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Blastwave in a rotating cloud PowerPoint PPT Presentation
Blastwave in a rotating cloud - Blastwave in a rotating cloud. Vary the blast intensity, nonrotating cloud. 0.304 mW. 0.363 mW. 0.221 mW. 0.460 mW. 0.415 mW. 0.515 mW ...
Blastwave in a rotating cloud. Vary the blast intensity, nonrotating cloud. 0.304 mW. 0.363 mW. 0.221 mW. 0.460 mW. 0.415 mW. 0.515 mW ...
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Flow at RHIC within the BlastWave framework PowerPoint PPT Presentation
Flow at RHIC within the BlastWave framework - A tool to study the system expansion. A tool to assess partonic collectivity? ... Hydro from: P. Kolb ,U.Heinz, review for 'Quark Gluon Plasma 3 , nucl-th/0305084 ...
A tool to study the system expansion. A tool to assess partonic collectivity? ... Hydro from: P. Kolb ,U.Heinz, review for 'Quark Gluon Plasma 3 , nucl-th/0305084 ...
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Why would I want to look at strange particle production? PowerPoint PPT Presentation
Why would I want to look at strange particle production? - Freeze-out T different Is blastwave realistic? ... Blastwave parameterization. STAR Preliminary. Helen Caines. Hot Quarks July 2004. 8 ...
Freeze-out T different Is blastwave realistic? ... Blastwave parameterization. STAR Preliminary. Helen Caines. Hot Quarks July 2004. 8 ...
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PowerPoint-Pr PowerPoint PPT Presentation
PowerPoint-Pr - Results: Blastwave analysis ... Results: Blastwave analysis fit results. open symbols: results from fit to mt - spectra only ...
Results: Blastwave analysis ... Results: Blastwave analysis fit results. open symbols: results from fit to mt - spectra only ...
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GRB afterglows in the Non-relativistic phase PowerPoint PPT Presentation
GRB afterglows in the Non-relativistic phase - For adiabatic blastwave: For highly radiative blastwave: The evolution of external shocks: ... For Newtonian blastwave (Sedov solution) ...
For adiabatic blastwave: For highly radiative blastwave: The evolution of external shocks: ... For Newtonian blastwave (Sedov solution) ...
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GRBs and Magnetic Fields PowerPoint PPT Presentation
GRBs and Magnetic Fields - Blastwave (FS ambient medium) Emission from Ejecta: Prompt gamma-rays ... Emission from Blastwave. Afterglows (X/Opt/Radio) Insensitive to the properties ...
Blastwave (FS ambient medium) Emission from Ejecta: Prompt gamma-rays ... Emission from Blastwave. Afterglows (X/Opt/Radio) Insensitive to the properties ...
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Spectra Physics at RHIC PowerPoint PPT Presentation
Spectra Physics at RHIC - Blastwave Fits at 130 & 200 GeV. Fits M. ... blastwave fit (green line) pT prediction for. Tch = 170 MeV. and b =0 ... with a blastwave fit at RHIC ...
Blastwave Fits at 130 & 200 GeV. Fits M. ... blastwave fit (green line) pT prediction for. Tch = 170 MeV. and b =0 ... with a blastwave fit at RHIC ...
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PHENIX Overview: Status of QGP PowerPoint PPT Presentation
PHENIX Overview: Status of QGP - Goal of Relativistic Heavy Ion collisions - to produce and characterize QGP state. ... analyses) using a hydro inspired 'Blastwave' model (F. Retiere, nucl-ex/0404024) ...
Goal of Relativistic Heavy Ion collisions - to produce and characterize QGP state. ... analyses) using a hydro inspired 'Blastwave' model (F. Retiere, nucl-ex/0404024) ...
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Azimuthallysensitive HBT in STAR PowerPoint PPT Presentation
Azimuthallysensitive HBT in STAR - full blastwave. STAR data. Au Au 130 GeV minbias. significant oscillations observed ... consistent with blast-wave parameterization of v2(pT,m), spectra, R(pT), K-p ...
full blastwave. STAR data. Au Au 130 GeV minbias. significant oscillations observed ... consistent with blast-wave parameterization of v2(pT,m), spectra, R(pT), K-p ...
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Particle correlations at STAR PowerPoint PPT Presentation
Particle correlations at STAR - 'Blast wave' parameterization (Sollfrank model) can approximately ... A model of the freezeout - BlastWave. BW: hydro-inspired parameterization. of freezeout ...
