Energetic particle environment as seen by RESIK Royal Observatory of Belgium 04-05-2012 Szymon Gburek SRC-PAS.

Slides:

Advertisements

Similar presentations

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.

Advertisements

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

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

Locations of Boundaries of the Outer and Inner Radiation Belts during the Recent Solar Minimum, as Observed by Cluster and Double Star Natalia Ganushkina.

RHESSI observations of LDE flares – extremely long persisting HXR sources Mrozek, T., Kołomański, S., Bąk-Stęślicka, U. Astronomical Institute University.

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

Saeedeh Ghaffari Nanofabrication Fall 2011 April 15 1.

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,

21 ECRS, Kosice, 12/09/2008 Trapped charge particles measurements in the radiation belt by PAMELA instrument Vladimir V. Mikhailov (MEPHI) for PAMELA collaboration.

Atomic X-Ray Spectroscopy Chapter 12 X-ray range  Å to 100 Å Used  0.1Å to 25 Å.

Working Group 2 - Ion acceleration and interactions.

RHESSI/GOES Observations of the Non-flaring Sun from 2002 to J. McTiernan SSL/UCB.

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.

RHESSI observations of LDE flares – extremely long persisting HXR sources Mrozek, T., Kołomański, S., Bąk-Stęślicka, U. Astronomical Institute University.

RHESSI/GOES Observations of the Non-flaring Sun from 2002 to J. McTiernan SSL/UCB.

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,

etc… Analysing samples with complex geometries Particles Inclusions

Shu Zhang (on behalf of the HXMT team) Institute of High Energy Physics, Chinese Academy of Science The current status of HXMT and its calibrations.

Examples: Orbital Filling, Valence Electrons, and Noble Gas Notation.

PROBA2 a Space Weather Monitor Matthew J West ESWW10 - Nov 2013.

Absolutely Calibrating an Energy Dispersive Detector Patrick Ross Spring Research Conference.

X-ray Timing and Polarization mission & instrumentation DONG Yongwei Center for Particle Astrophysics Institute of High Energy Physics, Chinese Academy.

Radiation conditions during the GAMMA-400 observations:

Chapter 12 Atomic X-Ray Spectroscopy

The Hard X-ray Modulation Telescope Mission

Ion Beam Analysis Dolly Langa Physics Department, University of Pretoria, South Africa Blane Lomberg Physics Department, University of the Western Cape,

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.

Degradation of LYRA on PROBA2 after two years in orbit I. E. Dammasch STCE Workshop Brussels, 03 May 2012 LYRA the Large-Yield Radiometer onboard PROBA2.

Hayabusa Data Archives Makoto Yoshikawa (JAXA) COSPAR Capacity Building Workshop on Planetary Science July 23 - Aug. 3, 2007 Montevideo, Uruguay.

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

Gamma-Ray Bursts observed with INTEGRAL and XMM- Newton Sinead McGlynn School of Physics University College Dublin.

6 October 2005 Geant4 Workshop, Leuven, Belgium Geant4 Model of SIXS Particle Instrument and Preliminary Simulation Results Lehti, J. (ASRO) Valtonen,

GOES fluence in Å and Å (1 min data) GOES fluence in Å and Å (1 min data) Areas in black correspond to times with the data missing.

Geant4 simulation for the study of origins of the background of the X-ray CCD camera onboard the Suzaku satellite ○ Takayasu Anada, Masanobu Ozaki, Tadayasu.

Final Presentation By Matthew Lewis 17 th March 2006 “To Determine the Accuracy that GOES True Numbers can Reproduce the Full X-ray Spectrum of the Sun”

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

In Situ Measurements of Auroral Acceleration Regions Wu Tong

D. E. McKenzie (Montana State University), S. Gburek (Space Research Centre, Polish Academy of Sciences), L. W. Acton, P. C. Martens (Montana State University)

Aug , 2006 KJYAM 慶州 1 Suzaku Observation of Nearby Seyfert 2 Galaxy NGC 4945 Naoki Isobe (RIKEN, Japan) and Suzaku NGC 4945 team.

