'Pickup ions' diaporamas de présentation

NSO Summer School Lecture 1: Solar Wind Structure and Waves

NSO Summer School Lecture 1: Solar Wind Structure and Waves. Charles W. Smith Space Science Center University of New Hampshire Charles.Smith@unh.edu. Good References:.

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cosmic ray acceleration and shocks in heliosphere

cosmic ray acceleration and shocks in heliosphere. chung-ming ko institute of astronomy and department of physics, national central university, taiwan (R.O.C.). SC4, Lebedev Institute, Moscow, Russia, 2009.05.18. a short discussion on. cosmic ray acceleration basics propagation

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Review of CIR-related Particle Composition, Charge States, & Energy Spectra

Review of CIR-related Particle Composition, Charge States, & Energy Spectra. Joe Mazur The Aerospace Corporation Glenn Mason Johns Hopkins/APL Joe Dwyer Florida Institute of Technology Mihir Desai Southwest Research Institute. Processes for 1 AU observations of solar material.

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Review of CIR-related Particle Composition, Charge States, & Energy Spectra

Review of CIR-related Particle Composition, Charge States, & Energy Spectra. Joe Mazur The Aerospace Corporation Glenn Mason Johns Hopkins/APL Joe Dwyer Florida Institute of Technology Mihir Desai Southwest Research Institute. Processes for 1 AU observations of solar material.

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STEREO SWG: PLASTIC Science Snipits Toni Galvin (UNH) for the PLASTIC Team

STEREO SWG: PLASTIC Science Snipits Toni Galvin (UNH) for the PLASTIC Team Special thanks to K. Simunac, B. Klecker. STEREO PLASTIC Institutions: UNH, U Bern, MPE, U Kiel, NASA/GSFC IDPU/LVC provided by UCB (IMPACT). The Sun in EUV courtesy STEREO/SECCHI/NRL.

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Interstellar and Interplanetary Material

Interstellar and Interplanetary Material. HST Astrobiology Workshop: May 5-9, 2002 P.C. Frisch University of Chicago. Outline:. The solar system is our template for understanding interplanetary material Heliosphere, solar wind, ISM Astrospheres Interstellar and interplanetary matter

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Importance of Pickup Ions & Suprathermal Ions in the Inner Heliosphere

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Inner Source Pickup Ions

Inner Source Pickup Ions. Pran Mukherjee. Outline. Introduction Current theories and work Addition of new velocity components Summary Questions. Introduction. First, a few definitions:

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Pre-accelerated seed populations of energetic particles in the heliosphere

Pre-accelerated seed populations of energetic particles in the heliosphere. N. A. Schwadron* and M. Desai Southwest Research Institute *Also, Boston University. Miracle occurs. Where do energetic particles and cosmic rays come from?. Plasma : Solar Wind, Coronal Plasma.

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Pre-accelerated seed populations of energetic particles in the heliosphere

Pre-accelerated seed populations of energetic particles in the heliosphere. N. A. Schwadron* and M. Desai Southwest Research Institute *Also, Boston University. Miracle occurs. Where do energetic particles and cosmic rays come from?. Plasma : Solar Wind, Coronal Plasma.

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ACE uses Solar Gravitational Lensing of Interstellar Helium to infer Interstellar Gas Temperature

ACE uses Solar Gravitational Lensing of Interstellar Helium to infer Interstellar Gas Temperature. The temperature of the interstellar gas surrounding our solar system has been inferred from observations of pickup ions with the SWICS instrument on ACE.

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Adiabatic Modeling of Inner Source Pickup Ions

Abstract.

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