Workshop Program:
The workshop abstract booklet can be seen below. It can also be downloaded here.
Poster presenters: We kindly ask that posters be prepared in A0 size, if possible.
First Workshop on Sun and Space Weather Program
28 September - 2 October 2026 | Antalya, Türkiye
IT: Invited Talk (30 min presentation + 10 min Q & A) | CT: Contributed Talk (15 min presentation + 5 min Q & A)
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September 28, Monday |
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10:15 – 10:30 |
Opening Remarks |
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Morning Session |
Cyclic behaviors of solar and geomagnetic activity |
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Time |
Speaker |
Presentation Title |
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10:30 - 11:10 |
1.1 K. Mursula (IT) |
What happens during a Gleissberg cycle and why? |
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11:10 - 11:30 |
1.2 V. Bezrukovs (CT) |
Novel Approaches to Solar Flare Forecasting and Space Weather Monitoring: Results from the FLARE and IONEX Projects |
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11:30 - 11:50 |
1.3 H. S. Mohamed (CT) |
Impact of F10.7 Flux and Proton Intensity on Delayed Ionospheric TEC Responses at Low Latitudes During Geomagnetic Storms Across Solar Cycles 23–25 |
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12:00 - 14:00 |
Lunch |
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Afternoon Session |
Solar and geomagnetic activity prediction — I |
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Time |
Speaker |
Presentation Title |
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14:00 - 14:40 |
2.1 J.-P. Rozelot (IT) |
The crucial role of the leptocline in improving predictions of solar activity. |
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14:40 - 15:00 |
2.2 K. Gerçeker (CT) |
Assessing the Short-Term Predictability of Daily Space Weather Indices with Simplex Projection |
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September 29, Tuesday |
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Morning Session |
Solar and geomagnetic activity prediction — II |
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Time |
Speaker |
Presentation Title |
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10:30 - 11:10 |
3.1 K. Ryu (IT) |
Korea’s Space Environment Missions Advancing from LEO, GEO, Cis-Lunar, L4, and Beyond: Current Status and Future Plans |
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11:10 - 11:30 |
3.2 N. Karapınar (CT) |
Automated Umbra–Penumbra Delineation and Machine-Learning-Based McIntosh Classification of Sunspot Groups |
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11:30 – 11:50 |
3.3 B. Habashy (CT) (Online) |
Solar Hemispheric Asymmetry and Its Impact on Geomagnetic Activity During Solar Cycles 21–24 |
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12:00 - 14:00 |
Lunch |
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Afternoon Session |
Eruptive solar phenomena (Flares, CMEs, SEPs, Shocks) — I |
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Time |
Speaker |
Presentation Title |
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14:00 - 14:40 |
4.1 P. Devi (IT) |
Relationship of prominence eruptions with CMEs and their dependence on Solar Cycle |
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14:40 - 15:00 |
4.2 N. Gopalswamy (CT) |
Double-whammy Space Weather Events in the SOHO Era |
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15:00 - 15:20 |
Tea Break |
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15:20 - 16:00 |
4.3 S. Yashiro (IT) (Online) |
White-Light Emissions in Gamma-Ray Solar Flares |
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16:00 - 16:40 |
4.4 P. Mäkelä (IT) (Online) |
Durations of solar hard X-ray bursts with and without an associated coronal mass ejection |
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17:00 - 19:00 |
Poster Session |
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September 30, Wednesday |
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Morning Session |
Eruptive solar phenomena (Flares, CMEs, SEPs, Shocks) — II |
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Time |
Speaker |
Presentation Title |
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09:00 - 09:40 |
5.1 N. Gopalswamy (IT) |
The association rates of type II bursts and large solar energetic particle events in CME populations |
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09:40 - 10:00 |
5.2 M. Tirnakci (CT) |
The Role of Impact Parameter in Forbush Decrease Profiles |
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10:00 - 10:20 |
5.3 H. Bhati (CT) (Online) |
Study of ICME-ICME interactions, ICME-in-sheath and associated GLE 77 during 11-12th Nov 2025 |
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10:20 - 10:50 |
Tea Break |
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10:50 - 11:30 |
5.4 S. Akiyama (IT) (Online) |
A Comparative Study of CME and PEA Properties in Quiescent Filament Eruptions with and without SEP Events (1996–2025) |
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11:30 - 12:10 |
5.5 R. Joshi (IT) |
Solar Flare Ribbons at Unprecedented Resolution |
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12:10 onward |
FREE TIME |
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October 1, Thursday |
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Morning Session |
Response of the Magnetosphere to the Impact of CMEs and Stream Interaction Region |
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Time |
Speaker |
Presentation Title |
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10:00 - 10:40 |
6.1 P. Koucká Knížová (IT) |
Sporadic E Behavior over Central Europe during a Geomagnetically Quiet Period in 2019 |
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10:40 – 11:00 |
6.2 O. Kryakunova (CT) |
On solar sources of interplanetary disturbances before the high-energy magnetospheric electrons enhancements |
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11:00 - 11:30 |
Tea Break |
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12:00 - 14:00 |
Lunch |
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Afternoon Session |
Magnetosphere–Ionosphere–Thermosphere coupling — II |
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Time |
Speaker |
Presentation Title |
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14:00 – 14:20 |
7.1 V. Truhlík (CT) |
Performance of the IRI Model during Quiet Space Weather Periods at Swarm Altitudes and First Results on the Inclusion of Atmospheric Wave Indices |
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14:20 - 15:00 |
7.2 W. Ward (IT) (Online) |
Knowledge Gaps in the Mesosphere and Lower Thermosphere: Potential Keystone Contributions |
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October 2, Friday |
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Morning Session |
Space weather effects on technological systems — I |
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Time |
Speaker |
Presentation Title |
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09:30 - 10:10 |
8.1 F. İnceoğlu (IT) (Online) |
Space Weather and Machine Learning: What Works and What Does Not |
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10:30 - 10:50 |
8.2 V.B. Belakhovsky (CT) (Online) |
The analyses of the sources of extreme geomagnetically induced currents in power lines based on observations over 11 years |
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10:50 - 11:20 |
Tea Break |
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11:20 – 12:00 |
8.3 V. Dobrica (IT) |
Assessing geoelectric hazard over Romania during extreme geomagnetic storms in March 1989, November 2003 and May 2024 |
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12:00 - 12:20 |
8.4 F.O. Grodji (CT) (Online) |
A study of solar flare effects on the geomagnetic field elements during solar cycles 23 and 24 |
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12:20 – 12:40 |
8.5 V. Pilipenko (CT) (Online) |
Geomagnetically Induced Currents Generated by Interplanetary Shock Waves and Solar Flares |
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12:40 - 14:30 |
Lunch |
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Afternoon Session |
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Time |
Speaker |
Presentation Title |
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14:30 - 15:30 |
Closing Remarks |
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Son güncelleme : 1.10.2026 10:17:27