X-POL Solar X- ray Pol arimeter Rudawy, P., Sylwester, J., Zawistowski, T., Siarkowski, M., Bąkała, J., Podgórski, P., Kowaliński, M. and Gburek, S. Space.

Slides:

Advertisements

Similar presentations

Line Features in RHESSI Spectra Kenneth J. H. Phillips Brian R. Dennis GSFC RHESSI Workshop Taos, NM 10 – 11 September 2003.

Advertisements

Thermal and nonthermal contributions to the solar flare X-ray flux B. Dennis & K. PhillipsNASA/GSFC, USA J. & B. SylwesterSRC, Poland R. Schwartz & K.

The Science of Solar B Transient phenomena – this aim covers the wide ranges of explosive phenomena observed on the Sun – from small scale flaring in the.

000509EISPDR_SciInvGIs.1 EIS Performance and Operations Louise Harra Mullard Space Science Laboratory University College London.

Low energy payload of Solar X-ray Spectrometer (SOXS) mission: instrument description and first results Dr. Tomasz Mrozek Astronomical Institute University.

SPHINX DATA ANALYSIS Magdalena Gryciuk Astronomical Institute, University of Wroclaw Space Research Centre, Polish Academy of Sciences I SOLARNET SPRING.

J. Sylwester, W. Trzebiński, M. Kowalinski, J. Bakala, Z. Kordylewski, J. Barylak, S. Gburek Space Research Centre, PAS, Wrocław, Poland I. Myagkova Skobel’tsyn.

Dipartimento di Scienze Fisiche & Astronomiche – Universita’ di Palermo INAF/Osservatorio Astronomico G.S. Vaiana Fabio Reale RESIK,RHESSI &SPIRIT workshop.

L. Teriaca, IMPRS Seminar, Lindau 08/12/04 Spectroscopy of the solar Transition Region and Corona L. Teriaca.

Masuda Flare: Remaining Problems on the Looptop Impulsive Hard X-ray Source in Solar Flares Satoshi Masuda (STEL, Nagoya Univ.)

THE IMPULSIVE X-RAY RESPONSE IN FLARE FOOTPOINTS TOMASZ MROZEK WROCLAW UNIWERSITY ASTRONOMICAL INSTITUTE POLAND.

COSPAR E July 22, Paris revised for Nobeyama Symposium 2004 October 29, Kiyosato Takeo Kosugi (ISAS/JAXA, Japan)

Physical characteristics of selected X-ray events observed with SphinX spectrophotometer B. Sylwester, J. Sylwester, M. Siarkowski Space Research Centre,

Cristina Chifor SESI Student Intern 2005 Solar Physics, Code 612 NASA/Goddard Space Flight Center Mentors: Dr. Ken Phillips & Dr. Brian Dennis FE AND FE/NI.

Workshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”, 6 – 8 December 2005, Wrocław Spectroscopy Department.

Page 1 Cristina Chifor (a) Ken Phillips (b), Brian Dennis (c) a) DAMTP, University of Cambridge, UK b) Mullard Space Science Lab, UK c) NASA/GSFC, Maryland,

The Focusing Optics X-ray Solar Imager (FOXSI) Steven Christe 1, S. Krucker 2, L. Glesener 2, S. Ishikawa 3, B. Ramsey 4, T. Takahashi 3, R.P. Lin 2 1.

High Altitude Observatory (HAO) – National Center for Atmospheric Research (NCAR) The National Center for Atmospheric Research is operated by the University.

Science With the Extreme-ultraviolet Spectrometer (EIS) on Solar-B by G. A. Doschek (with contributions from Harry Warren) presented at the STEREO/Solar-B.

Super-Hot Thermal Plasmas in Solar Flares

X-Ray Observation and Analysis of a M1.7 Class Flare Courtney Peck Advisors: Jiong Qiu and Wenjuan Liu.

The Non-Flare Temperature and Emission Measure Observed by RHESSI J.McTiernan (SSL/UCB) J.Klimchuk (NRL)

Measuring the Temperature of Hot Solar Flare Plasma with RHESSI Amir Caspi 1,2, Sam Krucker 2, Robert P. Lin 1,2 1 Department of Physics, University of.

The Non-Flare Temperature and Emission Measure Observed by RHESSI and SXI J.McTiernan (SSL/UCB) J.Klimchuk (NRL) Fall 2003 AGU Meeting.

From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.

35th COSPAR: Scientific Commission E1.9; Paris, July 2004 Identification of Lines in the Range 3.3 Å Å Observed in RESIK Spectra B. Sylwester,

S R CS R C 35th COSPAR Scientific Commission E1.9 Paris, July 2004 Analysis of Potassium Abundance in Selected Solar Flares J. Sylwester, B. Sylwester.

990901EIS_RR_Science.1 Science Investigation Goals and Instrument Requirements Dr. George A. Doschek EIS US Principal Investigator Naval Research Laboratory.

Science Specification of SOLAR-C payload SOLAR-C Working Group 2012 July 23.

