Yohkoh Gallileo Kick-off Nobeyama 10~11-Jul-2002 Wide Band Spectrometer Archives (Draft Plan) Tetsuya Watanabe Nat. Astron. Obs. Japan.

Slides:

Advertisements

Similar presentations

Workshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”, 6 – 8 December 2005, Wrocław Spectroscopy Department.

Advertisements

Ryo Yamazaki (Osaka University, Japan) With K. Ioka, F. Takahara, and N. Shibazaki.

1 T. Mizuno et al. August 23, 2014 HEAPA Symposium on Future T. Mizuno (Hiroshima Univ.) on behalf of the SGD team and Polarization team.

Yohkoh Galileo meeting J. Sato The Goal of the Flare Catalogue 1: Sufficient information for flare analysis 2: Easy access to the Catalogue Direct and.

EGRET unidentified sources and gamma-ray pulsars I. CGRO mission and the instrument EGRET and it’s scientific goals II. Simple introduction of EGRET sources.

X-Ray Observation and Analysis of a M1.7 Class Flare Courtney Peck Advisors: Jiong Qiu and Wenjuan Liu.

Terrestrial Gamma-ray Flashes. Gamma Ray Astronomy Beginning started as a small budget research program in 1959 monitoring compliance with the 1963 Partial.

Measuring the Temperature of Hot Solar Flare Plasma with RHESSI Amir Caspi 1,2, Sam Krucker 2, Robert P. Lin 1,2 1 Department of Physics, University of.

Important Work for Today Definition of HXT data archive Definition of WBS data archive Assign responsibilities and agree SCHEDULE Discuss new or improved.

Uses of solar hard X-rays Basics of observations Hard X-rays at flare onset The event of April 18, 2001 Conclusions Yohkoh 10th Jan. 21, 2002Hugh Hudson,

Danish Space Research Institute Danish Small Satellite Programme FH Space_Environment.ppt Slide # 1 Flemming Hansen MScEE, PhD Technology Manager.

Paul Sellin, Radiation Imaging Group Digital pulse shape discrimination applied to capture-gated neutron detectors P.J. Sellin, S. Jastaniah, W. Catford.

Photons of Light The smallest unit of light is a photon A photon is often called a particle of light The Energy of an individual photon depends on its.

GAMMA RAY SPECTROSCOPY

S. Zuberi, University of Rochester Digital Signal Processing of Scintillator Pulses Saba Zuberi, Wojtek Skulski, Frank Wolfs University of Rochester.

AGATA Demonstrator Test With a 252 Cf Source: Neutron-Gamma Discrimination Menekşe ŞENYİĞİT.

Henry L. Clark, Ph D Accelerator Physicist / SEE Line Project Manager / Upgrade Project Manager Cyclotron Institute, Texas A&M University.

GLAST Simulations Theodore E. Hierath Louisiana State University August 20, 2001.

The Yohkoh Galileo Project --- International Coordination Meeting Nobeyama, Japan July 2002.

HETE- 2 OBSERVATIONS OF THE EXTREMELY SOFT X-RAY FLASH XRF Liang Jau-shian Institute of Physics, NTHU.

Tests of a 10cm by 10cm triple GEM detector

WHAT ASTRONOMERS LEARN ABOUT THE ELECTROMAGNETIC SPECTRUM.

Something about Institute of Automatics, neutron generators and radiation hardness Institute of Automatics, Neutron Generators, Detectors and Radiation.

2009 Jun 24The Solar Science Data Center F. Breitling 1 The Solar Science Data Center F. Breitling, G. Mann, C. Vocks, H. Enke 2 nd Workshop of the Solar.

Martin Cupák seznam.cz)‏ The First SphinX Workshop May 2007, Wroclaw, Poland Experience with the software of Czech HXRS X-ray photometer.

R. Jansen TEC-EDM 1 Cosmic Vision Instrumentation ASIC 24-September 2009.

Interrelation between Cosmic Rays, Magnetosphere particles and the Earth Atmospheric Phenomena- Prospects of Experimental Study from Satellites M.I. Panasyuk.

RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.

High Energy Measurements for Solar, Heliospheric, Magnetospheric, and Atmospheric Physics R. P. Lin J. Sample, A. Shih, S. Christe, S. Krucker, I. Hannah.

