GIS – an update Dr Lucie Green Mullard Space Science Laboratory UCL.

Slides:



Advertisements
Similar presentations
GIS-UDRIL Project Current Activities and Plans May, 2003 Compilation Databases Atlases Archives Enhancement Databases Archives.
Advertisements

000509EISPDR_SciInvGIs.1 EIS Performance and Operations Louise Harra Mullard Space Science Laboratory University College London.
Overview Review of the Goddard method Update on instrument/detector evolution (a purely phenomenological approach) Characterization of the soft proton.
XMM EPIC MOS Jenny Carter 4 th EPIC BG WG Meeting Mallorca, 25/10/06 BGWG blank sky data analysis Jenny Carter, University of Leicester.
Hinode/EIS Data Products and Archive Access Jian Sun (MSSL)
Transition Region Redshifts in Quiet Sun, Coronal Hole, and Active Region Ingolf E. Dammasch Solar Influences Data Analysis Center, Royal Observatory of.
Initial Results of EIS Shinsuke Imada (NAOJ) EIS Team.
1 Hinode Coordinated Observations: Heat Transfer Contributed by the Hinode/EIS team through the Naval Research Laboratory and University College London.
Hinode’s Extreme ultraviolet Imaging Spectrometer (EIS) Data acquisition and calibration primer Presented by Jason Scott.
990901EIS_Opt.1 The Instrument: Optical Design Dr. John T. Mariska Data Coordination Scientist Naval Research Laboratory
000509EISPDR_SciInvGIs.1 EIS Science Goals: The First Three Months…. Louise Harra Mullard Space Science Laboratory University College London.
Ingolf E. Dammasch ROB/SIDC Brussels, Belgium Solar UV Spectroscopy with SUMER on SOHO.
ALFVEN WAVES IN A POLAR CORONAL HOLE FROM HINODE/EIS OFF LIMB OBSERVATIONS Bemporad A. & Abbo L. –
GRID Activities at ESAC Science Archives and Computer Engineering Unit Science Operations Department ESA/ESAC – Madrid, Spain.
Important Work for Today Definition of HXT data archive Definition of WBS data archive Assign responsibilities and agree SCHEDULE Discuss new or improved.
The EUV spectral irradiance of the Sun from minimum to maximum Giulio Del Zanna Department of Space and Climate Physics University College London Vincenzo.
Chandra Calibration Status Summary 1.The gratings and mirrors are very well calibrated at this time and there are no time-dependent effects as far as we.
Chandra Calibration Status  Recent releases  Current Calibration projects  Cross-Calibration between Chandra and other X-ray telescopes  Revisions.
High-latitude activity and its relationship to the mid-latitude solar activity. Elena E. Benevolenskaya & J. Todd Hoeksema Stanford University Abstract.
Ingolf E. Dammasch ROB/SIDC Brussels, Belgium Solar UV Spectroscopy with SUMER on SOHO (extended version for 11 Oct 2007)
08__050610_SCIP/SEB_PSR_Delivery.1 Temperature and Density Diagnostics with SECCHI EUVI J.S. Newmark Naval Research Laboratory (202)
The Solar-B EUV Imaging Spectrometer: an Overview of EIS J. L. Culhane Mullard Space Science Laboratory University College London.
Sunspot Studies in Oslo Nils Brynildsen, Per Maltby, Terje Fredvik and Olav Kjeldseth-Moe Institute of Theoretical Astrophysics University of Oslo.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
CDS Session NAM Dublin April Active Region Loop Studies in Oslo Olav Kjeldseth-Moe and Terje Fredvik Institute of Theoretical Astrophysics University.
Astronomical GRID Applications at ESAC Science Archives and Computer Engineering Unit Science Operations Department ESA/ESAC.
990901EIS_RR_Science.1 Science Investigation Goals and Instrument Requirements Dr. George A. Doschek EIS US Principal Investigator Naval Research Laboratory.
1 Long-term Solar Synoptic Measurements with Implications for the Solar Cycle Leif Svalgaard Stanford University 23 April 2013.
1 TIPS 2011 May Persistence in the WFC3 IR detector Knox S. Long.
Solar-B Mission Preparation Len Culhane – UK EIS Principal Investigator Louise Harra – UK Project Scientist David Williams – UK EIS Chief Observer Mullard.
Detecting EUV waves Detecting Dimmings www. SolarDemon.oma.be near real-time, Flare, Dimming, and EUV wave Monitoring E. Kraaikamp 1, C. Verbeeck 1, and.
EIS - MSSL/NRL EUV Imaging Spectrometer SOT - ISAS/NAOJ Solar Optical Telescope XRT - SAO/ISAS X-ray Telescope FPP - Lockheed/NAOJ Focal Plane Package.
