ISEST 2018 Workshop

The 2018 ISEST Workshop will be held in September 24-28, 2018, Hvar, Croatia. Here is the link to the meeting website

Opening, Plenary Talk, and WG Reports (Monday, Sep. 24, 2018) (Chair persons: M. Temmer, J. Zhang)

• Opening Remark ---- by Bojan Vrsnak
  
• Plenary Talk ---- by Jie Zhang
  
• Working Group 1 Report (data)---- by Jie Zhang
  
• Working Group 2 Report (Theory)---- by Bojan Vrsnak
  
• Working Group 3 Report (Simulation)---- by Dusan Odstrcil
  
• Working Group 4 Report (Campaign Events)---- by Dave Webb
  
• Working Group 5 Report (Bs Challenge) ---- by Spiros Pastourakos
  
• Working Group 6 Report (Solar Energetic Particles)---- by Olga Malandraki
  
• Working Group 7 Report (MiniMax24)---- by Manuela Temmer
  

Data & Observation related to solar-terrestrial phenomena (WG1 (data), WG5 (Bs challenge) and related abstracts from the General session on Sun & Heliosphere (Monday, Sep. 24, 2018) (Chair Persons: - J. Zhang, A. Veronig)

• Observations of magnetic flux ropes in the solar atmosphere: what next? ---- by Lucie Green (Invited)
  
• Evolution of coronal cavities leading to CMEs ---- by N. Srivastava
  
• Identifying the source complexity of a complex ejecta---- by R. Liu
  
• Which factors of an active region determine whether a strong flare will be CME-associated or not? ---- by A. Veronig
  
• The catalogue of solar failed eruptions---- by T. Mrozek
  
• Features of spectral-polarization dynamics of flare active regions bymicrowave observations ---- by T. Kaltman
  
• Can superflares occur on the Sun? A view from dynamo theory ---- by D. Sokoloff
  

Data & Observation related to solar-terrestrial phenomena (WG1 (data), WG5 (Bs challenge) and related abstracts from the General session on Sun & Heliosphere (Tuesday, Sep. 25, 2018) (Chair Persons: S. Patsouralos, J. Zhang)

• The Effects of Uncertainty on Deflection, Rotation and Bs predictions ---- by C. Kay (Invited)
  

• What can we learn from coronal dimmings about the early evolution of Earth-directed CMEs?---- by K.Dissauer
  

• Clustering of Coronal Mass Ejections---- by A. Ruzmalkin
  

• Unraveling the internal magnetic configuration of the ICMEs ---- by T. Nieves-Chinchilla (Invited)
  

• On the role of the topology of magnetic clouds on galactic cosmic-ray Forbush decreases at energies above 70 MeV---- by S. Benella
  

• Statistical analysis of Forbush decreases observed during past five solar cycles and associated to coronal mass ejections or coronal holes ---- by A. Melkumyan
  

• The dependence of high-speed stream peak velocities and of the Kp index on the positions of their source coronal holes on the Sun ---- by S. Hofmeister
  

• Preparing for the Future of Heliospheric Observations---- by P. Hess (Invited)
  

• Long-term periodicities in the heliospheric magnetic flux density and the effects on planetary space weather ---- by M. Dosa
  

• Solar Radio Imaging-Spectroscopy and Heliospheric Imager ---- by Y. Yan
  

Simulations and theoretical aspects of solar-terrestrial phenomena (WG2 (theory), WG3 (simulation) and related abstracts from the General session on Sun & Heliosphere (Tuesday, Sep. 25, 2018; Wednesday, Sep. 2018) (Chair Persons: F. Shen, B. Vrsnak, D. Odstrcil)

• Interaction between multiple CMEs and its impact on space weather---- by C. Shen (Invited)
  

• DBEM web application for heliospheric propagation of CMEs---- by J. Calogovic
  

• Forbush decrease model for expanding CMEs (ForbMod)---- by M. Dumbovic
  

• Near Real-Time Simulation of Heliospheric Space Weather---- by D. Odstrcil (Invited)
  

• Three-dimensional MHD simulation of solar wind using a new boundary treatment: Comparison with in-situ data at Earth --- by F. Shen
  

• Influence of the Magnetic Decay Index Spatial Distribution on the Kinematics of the Solar Eruptive Prominence--- by I. Myshyakov
  

• Simulation of fast-mode MHD waves interacting with low density regions such as coronal holes ---- by I. Piantschitsch
  

• Numerical simulations of coronal loop kink oscillations excited by different driver frequencies ---- by A. Alfanasev
  

Parker Solar Probe and Solar Orbiter (Wednesday, Sep. 26, 2018) (Chair Person: M. Temmer)

• Modeling and data analysis tools to support science at the Parker Solar Probe and Solar Orbiter era (including the hands-on-session) ----- by R. Pinto (Invited)
  

• STIX Software Development at Graz ----- by E. Dickson
  

• GEANT4 simulation of the Helios E6 - Proton contamination of relativistic electron measurements----- by B. Heber
  

Solar energetic particles (WG6 (SEPs) and related abstracts from the General session on Sun & Heliosphere (Thursday, Sep. 27, 2018) (Chair Person: O. Malandraki)

• Solar Energetic Particles: Origin, Acceleration, and Transport ----- by C. Cohen (Invited)
  

• The features of plasma turbulence associated with solar transients ----- by M. Riazantseva
  

• Acceleration of particles in 3D magnetic islands with low plasma density and their diagnostics in the heliosphere ----- by V. Zharkova
  

• Challenges of Space Weather and space radiation predictions for human explorations to Mars----- by J. Guo
  

Event studies using solar-terrestrial data & modeling (WG4 (campaign events) and related abstracts from the General session on Sun & Heliosphere (Thursday, Sep. 27, 2018) (Chair Persons: D. Webb, N. Srivastava)

• Sun-to-Earth Modeling of Coronal Mass Ejections with a Global MHD Model: Facilitating Physical Understanding and Space Weather Forecasting----- by M. Jin (Invited)
  

• Solar photospheric plasma and magnetic field dynamics: modelling of the temporal evolution of flow motions--- by J.I. Campos Rozo
  

• Multi-instrument observations of an X9.3 flare--- by I. Dammasch
  

• Coronal Hole and Active Region Interaction observed through a CME-HSS Interaction--- by S. Helnemann
  

• Observation-based Sun-to-Earth simulations of geo-effective Coronal Mass Ejections with EUHFORIA --- by S. Scolini (Invited)
  

• Dynamic properties of prominence eruptions observed by AIA and LASCO--- by T. Tsvetkov
  

• CME acceleration and EUV wave kinematics for September 10th 2017 event--- by T. Podladchikova
  

• Evolution of plasma parameters during the early acceleration phase of the June 13 2010 CME event --- by J. Selbezeder