The program is updated on 31th October (PDF).
The abstract book is now available (PDF).

If you registered for a poster presentation, please check here.

Sessions

Session 1 (S1): New facility and technology of solar polarimetry
Session 2 (S2): Solar phenomena revealed by polarimetry
Session 3 (S3): Theory and modeling of polarization
Session 4 (S4): Techniques for Stokes inversions and disambiguation
Session 5 (S5): Synergy to other fields (stellar physics, planetary science, plasma physics)

Program table

Day1-Monday 7 Nov
Day2-Tuesday 8 Nov
Day3-Wednesday 9 Nov
Day4-Thursday 10 Nov
Day5-Friday 11 Nov


Monday 7 Nov

12:30-13:30

Registration

Chair: Yukio Katsukawa

13:30-13:40

Opening

13:40-14:20

Review

L. Bellot Rubio

S1

EST: The future facility for accurate high-spatial resolution spectropolarimetry

14:20-14:40

(Remote)

N. Hurlburt

S1

Early laboratory testing of a photonic magnetograph

14:40-15:10

Keynote (remote)

Z. Xu

S1

Coronagraph-COronal Magnetism and Plasma ASsembled Scopes(COMPASS)

15:10-16:10

Break & Poster (60 min)

16:10-16:40

Keynote

D. Song

S1

The CLASP2 and CLASP2.1 missions for measuring chromospheric magnetic fields

16:40-17:00

(Remote)

S. K. Dubey

S1

Multi-Application Solar Telescope (MAST) : Polarimeter and telescope polarization characterization

17:00-17:20

(Remote)

Z. Qu

S1

Recent Progresses in Shaping the FASOT

17:20-17:50

Keynote

D. Orozco Suárez

S1

The polarimetric and helioseismic imager of solar orbiter






Tuesday 8 Nov

Chair: Kiyoshi Ichimoto

09:00-09:40

Review

J. Trujillo Bueno

S3

Highlights of observational and theoretical high-precision spectropolarimetry

09:40-10:00

(Remote)

T. Schad

S3

Non-symmetric Radiative Excitation of Polarized Lines in the Upper Atmosphere

10:00-10:20


A. Vicente Arevalo

S3

Formation of the polarized solar He I 10830 Å line

10:20-10:50

Break & Poster (30 min)

10:50-11:20

Keynote

E. Alsina Ballester

S3

Modeling the polarization of the Na I and K I D lines

11:20-12:10

Poster flash talk (1)


(Remote)

Y. Huang

S1

Development of DST Spectro-Polarimeter at Hida Observatory


(Remote)

T. Sakurai

S1

Calibration and Data Analysis Pipeline of the Infrared Spectro-Polarimeter at NAOJ/Mitaka


(Remote)

J. Batmunkh

S1

Building an efficient compression method for solar spectro-polarimetry data accumulated by Hinode/SP


(Remote)

X. Sun

S4

SpIn4D: Spectropolarimetric Inversion in Four Dimensions with Deep Learning


(Remote)

T. Kawate

S5

A tabletop device for investigating spectropolarimetric responses to anisotropic/magnetized plasmas



Y. Hanaoka

S2

Polarization of the Corona Observed During the 2017 and 2019 Total Solar Eclipses



R. T. Ishikawa

S2

Spectral line broadening associated with the turbulence in fading granules



J. Jurcak

S2

The stability of sunspots and pores related to the magnetic field properties

12:10-13:40

Lunch Break (90 min)

Chair: Rebeca Centeno

13:40-14:10

Keynote (remote)

T. del Pino Alemán

S3

Magnetic field diagnostics with UV spectropolarimetry

14:10-14:30


D. Afonso Delgado

S3

Exploring the UV solar spectrum: the polarization of Fe II lines between 250-280 nm

14:30-14:50

(Remote)

J. Zhao

S3

Simulating the Solar Corona in the Forbidden and Permitted Lines with Forward Modeling

14:50-15:10


S. Hebbur Dayananda

S3

P-CORONA : A new forward modeling code to study the polarization of solar coronal lines

