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Download the program in PDF form.
Download the list of posters in PDF form.
Important dates
18 September 2022 |
Welcome reception |
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19-23 September 2022 |
Hinode 15 / IRIS 12 joint science meeting |
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Program overview
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Sun -18 Sep |
Mon -19 Sep |
Tue -20 Sep |
Wed -21 Sep |
Thu -22 Sep |
Fri -23 Sep |
8:00 - 9:00 |
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Registration |
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9:00 - 10:30 |
Welcome
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Session 1 |
Session 2
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Session 3 |
Session 4 |
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10:30 - 12:00 |
Poster session |
Poster session |
Poster session |
Poster session |
Poster session |
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12:00 - 13:00 |
Session 5 |
Session 2 |
Session 3 |
Session 3 |
New missions
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13:00 - 14:30 |
Lunch break |
Lunch break |
Lunch break |
Lunch break |
Lunch break |
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14:30 - 15:30 |
Session 5 |
Session 2 |
Organized tour |
Session 4 |
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15:30 - 17:00 |
Poster session |
Poster session |
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Poster session |
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17:00 - 18:00 |
Session 1 |
Session 2 |
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Session 4 |
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18:00 - 22:00 |
Welcome reception |
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19:30 - 23:00 |
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Conference dinner |
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Scientific program
Monday, September 19
Chair: Yukio Katsukawa |
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9:00 - 9:15 |
Welcome address |
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S5 Review |
9:15 - 9:45 |
C. J. Diaz Baso |
Application of machine learning and neural networks to data processing in solar physics |
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S5 Inv. |
9:45 - 10:05 |
R. Ishikawa |
Solar magnetic fields from the photosphere to the top chromosphere revealed by CLASP2 and Hinode |
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S5 Inv. |
10:05 - 10:25 |
J. Stepan |
Novel framework for the three-dimensional NLTE inverse problem |
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S5 |
12:00 - 12:15 |
N. Zambrana Prado |
Elemental composition diagnostics for Hinode/EIS |
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S5 |
12:15 - 12:30 |
B. Panos |
Explainable solar flare prediction using IRIS Mg II spectra |
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S5 |
12:30 - 12:45 |
K. Fukumitsu |
Image Restoration based on Deep Learning for High-Resolution Solar Images |
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S5 |
12:45 - 13:00 |
T. Pereira |
SunnyNet: Speeding up 3D non-LTE spectral synthesis with neural networks |
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Chair: Jana Kasparova |
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S5 |
14:30 - 14:45 |
D. Nobrega-Siverio |
Solar surges related to UV bursts: Characterization through k-means, inversions, and density diagnostics |
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S5
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14:45 - 15:00 |
N. Karna |
The study of polar coronal holes since the launch of Hinode |
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S5 |
15:00 - 15:15 |
J. M. Jenkins |
The Lightweaver 1.5D Spectral Synthesis of an MPI-AMRVAC Solar Prominence/Filament |
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S5 |
15:15 - 15:30 |
D.F. Ryan |
Deriving and Visualizing X-ray Source Properties in 3-D Using Hinode/XRT and SolO/STIX |
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S1 Review |
17:00 - 17:30 |
N. Bello Gonzalez |
Convective cells and magnetic fields |
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S1 |
17:30 - 17:45 |
N. Nitta |
How much do we know about the polar field? |
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S1 |
17:45 - 18:00 |
A. Popovas |
First results from global MHD simulations of Solar convective zone |
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Tuesday, September 20
Chair: Graham Kerr |
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S1 Inv. |
9:00 - 9:20 |
S.S.A. Silva |
Formation of vortex tubes |
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S1 Inv. |
9:20 - 9:40 |
K. Cho |
Generation of umbral oscillations and subsurface structure of sunspots |
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S1 Inv. |
9:40 - 10:00 |
R.T. Ishikawa |
Multi-scale deep learning for estimating horizontal velocity fields on the solar surface |
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S1 |
10:00 - 10:15 |
T. Oba |
Study of the relation between the reversed granulation and the gas compression/expansion |
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S1 |
10:15 - 10:30 |
L. Bellot Rubio |
Unipolar and bipolar magnetic flux appearance in the solar internetwork |
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S2 Review |
12:00 - 12:30 |
K. Reeves |
A Review of the Hinode and IRIS Contributions to Understanding Magnetic Reconnection and Prospects for the Future |
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S2
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12:30 - 12:45 |
Ying Li |
Spectroscopic observations of a solar flare from IRIS and CHASE |
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S2 |
12:45 - 13:00 |
S. Jejcic |
Non-LTE Inversion of Prominence Spectroscopic Observations in H-alpha and MgII lines |
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Chair: Sabrina Savage |
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S2 Inv. |
14:30 - 14:50 |
W. Ashfield |
Condensation in flares, observation and modeling |
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S2 Inv. |
14:50 - 15:10 |
R.J. French |
Probing Current Sheet Instabilities from Flare Ribbon Dynamics |
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S2 |
15:10 - 15:25 |
I. Cabello |
