Michael L. Kaiser STEREO Project Scientist NASA/Goddard Space Flight Center STEREO May 2, 2008 STEREO at 1.25 years.

Slides:

Advertisements

Similar presentations

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

Advertisements

© Crown copyright Met Office Requirement for transitioning radio heliophysics research into operations David Jackson Radio Heliophysics Infrastructure.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG #22 (via telecon)

Sun Earth Connection Coronal and Heliospheric Investigation STEREO and SECCHI Status Consortium Meeting, Abingdon July 2001 Russ Howard.

1 STEREO Today Status report presented by Janet Luhmann and Peter Schroeder for the ACE/STEREO/WIND/SOHO Workshop 2010 June 8-10, Kennebunkport (Material.

CStCyr—SECCHI Paris-Mar #1 STEREO SECCHI COR1 Status O. C. St. Cyr for J.M. Davila and COR1 science team Heliophysics Science Division – Code 670.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center Phase E Kickoff Meeting February 23, 2007.

COR1 Science Overview Joseph M Davila Goddard Space Flight Center.

STEREO Space Weather Beacon: December 2003 D.A. Biesecker NOAA/SEC.

IMPACT Report SSMO Receiving Review– January 23, 2007.

The Solar and Space Weather Reseach Group in Lund Space weather Solar activity - the driver Modelling and forecasting space weather and effects using KBN.

SECCHI – Sun-Earth Connections Coronal and Heliospheric Investigation SECCHI Synoptic and Special Observing Programs Simon Plunkett SECCHI Operations Lead.

2007 March 61 The SECCHI Campaign Jean-Pierre Wuelser SECCHI Consortium Meeting Orsay.

Solar Polar Orbit Radio Telescope (SPORT): A Mission Concept for Interplanetary CMEs Imaging WU Ji, LIU Hao, SUN Weiying, ZHENG Jianhua, FENG Xueshang,

STEREO Science Center SWG – Dec 2004 William Thompson NASA Goddard SFC Code Greenbelt, MD

STEREO Science Center SWG – May 2005 William Thompson NASA Goddard SFC Code Greenbelt, MD

STEREO Science Center William Thompson NASA Goddard SFC Code Greenbelt, MD

Terry Kucera Deputy Project Scientist NASA/Goddard Space Flight Center STEREO: 360° of Sun Museum Alliance & Solar System.

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.

NASA, CGMS-41, July 2013 Coordination Group for Meteorological Satellites - CGMS NASA Space Weather Activities Presented to CGMS-41 Ad-hoc meeting on space.

3D Heliospheric Reconstructions from the SECCHI White Light Coronagraphs Onboard STEREO: Overview of the NRL Approach J. Newmark, J. Cook, P. Reiser, P.

7/12/20011 Observing Sequences in View of the SECCHI Science Goals From the EUVI Perspective J-P. Wülser.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG #23 29 March 2012 (via telecon)

STEREO Space Weather Group update Dave Webb ISR, Boston College and Air Force Research Laboratory STEREO SWG October 2009 Meredith, NH.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG 3-5 February 2009 Pasadena, California.

STEREO - Solar Terrestrial Relations Observatory Mission STEREO STEREO Science Team Meeting May 2, 2005 Presented by Edward Reynolds APL STEREO Project.

System for Radiation Environment characterization (fluxes, doses, dose equivalents at Earth, Moon and Mars) on hourly thru yearly time frame Example: Snapshots.

Instrument Performance Spefication 13 July 2001 SECCHI Consortium Meeting Cosner’s House, Abington Dan Moses.

195 Å image – behind 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – ahead SECCHI Extreme.

China National Report , Uppsala, Sweden China National Space Administration.

STEREO: Beyond 3D. Why the Sun? The sun provides energy for the development of life on our planet. Our orbit looks calm and peaceful, but there is nothing.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG April 2008 Meudon, France.

Advances in Space Imaging Russell A. Howard Naval Research Laboratory NSF Workshop on Small Missions, May 2007.

SUN, EARTH AND SPACE. THE SUN CLOSE UP: INSIDE AND OUT.

Michael L. Kaiser STEREO Project Scientist NASA/Goddard Space Flight Center STEREO June 11, 2008 STEREO at 1.4 years.

IMPACT SWG Status Report – December 11, Early IMPACT Timeline Status Day 3,410-28, 10-29IDPU/MAG/SWEA and STE turned on Day 711-1Booms deployed.

SECCHI Status Russell A. Howard & The SECCHI Team 3 Feb 2009 STEREO SWG - Pasadena.

IMPACT Data Plans May 2006 Peter Schroeder UC-Berkeley

William Thompson L-3 Communications NASA Goddard Space Flight Center STERE The STEREO Science Center.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG March 27-28, 2007.

STEREO - Solar Terrestrial Relations Observatory Mission SECCHI Calibration Activities Simon Plunkett SECCHI Operations Scientist Naval Research Laboratory.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG November 2007 Pasadena, California.

Solar Terrestrial Relations Observatory In-Situ “STEREO” Science Plans Presentation to STEREO SWG, Hamburg, May, 2005 (J. Luhmann and A. Galvin for the.

Solar weather consists of the Sun’s effects upon its planetary system and the solar activities it causes. Solar activities, such as flares and CMEs, form.

STEREO Space Weather Beacon: March 2004 D.A. Biesecker NOAA/SEC.

SECCHI Status Russell A. Howard & The SECCHI Team March 2010 STEREO SWG – Trinity College, Dublin.

SSC Support for Sim #3 Archived MOC Data Products, and distributed via web. –Level-0 telemetry files organized by year and month –SPICE orbit and attitude.

SSC Data Access Plans All data will be available through web –Also setting up anonymous ftp site –SECCHI images will be password protected during embargo.

