'Hard x' presentation slideshows

Overview of what we saw in Lectutre 07

Heliosphere - Lecture 8 November 08, 2005 Space Weather Course Electromagnetic Radiation in the Heliosphere Radio Emission Numerical studies of CME Acceleration and Transport of Particles SEP in Shocks Chapter 7 - Kallenrode (Energetic Particles in the Heliosphere). What we saw:

938 views • 68 slides

Recent Progress in MHD studies on HL-2A tokamak and Future plans

Recent Progress in MHD studies on HL-2A tokamak and Future plans. Yi Liu, Y.B.Dong, W. Deng, J.Zhou, X.T.Ding. South w estern Institute of Physics, Chengdu 610041 , China e-mail contact of main author:yiliu@swip.ac.cn. Outline. Experimental results on MHD activities

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NB: Those slides dedicated to real observations are just white like this one.

NB: in the presentation, those slides describing virtual observations in the project have a light blue background like this one -. NB: Those slides dedicated to real observations are just white like this one. Project Description :. = astro-ph/0110511

432 views • 35 slides

TSI and VUV Radiative Energies During X-Class Solar Flares

TSI and VUV Radiative Energies During X-Class Solar Flares . Chris Moore Undergraduate Student U. of Iowa (2 summers at LASP/U. Of Colorado) Phillip Chamberlin, Rachel Hock, Greg Kopp LASP/U. of Colorado. Research Objectives.

369 views • 24 slides

Modelling the high mass accretion rate spectra of GX 339-4

Modelling the high mass accretion rate spectra of GX 339-4. Mari Kolehmainen & Chris Done Durham University Maria Diaz Trigo, ESO. High Energy View of Accreting Objects: X-ray Binaries Agios Nikolaos, Crete 2010. High mass accretion rate spectra. classical high/soft state disc dominated

352 views • 22 slides

Coronal hard X-ray sources and associated radio emissions

Coronal hard X-ray sources and associated radio emissions. N. Vilmer D. Koutroumpa (Observatoire de Paris- LESIA; Thessaloniki University) S.R Kane G. Hurford (Space Sciences Laboratory Berkeley). Background: CORONAL ABOVE THE LOOP TOP SOURCES

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T0 MY PRESENTATION MD. SHOBHAN

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The PHENEX Experiment Results in 2006 and Future Plan

The PHENEX Experiment Results in 2006 and Future Plan. P olarimetry for H igh ENE rgy X rays. S. Gunji* a , Y. Kishimoto a ,H. Sakurai a , F. Tokanai a , M. Kanno a , Y. Ishikawa a , Hayashida b , N. Anabuki b , H. Tsunemi b , T. Mihara c ,

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Comment on the observational aspects of M82X-1: intermediate-mass BH?

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ULIRGs in hard X-ray: From XMM to Simbol X

ULIRGs in hard X-ray: From XMM to Simbol X. V. Braito. Review past X-ray observations of ULIRGs Open questions: relative contribution SB and AGN Need of observation above 10 keV. 1.ULI R Gs are predominantly powered by heavily d ust enshrouded AGN or circumnuclear SB ?.

278 views • 14 slides

Reconstruct the FEL x-ray profile with X-TCAV after undulator

Reconstruct the FEL x-ray profile with X-TCAV after undulator. Y. Ding, C. Behrens 3/18/2011. Thanks Zhirong and Paul for helpful discussions. Laser Heater Measurements. I nteraction between laser and electrons in wiggler leads to the increase of energy spread;

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Ay 191 Experiment Development of Hard X-ray Imaging Detectors J. Hong, B. Allen and J. Grindlay

Ay 191 Experiment Development of Hard X-ray Imaging Detectors J. Hong, B. Allen and J. Grindlay. Hard X-rays (~5-600 keV) are direct probes of black holes : GRBs, AGNs, Stellar BHs, etc.

177 views • 6 slides

Wide Band Spectrometer Archives (Draft Plan)

Wide Band Spectrometer Archives (Draft Plan). Tetsuya Watanabe Nat. Astron. Obs. Japan. - 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

163 views • 6 slides

ERL working modes

ERL working modes. Georg Hoffstaetter, Professor Cornell University / CLASSE / SRF group & ERL effort. High Current mode High Coherence mode High Buch charge mode HGHG FEL mode ? SASE FEL mode ? XFEL-O mode ?. Beam goals for ERLs. Hard x-rays: 5GeV, competitive current: up to 100mA

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Discussions/Clarifications on technical subjects:

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C. Y. Hui & W. Becker

X-Ray Studies of the Central Compact Objects in Puppis-A & RX J0852.0-4622. C. Y. Hui & W. Becker. Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse 85748 Garching, Germany.

165 views • 1 slides

Hard X-ray Telescope for the FFAST project

Hard X-ray Telescope for the FFAST project. Hironori Matsumoto (Nagoya University) Miyata, Y., Furuzawa , A., Kunieda , H. (Nagoya Univ.), Ishida, N., Furuta , H., Yamamoto, Y. ( Tamagawa Engineering), Tsunemi , H. (Osaka Univ.) & FFAST team. 1. The FFAST project. 3 . Mirror design.

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1. Introduction

Table 1. Summary of the XMM-Newton observations of Her X-1 . For the orbital phase we used the ephemeris of Deeter et al. (1991); for the 35d phasing we define ? 35 =0 at the main-on turn-on. XMM-NEWTON EPIC OBSERVATIONS OF Her X-1

107 views • 1 slides