STCE Meeting – 06/06/2011 Summary of the « Radio Science Workshop » Hervé Lamy (BISA) Petra Van Lommel (STCE)

Slides:



Advertisements
Similar presentations
MMMM T S R S Summary of TSRS Objectives The Trieste Solar Radio System (TSRS; INAF-Trieste Astron. Obs.), is a set of two multichannel solar radio polarimeters.
Advertisements

2006/06/29 S. Poedts Centre for Plasma Astrophsyics, Leuven (B)
1 SWWT Initiatives - Long term monitoring of Sun-Earth Interactions F. Lefeuvre + contributions from 16 groups or individual SWWT members.
STCE Workshop : radio and optical observations of meteors 30/01/2014 BRAMS : status and perspectives Hervé Lamy Belgian Institute for Space Aeronomy (BISA)
Belgian Institute for Space Aeronomy
BELGRADE DATABASES - ionospheric observations and detections astro- and geophysical phenomena by radio signals Aleksandra Nina Institute of Physics, Belgrade.
G.N. Rajasekhara Girish Kumar Beeharry Mauritius Radio Telescope The CALLISTO spectrograph in Mauritius.
Planets and Solar System Science at Low Frequencies Philippe Zarka LESIA, CNRS-Observatoire de Paris France Towards a European.
The EISCAT Radar Facilities Ian McCrea STFC RAL. What is EISCAT? International Scientific Association Established agreeement since 1975 First observations.
Solar radio observations in Belgium C. Marqué, F. Clette, J.-L. Dufond, A. Ergen, J. Magdalenic, B. Dabrowski Royal Observatory of Belgium 2 nd LOFAR Solar.
Groundbased meteor/dust observations Asta Pellinen-Wannberg Swedish Institute of Space Physics & Umeå University Department of Space Science.
Radio Mobile Software for Wireless Systems Javier Triviño Universidad de Los Andes Merida – Venezuela.
Mesoscale ionospheric tomography over Finland Juha-Pekka Luntama Finnish Meteorological Institute Cathryn Mitchell, Paul Spencer University of Bath 4th.
CISM Advisory Council Meeting 4 March Ionosphere-Thermosphere Modeling Tim Killeen, Stan Solomon, and the CISM Ionosphere-Thermosphere Team.
Why are they so important?
Radio Astronomy in School Suceava “Ştefan cel Mare” State University Planetarium / Observatory Cezar Leşanu
How Global Positioning Devices (GPS) work
1 UNCLASSIFIED – FOUO – Not for Public Release Operational Space Environment Network Display (OpSEND) & the Scintillation Network Decision Aid Dr. Keith.
Geospace Variability through the Solar Cycle John Foster MIT Haystack Observatory.
Workshop on Earthquakes: Ground- based and Space Observations 1 1 Space Research Institute, Austrian Academy of Science, Graz, Austria 2 Institute of Physics,
Heliosphere impact on geospace IPY core project (#63) conducted by ICESTAR, IHY (International Heliophysical Year) and 27 other consortia with scientists.
“Quickmaps and history of the effects of ionospheric scintillations on GPS/GLONASS signals” SDA for ESA Space Weather Applications Pilot Project J.J. Valette,
I.U.C.A.F Summer School May / June CRAF Committee for Radio Astronomy Frequencies.
RADAR Detection of Extensive Air Showers Nils Scharf III. Physikalisches Institut A Bad Honnef Nils Scharf III. Physikalisches Institut A Bad.
European Planetary Science Congress 2012 – Madrid – September 2012 BRAMS: a Belgian Am-Pro collaboration to detect and characterize meteors with.
Requirements for meteor and dust studies with the new EISCAT_3D facility Asta Pellinen-Wannberg Umeå University and Swedish Institute of Space Physics.
Printed by With the help of scientists and staff at NRAO and WVU, high school students in West Virginia and neighboring states are.
IMC 2012 – La Palma – 21/09/2012 BRAMS, the Belgian Radio Meteor Stations : latest developments Hervé Lamy.
Splinter 1: Space science & weather Chair: J. De Keyser Summary: F. Clette 03/06/20101STCE: Space Science & Weather.
Meteorological Spectrum Issues- Outcome of the 2003 World Radiocommunication Conference Presented By: David Franc National Weather Service December 2,
Stanford VLF Remote Sensing Science, Engineering, Educational outreach Morris Cohen Along with Phil Scherrer, Deborah Scherrer, Umran Inan, Ray Mitchell,
China National Report , Uppsala, Sweden China National Space Administration.