'Blast wave' parameterization (Sollfrank model) can approximately ... A model of the freezeout - BlastWave. BW: hydro-inspired parameterization. of freezeout ...
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Phenomenology I: Phase transition PowerPoint PPT Presentation
Phenomenology I: Phase transition - The energy density of (massless) quarks and gluons is derived ... blastwave fit (green line) pT prediction for. Tch = 170 MeV. and b =0. pp no rescattering, ...
The energy density of (massless) quarks and gluons is derived ... blastwave fit (green line) pT prediction for. Tch = 170 MeV. and b =0. pp no rescattering, ...
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Modern Nuclear Physics with STAR @ RHIC: Recreating the Creation of the Universe PowerPoint PPT Presentation
Modern Nuclear Physics with STAR @ RHIC: Recreating the Creation of the Universe - Modern Nuclear Physics with STAR @ RHIC: Recreating the Creation of the Universe Rene Bellwied Wayne State University (bellwied@physics.wayne.edu)
Modern Nuclear Physics with STAR @ RHIC: Recreating the Creation of the Universe Rene Bellwied Wayne State University (bellwied@physics.wayne.edu)
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Azimuthally-sensitive HBT (asHBT) in Au Au collisions at ?sNN=200 GeV PowerPoint PPT Presentation
Azimuthally-sensitive HBT (asHBT) in Au Au collisions at ?sNN=200 GeV - Freeze-out anisotropy as an evolution 'clock' anisotropic pressure gradients ... Reaction-plane estimation (from event-wise p-space anisotropy) is imperfect ...
Freeze-out anisotropy as an evolution 'clock' anisotropic pressure gradients ... Reaction-plane estimation (from event-wise p-space anisotropy) is imperfect ...
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John M. Blondin PowerPoint PPT Presentation
John M. Blondin - Discovering the Complexity of Supernovae through 3D Simulations John M. Blondin NC State University We begin our story in 1572 In One Dimension: We begin our story ...
Discovering the Complexity of Supernovae through 3D Simulations John M. Blondin NC State University We begin our story in 1572 In One Dimension: We begin our story ...
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Low pT??????????? ???????? -- What we learned from low pT phenomena at RHIC? -- PowerPoint PPT Presentation
Low pT??????????? ???????? -- What we learned from low pT phenomena at RHIC? -- - Low pT ?-- What we learned from low pT phenomena at RHIC? --KANETA, Masashi -BNL ...
Low pT ?-- What we learned from low pT phenomena at RHIC? --KANETA, Masashi -BNL ...
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A Coarse 3D Model of E0102-72 Derived from HETG Data PowerPoint PPT Presentation
A Coarse 3D Model of E0102-72 Derived from HETG Data - http://www.pantheon.org/areas/gallery/folklore/greek_heroic/hydra.html) ... describe Hydra concepts and goals in the. pages at right. Dan Dewey ...
http://www.pantheon.org/areas/gallery/folklore/greek_heroic/hydra.html) ... describe Hydra concepts and goals in the. pages at right. Dan Dewey ...
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Femtoscopy in heavy ion collisions: Two decades of progress PowerPoint PPT Presentation
Femtoscopy in heavy ion collisions: Two decades of progress - mike lisa - Femtoscopy in relativistic heavy ion collisions ... regions or fancy stuff. ... neglect time/dynamics: gross F.O. geometry appears determined ...
mike lisa - Femtoscopy in relativistic heavy ion collisions ... regions or fancy stuff. ... neglect time/dynamics: gross F.O. geometry appears determined ...
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Experimental%20evidence%20for%20color-neutral%20pre-hadronic%20states%20above%20the%20critical%20temperature%20at%20RHIC%20and%20LHC PowerPoint PPT Presentation
Experimental%20evidence%20for%20color-neutral%20pre-hadronic%20states%20above%20the%20critical%20temperature%20at%20RHIC%20and%20LHC - Experimental evidence for color-neutral pre-hadronic states above the critical temperature at RHIC and LHC Rene Bellwied (University of Houston)
Experimental evidence for color-neutral pre-hadronic states above the critical temperature at RHIC and LHC Rene Bellwied (University of Houston)
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Recent results from RHIC experiments -- QGP search and the spin program -- PowerPoint PPT Presentation
Recent results from RHIC experiments -- QGP search and the spin program -- - Recent results from RHIC experiments-- QGP search and the spin program -- -BNL Outlook RHIC QGP PHENIX, STAR ...