Solar-B/EIS high-cadence observation for diagnostics of the corona and TR S. Kamio (Kyoto Univ.) Solar-B domestic meeting.

Co-spatial White Light and Hard X-ray Flare Footpoints seen above the Solar Limb: RHESSI and HMI observations Säm Krucker Space Sciences Laboratory, UC.

EIS - MSSL/NRL EUV Imaging Spectrometer SOT - ISAS/NAOJ Solar Optical Telescope XRT - SAO/ISAS X-ray Telescope FPP - Lockheed/NAOJ Focal Plane Package.

EUV Spectroscopy. High-resolution solar EUV spectroscopy.

Evolutionary pattern of DEM variations in flare(s) B. Sylwester, J. Sylwester, A. Kępa, T. Mrozek Space Research Centre, PAS, Wrocław, Poland K.J.H. Phillips.

Multiwavelength observations of a partially occulted solar flare Laura Bone, John C.Brown, Lyndsay Fletcher.

Compelling Theoretical Issues Driven by Observations / Theoretical Wish List of Observations WG5 Hamish Reid.

The Hard X-ray Modulation Telescope Mission

Probing Energy Release of Solar Flares M. Prijatelj Carnegie Mellon University Advisors: B. Chen, P. Jibben (SAO)

A Imaging Parameters A Imaging Parameters A

Spectroscopy Department Lebedev Physical Institute Moscow Solar Extreme Events: Fundamental Science and Applied Aspects (SEE-2005) International Symposium.

The Solar-B EUV Imaging Spectrometer: an Overview of EIS J. L. Culhane Mullard Space Science Laboratory University College London.

Energetic particle environment as seen by SphinX P. Podgorski 1, O. V. Dudnik 2, S. Gburek 1, M. Kowalinski 1, J. Sylwester 1, M. Siarkowski 1, S. Plocieniak.

Coronal hard X-ray sources and associated decimetric/metric radio emissions N. Vilmer D. Koutroumpa (Observatoire de Paris- LESIA) S.R Kane G. Hurford.

TESIS on CORONAS-PHOTON S. V. Kuzin (XRAS) and TESIS Team.

Outstanding Issues Gordon Holman & The SPD Summer School Faculty and Students.

Diagnostics of non-thermal n-distribution Kulinová, A. AÚ AVČR, Ondřejov, ČR FMFI UK, Bratislava, SR.

Solar space-born instruments and detectors for X-ray observations of the solar corona. Szymon Gburek Space Research Centre Polish Academy of Sciences,

Solar and STP science with AstroGrid Silvia Dalla School of Physics & Astronomy, University of Manchester A PPARC funded project.

Pre-flare activity of M1.2 flare 김수진 1,2, 문용재 1, 김연한 1, 박영득 1, 김갑성 2 1. Korea Astronomy and Space Science Institute 2. Kyung Hee University.

First SphinX Workshop 29 – 31 May, 2007, Wrocław Poland Janusz Sylwester Janusz Sylwester Space Research Centre, Polish Academy of Sciences, Wrocław Sergey.

Flare Differential Emission Measure from RESIK and RHESSI Spectra B. Sylwester, J. Sylwester, A. Kępa Space Research Centre, PAS, Wrocław, Poland T. Mrozek.

Flare Prediction and the Background Corona Coronal Diagnostic Spectrometer Wolter-Schwarzschild Type 2 telescope Two separate spectrometers- the Normal.

1 Coronas-F: payload, orbit, performance V. Slemzin CORONAS – Complex ORbital ObservatioNs of Activity of the Sun.

Preliminary Presentation By Matthew Lewis 2 nd December 2005.

RHESSI and the Solar Flare X-ray Spectrum Ken Phillips Presentation at Wroclaw Workshop “ X-ray spectroscopy and plasma diagnostics from the RESIK, RHESSI.

Energetic particle environment as seen by RESIK Royal Observatory of Belgium Szymon Gburek SRC-PAS.

Coronal X-ray Emissions in Partly Occulted Flares Paula Balciunaite, Steven Christe, Sam Krucker & R.P. Lin Space Sciences Lab, UC Berkeley limb thermal.

High Energy Observational Astrophysics. 1 Processes that emit X-rays and Gamma rays.

X-ray Spectroscopy of Coronal Plasmas Ken Phillips Scientific Associate, Natural History Museum, and Honorary Prof., QUB 1.

Spectroscopic Observations with SolarB-EIS Helen E. Mason DAMTP, Centre for Mathematical Sciences Giulio Del Zanna, MSSL.