(a) (b) (c) DETX DETY DETX DETY XIS2 DETX DETY XIS0 XIS2 Counts keV -1 ACTY N. Tawa, M. Nagai, K. Hayasida, H. Nakamoto, M. Namiki (Osaka-U), H. Yamaguchi.

Nishu Karna Mentor:Dr. William Dean Pesnell Code: 671 SESI Program-2009 Goddard Space Flight Center St. Cloud State University Date: August 5, 2009 RELATIVISTIC.

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

2 Jun 2022 Jan 2030 Sep 2032 Jun months 1 month 9 months 11 months 9 months Launch Ariane-5 Jupiter orbit insertion Transfer to Callisto Europa.

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

Spitzer Space Telescope

Observation of cosmic gamma-ray bursts and solar flares in the ''RELEC'' experiment on the ''VERNOV'' satellite.

Example of the output produced by XRF

XUV monochromatic imaging spectroscopy in the SPIRIT experiment on the CORONAS-F mission I. Diagnostics of solar corona plasma by means of EUV Spectroheliograph.

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.

Exploring an evidence of supermassive black hole binaries in AGN with MAXI Naoki Isobe (RIKEN, ) and the MAXI

HISAKI mission – ひさき – Chihiro Tao 1,2, Nicolas Andre 1, Hisaki/EXCEED team 1. IRAP, Univ. de Toulouse/UPS-OMP/CNRS 2. now at NICT

RESIK & Diogeness on the Payload & Coronas-F pointing This week, we show the location of both Polish spectrometers within the CORONAS-F satellite payload.

Introduction to SEPs Christina Cohen Caltech. Outline What are SEPs? ›And why do we care? How are the measured? ›on the ground ›in space What is the SEP.

SS Special Section of JGR Space Physics Marks Polar’s 5th Anniversary September 4, 1996 This April special section is first of two Polar special sections.

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

Dose Mapping for the SIXS Module and X-ray detector BepiColombo Mission 7 th GEANT4 Space Users’ Workshop August 18 – 20, 2010 Seattle - USA F. García,

Gyeongbok Jo 1, Jongdae Sohn 2, KyeongWook Min 2, Yu Yi 1, Suk-bin Kang 2 1 Chungnam National University 2 Korea Advanced Institute of Science.

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

Physics of Solar Flares

Solar gamma-ray and neutron registration capabilities of the GRIS instrument onboard the International Space Station Yu. A. Trofimov, Yu. D. Kotov, V.

A joint study of the University of Göttingen (1) and Astrium (2)

LET Performance Requirements Presenter: Richard Mewaldt

THEMIS and Space Weather

R. Bucˇık , K. Kudela and S. N. Kuznetsov

Monitor of All sky X-ray Image (MAXI)

Presentation transcript:

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

RESIK REntgenovsky Spektrometr s Izognutymi Kristalami X-ray Spectrometer with bent cristals

Primary scientific objectives of RESIK − the chemical composition of X-ray flare and active region plasmas using emission line and continuum intensities − the temperature & differential emission measure studies.

Gas filled proportional counters The same as for BCS on Yohkoh Fe55 Calibration source RESIK Detectors and operation principle + Four PIN diods behind the thick Al shield Particle detectors

X-ray data obtained from RESIK spectra, lightcurves 2.0 keV keV (3.3 Å Å) resolving power (λ/Δλ) of ∼ 1000 (10 m Å) Aug 24, May 22, 2003

RESIK WWW data visualization catalogue

A sample plot from RESIK daily pages of WWW catalogue

RESIK Diogeness Location of RESIK & DIOGENESS instruments on the satellite platform Drawing of the CORONAS-F payload

CORONAS-F launch, 2001 July 31

ORBIT Near-circular orbit around the Altitude from ~501 km to ~ 549 km Inclined at 82.5 ◦ Period is 94.9 min SAA + Rad Belt Nights up to ~35 min, Long days ~2 – 3 weeks

Correlation diagram between PIN and MKL rates. Distri-bution of rates as seen by RESIK PIN detectors in May 2002.

Changes in time 05-May 15-May 30-May

What kind of particles We see? AE-8, AP-8 Geometry -> shielding GEANT 4 modeling

Complementary data sets RESIK/DIOGENESSSphinX