Doug Biesecker NOAA/Space Environment Center. Beacon Ground Station Network Almost together –CNES – signed letter of agreement received Toulouse – 9m.

SWG040322SECCHI_STATUS.1 SECCHI Status R.A. Howard Presentation to STEREO SWG 22 March 2004 Boulder, Colorado.

STEREO Science Center Status Report William Thompson NASA Goddard Space Flight Center STEREO SWG October 2009 Meredith, NH.

1 P. C. Liewer, E. M. DeJong, J. R. Hall, JPL/Caltech; K. E. J. Huttunen, Y. Li, J. Luhmann, B. Lynch, UCB/SSL; Angelos Vourlidas & R. A. Howard, NRL;

IMPACT Status and Data Updates SWG Meudon, April 21-22, 2008 Janet Luhmann, Peter Schroeder, and Chris Russell for the IMPACT team.

IMPACT Conjunction and Sidelobe Operations Janet Luhmann, Dave Curtis, Peter Schroeder, Dick Mewaldt and the IMPACT Team July 2, 2014.

Space Weather Aspects of the STEREO Mission D.A. Biesecker 1 and D.F. Webb 2 1 NOAA Space Environment Center; 2 ISR/Boston College Introduction The STEREO.

Analysis of 3 and 8 April 2010 Coronal Mass Ejections and their Influence on the Earth Magnetic Field Marilena Mierla and SECCHI teams at ROB, USO and.

1 NASA’s STEREO Mission J.B. Gurman STEREO Project Scientist W.T. Thompson STEREO Chief Observer Solar Physics Laboratory, Helophysics Division NASA Goddard.

SSC Preflight Status Tested during Sim #3: –Telemetry ingest –Beacon processing –Science planning –Archiving of MOC data products, including level-0 telemetry.

1 Determination of CME 3D Trajectories using Stereoscopy STEREO CMES of 16Nov2007 and 31AUG2007 P. C. Liewer, E. M. DeJong, J. R. Hall, JPL/Caltech; R.

Coronal and Interplanetary Structures associated with type III bursts M. Pick, F. Auchère, A. Kerdraon, A. Bouteille, G. Stenborg Stereo Science Workshop,

NASA Endeavour Program North Pocono Middle School

An Introduction to Observing Coronal Mass Ejections

L4+L5 Mission as an Ideal Project for International Collaboration

The Instruments Faraday Cup CfA/U of Mich & MIT

SWAVES-like radio instrument?

L4+L5 Mission as an Ideal Project for International Collaboration

STEREO Michael L. Kaiser STEREO Project Scientist

esa. int/solar-orbiter/51168-summary/;

The STEREO Space Weather Broadcast

Space Weather and HI Richard A. Harrison, RAL

Presentation transcript:

Michael L. Kaiser STEREO Project Scientist NASA/Goddard Space Flight Center STEREO May 2, 2008 STEREO at 1.25 years

STEREO-B (BEHIND) OBSERVATORY Deployed SWAVES Electric Field Antenna (3 places) Deployed IMPACT Boom IMPACT Solar Wind Electron Analyzer (SWEA) IMPACT Suprathermal Electron Detector (STE) IMPACT Magnetometer (MAG) SECCHI Heliospheric Imager (HI) SECCHI Sun-Centered Imaging Package (SCIP) Assy (COR-1, COR-2, EUVI, GT) PLASTIC Instrument IMPACT SEP 1.1m X 2.0 m X 1.2 m 610 kg ≥ 600 W

STEREO Orbits Sun Earth +22  /year -22  /year Heliocentric Inertial Coordinates (Ecliptic Plane Projection) Geocentric Solar Ecliptic Coordinates Fixed Earth-Sun Line (Ecliptic Plane Projection) Ahead Behind Earth 1 yr. 2 yr. 3 yr. 4 yr. 1yr. 2yr. 3 yr. 4 yr.

STEREO Space Weather Data Products Highest resolution data – available hrs SECCHI: 2048 X 2048 images IMPACT: fluxes (10s sec), moments (few sec) and B (<1 sec) PLASTIC: fluxes and moments 1 min resolution SWAVES: intensities from all frequencies (~367) every 15 sec Other data products – available TBD Key parameters Catalogs and event tables Movies Research Beacon (space weather) data – available ‘immediately’ SECCHI: ~7 256 X 256 images every hour IMPACT: 1 min aves of B, 1 min aves solar wind moments and selected SEP fluxes PLASTIC: 1 minute resolution selected moments and fluxes SWAVES: 1 minute summaries of alternate frequencies ( MHz) ‘Operational’

SECCHI

IMPACT/PLASTIC

IMPACT SEP

Beacon Status Receive beacon telemetry from England, Japan, and France on a regular basis – overall coverage 50-90% –Toulouse station recently added –Not certain about continued funding for station in England –Wallops tracking is top priority—paperwork is main delay –NOAA examining link margins for extended mission All SECCHI telescopes are now included in the beacon pages. SWAVES radio plots are now generated in realtime.

March 25, 2008 – Our first big success

Eruption in the Low Corona A-B separation = 28 deg Cadence = 10 min Mild wavelet enhancement

Eruption in the Low Corona (Implications) Visibility of prominence top depends on projection – Gap of several hours between A &B. – Height-time analyses of eruptive prominences from single viewpoint are unreliable for CME studies! The existence of kinked structures is projection- depended –“kinked” structure seen in B, not A –Footpoints of eruptive prominence seen in B, not A –Shape, configuration of erupting structures is very uncertain from single viewpoint. Kinked structures

STEREO Actually ‘sees’ CIRs

90 ° 180 ° STEREO separation STEREO into cycle 24

or