15:10-16:10

Break & Poster (60 min)

16:10-16:30

(Remote)

M. Derouich

S3

Comprehensive data on atom+hydrogen and atom+electron collisions for spectroscopic and spectropolarimetric applications

16:40-17:30

Poster flash talk (2)


(Remote)

A. Korpi-Lagg

S1

SUNRISE III: The Solar Atmosphere in 3D and High Resolution


(Remote)

D. Kansabanik

S1

Tackling the unique challenges for low-frequency solar polarimetric calibration and imaging for Sun with the Murchison Widefield Array


(Remote)

S. Dey

S2

First detailed polarimetric study of a group of type-III solar radio bursts with the Murchison Widefield Array


(Remote)

P. Majee

S2

First detailed polarimetric study of a type II solar radio burst with the Murchison Widefield Array


(Remote)

S. Riva

S3

Suitability of the CRD approximation for the RIII redistribution matrix in the RT modeling of scattering polarization


(Remote)

M. Derouich

S3

Depolarization of solar molecular lines by collisions with neutral hydrogen atoms and with electrons


(Remote)

N. Guerreiro

S3

Theoretical modelling of the scattering polarisation signal of the Ca I 4227 A line accounting for angle-dependent PRD effects and bulk velocities


(Remote)

A. V. Sukhorukov

S3

3D RT Modeling of the Scattering Polarization in the Wings of Mg II h&k


(Remote)

M. E. M. Gangi

S5

SPOTS – SpectroPolarimetric Observations of T Tauri Stars: preliminary results



Y. Katsukawa

S1

Spectro-polarimetric capability of SUNRISE III SCIP



Y. Hashimoto

S2

Spectropolarimetry of solar prominences in He I 10830 Å with the Domeless Soler Telescope at Hida observatory






Wednesday 9 Nov

Chair: Krishnappa Nagaraju

09:00-09:30

Keynote

F. Zeuner

S2

Hanle rotation finally revealed in Sr I 4607

09:30-09:50


Y. Katsukawa

S2

Polarization measurement of the O V 121.83 nm intercombination line with CLASP

09:50-10:10


R. Ishikawa

S2

Observational Evidence for the Hanle and Magneto-Optical Effects in the Polarization of the Mg II h & k Lines Observed by CLASP2

10:10-10:40

Break & Poster (30 min)

10:40-11:20

Review

R. Centeno

S4

Magnetic field diagnostic for the Solar Chromosphere

11:20-11:40


J. Jurcak

S4

Mapping the magnetic field azimuth in the chromosphere

11:40-12:00


X. Zhou

S2

Synthetic Ca II 8542Å Stokes profile of chromospheric magnetic reconnection in emerging flux region

12:00-13:30

Lunch Break (90 min)

Chair: Ernest Alsina Ballester

13:30-14:00

Keynote

Y. Kawabata

S2

Chromospheric magnetic field in active regions

14:00-14:20


H. Mathur

S2

Does the Hα Stokes V profiles probe the chromospheric magnetic field? An observational perspective

14:20-14:40


A. G. M. Pietrow

S2

Inference of the chromospheric magnetic field configuration of solar plage using the CaII 8542 angstrom line

14:40-15:00

(Remote)

K. Nagaraju

S2

Velocity and Magnetic Field of Outflows from a Magnetic Reconnection Event

15:00-15:50

Break & Poster (50 min)

15:50-16:20

Keynote

M. Goto

S5

Electron temperature anisotropy explored by the impact polarization of the Lyman-alpha line in fusion plasma

16:20-16:40

(Remote)

L. Belluzzi

S3

Modeling scattering polarization accounting for angle-dependent PRD effects

16:40-17:10

Keynote (remote)

G. Janett

S3

Multi-fidelity preconditioning of Krylov solvers for linear transfer problems of polarized radiation

17:10-17:30

P. Benedusi

S3

Scalable Matrix-free Solver for 3D Polarized Radiative Transfer in Stellar Atmospheres