NASSP Masters 5003F - Computational Astronomy Lecture 19 EPIC background Event lists and selection The RGA Calibration quantities Exposure calculations.

Laue lenses for hard X-rays (> 60 keV) F. Frontera and A. Pisa on behalf of a Large Collaboration Rome, 18 March 2005.

2001 Mars Odyssey GRS RDS 1 HEND Workshop 2002 May 20 th – 22 nd 2002 Mars Odyssey Gamma-Ray Spectrometer Richard Starr NASA/GSFC – Catholic University.

Aspen 4/28/05Physics at the End of the Galactic Cosmic Ray Spectrum - “Below the Knee” Working Group “Below the Knee” Working Group Report - Day 3 Binns,

Gamma-Ray Bursts observed with INTEGRAL and XMM- Newton Sinead McGlynn School of Physics University College Dublin.

Jacques Paul Soft Gamma-Ray Astronomy 23 January 2001 Rencontres de Moriond Les Arcs Expected Impact on VHE Phenomena Panorama in the Coming Years INTEGRAL.

Gamma-Ray Telescopes. Brief History of Gamma Ray Astronomy 1961 EXPLORER-II: First detection of high-energy  -rays from space 1967 VELA satelllites:

Hard X and Gamma-ray Polarization: the ultimate dimension (ESA Cosmic Vision ) or the Compton Scattering polarimetery challenges Ezio Caroli,

11 th iWoRiD, Prague, Czech Republic Low-power Wide-dynamic-range Readout System for a 64-channel Multi-anode PMT of a Scintillation Gamma Camera Satoru.

MEASUREMENT Of γ-RAY ENERGY SPECTRA BY A SCINTILLATION COUNTER

Electromagnetic Spectrum. Different Types of Light  Light is a form of energy  It travels in waves  Also called Electromagnetic Radiation  Some Electromagnetic.

Electromagnetic Spectrum. The Universe The Big Bang forms the universe….. The energy creates stars. Gravity pulls stars together into Galaxies. The stars.

The AMS Transition Radiation Detector and the Search for Dark Matter Gianpaolo Carosi Lab for Nuclear Science, MIT The AMS Collaboration Lake Louise Winter.

Development of X-ray Spectrometry for Nuclear Decay Data Applications at IFIN-HH Aurelian Luca Horia Hulubei National Institute of Physics and Nuclear.

What does mean neighbours ? At the same epoch –simultaneous (transient phenomenae) –before (can affect the SIMBOL-X observing plan) –after (can complement.

XIS Calibration at Osaka K. Hayashida, K. Torii, M. Namiki, T. Shiroshoji, M. Shoji, S. Kastuda, H. Tsunemi (Osaka University) T. Kohmura (Kougakuin University)

IDEE, The Electron Spectrometer of the Taranis Mission J.-A. Sauvaud 1, A. Fedorov 1, P. Devoto 1, C. Jacquey 1, L. Prech 2, Z. Nemecek 2, F. Lefeuvre.

X-ray follow-ups of TeV unID sources using Suzaku Aya, T. Bamba (ISAS/JAXA, Japan) R. Yamazaki, K. Kohri, H. Matsumoto, H. Yamaguchi, G. Pühlhofer, S.

The science objectives for CALET Kenji Yoshida (Shibaura Institute of Technology) for the CALET Collaboration.

Watch This Space! Monsters at Work Liz Puchnarewicz Mullard Space Science Laboratory University College London.

Accelerator Physics, JU, First Semester, (Saed Dababneh). 1 In the figure: Photoelectric suppressed. Single Compton (effect of crystal dimensions).

LYRA Calibration, Data Products, Plans I. E. Dammasch, ROB/SIDC PROBA2 Science Meeting Sun 360, Kiel, Jul 2011 LYRA the Large-Yield Radiometer onboard.

RHESSI Observation of Atmospheric Gamma Rays from Impact of Solar Energetic Particles on 21 April 2002.

Observation of cosmic gamma-ray bursts and solar flares in the ''RELEC'' experiment on the ''VERNOV'' satellite.

Space Telescopes.

RHESSI and the Solar Flare X-ray Spectrum Ken Phillips Presentation at Wroclaw Workshop “ X-ray spectroscopy and plasma diagnostics from the RESIK, RHESSI.

