BORÓWIEC PL610. Hanna Rothkaehl, Mariusz Pożoga,Barbara Matyjasiak, Marcin Grzesiak, Roman Wronowski
|
|
- Brice Rodgers
- 5 years ago
- Views:
Transcription
1 BORÓWIEC PL610 Hanna Rothkaehl, Mariusz Pożoga,Barbara Matyjasiak, Marcin Grzesiak, Roman Wronowski
2 BORÓWIEC SRC PAS astrogeodynamic observatory φ = N λ = E h = m
3 Additional Diagnostics POLISH LOFAR STATIONS Scintilation reciver, Riometr Ionosondes, Warsaw, Olsztyn, Spitsbergen(Horsund) Radio reciver for DAB and oblique sounding
4 1. Research subjects out of CBK s interest: analysis of ionospheric and magnetometer scintillations. Results of both theoretical and observation analyses data will serve to this phenomenon s model construction and will be applied both in making ionospheric corrections at radio astronomy observation corrections and in Space Weather services. 2. Solar Wind parametres analysis, mainly an intraplanetary scintillation analysis. That to verify data provided by an American mission IBEX. 3. Sun s radio frequency analysis, in particular its solar radio burst. 4. Analysis of electromagnetic noise and pollution close to Earth. Apart from measurement data from LOFAR, ionospheric diagnosis located in a station and other ground equipment: ionosondes and digital radio receivers have been used here. 5. Jupiter and other Solar System s planets radio frequency analysis and radiation diagnosis of Jupiter s radiation strip. Those have just been coordinated within the world earthly enhancement programme of the mission NASA JUNO towards Jupiter. This activity has been conducted within EUROPLANET, the Paris Observatory being the closest partner in cooperation. That work may be helpful in ESA s scientific programme s preparations of JUICE mission. 6. Space mission design to take advantage from the rules of interferometry applied in LOFAR s infrastructure and to create a complementary LOFAR for the outer space. That works will be useful for two Projects: NCLE i DLSP missions of China Space Agency Chang E-4 towards the Moon s neighbourhood. That has been the subject of cooperation with ASTRON and the University of Nijmegen in Holland.
5 Technical activities Local observation depository computers and adequate software were installed. Replacement of local LCU system Identification MHz RFA for selected LBA antennas and some different action for mitigation this effect. Removing a computer switch failure
6 RFI Some part of LBA antennas located near observation building are affected by power supply located in the basement
7 Local observation activity - software to manage the station on a local basis to facilitate its independence - software to create dynamic spectrum in real time - measurements of EM waves scintillation on irregularities of plasma in Solar Wind - possibility to use the Transient Buffer Board (TBB) to parallel observations - possibility of creating dynamic spectrum based on previous data registry; special software development was applied to test the above.
8 Local observation activity - In cooperation with a University in Bielefield pulsar observation was initiated - observation of ionospheric scintillations based on strong radio sources; the options of various station configurations were checked
9 Local observation activity -the Sun observations were made to check the optimum capabilities to monitor Solar emissions - the observations of Jupiter at low frequencies were made to proceed in DAM observations (dacametric radio emissions) - sources of electromagnatic radiation within the short-wave range were monitored
10 VESPA implementation workshop , Graz, Austria VESPA - Virtual European Solar and Planetary Access LOFAR PL610 observations of decametric Jupiter radio emissions will be avaliable via VESPA platform with open acces. Measurements will be a part of followup monitoring for space mission JUNO. In future also observations of solar radio emissions will be available. SRC PAS will also provide space weather alerts. Web page:
11 LOFAR FUTURE SKA Synergy ground based radio astronomy and satellite diagnostics Cluster radio diagnostics near L2 MOON FAR SIDE
12 NSSC CAS- CBK PAN National Space Science Center CAS- Space Research Center PAS DSL-P 1st stage Chang E-4 satellite mission Pathfinder of DSL (Discovery the Sky at Longest Wavelength) Space Physics and Radio Astronomy Launch summer 2018
13 Netherlands-China Low-Frequency Explorer (NCLE) PI - Heino Falcke Co-PI Marc Klein Wolt Co-PI Hanna Rothkaehl
PoS(ISKAF2010)083. FRATs: a real-time search for Fast Radio Transients with LOFAR
FRATs: a real-time search for Fast Radio Transients with LOFAR Radboud University Nijmegen (Department of Astrophysics) E-mail: s.terveen@astro.ru.nl H. Falcke Radboud University Nijmegen (Department of
More informationVLBI observations of spacecraft
VLBI observations of spacecraft Joining space science and planetary data with almost classical radio astronomy Giuseppe Cimò Joint Institute for VLBI - ERIC (JIVE) Netherlands Institute for Radio Astronomy
More informationWhat we (don t) know about UHECRs
What we (don t) know about UHECRs We know: their energies (up to 10 20 ev). their overall energy spectrum We don t know: where they are produced how they are produced what they are made off exact shape
More informationLOFAR Key Science Projects and Science Network in Germany
LOFAR Key Science Projects and Science Network in Germany Rainer Beck MPIfR Bonn LOFAR A revolution in radio telescope design: Software telescope: no moving parts, no mirrors, simultaneous multi-beaming,
More informationSpace mission BRАUDE-M. Radio telescope on the farside of the Moon
Bilateral Workshop on Astrophysics V.N. Karazin Kharkiv National University INAF Space mission BRАUDE-M. Radio telescope on the farside of the Moon Dr. Vyacheslav Zakharenko, Director of the Institute
More informationSpace Ultra Long Wavelength Array
Space Ultra Long Wavelength Array Maohai Huang 1, Yihua Yan 1, Linjie Chen 1 *, Mo Zhang 1, Leonid Gurvits 2,6, Heino Falcke 3,4, Marc Klein Wolt 3,5 1 National Astronomical Observatories, Chinese Academy
More informationHOW TO GET LIGHT FROM THE DARK AGES
HOW TO GET LIGHT FROM THE DARK AGES Anthony Smith Lunar Seminar Presentation 2/2/2010 OUTLINE Basics of Radio Astronomy Why go to the moon? What should we find there? BASICS OF RADIO ASTRONOMY Blackbody
More informationESASky, ESA s new open-science portal for ESA space astronomy missions
ESASky, ESA s new open-science portal for ESA space astronomy missions Bruno Merín ESAC Science Data Centre European Space Agency bruno.merin@esa.int Visit to NAOC, Beijing, 19/05/2017 ESA UNCLASSIFIED
More informationSwedish Institute of Space Physics Research Strategies
Dnr 1.1-147/14 (replaces Dnr 1-309/04) Swedish Institute of Space Physics Research Strategies The Swedish Institute of Space Physics (IRF) is a national research institute under the auspices of the Swedish
More informationDetecting High Energy Cosmic Rays with LOFAR
Detecting High Energy Cosmic Rays with LOFAR Andreas Horneffer for the LOFAR-CR Team LOFAR CR-KSP: Main Motivation Exploring the sub-second transient radio sky: Extensive Air showers as guaranteed signal
More informationUNIT E: SPACE EXPLORATION
UNIT E: SPACE EXPLORATION S C I E N C E 9 1 Science 9 Unit E Section 3.0 OPTICAL TELESCOPES, RADIO TELESCOPES, AND OTHER TECHNOLOGIES ADVANCE OUR UNDERSTANDING OF SPACE SECTI ON 3.0 Science 9 Unit E Section
More informationExploring the Universe: Synergies in the ESA Science Programme
Exploring the Universe: Synergies in the ESA Science Programme Günther Hasinger, ESA Director of Science (D/SCI) 14 th Appleton Space Conference, RAL, 6.12.2018 Towards ESA UNCLASSIFIED - For Official
More informationThoughts on LWA/FASR Synergy
Thoughts on LWA/FASR Synergy Namir Kassim Naval Research Laboratory 5/27/2003 LWA-FASR 1 Ionospheric Waves 74 MHz phase 74 MHz model Ionosphere unwound (Kassim et al. 1993) Ionospheric
