Difference between revisions of "ISEST 2018 Workshop"
(→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)) |
(→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)) |
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2018_workshop/Tuesday/2_morning_Heber/benella_isest_pres.pdf On the role of the topology of magnetic clouds on galactic cosmic-ray Forbush decreases at energies above 70 MeV---- by S. Benella] <br> | *[http://solar.gmu.edu/wiki/presentations/ISEST_2018_workshop/Tuesday/2_morning_Heber/benella_isest_pres.pdf On the role of the topology of magnetic clouds on galactic cosmic-ray Forbush decreases at energies above 70 MeV---- by S. Benella] <br> | ||
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2018_workshop/Tuesday/2_morning_Heber/Melkumyan.pdf Statistical analysis of Forbush decreases observed during past five solar cycles and associated to coronal mass ejections or coronal holes ---- by A. Melkumyan ] <br> | *[http://solar.gmu.edu/wiki/presentations/ISEST_2018_workshop/Tuesday/2_morning_Heber/Melkumyan.pdf Statistical analysis of Forbush decreases observed during past five solar cycles and associated to coronal mass ejections or coronal holes ---- by A. Melkumyan ] <br> | ||
*[http://solar.gmu.edu/wiki/presentations/ISEST_2018_workshop/Tuesday/2_morning_Heber/Presentation_Hvar_Hofmeister.pdf 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] <br> | *[http://solar.gmu.edu/wiki/presentations/ISEST_2018_workshop/Tuesday/2_morning_Heber/Presentation_Hvar_Hofmeister.pdf 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] <br> | ||
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+ | *[http://solar.gmu.edu/wiki/presentations/ISEST_2018_workshop/Tuesday/3_afternoon_Zhang/hvar2018_hess.pdf Preparing for the Future of Heliospheric Observations---- by P. Hess (Invited)] <br> |
Revision as of 14:14, 28 November 2018
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
- 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