FORGES-2008

Monday, 29 September

Session 1: Chairperson - RainerHippler

 

  • Ashot Chilingarian, Alikhanian Physics Institute, Armenia
SurfaceParticle Detectors in Space Weather research and forecast
  • Nat Gopalswamy, NASA GSFC, USA

SolarSources of GLE Events of Cycle 23

  • Karel Kudela, Institute of Experimental Physics, Slovakia

Cosmicray transmissivity in variable magnetosphere on various time scales

 

Session2: Chairperson- YuriStozhkov

 

  • Leonid  Lazutin,Moscow State University, Scobeltsyn Institute for Nuclear Physics, Space Physics Division, Moscow, Russia

 Penetrationof the solar 1-100 MeV protons into the Earths magnetosphere during strongmagnetic storms

  • Leonid  Lazutin, Yuri  Logachev,            

Solar 1-20 MeV protons as a sourceof the proton radiation belt

  • Ashot Chilingarian, Armen Hovhanissyan, Alikhanyan Physics Institute, Armenia.

FilteringAlgorithms For smoothing Time Series measured by particle detectors at AragatsSpace

  • Mary  Zazyan, Ashot Chilingarian, Alikhanyan Physics Institute, Armenia.                                                               

Sensitivityof Aragats Space Environmental Center (ASEC) Particle Detectors to PrimaryCosmic Rays

  • Masoud Mirmomeni, Caro Lucas, Babak Nadjar Araabi, Behzad Moshiri, Tehran University, Iran

Forecasting Solar and GeomagneticActivity Indices Using Neurofuzzy Modeling and Mutual Information approaches.

 

Tuesday, 30  September

Session 3: Chairperson - Nat Gopalswamy

 

  • Yuri Stozhkov,  Lebedev Physical Institute, Russian Academy of science,

Somequestions of cosmic ray modulation and cosmic ray time dependence in the 24-thsolar cycle

  • Valery Korepanov, Lviv Centre of Institute of Space Research, Ukraine                                                                    

Magnetic field monitoring -instrumentation and methodology

  • P.Spillantini, University and INFN, Firenze,M.Casolino, University and INFN, Roma Tor Vergata, P.Papini, INFN, Firenze, F.Taccetti, INFN, Firenze (Italy)

EnergeticSolar Cosmic Ray surveyor and monitor for Earth-Mars missions (CREAM surveyorand monitor)

  • Rainer Hippler, University of Greifswald, Germany

Integrationof MuSTAnG in the international muon telescope network

  • Arash Arami, Mahdi Rezaei Yousefi, Babak Kasmaei, Masoud Mirmomeni, Caro Lucas, Tehran University, Iran

InformationTheoretical Approach to Attention inGeomagnetic Storm Forecasting



Session 4: Chairperson - Karel Kudela


  • S. Chilingaryan1, A. Chilingarian2, V. Danielyan2, W. Eppler1, A. Kopmann1,

1 - Forschungszentrum Karlsruhe (FZK), Institute of Data Processingand Electronics, Karlsruhe,Germany

2 –Alikhanyan PhysicsInstitute, Armenia.                             

Treatmentof Experimental and Slow Control Data for Large Scale Cosmic Ray DetectionNetworks

  • Valery Korepanov, Georgy Lizunov, Alla Fedorenko, Lviv Centre of Institute of Space Research, Ukraine, 
Seismoionosphericcoupling
  • Ashot Chilingarian, Bagrat Mailyan, Alikhanyan Physics Institute, Armenia                                             

Dailyvariation in intensity of different species of secondary cosmic rays asmeasured by the particle detectors of Aragats Space Environmental Center atminimum of solar activity

  • Babak Salehi Kasmaei, Mohammadmahdi Rezaei Yousefi, Caro Lucas,Tehran University, Iran        

Recurrence Analysis ofSolar-Terrestrial System

  • Ashot Chilingarian, Gagik Hovsepyan, Alikhanyan Physics Institute, Armenia.

New type of particle detectors for the Space Weatherresearch

 

 

Wednesday, 1October

Session 5: Chairperson - ValeryKorepanov

 

  • Vahe Peroomian, Mostafa El-Alaoui, University of California, Los Angeles, USA                                   

TheImpact of Sudden Storm Commencement on Magnetospheric ion distributions

  • A.Chilingarian, G.Hovsepyan, K.Arakelyan, S.Abovyan, S.Chilingarian, V.Danielyan, K.Avakyan, D.Pokhsraryan, A.Reymers, S.Tserunyan, A.Yegikyan, Cosmic Ray Division of Alikhanian Physics Institute, Armenia                                          

SEVANparticle-detector network located at Middle-Low latitudes for Solar Physics andSpace Weather research  

  • Youra Taroyan, University of Sheffield, United Kingdom

 Hinode EUV spectroscopic observationsof coronal oscillations

 

Thursday, October 2

Session 6: Chairperson - VahePeroomian

 

  • Ashot Chilingarian, Nikolay Bostanjyan, Alikhanyan Physics Institute, Armenia, 

Forbush decreases detected by ASECmonitors during 23rd solar activity cycle  

  • Ashot Chilingarian, Nikolay Bostanjyan, Alikhanyan Physics Institute, Armenia, 

Cosmic Ray Intensity increasesdetected by ASEC monitors during 23rd solar activity cycle in correlation withGeomagnetic storms  

  • Grigori Karapetyan, Cosmic Ray Division, Alikhanyan Physics Institute, Armenia,                                              

Detectionof high energy solar protons during ground level enhancements  

  • Ashot Chilingarian, Tigran Karapetyan, Alikhanyan Physics Institute, Armenia                                                               

Barometriccoefficients of the particle detectors of Aragats Space Environmental Center (ASEC) as measured at thebeginning of the 24th Solar activity cycle  

  • Omid Ghiasvand, Caro Lucas, Ahmad Kalhor, Mohammad Reza Feizi Derakhshi, Tehran University, Iran 

Using fuzzy neural networks topredict arrival time of interplanetary shocks  

  • Sahar Parsapoor, Caro Lucas, Tehran University, Iran,

Predicting of solar geometry indicesby utilizing the emotional learning method

  • S.Abovyan, K.Arakelyan, A.Chilingarian, V.Danielyan, D.Pokhsraryan, Alikhanyan Physics Institute, Armenia   

Electronics for the Space Environmental Viewing and Analysis Network(SEVAN)