17:30-17:50

(Remote)

M. Sampoorna

S3

Influence of Thomson Scattering Redistribution on Resonance Line Polarization






Thursday 10 Nov

Chair: Jan Jurcak

09:00-09:30

Keynote (remote)

T. Anan

S2

The impact of He I 1083 nm spectropolarimetry in solar physics

09:30-09:50


D. Yamasaki

S2

Investigation of the magnetic field structure of dark filaments by using a spectro-polarimetric observation with He I 1083 nm

09:50-10:10


S. Castellanos Duran

S2

Superstrong magnetic fields in bipolar light bridges

10:10-10:30


J. Okamoto

S2

The strongest magnetic fields in sunspots and their statistical properties

10:30-11:00

Break & Poster (30 min)

11:00-11:30

Keynote

G. Barnes

S4

An Overview of Disambiguation Techniques

11:30-11:50


L. Bellot Rubio

S2

Unipolar and bipolar magnetic flux appearance in the quiet Sun internetwork

11:50-12:10

(Remote)

A. Kaithakkal

S2

Traits of a quiet Sun Ellerman Bomb

12:10-13:40

Lunch Break (90 min)

Chair: KD Leka

13:40-14:10

Keynote

D. Kuridze

S2

Spectropolarimetry of flaring active region

14:10-14:30


R. Yadav

S2

Stratification of physical parameters in a C-class solar flare using multi-line observations

14:30-14:50


A. B. Griñón Marín

S2

A new view into flaring sunspots

14:50-15:10

(Remote)

D. Kansabanik

S2

Recent Developments in Low-frequency Spectro-Polarimetric Snapshot Imaging Studies of the Radio Sun

15:10-15:30

(Remote)

M. Murabito

S2

The formation and disappearance of penumbra

15:30-16:30

Break & Poster (60 min)

16:30-17:10

Review (remote)

S. Bagnulo

S5

Magnetism in isolated white dwarfs

17:10-17:40

Keynote

J. Stepan

S4

Novel framework for the three-dimensional NLTE inverse problem






Friday 11 Nov

Chair: Ayumi Asai

09:00-09:30

Keynote

A. Pastor Yabar

S4

Spectropolarimetric inversions including magneto-hydrostatic constraints

09:30-09:50


S. Yang

S4

A fast approach to calibrate the vector magnetic field from the polarization measurement in Huairou Solar Observing Station

09:50-10:10


M. Kubo

S4

Comparison of polar magnetic fields derived from MILOS and MERLIN inversion for Hinode/SOT-SP data

10:10-10:30

(Remote)

Y. Liang

S4

The reliable noise reduction method for the Stokes spectral profiles

10:30-11:00

Break & Poster (30 min)

11:00-11:30

Keynote

C. J. Díaz Baso

S4

Unlocking the potential of deep learning for the analysis of spectropolarimetric observations

11:30-11:50


J. Sinjan

S2

SO/PHI-HRT SDO/HMI Cross-Calibration and the True Solar Magnetic Flux

11:50-12:30

Review

K. Ichimoto

S2

Spectro-polarimetry of the sun from space and ground: : What we learned and issues for the future

12:30

Adjourn


Poster

[On-line poster presentation]
Please send your PDF file (10 MB max) of your poster presentation to the LOC email address
(spw10-loc@kwasan.kyoto-u.ac.jp) by Thursday, November 3, 23:59 JST. It will be posted on the SPW10 website for the participants
to view. We are going to setup Slack channels for communication among the participants.

[On-site poster]
Poster boards are available in the conference hall. If you are an in-person participant and wish to
display a poster on-site, please bring your poster (smaller than A0 size).

[Poster flash talk]
We have flash talk sessions on Tuesday 8 Nov. Please prepare a slide for your short presentation.
For each presentation, a 4-minute talk and a 1-minute Q&A will be allocated.


Top image is the dome of the 45 cm refractor telescope in the Kwasan Observatory, Kyoto University.