Recent results from RHIC experiments-- QGP search and the spin program -- -BNL Outlook RHIC QGP PHENIX, STAR ...
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Experimental Probes of QGP (Part I) PowerPoint PPT Presentation
Experimental Probes of QGP (Part I) - Bjorken-Formula for Energy Density: PRD 27, 140 (1983) watch out for typo (factor 2) ... Calculations of energy loss of high-pT particles e 15 GeV/fm3 ...
Bjorken-Formula for Energy Density: PRD 27, 140 (1983) watch out for typo (factor 2) ... Calculations of energy loss of high-pT particles e 15 GeV/fm3 ...
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STAR Strangeness Summary 2003 PowerPoint PPT Presentation
STAR Strangeness Summary 2003 - mt scaling in Au-Au and p-p. Works for p-p. not for Au-Au. Again evidence for flow. ... UA1 data from p p collisions at s= 630 GeV. ...
mt scaling in Au-Au and p-p. Works for p-p. not for Au-Au. Again evidence for flow. ... UA1 data from p p collisions at s= 630 GeV. ...
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John%20M.%20Blondin PowerPoint PPT Presentation
John%20M.%20Blondin - I noticed that a new and unusual star, surpassing the ... If the progenitor star possessed an asymmetric stellar wind (e.g., due to ...
I noticed that a new and unusual star, surpassing the ... If the progenitor star possessed an asymmetric stellar wind (e.g., due to ...
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Flow in p p data PowerPoint PPT Presentation
Flow in p p data - Only type of transverse flow in central collision (b=0) is radial flow ... anisotropy. momentum. anisotropy. sensitive to the EoS ...
Only type of transverse flow in central collision (b=0) is radial flow ... anisotropy. momentum. anisotropy. sensitive to the EoS ...
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Computational Astrophysics: Research to Teaching and Beyond PowerPoint PPT Presentation
Computational Astrophysics: Research to Teaching and Beyond - Andrew Cunningham (UR, UC Berkeley, LLNL) Alexei Poludnenko (UR, NRL) ... 2nd Age: Moderate rez 2-D calculations. Supercomputers: Cray, etc ...
Andrew Cunningham (UR, UC Berkeley, LLNL) Alexei Poludnenko (UR, NRL) ... 2nd Age: Moderate rez 2-D calculations. Supercomputers: Cray, etc ...
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Starting the Energy Scan - First Results from 62.4 GeV Au Au Collisions PowerPoint PPT Presentation
Starting the Energy Scan - First Results from 62.4 GeV Au Au Collisions - Starting the Energy Scan - First Results from 62.4 GeV. Au Au Collisions. Introduction. ... is a suppression for most central data. Maximum significantly higher ...
Starting the Energy Scan - First Results from 62.4 GeV. Au Au Collisions. Introduction. ... is a suppression for most central data. Maximum significantly higher ...
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Monte Calor Study of Hard and Soft Interactions: PowerPoint PPT Presentation
Monte Calor Study of Hard and Soft Interactions: - Charm quarks are believed to be produced at early stage by initial ... The low pT muon yields are uniform from whatever shape of the charmed hadron. 6/5/09 ...
Charm quarks are believed to be produced at early stage by initial ... The low pT muon yields are uniform from whatever shape of the charmed hadron. 6/5/09 ...
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IMHO In Mikes Humble Opinion PowerPoint PPT Presentation
IMHO In Mikes Humble Opinion - Mike Lisa. Ohio State University. what have we learned (so far)? what is exciting (to me) ... ma lisa - QM04. 3. Sophisticated tools to study a complex system ...
Mike Lisa. Ohio State University. what have we learned (so far)? what is exciting (to me) ... ma lisa - QM04. 3. Sophisticated tools to study a complex system ...
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Bulk matter properties in RHIC collisions PowerPoint PPT Presentation
Bulk matter properties in RHIC collisions - Models to evaluate Tch and. B Compare particle ratios to experimental data ... little difference in lifetime! Helen Caines. GHPM Oct. 2004. 23 ...
Models to evaluate Tch and. B Compare particle ratios to experimental data ... little difference in lifetime! Helen Caines. GHPM Oct. 2004. 23 ...
