Invited Talks at International Scientific Conferences:
 Invited Talks at International Scientific Conferences:
 
    -  Attracted by the Fascinating Magnetism of the Sun, 
         
@ Sohe3: Third Meeting of the Italian Solar and Heliospheric Community, 
         Turin (Italy) October 28-31, 2018.
    
 -  Shell Models for Astrophysical Phenomena Descriptions, 
         @ Nonlinear Waves and Chaos 9, 
         La Jolla - San Diego, California - USA, 4-8 March 2013.
    
 -  Zonal Shear in a Solar Dynamo Model,
         @ 2012 AGU Fall Meeting, 3-7 December, 
         - San Francisco, California - USA, Oral session.
    
 -  Reduced MHD Turbulence Model of a Coronal Loopi,
         Special Contribution for a new member of American Astronomical Society 
         
@ America Astronomical Society 210th Meeting 
         - Honolulu, Hawaii, USA, May 2007. 
         Bulletin of the American Astronomical Society, Vol. 38, p.150 (2007) 
    
 -  Turbulent Model for Solar Flares and Astrophysical Dynamo,
         @ Grand Challenge Problems in Computational Astrophysics Reunion Conference I, 
         
Institute for Pure & Applied Mathematics, 
          University of California 
          - Los Angeles, CA - USA, December 2006.
    
 -  Large Amplitude Velocity Fluctuations as Precursor of Nanoflares in 
         Solar Coronal Loops,
         @ PCA Culminating Conference, Institute for Pure & Applied Mathematics 
              
University of California - 
              Lake Arrowhead, CA - USA, May 2005.
    
 -  Large Amplitude Velocity Fluctuations as Precursor of Nanoflares in 
         Solar Coronal Loops,
         
@ Solar Coronal Loops Workshop - Palermo - Italy, 
             September 2004.
  
 Invited Colloquia at International Institutes and Universities:
 
    -  Small-scale Turbulence as Regenerating Source of the Stellar 
         Magnetic Fields,
         @ Department of Physics and Astronomy,  Georgia State University 
           - Atlanta GA - USA, February 2017.
    
 -  Velocity Fluctuations in Coronal Loops as Flare Drivers,
 @ Naval Research Laboratory - Washington DC - USA, July 2006.
    
 -  Reduced MHD Shell Model for Turbulence in Coronal Loops,
         @ Jet Propulsion Laboratory - NASA - Pasadena CA - USA, May 2005.
 
 
 
 
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