) events, although SEP acceleration in Particle acceleration in shocks driven by Coronal Mass Ejections (CMEs) is usually considered to be the most important mechanism in the genesis of large solar energetic particle (SEP) events, although SEP acceleration in](https://www.pdfsearch.io/img/6df9b30439e4b828cbd0c01655483d23.jpg) | Add to Reading ListSource URL: solarorbiter4.org- Date: 2011-05-17 20:49:54
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69![EGU General Assembly[removed]ST – Solar-Terrestrial Sciences – Orals Monday, 28 April MO1, 08:30–10:00 ST1.3, Particle acceleration mechanisms in solar system plasmas: observations and theory, 08:30–10:00, Room Y10 EGU General Assembly[removed]ST – Solar-Terrestrial Sciences – Orals Monday, 28 April MO1, 08:30–10:00 ST1.3, Particle acceleration mechanisms in solar system plasmas: observations and theory, 08:30–10:00, Room Y10](https://www.pdfsearch.io/img/de7a6d28e36dfc74648115928e6bca2e.jpg) | Add to Reading ListSource URL: www.egu2014.euLanguage: English - Date: 2014-04-02 08:35:07
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70![Combining lasers could shrink particle accelerators from kilometers to meters Combining lasers could shrink particle accelerators from kilometers to meters](https://www.pdfsearch.io/img/10b3b0d492f600d38d4e46d4aa129809.jpg) | Add to Reading ListSource URL: phys.orgLanguage: English - Date: 2015-04-16 07:59:22
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