'100 kev' presentation slideshows

Lattice, Injection Line and General ELENA Performance Limitations

Lattice, Injection Line and General ELENA Performance Limitations. Pavel Belochitskii. Choice of extraction energy. Extraction energy E kin =100 keV allows to increase significantly an amount of captured antiprotons ( ~30%) If go to lower energy, one meets strong limitations imposed by:

521 views • 43 slides

Lattice, Injection Line and General ELENA Performance Limitations

Lattice, Injection Line and General ELENA Performance Limitations. Pavel Belochitskii. Choice of extraction energy. Extraction energy E kin =100 keV allows to increase significantly an amount of captured antiprotons ( ~30%) If go to lower energy, one meets strong limitations imposed by:

432 views • 43 slides

Missioni in Corso INTEGRAL: UN ANNO IN ORBITA XMM-NEWTON: QUATTRO ANNI DI SCIENZA

473 views • 35 slides

Astrophysics and Evolution of Supermassive Black Holes

396 views • 26 slides

Physics Board Review X-Ray Attenuation Interactions of x-rays with matter

802 views • 26 slides

INTEGRAL producing science for more than 4 years in the soft g -ray range (15 keV to MeV)

P. Ubertini on behalf of the IBIS Survey Team. INTEGRAL producing science for more than 4 years in the soft g -ray range (15 keV to MeV). The INTEGRAL Sky. The lower image shows a false colour image of the central region of our galaxy.

359 views • 25 slides

HES-HKS analysis meeting

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Status report of the new Darmstadt polarized electron injector*

Status report of the new Darmstadt polarized electron injector*. Yuliya Poltoratska PESP2008, 1.10.2008. S-DALINAC Polarized electron source Requirements Electron gun Characterization of the electron beam Implementation at the S-DALINAC. *Supported by DFG through SFB 634 and GRK 410.

386 views • 21 slides

Cosmic X-ray Background with Swift/BAT: un update (and some new results)

Cosmic X-ray Background with Swift/BAT: un update (and some new results). M. Ajello (MPE-Garching) with G.Sato, J. Greiner, G. Hasinger, G. Kanbach, A. Strong, N. Gehrels, J. Tueller, C. Markwardt. Submitted on Apr. 2nd. Gilli et al. 2007. CXB problem.

291 views • 19 slides

Extra Low Energy Antiproton Ring (ELENA) for antiproton deceleration after the AD

Extra Low Energy Antiproton Ring (ELENA) for antiproton deceleration after the AD. Pavel Belochitskii for the AD team On behalf of the AD users community. Beam from AD: 3 10 7 antiprotons per cycle at energy 5.3 MeV with transverse emittances 1 to 2 ? mm mrad.

283 views • 18 slides

Validation of GEANT4 versus EGSnrc

Validation of GEANT4 versus EGSnrc. Yann PERROT LPC, CNRS/IN2P3 perrot@clermont.in2p3.fr. Motivation. Electron transport crucial to provide accurate dose estimation for medical physics applications ( accuracy ~2-3%)

339 views • 17 slides

Microwave emission from the trapped and precipitated electrons in solar bursts

Microwave emission from the trapped and precipitated electrons in solar bursts. J. E. R. Costa and A. C. Rosal1 2005, A&A, 436, 347. Abstract.

297 views • 17 slides

PLASMA KINETICS MODELS FOR FUSION SYSTEMS BASED ON THE AXIALLY-SYMMETRIC MIRROR DEVICES

PLASMA KINETICS MODELS FOR FUSION SYSTEMS BASED ON THE AXIALLY-SYMMETRIC MIRROR DEVICES. A . Yu . Chirkov 1) , S . V . Ryzhkov 1) , P . A . Bagryansky 2) , A . V . Anikeev 2) 1) Bauman Moscow State Technical University, Moscow, Russia

238 views • 16 slides

Jacques Paul

Soft Gamma-Ray Astronomy. Expected Impact on VHE Phenomena Panorama in the Coming Years. Jacques Paul. INTEGRAL Mission Scientist CEA/DSM/DAPNIA/Service d'Astrophysique CEA-Saclay, France. 23 January 2001. Rencontres de Moriond Les Arcs. Foreword.

297 views • 16 slides

HAPPY NEW YEAR 2019 !!! YEAR OF THE FCC !!!

HAPPY NEW YEAR 2019 !!! YEAR OF THE FCC !!!. Welcome to the XIth FCC- ee Work shop*): THEORY AND EXPERIMENTS. *) Work : 107 ( registered ) participants for ~100 presentations O rganization : c ongratulations and many thanks to

154 views • 15 slides

Dave Tierney S. McBreen, R. Preece, G. Fitzpatrick and the GBM Team

Low-Energy Spectral Deviations in a Sample of GBM GRBs. Dave Tierney S. McBreen, R. Preece, G. Fitzpatrick and the GBM Team. DT acknowledges support from SFI under grant No. 09-RFP-AST-2400. Introduction. Band Model Spectral model for fitting prompt GRB emission Consistent across GRBs

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Update on science with Suzaku HXD

Update on science with Suzaku HXD. G. Madejski, on behalf of the HXD Team: K. Abe, Y. Ezoe, Y. Fukazawa, S. Hong, H. Inoue, K. Ito, T. Itoh, T. Kamae, D. Kasama, M. Kawaharada, N. Kawano, K. Kawashima, S. Kawasoe, Y. Kobayashi, M. Kokubun, J. Kotoku,

222 views • 8 slides

Update on science with Suzaku HXD

Update on science with Suzaku HXD. G. Madejski, on behalf of the HXD Team: K. Abe, Y. Ezoe, Y. Fukazawa, S. Hong, H. Inoue, K. Ito, T. Itoh, T. Kamae, D. Kasama, M. Kawaharada, N. Kawano, K. Kawashima, S. Kawasoe, Y. Kobayashi, M. Kokubun, J. Kotoku,

195 views • 8 slides

Thoughts on why G0 needed position feedback and HAPPEX didn't

Thoughts on why G0 needed position feedback and HAPPEX didn't. The practical reason why G0 needed position feedback and HAPPEX didn't is simple: Values of HAPPEX position differences (with no feedback) were typically < 20 nm (see figures in following slides)

71 views • 7 slides

Beam Test on Astronomical Hard X-ray Polarimeter PoGO

Beam Test on Astronomical Hard X-ray Polarimeter PoGO. Abstract:.

99 views • 1 slides