Determining the rp-Process Flow through 56 Ni 56 Ni is a Waiting Point and imposes a delay Decay Lifetime: 2.3x10^4 s ; Burst Time: 10 – 100 s Largest.

GLAST GLAST Burst Monitor Charles Meegan Principal Investigator NASA MSFC Steve Elrod Project Manager NASA MSFC

PoGO_G4_ ppt1 Study of BGO/Collimator Optimization for PoGO August 8th, 2005 Tsunefumi Mizuno, Hiroshima University/SLAC

Sep. 22, 2011 Seoul National University Jae Keum Lee KIMS Background 1 China-Korea Workshop 2011 September 22-23, 2011.

A New Solar Neutron Telescope working at the International Space Station K. Koga, T. Goka (PI), H. Matsumoto, T. Obara, O. Okudaira (JAXA) Y. Muraki (Nagoya)

April 28, 2009 IACHECH. Matsumoto1 Introduction of the Soft X-ray Imager (SXI) on board the Astro-H satellite H. Matsumoto (Kyoto Univ.) on behalf of the.

High Energy Observational Astrophysics. 1 Processes that emit X-rays and Gamma rays.

Fermi Gamma-ray Burst Monitor

for Lomonosov-GRB collaboration

GRM brief introduction

DAMA Calibrations – low energy

Energy Response of the X-ray Imaging Spectrometer (XIS) on Suzaku

GRB spectral evolution: from complex profile to basic structure

TWO-CHANNEL SPECTROMETRIC SYSTEM BASED ON UNCOOLED Si-DETECTORS AND GADOLINIUM CONVERTER FOR THERMAL NEUTRONS REGISTRATION G.P. Vasiliev1, V.M. Dubina1,

Hard X-ray Spectral Evolution and SEP Events

Presentation transcript:

Yohkoh Gallileo Kick-off Nobeyama 10~11-Jul-2002 Wide Band Spectrometer Archives (Draft Plan) Tetsuya Watanabe Nat. Astron. Obs. Japan

Yohkoh Gallileo Kick-off Nobeyama 10~11-Jul Data PC data Gamma-Ray Spectrometer (GRS) GRS-PC11, 12, 13, 14, 15, 16 GRS-PC21, 22, 23, 24, 25, 26 Hard X-ray Spectrometer (HXS) HXS-PC1,2 Soft X-ray Spectrometer (SXS) SXS-PC11, 12, 21, 22 Radiation Belt Monitor (RBM) RBM-SC-PC1,2 RBM-SSD-PC Gamma Burst Detector (GBD) GBD-PC1 (HXS) GBD-PC2 (RBM)

Yohkoh Gallileo Kick-off Nobeyama 10~11-Jul Data PH data Gamma-Ray Spectrometer (GRS) GRS-PHL1, 2 GRS-PHH Hard X-ray Spectrometer (HXS) HXS-PH Soft X-ray Spectrometer (SXS) SXS-PH1, 2 Radiation Belt Monitor (RBM) RBM-SC-PH

Yohkoh Gallileo Kick-off Nobeyama 10~11-Jul Data DHK data Gamma-Ray Spectrometer (GRS) GRS-UDH1, 2 GRS-CAL GRS-ADCLT1, 2 GRS-ADCHT1, 2 Hard X-ray Spectrometer (HXS) HXS-UD HXS-CAL HXS-ADCT Soft X-ray Spectrometer (SXS) SXS-UD1, 2 SXS-ADCT1, 2 Radiation Belt Monitor (RBM) RBM-SC-UD

Yohkoh Gallileo Kick-off Nobeyama 10~11-Jul Calibration Gamma Ray Spectrometer (GRS) channel vs. energy (root-square) gain ( 60 Co) +De-excitation Lines spectral resolution Hard X-ray Spectrometer (HXS) channel vs. energy (root-square) gain ( 241 Am) + annihilation line spectral resolution Soft X-ray Spectrometer (SXS) channel vs. energy (linear) gain ( 55 Fe) spectral resolution

Yohkoh Gallileo Kick-off Nobeyama 10~11-Jul Processed Data Gamma-Ray Spectrometer (GRS) Gamma-Ray Event & Spectra 14 Spectra among 38 events (Matsumoto 2002) & CalibrationCalibration Hard X-ray Spectrometer (HXS) “Big Event” Spectra  Time Plot /WBS Plot (digital ver) (cosmic) Gamma Burst Event List