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GRB Physics in the Swift Era PowerPoint PPT Presentation
GRB Physics in the Swift Era - Title: Astronomy 103 Author: bing zhang Last modified by: Bing Zhang Created Date: 8/28/2004 6:47:00 PM Document presentation format: On-screen Show
Title: Astronomy 103 Author: bing zhang Last modified by: Bing Zhang Created Date: 8/28/2004 6:47:00 PM Document presentation format: On-screen Show
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SNR E0102: Building a Supernova Remnant PowerPoint PPT Presentation
SNR E0102: Building a Supernova Remnant - X-ray Images... Bright thin ring of reverse-shocked ejecta, primarilly O and Ne. ... of Type Ia spectra from 1D hydro code fed into X-ray emission calculation. ...
X-ray Images... Bright thin ring of reverse-shocked ejecta, primarilly O and Ne. ... of Type Ia spectra from 1D hydro code fed into X-ray emission calculation. ...
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Chandra%20HETG%20Spectra%20of%20SN%201987A%20at%2020%20Years PowerPoint PPT Presentation
Chandra%20HETG%20Spectra%20of%20SN%201987A%20at%2020%20Years - Chandra HETG Spectra of SN 1987A at 20 Years. D. Dewey1, S.A. Zhekov2,3, ... This work was supported by NASA through SAO contract SV3-73016 to MIT for ...
Chandra HETG Spectra of SN 1987A at 20 Years. D. Dewey1, S.A. Zhekov2,3, ... This work was supported by NASA through SAO contract SV3-73016 to MIT for ...
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Twoparticle correlations and Heavy Ion Collision Dynamics at RHICSTAR PowerPoint PPT Presentation
Twoparticle correlations and Heavy Ion Collision Dynamics at RHICSTAR - x-anisotropy in entrance channel p-space anisotropy at freezeout ... Experimental indications of x-space anisotropy @ RHIC. solid. dashed. 0.04 0.01. 0.09 0.02 ...
x-anisotropy in entrance channel p-space anisotropy at freezeout ... Experimental indications of x-space anisotropy @ RHIC. solid. dashed. 0.04 0.01. 0.09 0.02 ...
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Itanium 2 Profiling Tools: Performance monitoring events Pfmon (Open Source) Intel Vtune Analyzer PowerPoint PPT Presentation
Itanium 2 Profiling Tools: Performance monitoring events Pfmon (Open Source) Intel Vtune Analyzer - Itanium 2 Profiling Tools: Performance monitoring events Pfmon (Open Source) Intel Vtune Analyzer Arthur Raefsky raefsky@sgi.com Overview Profiling Tools: The Intel ...
Itanium 2 Profiling Tools: Performance monitoring events Pfmon (Open Source) Intel Vtune Analyzer Arthur Raefsky raefsky@sgi.com Overview Profiling Tools: The Intel ...
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FOT ACIS Training PowerPoint PPT Presentation
FOT ACIS Training - FOT ACIS Training
FOT ACIS Training
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The formation of realistic disk galaxies in PowerPoint PPT Presentation
The formation of realistic disk galaxies in - High resolution galaxy formation ... Images with SUNRISE (Patrik Jonsson) Effect of increasing resolution on the size of disks ...
High resolution galaxy formation ... Images with SUNRISE (Patrik Jonsson) Effect of increasing resolution on the size of disks ...
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Recombination PowerPoint PPT Presentation
Recombination - R.J. Fries, C. Nonaka, B. M ller & S.A. Bass, PRL 90, 202303 (2003) ... C. Nonaka, R.J. Fries & S.A. Bass, nucl-th/0308051, submitted to PLB ...
R.J. Fries, C. Nonaka, B. M ller & S.A. Bass, PRL 90, 202303 (2003) ... C. Nonaka, R.J. Fries & S.A. Bass, nucl-th/0308051, submitted to PLB ...
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From RHIC to LHC The Little Bang Evolution Rene Bellwied Wayne State University PowerPoint PPT Presentation
From RHIC to LHC The Little Bang Evolution Rene Bellwied Wayne State University - From RHIC to LHC The Little Bang Evolution Rene Bellwied Wayne State University
From RHIC to LHC The Little Bang Evolution Rene Bellwied Wayne State University
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Geometry-driven physics at RHIC A work in progress PowerPoint PPT Presentation
Geometry-driven physics at RHIC A work in progress - (connection between simple and bulk systems nontrivial & theoretically ... (Wow, was it really only last summer? I feel like I've seen this data for 100 years...
