Apr 3 – 28, 2023
Albano Building 3
Europe/Stockholm timezone

Schedule - Week 4

Theme 1: Statistical modeling of polarization observations. Coordinator: François Boulanger

Theme 2: Modelling Galactic magnetic fields. Coordinator: Tess Jaffe

Theme 3: IMAGINE pipeline. Coordinator: Sebastian Hutschenreuter


 

Monday, 24 April

9:30 Welcome (Lärosal 7, House 1, zode D)

9:45 One-minute introductions (Lärosal 7, House 1, zode D)

10:00 Introduction to Theme 1 (Lärosal 7, House 1, zode D)

10:30 Discussion Theme 1 and planning of continuation during the week (Lärosal 7, House 1, zode D)

10:45 ☕☕☕Coffee break (Nordita lounge areas, floor 6)

11:15 Introduction to Theme 2 (Lärosal 7, House 1, zode D)

11:45 Discussion Theme 2 and planning of continuation during the week (Lärosal 7, House 1, zode D)

12:00 Introduction to Theme 3 (Lärosal 7, House 1, zode D)

12:30 Discussion Theme 3 and planning of continuation during the week (Lärosal 7, House 1, zode D)

13:00 Lunch

14:00 Tutorial by François on wavelet scattering tools to characterize interstellar turbulence (Nordita, Room 6335-Hekto, floor 6)

16:00 Discussion of E versus B modes in polarization of interstellar turbulence (Nordita, Room 6335-Hekto, floor 6)

 

Tuesday, 25 April

10:00 Contributed Talks. Chair: François Boulanger

10:00 Huirong Yan, "Turbulent magnetic fields: theory and detection, implication on CRs" (Lärosal 7, House 1, zode D)

10:20 Raphael Skalidis, “Towards a comprehensive map of the Galactic magnetic field strength” (Lärosal 7, House 1, zode D)

10:40 Sebastian Hutschenreuter, "The Faraday sky and its connection to the Galactic magnetic field" (Lärosal 7, House 1, zode D)

11:00 ☕☕☕Coffee break (Nordita lounge areas, floor 6)

11:30 Independent work and group discussions (Nordita offices, floor 6)

13:00 Lunch

14:00 Discussion of variance in magnetic field modeling. Lead: Tess Jaffe (Nordita, Room 6335-Hekto, floor 6)

15:00 :  Seminar:  Non-equilibrium turbulence transport in convenction and dynamos (Nordita, Room 6335-Hekto, floor 6)

16:30 :  IMAGINE software demo/tutorial. Lead: Sebastian Hutschenreuter (Nordita, Room 6335-Hekto, floor 6)

 

Wednesday, 26 April

10:00 Contributed Talks. Chair: Katia Ferrière

10:00 Shinsuke Ideguchi, "Application of Faraday tomography to the combined data from GMIMS-South and S-PASS surveys"  (Lärosal 7, House 1, zode D)

10:20 Andrea Bracco, "Synthetic observations of the low-frequency radio sky: progress, applications, and prospects." (Lärosal 7, House 1, zode D)

10:40 Ana Erceg, "Determining the distances to LoTSS-DR2 structures using multi-tracer analysis" (Lärosal 7, House 1, zode D)

11:00 Amit Seta, "Rotation measure structure function with higher order stencils as a probe of large-scale magnetic fields" (Lärosal 7, House 1, zode D)

11:20 ☕☕☕Coffee break & Discussion (Nordita lounge areas, floor 6)

12:20 Independent work and group discussions (Nordita offices, floor 6)

13:00 Lunch

14:00 Discussion of turbulent instabilities in the ISM (Nordita, Room 6335-Hekto, floor 6)

15:00 Continued discussion of Faraday tomography degeneracies after Shinsuke's talk (Hekto)

16:00 Discussion of non-parametric modeling (Nordita, Room 6335-Hekto, floor 6)

18:30–21:00 Dinner at restaurant Cypern

 

Thursday, 27 April

10:00 Contributed Talks. Chair: Alex Tsouros 

10:00 Günther Sigl, "The Influence of Galactic Magnetic Fields on Ultra-High Energy Cosmic Rays: CRPropa Simulations" (Lärosal 7, House 1, zode D)

10:20 François Boulanger (TBC) (Lärosal 7, House 1, zode D)

11:00 ☕☕☕Coffee break (Nordita lounge areas, floor 6)

11:15 Discussion of cosmic rays 

11:30 Independent work and group discussions (Nordita offices, floor 6)

13:00 Lunch

14:00 Discussion of current constraints to add to IMAGINE (Nordita, Room 6335-Hekto, floor 6)

16:00 Discussion of spectro-polarimetry. Lead: Huirong Yan (Nordita, Room 6335-Hekto, floor 6)

 

Friday, 28 April

10:00 Week summary and closing: Francois Boulanger, Tess Jaffe (Lärosal 7, House 1, zode D)

11-17 Independent work and group discussions (Nordita offices, floor 6)