logging in or signing up SWW3 Chilingaryan Marian Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINTLite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 141 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: November 02, 2007 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript Cosmic Rays in Space Weather researchA.ChilingarianCosmic Ray Division, Alikhanyan Physics Institute, Armenia: Cosmic Rays in Space Weather research A.Chilingarian Cosmic Ray Division, Alikhanyan Physics Institute, ArmeniaAragats Space-Environmental Center (ASEC), Cosmic Ray Division (CRD), Alikhanyan Physics Institute: Aragats Space-Environmental Center (ASEC), Cosmic Ray Division (CRD), Alikhanyan Physics InstituteAragats Space-Environmental Center: Aragats Space-Environmental Center Measure as much as possible secondary CR fluxes with different energy thresholds; Measure the histogram of energy releases on minute-by-minute basis; Monitor correlations between changing CR fluxes; Measure particle arrival directions; Use same detectors for SW and high energy CR; Perform simulation of the time-series registered by the ASEC monitors; Correlate surface and space-born detectors data assessable from the Internet; Be part of world-wide networks and create new networks; Provide forecasting and alerts on severe conditions of the SW. List of ASEC Particle Detectors: List of ASEC Particle DetectorsSolar Neutron Telescope: Solar Neutron TelescopeNor Amberd Multidirectional Muon Monitor : Nor Amberd Multidirectional Muon Monitor Aragats Multidirectional Muon Monitor (AMMM): Aragats Multidirectional Muon Monitor (AMMM)ASEC monitor are “selecting” different energy populations of GCR and SCR: ASEC monitor are “selecting” different energy populations of GCR and SCREnergy Spectrum of the GLE from 20 January 2005: Energy Spectrum of the GLE from 20 January 2005 Famous “Halloween” events of 2003, detected in electron & muon and neutron fluxes by ASEC monitors: Famous “Halloween” events of 2003, detected in electron & muon and neutron fluxes by ASEC monitorsCorrelation Matrix of ASEC monitors for 29 October 2003 (6:09 – 14:39), Fd: Correlation Matrix of ASEC monitors for 29 October 2003 (6:09 – 14:39), FdASEC Monitors Correlation Matrix 25 Jan 2003, (quiet time): ASEC Monitors Correlation Matrix 25 Jan 2003, (quiet time)Neutron and Proton GLEs as seen by the SNT: Neutron and Proton GLEs as seen by the SNTPrecursor of largest GMS from 20 November 2003: Precursor of largest GMS from 20 November 2003 Correlation Matrix of ASEC monitors for 20-21 November 2003 г. (14:40 – 6:00), Geomagnetic Storm: Correlation Matrix of ASEC monitors for 20-21 November 2003 г. (14:40 – 6:00), Geomagnetic StormSevan DetectorSpace Environmental Viewing and Analysis Network : Sevan Detector Space Environmental Viewing and Analysis Network Software Trigger (Microcontroller based) 111 – Charged particle-high; 300 MeV muon 010 – Neutral particle 100 – Low energy charged particle 011 – High energy neutral particle 001 – horizontal muon 101 – 2 horizontal muons MMM – Extensive Air ShowerSpace Environment Viewing and Analysis Network (SEVAN): Space Environment Viewing and Analysis Network (SEVAN) Proceedings of the International Conference Solar Extreme Events - 2005: Proceedings of the International Conference Solar Extreme Events - 2005 http://crdlx5.yerphi.am/index.php?Page=/Online_News/CRDSEE/Proceedings/&Title=0 You do not have the permission to view this presentation. In order to view it, please contact the author of the presentation.
SWW3 Chilingaryan Marian Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINTLite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 141 Category: Entertainment License: All Rights Reserved Like it (0) Dislike it (0) Added: November 02, 2007 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript Cosmic Rays in Space Weather researchA.ChilingarianCosmic Ray Division, Alikhanyan Physics Institute, Armenia: Cosmic Rays in Space Weather research A.Chilingarian Cosmic Ray Division, Alikhanyan Physics Institute, ArmeniaAragats Space-Environmental Center (ASEC), Cosmic Ray Division (CRD), Alikhanyan Physics Institute: Aragats Space-Environmental Center (ASEC), Cosmic Ray Division (CRD), Alikhanyan Physics InstituteAragats Space-Environmental Center: Aragats Space-Environmental Center Measure as much as possible secondary CR fluxes with different energy thresholds; Measure the histogram of energy releases on minute-by-minute basis; Monitor correlations between changing CR fluxes; Measure particle arrival directions; Use same detectors for SW and high energy CR; Perform simulation of the time-series registered by the ASEC monitors; Correlate surface and space-born detectors data assessable from the Internet; Be part of world-wide networks and create new networks; Provide forecasting and alerts on severe conditions of the SW. List of ASEC Particle Detectors: List of ASEC Particle DetectorsSolar Neutron Telescope: Solar Neutron TelescopeNor Amberd Multidirectional Muon Monitor : Nor Amberd Multidirectional Muon Monitor Aragats Multidirectional Muon Monitor (AMMM): Aragats Multidirectional Muon Monitor (AMMM)ASEC monitor are “selecting” different energy populations of GCR and SCR: ASEC monitor are “selecting” different energy populations of GCR and SCREnergy Spectrum of the GLE from 20 January 2005: Energy Spectrum of the GLE from 20 January 2005 Famous “Halloween” events of 2003, detected in electron & muon and neutron fluxes by ASEC monitors: Famous “Halloween” events of 2003, detected in electron & muon and neutron fluxes by ASEC monitorsCorrelation Matrix of ASEC monitors for 29 October 2003 (6:09 – 14:39), Fd: Correlation Matrix of ASEC monitors for 29 October 2003 (6:09 – 14:39), FdASEC Monitors Correlation Matrix 25 Jan 2003, (quiet time): ASEC Monitors Correlation Matrix 25 Jan 2003, (quiet time)Neutron and Proton GLEs as seen by the SNT: Neutron and Proton GLEs as seen by the SNTPrecursor of largest GMS from 20 November 2003: Precursor of largest GMS from 20 November 2003 Correlation Matrix of ASEC monitors for 20-21 November 2003 г. (14:40 – 6:00), Geomagnetic Storm: Correlation Matrix of ASEC monitors for 20-21 November 2003 г. (14:40 – 6:00), Geomagnetic StormSevan DetectorSpace Environmental Viewing and Analysis Network : Sevan Detector Space Environmental Viewing and Analysis Network Software Trigger (Microcontroller based) 111 – Charged particle-high; 300 MeV muon 010 – Neutral particle 100 – Low energy charged particle 011 – High energy neutral particle 001 – horizontal muon 101 – 2 horizontal muons MMM – Extensive Air ShowerSpace Environment Viewing and Analysis Network (SEVAN): Space Environment Viewing and Analysis Network (SEVAN) Proceedings of the International Conference Solar Extreme Events - 2005: Proceedings of the International Conference Solar Extreme Events - 2005 http://crdlx5.yerphi.am/index.php?Page=/Online_News/CRDSEE/Proceedings/&Title=0