(connection between simple and bulk systems nontrivial & theoretically ... (Wow, was it really only last summer? I feel like I've seen this data for 100 years...
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Using WAS on a Unix Platform by Colin Renouf Version 1.4 PowerPoint PPT Presentation
Using WAS on a Unix Platform by Colin Renouf Version 1.4 - The Bourne, Korn, and C Shells are commonly used. Bash, from Linux, is ... Learn shell scripting either Korn or Bash and automate as much management as ...
The Bourne, Korn, and C Shells are commonly used. Bash, from Linux, is ... Learn shell scripting either Korn or Bash and automate as much management as ...
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Femtoscopy in HIC' Theory R' Lednick, JINR Dubna PowerPoint PPT Presentation
Femtoscopy in HIC' Theory R' Lednick, JINR Dubna - KP'71-75: settled basics of correlation femtoscopy. proposed CF= Ncorr /Nuncorr & mixing techniques to construct Nuncorr ... approximation: Remitter Rsource ...
KP'71-75: settled basics of correlation femtoscopy. proposed CF= Ncorr /Nuncorr & mixing techniques to construct Nuncorr ... approximation: Remitter Rsource ...
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WHERE PowerPoint PPT Presentation
WHERE - Avg density 1 grain/million m3. Whirlpool' Galaxy. Looking at a ... Supernova blast wave. Expanding emission nebula. Galactic density wave. p. 271. Molecular ...
Avg density 1 grain/million m3. Whirlpool' Galaxy. Looking at a ... Supernova blast wave. Expanding emission nebula. Galactic density wave. p. 271. Molecular ...
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Diapositive 1 PowerPoint PPT Presentation
Diapositive 1 - Halo CME May 02 1998. Disk observations. CMEs and shocks. CME wrapped by shock ... Flanks: blast wave .5. Coronal shocks and CME driven shocks. FASR Freq. range ...
Halo CME May 02 1998. Disk observations. CMEs and shocks. CME wrapped by shock ... Flanks: blast wave .5. Coronal shocks and CME driven shocks. FASR Freq. range ...
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Osservabili%20 PowerPoint PPT Presentation
Osservabili%20 - Luciano Ramello Universit del Piemonte Orientale & I.N.F.N.. for the ALICE Collaboration ... Tsallis blast-wave (power law in mT) B. Hippolyte, H. Ricaud ...
Luciano Ramello Universit del Piemonte Orientale & I.N.F.N.. for the ALICE Collaboration ... Tsallis blast-wave (power law in mT) B. Hippolyte, H. Ricaud ...
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Blast%20waves%20from%20GRBs PowerPoint PPT Presentation
Blast%20waves%20from%20GRBs - Blast wave. 2. GeV TeV flashes. Meszaros, Rees (1993) Sari, Piran (1999) (Blandford, McKee 1976) ... A flat optical spectrum is expected from e /- loaded blast wave. ...
Blast wave. 2. GeV TeV flashes. Meszaros, Rees (1993) Sari, Piran (1999) (Blandford, McKee 1976) ... A flat optical spectrum is expected from e /- loaded blast wave. ...
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Progenitors: Mass loss determines SN Type. PowerPoint PPT Presentation
Progenitors: Mass loss determines SN Type. - Ib (only He core), Ic (only O core) Ejecta structure: Shock ... Hard from reverse shock & blast wave. Optical: Gr ningsson et al. X-rays: Park et al 2005 ...
Ib (only He core), Ic (only O core) Ejecta structure: Shock ... Hard from reverse shock & blast wave. Optical: Gr ningsson et al. X-rays: Park et al 2005 ...
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SNR 101 3rd X-ray Astronomy school Wallops Island May 12-16 May PowerPoint PPT Presentation
SNR 101 3rd X-ray Astronomy school Wallops Island May 12-16 May - SNRs also enrich the ISM by dispersing material produced both during the star's ... one expects thermal emission coming from a thin shell behind the blast wave. ...
SNRs also enrich the ISM by dispersing material produced both during the star's ... one expects thermal emission coming from a thin shell behind the blast wave. ...
