Presentation is loading. Please wait.

Presentation is loading. Please wait.

Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO SWG, Fall Hills, Meredith, NH STEREO/WAVES.

Published byTrevor Barnett Modified over 8 years ago

Similar presentations

Presentation on theme: "Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO SWG, Fall Hills, Meredith, NH STEREO/WAVES."— Presentation transcript:

1 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO SWG, Fall Hills, Meredith, NH STEREO/WAVES team status STEREO/WAVES studies in progress Instrument status report 1 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

2 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO/WAVES team status 68 members: 30 S/WAVES Co-Investigators 2 S/WAVES Co-I Emeritus 3 S/WAVES science team members 33 S/WAVES Associate and Participating scientists 2 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

3 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO/WAVES team status etc 5 pp. Member’s field of interest: 3 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

4 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center 4 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

5 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO/WAVES studies in progress We “adjusted“ to extended solar minimum! Still, work on few radio events! more time for calibrations, refining direction finding techniques more time for theoretical work focus on in situ studies (wave form analyzer: wave coupling, dust) radio emission from magnetospheres (Earth, Jupiter) 5 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

6 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO/WAVES studies in progress On-going work on radio events and observations: comprehensive analysis of a type III radio storm (Eastwood) beam pattern characterization (Bonnin) assocation of IP type III radio emission with CMEs, EUV waves and large scale coronal structures (Kerdraon) modeling of galactic radio background at LF using data from Ulysses, Cassini and STEREO (Lecacheux, MacDowall, Hoang) magnetic field topology of the inner heliosphere from combined observations of S/WAVES, IMPACT and RHESSI (Martinez-Oliveros) Multiwavelength analysis of the 19 May 2007 SEP event (Kerdraon) Radio signatures of EUV waves (Pick) 6 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

7 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO/WAVES studies in progress Calibrations, direction finding, search algorithms, theory: direction finding algorithms, source sizes, ray tracing simulations (Cecconi, Reiner, Lecacheux, Rucker, Santolik, Kasper, …) development of Wind-Ulysses radio tracking of CME driven shocks in preparation to STEREO (Hoang) Monte-Carlo modeling of radio wave propagation in the corona and solar wind (Golla, MacDowall) automated algorithm for identification of transients seen by both spacecraft (Kasper) characterization of the propagation of CME shocks (Cremades, Reiner) Non-linear plasma turbulence: Type III solar radio burst simulations (Robinson) 7 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

8 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO/WAVES studies in progress In situ studies with TDS (QTN): Dust, nano-particles (Kaiser, Goetz, StCyr, Meyer, Issautier, …) combined plasma and wave observations of electrons in the electron foreshock region upstream of thebow shock, WAVES and IMPACT (Pulupa) Wave coupling in Type III emission, simulations (Henri) Measurements of Rapid Density Fluctuations in the Solar Wind (Malaspina) small scale electrostatic turbulence; comparison with Vlasov- Maxwell simulations (Carbone) Foreshock Langmuir waves in STEREO data (Cairns) Langmuir waves in the solar wind, comparison to theory (Sundkvist) macroscopic properties of the solar wind (Issautier) 8 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

9 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center Mike Kaiser’s legacy! 9 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

10 Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center Instrument status Both A & B receivers continue to function nominally –No trend changes in HK parameters –A few anomalies are tracked with vigor One unexpected/unexplained reset EEPROM error Missing DMA Operations continue to go well –Commands go up – with routine operations and special sequences –Telemetry comes down –Associated data products are produced and made available –Special situations are handled e.g. S/C resets –Flight operations team at APL has been very accommodating We have slowly evolved our flight software –To improve science –To investigate anomalies 10 STEREO SWG 20 – 2009 October 27-29, Meredith, New Hampshire

Download ppt "Observatoire de Paris University of Minnesota University of California - Berkeley Goddard Space Flight Center STEREO SWG, Fall Hills, Meredith, NH STEREO/WAVES."

Similar presentations

The Johns Hopkins University Applied Physics Laboratory SHINE 2005, July 11-15, 2005 Transient Shocks and Associated Energetic Particle Events Observed.

The Johns Hopkins University Applied Physics Laboratory SHINE 2005, July 11-15, 2005 Transient Shocks and Associated Energetic Particle Events Observed.
SEP Data Analysis and Data Products for EMMREM Mihir I. Desai & Arik Posner Southwest Research Institute San Antonio, Texas Mihir I. Desai & Arik Posner.

SEP Data Analysis and Data Products for EMMREM Mihir I. Desai & Arik Posner Southwest Research Institute San Antonio, Texas Mihir I. Desai & Arik Posner.
R. P. Lin Physics Dept & Space Sciences Laboratory University of California, Berkeley The Solar System: A Laboratory for the Study of the Physics of Particle.

