Meeting Programme

 

 

Tuesday, December 09

 

Registration of participants, 09:00 – 10:00

 

Welcome addresses, 10:00 – 10:10

 

Chair J. Sylwester, SRC PAS

President of Wrocław PAS division - Prof. D.J. Bem

 

Morning Session, 10:10 – 12:50

 

Chair J. Sylwester, SRC PAS

The impact of CORONAS Multimission project.

 

10:10 - 10:40 S. Kuzin

The EUV imaging spectroscopy experiment TESIS onboard the CORONAS Photon

satellite.

 

10:40 – 11:10 A. Ignatiev

Planning of observations, data processing and storage for SPIRIT and

TESIS experiments.

 

11:10 – 11:40 A. Pertsov

The main control systems for X-ray imaging spectroscopy experiments

on Fobos-1 through CORONAS-PHOTON.

 

11:40 – 12:15 Coffee break

 

Chair E. Dzifč‡kov‡, Comenius University, Bratislava

Data analysis with RESIK spectrometer.

 

12:15 – 12:30 J. Sylwester, A. Kulinova & M. Kowaliński

Impact of local spacecraft environment on RESIK and SphinX measurements.

 

12:30 - 12:50 A. Kępa, B. Sylwester, J. Sylwester

Plans for further reduction, visualization and archiving of RESIK spectra.

 

12:50 – 15:00 Lunch break

 

Afternoon Session, 15:00 - 16:45

 

Chair S. Kuzin, FIAN

Dynamics of Solar Corona.

 

15:00 – 15:30 M. Livshits and M. Katsova

Test by observations for a new model of large CME/flare events on

the Sun and late-type stars.

 

15:30 – 16:00 Coffee break

 

16:00 – 16:30 V. Slemzin

EUV observations of the solar corona and transients at 1-5 Rsun with

the SPIRIT telescope-coronagraph.

 

16:30 – 16:45 E. Dzifcakova, A. Kulinova

Is it possible to diagnose the non-thermal distributions from EUV

spectra?

 

 

 

Wednesday, December 10

 

Morning Session, 10:00 - 12:40

 

Chair S. Bogachev, FIAN

Diagnostics of Solar Corona.

 

10:00 – 10:30 A.Urnov

Determination of coronal plasma densities from Coronas observations.

 

10:30 – 10:50 B. Sylwester

Plasma temperature distribution & composition for low activity solar

corona.

 

10:50 – 11:30 Coffee break

 

11:30 – 11:50 T. Mrozek and S. Kołomański

RHESSI observation of extremely long persisting HXR sources - SphinX

wanted immediately.

 

11:50 – 12:20 A. Kulinova, E. Dzifč‡kov‡ & J. Sylwester

The non-thermal diagnostics of flares observed by RESIK.

 

12:20 – 12:40 J. Kasparova

Application of kappa distribution to RHESSI flare spectra.

 

12:40 – 15:15  Lunch break

 

 

 

 

 

Afternoon Session, 15:15 - 16:45

 

Chair A.Pertsov, FIAN

SphinX instrument development

 

15:15 – 15:25 J. Bąkała

SphinX – mechanical construction, assembly with TESIS and final

launch preparations.

 

15:25 – 15:40 S. Gburek

SphinX data and software.

 

15:40 – 16:15 Coffee break

 

16:15 – 16:30 M. Siarkowski

SphinX data calibration.

 

16:30 – 16:45 P. Podg—rski

SphinX dead times and throughput.

 

 

Thursday, December 11

 

Morning Session, 10:00 - 12:30

 

Chair S. Gburek, SRC PAS

Solar flares – theory and observations.

 

10:00 – 10:30 S. Bogachev

Particle acceleration in collapsing magnetic traps and hard x-ray

emission of solar flares.

                                                                                      A work awarded with Zeldovich medal

 

10:30 – 11:00 F. Reale, P. Testa, J. Klimchuk, S. Parenti

Constraints on nano-flaring plasma from Hinode/XRT observations of

active regions.

 

11:00 – 11:30 Coffee break

 

Chair F. Reale, University of Palermo

SphinX operation and data analysis.

 

11:30 – 12:00 J. Sylwester & SphinX Team

Operation of SphinX during early phase of the CORONAS-Photon

Mission.

 

12:00 – 12:15 B. Sylwester & J. Sylwester

SphinX spectral synthesis for low activity corona.

 

12:15 – 12:30 J. Sylwester

Meeting summary talk.

 

12:30 – 15:00 Lunch break

 

Afternoon Session, 15:00 - 17:00

 

15:00 – 15:40 Discussion session

 

15:40 – 16:15 Coffee break

 

16:15 – 17:00 Discussion session

 

 

Friday, December 12

 

09:30 – approx. 15:00

Trip to Białk—w observatory.

 

11:00 – 11:30 Coffee break

 

 

Białk—w observatory belongs to Wrocław University and is managed andoperated by scientist from Astronomical Institute, University of Wrocław. The observatory is located 70 km north-west of Wrocław. Several solar and stellar instruments are used in Białk—w for observations including large coronagraph producing excellent

quality data. More information can be found at http://helio.astro.uni.wroc.pl/helio_bialkow_observatory.html (unfortunately

in Polish).