SOHO/CDS CDS Users’ Meeting, Sep 2005 Dr Peter Young, CCLRC/RAL Element Abundance Results from CDS Dr Peter Young Dr Peter Young SOHO/CDS Project Scientist.
STIS Closeout Plan Paul Goudfrooij 2005 HST Calibration Workshop, 10/26/2005.
Innovations in the Multimission Archive at STScI (MAST) M. Corbin, M. Donahue, C. Imhoff, T. Kimball, K. Levay, P. Padovani, M. Postman, M. Smith, R. Thompson.
The Solar-B EUV Imaging Spectrometer: an Overview of EIS J. L. Culhane Mullard Space Science Laboratory University College London.
1 “STEREO PLASTIC STATUS REPORT” A.B. Galvin Lorna Ellis (Data) Mark Popecki (Operations) Team (Science) STEREO SWG Meredith NH October 27, 2009.
Science with the new HST after SM4 WFC3 slitless spectroscopy Harald Kuntschner Martin Kümmel, Jeremy R. Walsh (ST-ECF) WFC3-team at STScI and NASA.
R-Alice Lutetia PDS/PSA Data Review Kurt Retherford.
April , 2006 HEASARC Users Group Steve Drake RXTE Archive at HEASARC Status and Plans Steve Drake.
KIM TOLBERT THE CATHOLIC UNIVERSITY OF AMERICA AND GODDARD SPACE FLIGHT CENTER FERMI Solar Data Availability and Quicklook Plots Fermi Solar Data Analysis.
EUV Imaging Spectrometer (EIS): Instrument Checkout, Performance Verification and Initial 90 Day Observing Plan Extended Solar Optical Telescope Meeting.
1-D Flat Fields for COS G130M and G160M Tom Ake TIPS 17 June 2010.
Joint Planning of SOT/XRT/EIS Observations Outline of 90 Day Initial Observing Plans T. Shimizu, L Culhane.
R-Alice Lutetia PDS/PSA Data Review Kurt Retherford.
Line Profile Characteristics of Solar Explosive Event Bursts Z. Ning et al 2004 A&A 419,1141 Speaker: Jinping Dun.
STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG March 27-28, 2007.
Modeling the UV/EUV and its relevance for PROBA2 observations Margit Haberreiter Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center,
14 January Observational Astronomy SPECTROSCOPIC data reduction Piskunov & Valenti 2002, A&A 385, 1095.
PACS NHSC Data Processing Workshop Aug 26-30, 2013 Page 1 SPIRE Spectrometer Data: Calibration Updates, User Data Reprocessing, and Other Issues Nanyao.
Page 1 NHSC PACS Web Tutorial PACS 301 nhsc.ipac.caltech.edu/helpdesk NHSC/PACS Web Tutorials Running the PACS Spectrometer pipeline for CHOP/NOD Mode.
The Mauna Loa Solar Observatory (MLSO) Data Archive Tony Darnell Joan Burkepile and Andrew Stanger High Altitude Observatory P.O.
NAM and UKSTP 11 April 2003 Sensitivity Differences in Pre-Loss and Post-Recovery NIS/CDS Spectrum By Steven Chapman Centre for Astrophysics University.
020116EIS_JTM.1 EIS Sensitivity Update John Mariska NRL 3-5 Feb 2003.
Spectrometer Throughput Dr Peter Young Consortium meeting, 3 March 2006.
EOVSA Data and Database System J. McTiernan EOVSA Technical DesignMeeting 7-Nov-2011.
UCL DEPT. OF SPACE & CLIMATE PHYSICS SOLAR & STELLAR PHYSICS GROUP Atomic Data for Astrophysics VOTada VO Tools and Atomic Data for Astrophysics Giulio.
DAA PEACE Status A. Fazakerley, B. Mihaljčić, I. Rozum, A. Lahiff, G. Watson, D. Kataria UCL Department of Space and Climate Physics Mullard Space Science.
The STIS NUV-MAMA objective prism … … and looking beyond for HST UV slitless spectroscopy Jes ú s Ma í z Apell á niz HST Calibration worskhop 26 October.
Coronal Hole recognition by He 1083 nm imaging spectroscopy O. Malanushenko (NSO) and H.P.Jones (NASA's GSFC) Tucson, Arizona, USA Solar Image Recognition.
1 MURI:NADIR Progress on Area 6 solar features forecast October 2010.
Using Solar-B EIS – lessons from SOHO/CDS Peter Young*, Andrzej Fludra CCLRC Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire, OX11 0QX, U.K.
A. Ealet Berkeley, december Spectrograph calibration Determination of specifications Calibration strategy Note in
Spectroscopic Observations with SolarB-EIS Helen E. Mason DAMTP, Centre for Mathematical Sciences Giulio Del Zanna, MSSL.
Dimming analysis 13/05/05 Gemma Attrill
COS FUV Flat Fields and Signal-to-Noise Characteristics
Spectral Line Measurement
First Assessments of EUVI Performance on STEREO SECCHI
Studying Transition Region Phenomena with Solar-B/EIS
Slit and Slot Interchange
Presentation transcript:

GIS – an update Dr Lucie Green Mullard Space Science Laboratory UCL

To get Good recent spectra Webpages to go through Giulio’s plot which show ghosted regions Ghost information file

GIS – New Web Pages

GIS – Users Guide

GIS – ghost information file The ghostbuster software generates an information file SPECTRAL ATLAS 4 / GIS Meridian Study T23:24:52.538, s31134r17.fits GSET: 66 ; Slit no/size: 2 / 4"x4" ; Pointing: [0,968] GIS Detector 1 - Likely Ghosting Regions Fe XI A line ghosts to 160 A, 1434 counts (15%) recovered Fe X A line ghosts to 157 A, 5791 counts (18%) recovered Fe X A line ghosts to 154 A, 6293 counts (16%) recovered Fe XII A line ghosts into 175 A --- Blend / unrecovered Fe XII 192. A line ghosts into A --- Blend / unrecovered Wavelengths affected by ghosting Locations of recovered counts Blended lines

GIS - Studies

GIS – Data Archive Synoptic observations run since the start of the mission. For example, quiet sun obs: -SPECT_1 Slit: 2x2" Raster area: 30x30" Exposure time: 30s -GIMCP Slit: 2x2" Raster area: 2x2" Exposure time: 100s Search the archive! IDL> headcat, cat96, year=1996 Search though cat96.SCI_OBJ to look for coronal holes, active region loops etc…

GIS – Line Intensities LTGD decreases line intensity and broadens lines Uncorrected intensities give an idea of detector evolution

SPECT_1 study Spectral line counts

GIS – LTGD methods Filament dumps GIS1 in 2001 GIMCPS1 study – line by line analysis 197 A 171A

GIS – Long-term Gain Depression Flat fields available Strong lines

bla

GIS – Line Profiles

No LTGD cor. Line widths with LTGD cor.

Summary Request observations Request data GIS is working well Revision of calibration is underway Comments on User Guide are welcome