R. P. Lin Physics Dept & Space Sciences Laboratory University of California, Berkeley The Solar System: A Laboratory for the Study of the Physics of Particle.
Session A Wrap Up. He Abundance J. Kasper Helium abundance variation over the solar cycle, latitude and with solar wind speed Slow solar wind appears.

Session A Wrap Up. He Abundance J. Kasper Helium abundance variation over the solar cycle, latitude and with solar wind speed Slow solar wind appears.
Feb. 3-5, 2009 Pasadena, CA. Late agenda update Page 2.

Feb. 3-5, 2009 Pasadena, CA. Late agenda update Page 2.
M. J. Reiner, 1 st STEREO Workshop, March, 2002, Paris.

M. J. Reiner, 1 st STEREO Workshop, March, 2002, Paris.
Electron Acceleration at the Solar Flare Reconnection Outflow Shocks Gottfried Mann, Henry Aurass, and Alexander Warmuth Astrophysikalisches Institut Potsdam,

Electron Acceleration at the Solar Flare Reconnection Outflow Shocks Gottfried Mann, Henry Aurass, and Alexander Warmuth Astrophysikalisches Institut Potsdam,
STEREO AND SPACE WEATHER Variable conditions in space that can have adverse effects on human life and society Space Weather: Variable conditions in space.

STEREO AND SPACE WEATHER Variable conditions in space that can have adverse effects on human life and society Space Weather: Variable conditions in space.
Coronal radiation belts? H. S. Hudson Space Sciences Lab, UC Berkeley.

Coronal radiation belts? H. S. Hudson Space Sciences Lab, UC Berkeley.
Solar Energetic Particle Production (SEPP) Mission Primary Contacts: Robert P. Lin (UC Berkeley), John L. Kohl (Harvard-Smithsonian CfA) Primary Science.

Solar Energetic Particle Production (SEPP) Mission Primary Contacts: Robert P. Lin (UC Berkeley), John L. Kohl (Harvard-Smithsonian CfA) Primary Science.
Coronal IP Shocks Nat Gopalswamy NASA/GSFC Elmau CME Workshop, 2003 February 7 Plenary talk Sun Earth.

Coronal IP Shocks Nat Gopalswamy NASA/GSFC Elmau CME Workshop, 2003 February 7 Plenary talk Sun Earth.
Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.

Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.
Solar Imaging Radio Array (SIRA) R. MacDowall, N. Gopalswamy, M. L. Kaiser, M. J. Reiner Code 695 NASA Goddard Space Flight Center Greenbelt, MD 20771.

Solar Imaging Radio Array (SIRA) R. MacDowall, N. Gopalswamy, M. L. Kaiser, M. J. Reiner Code 695 NASA Goddard Space Flight Center Greenbelt, MD
Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.

Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences A Solar and Heliospheric Research grant funded by the DoD MURI program.
SDO/AIA science plan: prioritization and implementation: Five Objectives in 10 steps [session no.] HMI/AIA science teams meeting; Monterey; Feb. 20061.

SDO/AIA science plan: prioritization and implementation: Five Objectives in 10 steps [session no.] HMI/AIA science teams meeting; Monterey; Feb
F1B: Determine the Dominant Processes of Particle Acceleration Phase 2005-2015, Open the Frontier UV Spectroscopic determin- ation of pre/post-shock density,

F1B: Determine the Dominant Processes of Particle Acceleration Phase , Open the Frontier UV Spectroscopic determin- ation of pre/post-shock density,
The “cone model” was originally developed by Zhao et al. ~10 (?) years ago in order to interpret the times of arrival of ICME ejecta following SOHO LASCO.

The “cone model” was originally developed by Zhao et al. ~10 (?) years ago in order to interpret the times of arrival of ICME ejecta following SOHO LASCO.
CME Workshop Elmau, Feb 6 - 12, 20031 WORKING GROUP C: ENERGETIC PARTICLE OBSERVATIONS Co-Chairs: Klecker, Kunow SUMMARY FROM SESSION 1B Discussion of.

CME Workshop Elmau, Feb , WORKING GROUP C: ENERGETIC PARTICLE OBSERVATIONS Co-Chairs: Klecker, Kunow SUMMARY FROM SESSION 1B Discussion of.
Stuart D. BaleFIELDS iCDR – Science Requirements Solar Probe Plus FIELDS Instrument CDR Science and Instrument Overview Science Requirements Stuart D.

Stuart D. BaleFIELDS iCDR – Science Requirements Solar Probe Plus FIELDS Instrument CDR Science and Instrument Overview Science Requirements Stuart D.
High-Cadence EUV Imaging, Radio, and In-Situ Observations of Coronal Shocks and Energetic Particles: Implications for Particle Acceleration K. A. Kozarev.

High-Cadence EUV Imaging, Radio, and In-Situ Observations of Coronal Shocks and Energetic Particles: Implications for Particle Acceleration K. A. Kozarev.

Similar presentations

Ads by Google