'Solar modulation' presentation slideshows

AMS as an Astroparticle Physics Experiment

AMS as an Astroparticle Physics Experiment. ? 4 ? ?????? ???? 6 ? 19 ? ( ? ) ? ??. Astroparticl Physics is Connecting Quarks with the Cosmos. Neutron. Proton. Periodic System of Elementary Particles. What Powered the Big Bang?. Inflation (Big Bang plus 10 -34 Seconds).

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John W. Bieber Bartol Research Institute, University of Delaware, Newark

APS Division of Plasma Physics Nov 15-19, 2004 Savannah, Georgia TRANSPORT AND MODULATION OF COSMIC RAYS IN THE SOLAR WIND. John W. Bieber Bartol Research Institute, University of Delaware, Newark Supported by NSF grant ATM-0000315 Visit our Website:

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Results from the PAMELA space experimen t

Results from the PAMELA space experimen t. Roberta sparvoli University of rome Tor Vergata & INFN ( italian National institute of nuclear physics). PAMELA Payload for Matter/antimatter Exploration and Light-nuclei Astrophysics. Direct detection of CRs in space

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Space Education

A.Chilingarian Particle detectors networks for the Fundamental Physics, Space Weather and Education Cosmic Ray Division, Alikhanyan Physics Institute,Yerevan, Armenia ASEC and ANI collaborations. Space Education.

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Ulysses: Cosmic rays in 4 Dimensions

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PAMELA measurements of proton and helium nuclei and cosmic ray acceleration in the galaxy

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GLAST Solar System Science Gerry Share, UMd/NRL Also see the following posters:

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The Gulmarg Neutron Monitor

The Gulmarg Neutron Monitor. Ramesh Koul Astrophysical Sciences Division Bhabha Atomic Research Centre Mumbai 400 085. NM configurations. # IGY 1957/58 eff. ~ 1.9% # NM64 1964 eff. ~ 5.7% # He3 based # Gd doped liquid scintillator. Gulmarg Neutron Monitor (GNM).

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Contents 1. Motivation of the Observation

To high altitude. The 28th ICRC (ICRC2003, Tsukuba, Japan) Oral session on Solar&Heliospheric Phenomena (SH3.4; Long-term variations) Solar modulation effect on the cosmic-ray proton spectra measured by BESS Yoshiaki Shikaze (Kobe University) for the BESS Collaboration. Balloon.

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AESOP and LEE Instruments

AESOP and LEE Instruments. A niti - E lectron S ub- O rbital P ayload. L ow E nergy E lectrons. AESOP and LEE 1999 tandem flight. AESOP departing Esrange 2006. LEE hangtest for Big-60 launch 2002. John Clem and Paul Evenson Bartol Research Institute. NASA grant: NNG05WC08G. Introduction.

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There are 4 major steps in determining fluxes in the atmosphere

There are 4 major steps in determining fluxes in the atmosphere Determine the composition and spectrum of cosmic rays at local interstellar space Solar Modulation Geomagnetic Cutoff Transport of particles through the atmosphere In this analysis 1 & 2 are combined

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Objectives for IMS group

Objectives for IMS group. Kenji Yoshida Shibaura Institute of Technology. Approval of M&S framework. CALET Team Organization |B. CALET Science Team. IEC ( International Executive Committee ). JAXA NASA ASI. - Science Data Handling - Science Analysis - Science Publications.

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Cosmic-Ray Background Flux Model for Hard X-ray/Gamma-ray Balloon and Satellite Experiments

Cosmic-Ray Background Flux Model for Hard X-ray/Gamma-ray Balloon and Satellite Experiments. T sunefumi Mizuno , T uneyoshi Kamae (Stanford Linear Accelerator Center) , Masanobu Ozaki (JAXA) and Yasushi Fukazawa (Hiroshima Univ.). Abstract:.

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Charge Sign Dependence in Cosmic Ray Solar Modulation

Abstract #2368. NASA grants: NNG05WC08G,NNX08BA62G. Charge Sign Dependence in Cosmic Ray Solar Modulation. John Clem and Paul Evenson Bartol Research Institute, Department of Physics and Astronomy, University of Delaware.

84 views • 1 slides