SCOSTEP 2023 program

SCOPE OF THE WORKSHOP

The Swiss National SCOSTEP committee is pleased to announce the 5th Swiss SCOSTEP workshop to be held from May 15-16, 2023 at FHNW in Windisch, Switzerland.

This workshop aims at bringing together scientists with an interest in solar-terrestrial science. It encourages a lively exchange between scientists from all fields within solar-terrestrial physics to identify synergies, foster collaborations, and strengthen the Swiss solar-terrestrial community.

Format

The workshop will consist of three invited talks plus contributed presentations (oral or poster). It covers the following topics:
1. Fundamental solar physics
2. Solar variability in the past and future
3. Sun-Earth relations in proxies, observations, and model simulations
4. Future (space) missions/observations

In-person participation is highly encouraged and recommended. A remote option will only be available on a best-effort basis.

Invited speakers:


TIME SCHEDULE:

Contributed talks are scheduled for 15 min + 5 min questions, invited talks for 25 min + 5 min questions.

Monday, 15.5.2023

10:30-11:00   coffee break
11:00-11:10 L. Kleint, S. Krucker welcome
11:10-11:40 T. Sukhodolov Solar influence on our climate (invited)
11:40-12:00 JP Montillet Discussion on the recent total solar irradiance products released by PMOD/WRC
12:00-12:20 O. Steiner Solar radiance variability in terms of the viral theorem
12:20:12:40 R. Sharma Detection and simulation of the weak nonthermal population from the Sun in meterwaves
12:40-14:00   lunch break
14:00-14:30 L. Hayes Solar Orbiter and Space Weather (invited)
14:30-14:50 S. Aregger Solar Energetic Particle Events and their Linkage to Solar Flares during the First Two Remote Sensing Windows of Solar Orbiter
14:50-15:10 N. Janitzek Linking Solar Flare Observations to Impulsive Solar Energetic Particle Events Measured with Solar Orbiter at 0.5 AU
15:10-15:30 A. Battaglia On the existence of hot X-ray onset precursor events in solar flares
15:30-16:00   coffee break
16:00-16:20 K. Barczynski First high-resolution coordinated observations of an active regions with Solar Orbiter and DKIST
16:20-16:40 L. Harra A spectral solar irradiance monitor (SoSpIM) on the JAXA Solar-C (EUVST) space mission
16:40-17:00 M. Rixen Flares monitoring during whole whole active region lifetime
18:00 (TBC)   social dinner

 

Tuesday, 16.5.2023

9:00-9:30 N. Brehm Studying solar variability with tree rings (invited)
9:30-9:50 S. Ulzega Shedding light on the sun through the calibration of solar dynamo models on millennial records of solar activity.
9:50-10:10 P. Judge A DKIST observation of magnetic structures from solar photosphere to corona
10:10-10:30 L. Kleint Statistical Analyses of IRIS spectra to determine properties of supersonic downflows and IRIS bursts
10:30-11:00   coffee break
11:00-11:20 B. Panos Flare prediction with explainable artificial intelligence
11:20-11:40 J. Zbinden Multiline flare prediction based on the IRIS spectral lines Mg II h&k, Si IV, and C II with machine learning
11:40-12:00 J. Canivete Cuissa Vortices and Alfvénic pulses in the simulated solar atmosphere
12:00-12:20 M. Stutz visualizing solar observations
12:20-12:30 M. Gabella Sun measurement site in Switzerland for the monitoring and calibration of weather radars
12:30-14:00   lunch break
14:00-14:20 S. Berdyugina Stochastic analysis of synoptic observations of solar turbulent magnetic fields at IRSOL
14:20-14:40 F. Zeuner Hanle rotation signatures in the Sr I 4607.3 Å line
14:40-15:00 L. Belluzzi A new tool for investigating the magnetism of the solar chromosphere
15:00-15:20 R. Ramelli Observations and instrumentation at IRSOL: present and future
15:20-15:30   closing remarks
 

posters:
C. Monstein: Contribution to IHY2007 and ISWI: Frequency Agile Radio Spectrometer CALLISTO
H. Collier: STIX Observations of Fast-Time Variations in Solar Flares
T. Egorova: Implication of the Sun transition to high Activity mode for the climate and ozone layer.
W. Hajdas: Aerospace Measurements Of Radiation Environment
W. Hajdas: COnstellation of Radiation BElt Survey program CORBES
 

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