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Stellar%20Nucleosynthesis PowerPoint PPT Presentation
Stellar%20Nucleosynthesis - The periodic chart contains 92 naturally-occurring elements in the universe ... This will cause a blast wave that ejects the star's envelope into interstellar space. ...
The periodic chart contains 92 naturally-occurring elements in the universe ... This will cause a blast wave that ejects the star's envelope into interstellar space. ...
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Particle Production from Soft Processes PowerPoint PPT Presentation
Particle Production from Soft Processes - Statistical Model, Blast-Wave and Hydro. Further Test of (Early) Thermalization and Hydro ... ? Tkinetic from Blast-Wave is not same as Temperature from Hydro Model ...
Statistical Model, Blast-Wave and Hydro. Further Test of (Early) Thermalization and Hydro ... ? Tkinetic from Blast-Wave is not same as Temperature from Hydro Model ...
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Cosmic Jets PowerPoint PPT Presentation
Cosmic Jets - Jet simulations and sources. Relativistic leptonic and hadronic ... SNs/SNRs: blast wave shock. Jet morphology. Jet simulation. M. Krause, LSW HD. t = 1.64 Myr ...
Jet simulations and sources. Relativistic leptonic and hadronic ... SNs/SNRs: blast wave shock. Jet morphology. Jet simulation. M. Krause, LSW HD. t = 1.64 Myr ...
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Relativistic Ideal and Viscous Hydrodynamics PowerPoint PPT Presentation
Relativistic Ideal and Viscous Hydrodynamics - Blast wave model (thermal boost) Kinetic equilibrium. inside matter. e.g. Sollfrank et al.('93) ... Applicability of Blast Wave Model. Dependence of Initial Conditions ...
Blast wave model (thermal boost) Kinetic equilibrium. inside matter. e.g. Sollfrank et al.('93) ... Applicability of Blast Wave Model. Dependence of Initial Conditions ...
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Diapositive 1 PowerPoint PPT Presentation
Diapositive 1 - Some SPS and RHIC results. ALICE detector performance ... This hints for the presence of radial flow blast wave analysis. F Production K K- and e e ...
Some SPS and RHIC results. ALICE detector performance ... This hints for the presence of radial flow blast wave analysis. F Production K K- and e e ...
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Shielding effects on radiation intensity and dose PowerPoint PPT Presentation
Shielding effects on radiation intensity and dose - ... shockwave, blast wave, column/plume, base surge, residual radiation, fallout, ... Traveling through air is called a blast wave, or air blast ...
... shockwave, blast wave, column/plume, base surge, residual radiation, fallout, ... Traveling through air is called a blast wave, or air blast ...
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Gamma-Ray Bursts PowerPoint PPT Presentation
Gamma-Ray Bursts - If you pretend being interested in the stuff about me, I'll click on the ... outburst phase (gamma-ray/x-ray): internal shocks in the relativistic blast wave. ...
If you pretend being interested in the stuff about me, I'll click on the ... outburst phase (gamma-ray/x-ray): internal shocks in the relativistic blast wave. ...
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PILOT Survey for Supernovae in Starbursts PowerPoint PPT Presentation
PILOT Survey for Supernovae in Starbursts - Core-collapse SNe (CCSNe) generate/liberate the bulk of the ... Can serve as probes of extinction and ISM. CCSNe blast wave probes progenitor mass-loss history. ...
Core-collapse SNe (CCSNe) generate/liberate the bulk of the ... Can serve as probes of extinction and ISM. CCSNe blast wave probes progenitor mass-loss history. ...
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New results from the NA57 experiment PowerPoint PPT Presentation
New results from the NA57 experiment - Universit degli Studi di Bari and INFN, Bari, ... 'Blast wave' analysis. Conclusions. XXXVIII Rencontres de Moriond 26 March 2003 ... A 'blast wave' analysis ...
Universit degli Studi di Bari and INFN, Bari, ... 'Blast wave' analysis. Conclusions. XXXVIII Rencontres de Moriond 26 March 2003 ... A 'blast wave' analysis ...
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Avalanche PowerPoint PPT Presentation
Avalanche - form in snow with little internal cohesion among individual ... strong blast wave. wet loose snow avalanches. occurs at spring 'Good conditions' for avalanche ...
form in snow with little internal cohesion among individual ... strong blast wave. wet loose snow avalanches. occurs at spring 'Good conditions' for avalanche ...
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