Chandrayaan-2 Large Area Soft X-ray Spectrometer (CLASS)

Xenon gamma-ray detector for “SIGNAL” experiment

Physics of Solar Flares

Planning Flare Observations for Hinode/EIS

RHESSI Working Group 4 Program – Taos workshop

Chromospheric and Transition Region Dynamics

Understanding solar flares from optical observations Heinzel, P

Nonthermal Electrons in an Ejecta Associated with a Solar Flare

Transition Region and Coronal Explorer (TRACE)

Future prospects for EUV and soft X-ray solar spectroscopy missions

Presentation transcript:

X-POL Solar X- ray Pol arimeter Rudawy, P., Sylwester, J., Zawistowski, T., Siarkowski, M., Bąkała, J., Podgórski, P., Kowaliński, M. and Gburek, S. Space Research Centre, Polish Academy of Sciences ul. Kopernika 11, Wroclaw, POLAND

PURPOSE Understanding impulsive particle acceleration and plasma heating processes in the solar flares through X-ray polarimetry High energy- and time-resolution polarimetric observations Active regions Solar flares (non-stationary processes in flares; energy release and energy transport processes in solar flares) Impulsive acceleration of the non-thermal electrons Beam diagnostics Energy deposition in the solar chromosphere Temperature and differential emission measure studies (plasma diagnostics) Chemical composition of the coronal plasma; Space Research Centre, Polish Academy of Sciences

INSTRUMENT Space Research Centre, Polish Academy of Sciences Detectors:4 CCD back-iluminated fully depleted Energy range:soft X-rays 1.86Å (Fe XXV), 3.20Å (CaXIX), 4.0Å (ArXVII) Energy resolution:10 4 :1 Sensitivity:>C GOES class events Orbit:Sun synchronous preferred, altitude: >500 and <800 km Pointing: 2-axes stabilization, detector axis pointed to +/-2 º Lifetime:>3 years The overall size of the instrument is approx.: 32 cm x 26 cm x 26 cm Mass approx. 4 kg

INSTRUMENT Space Research Centre, Polish Academy of Sciences TWO-AXES ADJUSTABLE FRAME WITH THREE DETECTOR MODULES TOP VIEW UV-FILTERS & ENTRANCE CAPILLARY MESH PINHOLE SOLAR FLARE LOCATOR

Space Research Centre, Polish Academy of Sciences TWO-AXES ADJUSTABLE FRAME WITH THREE DETECTOR MODULES BENT CRISTAL CCD COOLER ENTRANCE CAPILLARY MESH INSTRUMENT

Space Research Centre, Polish Academy of Sciences INSTRUMENT w x+y z ArXVII He-like triplet

ENTRANCE CAPILLARY MESH TWO-AXES ADJUSTABLE FRAME WITH THREE DETECTOR MODULES CCD SOLAR FLARE LOCATOR MOTOR 1 MOTOR 2

TWO-AXES SUSPENSION HEAT-BELT TWO-AXES ADJUSTABLE FRAME WITH THREE DETECTOR MODULES

OUR HERITAGE RF15-I X-ray spectrophotometer- Imager (Interball-Tail, ) PI RESIK Bragg Bent crystal spectrometer 3-6 Å (Coronas-F, ) PI in collab. NRL, RAL, IZMIRAN Diogeness Bragg scanning spectrometer (Coronas-F, 2001) PI Solar Photometer in X-rays (SphinX) (Coronas-Foton, 2009) PI, in collab. U. Palermo, AI CAS ChemiX (InterHelioProbe, in prep. 2018) PI, in collab. IZMIRAN Space Research Centre, Polish Academy of Sciences

TWO BRAGG SPECTROMETERS CONSTRUCTED AT SRC WITH INTERNATIONAL COOPERATION RESIK - bent crystal spectrometer Diogeness - flat scanning crystal spectrometer Space Research Centre, Polish Academy of Sciences

New X-Ray emission lines and continuum emitted by active solar corona successfully measured for the first time in the wavelength range 3.3 – 6.1 Å. RESIK RESULTS Absolute abundance of argon determined for the first time for the Sun using direct spectroscopic tools. Similar results for S, Cl, K (series of ApJ papers) Space Research Centre, Polish Academy of Sciences

SphinX SRC CONCEPT, DESIGN & MANUFACTURE Measures the X-ray emission of the Sun in the 0.8 – 15 keV band with: – Time resolution ~10 μ s – Sensitivity 100 x better than GOES (the standard for 30+ years) – Energy resolution 3x RHESSI (NASA ) Principal aim: to record quiet-Sun level of emission Space Research Centre, Polish Academy of Sciences

ChemiX SRC CONCEPT & DESIGN Space Research Centre, Polish Academy of Sciences Basic Instrument parameters Mass: ~5 -6 kg Power consumption: ~10 W Size: 30cm x 30cm x 120cm Telemetry: up to 12 kB/s Specific instrument Characteristics Wavelength coverage: 1Å –7 Å, Qartz and Si Spectral resolution : better than Å Detectors: 3 CCD back illuminated & particle PIN Sensitivity: 1.5 –2 x RESIK, S/N: 10 xRESIK Collimators: multi-grid, slit, Electronics: FPGA based

X-POL Solar X- ray Pol arimeter Space Research Centre, Polish Academy of Sciences ul. Kopernika 11, Wroclaw, POLAND