WP3: Science Planning and User Engagement Anita Aikio Coordinators: UOulu (FI) and STFC (UK) Objectives: Ensure consistency between the Science Case and.
TUTORIAL BRAMS ZOO. What is a meteoroid? A meteoroid is a solid object moving in interplanetary space, of a size considerably smaller than an asteroid.
An Efficient Propagation Simulator for High Frequency Signals And Results from HF radar experiment Kin Shing Bobby Yau Supervisors: Dr. Chris Coleman &
Joint International GRACE Science Team Meeting and DFG SPP 1257 Symposium, Oct. 2007, GFZ Potsdam Folie 1 Retrieval of electron density profiles.
NATIONAL INSTITUTE FOR SPACE RESEARCH – INPE/MCT SOUTHERN REGIONAL SPACE RESEARCH CENTER – CRS/CIE/INPE - MCT SOUTHERN SPACE OBSERVATORY– SSO/CRS/CIE/INPE.
Distributed Radar Networks Ray Greenwald JHU/APL.
GALOCAD GAlileo LOcal Component for nowcasting and forecasting Atmospheric Disturbances R. Warnant*, G. Wautelet*, S. Lejeune*, H. Brenot*, J. Spits*,
New results in polarimetry of planetary thermospheric emissions: Earth and Jovian cases. M. Barthelemy (1), J. Lilensten (1), C. Simon (2), H. Lamy(2),
Radio polarisation measurement of meteor trail echoes during the Perseids 2012 S. Ranvier (1), M. Anciaux (1), H. Lamy (1), J. De Keyser (1) ‏, S. Calders.
Comparison of the electron density profiles measured with the Incoherent Scatter Radar, Digisonde DPS-4 and Chirp-Ionosonde Ratovsky K.G., Shpynev* B.G.,
Analyzing the Effect of Interference in GNSS Scintillation Monitoring Rodrigo Romero Politecnico di Torino 11th European Space.
SPLINTER SESSION « RADIO SCIENCE » SUMMARY Hervé Lamy (BIRA) Christophe Marqué (ROB)
HAARP-induced Ionospheric Ducts Gennady Milikh, University of Maryland in collaboration with: Dennis Papadopoulos, Chia-Lee Chang, BAE systems Evgeny Mishin,
Stanford VLF Remote Sensing Science, Engineering, Educational outreach Morris Cohen Along with Phil Scherrer, Deborah Scherrer, Umran Inan, Ray Mitchell,
RADIO QUITE SITE QUALIFICATION FOR THE BRAZILIAN SOUTHERN SPACE OBSERVATORY BY MONITORING THE LOW FREQUENCY 10–240 MHZ ELECTROMAGNETIC SPECTRUM GUILHERME.
IMC 2012 – La Palma Sept Results of the Draconids 2011 observation with the BRAMS network Stijn Calders 1 & Cis Verbeeck 2 1 Belgian Institute for.
GALOCAD GAlileo LOcal Component for nowcasting and forecasting Atmospheric Disturbances R. Warnant, G. Wautelet, S. Lejeune, H. Brenot, J. Spits, S. Stankov.
STCE Meeting – 08/06/2009 PARTICIPATING IN SPACE/GROUND-BASED EXPERIMENTS (Hervé Lamy - WP BISA C.2) MEMS Magnetometer Radio detection of meteors Polarization.
In 1955 researchers discovered the planet Jupiter produced radio waves. For over 58 years these mysterious storms have been studied by radio astronomers.
NORWEGIAN-UKRAINIAN COOPERATION AIMED TO SUSTAINABLE DEVELOPMENT OF THE EDUCATION PROCESS IN GEOSPACE RESEARCHES Cesar La Hoz, UiT the Arctic University.
DETECTING WHISTLERS WITH A VLF ANTENNA LOCATED IN HUMAIN (BELGIUM) S. Ranvier (1), F. Darrouzet (1), H. Lamy (1), J. De Keyser (1) ‏, J. Lichtenberger.
The KUT meteor radar: An educational low cost meteor observation system by radio forward scattering IMC th International Meteor Conference June.
Lee-Anne McKinnell and Mpho Tshisaphungo
Status of the BRAMS project & plans for the future
Protection of the Humain station
Recent progress of WDC for Geophysics, Beijing
ICESTAR: Solar-terrestrial and aeronomy research during the International Polar Year Kirsti Kauristie1, Allan Weatherwax2, Richard Harrison3, Richard.
Space Geodesy Branch Highlights, August 2002 CONT02 VLBI Campaign
H. Lamy (1), S. Calders (1), C. Tétard (1), C. Verbeeck (2), A
AN EDUCATION AND OUTREACH PROJECT Jim Thieman and Chuck Higgins
Participation to the CAMS network & preliminary BRAMS/CAMS comparison
Overview of major shower observations by the BRAMS network
Hervé Lamy & Cédric Tétard Royal Belgian Institute for Space Aeronomy
Status of the BRAMS activities
Status of the BRAMS network and recent progress
Study of joint CAMS/BRAMS observations & comparison with simulations
SWWT Initiatives - Long term monitoring of Sun-Earth Interactions
Institut de mécanique céleste et de calcul des éphémérides
Presentation transcript:

STCE Meeting – 06/06/2011 Summary of the « Radio Science Workshop » Hervé Lamy (BISA) Petra Van Lommel (STCE)

STCE Meeting – 06/06/2011 OUTLINE Goals of the workshop Radio projects on the plateau Existing and potential collaborations Communication platform on the EU SW portal

STCE Meeting – 06/06/2011 GOALS OF THE WORKSHOP What are the radio science projects carried out on the plateau? What are the technical needs and the methods used? Can we share software / hardware? Can we benefit from experience of other groups?  increase efficiency in the framework of the STCE This workshop was the continuation of a « radio day » that we already organize on October

STCE Meeting – 06/06/2011 BRAMS : Belgian RAdio Meteor Stations BISA project Goal: detect and characterize meteors with forward scattering radio techniques Status: network in development, should be partly operational in August (Perseids), fully operational in October (Draconids) Contact person: Hervé Lamy, Sylvain Ranvier Website: brams.aeronomy.be

STCE Meeting – 06/06/2011 Whistler observations BISA project Goal: detect Whistler waves with a VLF antenna in Humain Status : system operational, preliminary results obtained, analysis will start soon. Part of an international project AWDANet (Automatic Whistler Detector and Analyzer system’s network) Contact persons : Fabien Darrouzet, Sylvain Ranvier

STCE Meeting – 06/06/2011 Lightning detection RMI project Goal: detect, locate and characterize lightnings above Belgium Status: system operational with 5 SAFIR antennas located in Belgium, accuracy of location ~ a few km Possibility of extending the network with stations located in France and Netherlands Contact persons: Dieter Poelman, Geert De Sadelaer Website : Lightning+detection.html

STCE Meeting – 06/06/2011 Monitoring station in Humain ROB/BIRA/RMI Goal: to monitor the elm perturbations induced by the future extension of the quarry in Humain. Status: hardware setup being procured, monitoring should start in July, duration of one year Contact Persons: Christophe Marqué, Sylvain Ranvier

STCE Meeting – 06/06/2011 Committee on Radio Astronomy Frequencies (CRAF) Christophe Marqué is a member Goal: coordinates activities to keep the frequency bands used by radio astronomy and space sciences free from interference. Contact person: Christophe Marqué Website :

STCE Meeting – 06/06/2011 Radio Science Geodesy and Rotation ROB Goal: planetary geodesy (retrieve internal physical parameters) from the position of a s/c orbiting a planet (mainly Mars at the moment) Contact persons : Véronique Dehant, Pascal Rosenblatt Website :

STCE Meeting – 06/06/2011 Solar radio observations in Humain ROB Goal: monitoring of solar activity and research : solar flares, CMEs, irradiance Status : Callisto spectrograph operating since 2008 ( MHz), Phoenix 2 spectrometer (300 MHz-3 GHz) fully operational in spring 2011, measurements of F10.7cm flux Contact persons : Jasmina Magdalenic, Christophe Marqué. Website : sidc.be/humain

STCE Meeting – 06/06/2011 Radar observations of auroral arcs BISA Goal: to use observations of auroral arcs with EISCAT facilities in Tromsø (Norway) to model magnetosphere- ionosphere coupling. Status : Observations carried out during 2008 and 2009 campaigns. Data have been reduced and are currently interpreted Contact persons : Cyril Simon, Hervé Lamy

STCE Meeting – 06/06/2011 Existing collaborations Radio astronomical site of Humain : currently used by the 3 institutes for various experiments. There is a strong need for a fast internet link in Humain. STCE funding?

STCE Meeting – 06/06/2011 Existing collaborations (2) Dourbes: the emitting beacon of BRAMS is located there Monitoring of the electromagnetic perturbations induced by the quarry in Humain  collaboration between Sylvain Ranvier (BISA) and Christophe Marqué (ROB) to select the hardware.

STCE Meeting – 06/06/2011 Possible future collaborations BRAMS/SAFIR teams: share experience about VHF interferometry and use of the PPS of a GPS to get accurate time measurements. In the 2 nd part of 2011, BISA will start developing a meteor radar system  located in Dourbes? To be discussed. Comparisons between strong irregularities in the TEC observed with GPS measurements, Galileo data or ionosonde data, and strong meteor VHF echoes.

STCE Meeting – 06/06/2011 Possible future collaborations (2) VLF measurements need use of ionospheric models for TEC Future measurements of the F10.7cm flux in Humain will be very interesting for many activities in BISA. Others?

STCE Meeting – 06/06/2011 Communication platform Set up by Stijn Calders (BISA) on spaceweather.eu Possibility to upload and share documents and/or softwares An idea was to make a list of hardware material that could be useful to all scientists on the plateau. This would avoid duplicity. Not very successful so far… but we’ll keep trying.