A textbook example of magnetic flux emergence leading to EBs, UV bursts, surges and EUV signatures |
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S2 |
17:00 - 17:15 |
S.L. Guglielmino |
Small-scale reconnection events observed by IRIS: microflares, UV bursts and their complex configurations |
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S2 |
17:15 - 17:30 |
M. Garcia-Rivas |
First co-temporal GREGOR and IRIS observations of a solar flare |
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S2 |
17:30 - 17:45 |
J. Zbinden |
How well can we predict flares based on IRIS Mg II, Si IV, and C II spectra? |
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S2
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17:45 - 18:00 |
G. Chintzoglou |
Revealing Strong Photospheric Downflows in Collisional Polarity Inversion Lines of Flare- and CME-Productive Active Regions |
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Wednesday, September 21
Chair: Bart De Pontieu |
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S2 |
9:00 - 9:15 |
S. Roy |
Thermal and Non-thermal Energy Evolution in Solar Flares |
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S2 |
9:15 - 9:30 |
J. Dudik |
Filament self-reconnection as a possible source of SADs |
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S3 Review |
9:30 - 10:00 |
D. Baker |
Upflows in active regions and their composition |
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S3 |
10:00 - 10:15 |
M. Gosic |
Emergence of internetwork magnetic fields into the chromosphere and transition region |
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S3 |
10:15 - 10:30 |
Yajie Chen |
Doppler shifts of spectral lines formed in the solar transition region and corona |
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S3 |
12:00 - 12:15 |
J. de la Cruz Rodriguez |
Spatially-resolved radiative losses in the chromosphere |
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S3 |
12:15 - 12:30 |
S. Bose |
On the correlation between chromospheric and coronal heating in an active region moss |
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S3 |
12:30 - 12:45 |
C.M.J. Osborne |
Considering the Radiative Interaction between Flares and Neighbouring Chromosphere |
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S3 |
12:45 - 13:00 |
M. Barta |
What is the temperature of solar prominences? First independent determination using ALMA, H-alpha, and IRIS |
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Thursday, September 22
Chair: Sarah Matthews |
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S3 Inv. |
9:00 - 9:20 |
J. M. da Silva Santos |
Heating of the solar chromosphere |
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S3 Inv.
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9:20 - 9:40 |
Leping Li |
Coronal condensations in hybrid prominence/coronal rain structures |
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S3 |
9:45 - 10:00 |
V. Hansteen |
Mg II formation in the Solar Chromosphere |
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S3 |
10:00 - 10:15 |
S. Sahin
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Prevalence of Thermal Non-Equilibrium over an Active Region |
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S3 |
10:15 - 10:30 |
P. Testa |
Evolution of coronal abundances in active regions |
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S3 |
12:00 - 12:15 |
T.A. Howson |
The atmospheric response to heating driven by random foot point driving |
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S3 |
12:15 - 12:30 |
R. Morosin |
Spatio-temporal analysis of chromospheric heating in a plage region |
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S3 |
12:30 - 12:45 |
T. Mihailescu |
What determines active region coronal plasma composition? |
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S3 |
12:45 - 13:00 |
S. Mulay |
A detailed investigation of molecular hydrogen at three flare ribbons |
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Chair: Patrick Antolin |
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S4 Review |
14:30 - 15:00 |
K. Karampelas |
MHD waves and instabilities in relation to oscillatory reconnection |
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S4 |
15:00 - 15:15 |
A. Sainz Dalda |
Turbulence in the chromosphere during flares: taking on the challenge. |
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S4 |
15:15 - 15:30 |
M. Murabito |
Relationship between high FIP bias and magnetic wave power |
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S4 |
17:00 - 17:15 |
J. Lorincik |
Rapid variations of Si IV line properties in an M-class flare observed by IRIS at very high cadence |
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S4 |
17:15 - 17:30 |
J. Joshi |
Properties of ubiquitous magnetic reconnection events in the lower solar atmosphere |
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S4 |
17:30 - 17:45 |
P. Kohutova |
Coronal oscillations in the self-consistent 3D MHD simulations of the solar atmosphere |
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S4 |
17:45 - 18:00 |
Y. Kotani |
Universal Correlation between the Ejected Mass and Total Flare Energy for Solar and Stellar Cold Plasma Ejection |
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Friday, September 23
Chair: Bernhard Fleck |
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S4 Inv.
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9:00 - 9:20 |
Wenxian Li |
Coronal magnetic fields measurement using MIT method |
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S4 Inv. |
9:20 - 9:40 |
B. Popescu Braileanu |
Ion-neutral interactions, MHD instabilities |
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S4 |
9:40 - 9:55 |
V. Polito |
IRIS and NuSTAR observations of a small B-class flare |
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S4 |
9:55 - 10:10 |
P. Ondratschek |
MgII spectra of an enhanced network region simulated with the MURaM code |
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S4 |
10:10 - 10:25 |
A.R.C. Sukarmadji |
Nanojets as pointers to the flare initiation process |
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12:00 - 12:20 |
B. De Pontieu |
The MUlti-slit Solar Explorer mission |
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12:20 - 12:40 |
T. Shimizu |
Solar-C EUVST |
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12:40 - 13:00 |
Closure of the meeting |
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