More informationRadio Emission from the Sun Observed by LOFAR and SKA
Radio Emission from the Sun Observed by LOFAR and SKA Gottfried Mann Leibniz-Institut für Astrophysik Potsdam (AIP) An der Sternwarte 16, D-14482 Potsdam, Germany e-mail: GMann@aip.de September 2011 LOFAR
More informationASTERICS Astronomy ESFRI & Research Infrastructure Cluster
ASTERICS Astronomy ESFRI & Research Infrastructure Cluster Giuseppe Cimò Joint Institute for VLBI - ERIC (JIVE) Netherlands Institute for Radio Astronomy (ASTRON) 1 what is ASTERICS? A major collaboration
More informationRadio Astronomy and Space Science VLBI observations of orbiters and landers Giuseppe Cimò
Radio Astronomy and Space Science VLBI observations of orbiters and landers Giuseppe Cimò for the PRIDE collaboration Planetary Radio Interferometry and Doppler Experiment DeltaDOR and VLBI DeltaDOR is
More information=> most distant, high redshift Universe!? Consortium of international partners
LOFAR LOw Frequency Array => most distant, high redshift Universe!? Consortium of international partners Dutch ASTRON USA Haystack Observatory (MIT) USA Naval Research Lab `best site = WA Novel `technology
More informationMax-Planck-Institut für Radioastronomie, Bonn Istituto di Radioastronomia - INAF, Bologna
RadioNet3 & SKA Franco Mantovani Project Scientist RadioNet3 Max-Planck-Institut für Radioastronomie, Bonn Istituto di Radioastronomia - INAF, Bologna RadioNet3 Advanced Radio Astronomy in Europe www.radionet-eu.org
More informationVery Low Frequency Observation On The Moon. H. Noda, N. Kawano, et al. NAOJ, Japan
Very Low Frequency Observation On The Moon H. Noda, N. Kawano, et al. NAOJ, Japan LLFAST Japan Lunar Low Frequency Astronomy Study Team A study team of voluntary base in Japan A subgroup of the study team
More informationSolar Observations with LOFAR
Solar Observations with LOFAR Gottfried Mann, C. Vocks and F. Breitling Astrophysikalisches Institut Potsdam An der Sternwarte 16, D-14482 Potsdam, e-mail: GMann@aip.de LOFAR: LOw Frequency ARray 30 240
More informationRecent Activities of NICT Space Weather Research and Operation
Recent Activities of NICT Space Weather Research and Operation Mamoru Ishii National Institute of Information and Communications Technology 2 2 Field of Space Weather GEO Sat. (More than 400) Satellite
More informationLudwig Combrinck HartRAO 3rd Space Geodesy Workshop 16 March 2009 Matjiesfontein
Space Geodesy and Space Science Ludwig Combrinck HartRAO 3rd Space Geodesy Workshop 16 March 2009 Matjiesfontein DST s Concept of Space Science SA Space Agency, commercial applications, CSIR Satellite
More informationAstronomical Experiments for the Chang E-2 Project
Astronomical Experiments for the Chang E-2 Project Maohai Huang 1, Xiaojun Jiang 1, and Yihua Yan 1 1 National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road,Chaoyang District,
More informationSun Earth Connection Missions
Sun Earth Connection Missions ACE Advanced Composition Explorer The Earth is constantly bombarded with a stream of accelerated particles arriving not only from the Sun, but also from interstellar and galactic
More informationESA Science Programme and the Ice Giants study
Outer Planets Assessment Group meeting 11-12 September 2018 ESA Science Programme and the Ice Giants study Luigi Colangeli Head Science coordination Office Directorate of Science ESA UNCLASSIFIED - For
More informationAstronomy. Catherine Turon. for the Astronomy Working Group
Astronomy Catherine Turon for the Astronomy Working Group Answers to the call for ideas Illustration of the strong expectation of the community from the ESA Science Programme: In astronomy 1983: Horizon
More informationFrom LOFAR to SKA, challenges in distributed computing. Soobash Daiboo Paris Observatory -LESIA
From LOFAR to SKA, challenges in distributed computing Soobash Daiboo Paris Observatory -LESIA Overview LOFAR telescope Data processing with LOFAR NenuFar SKA Summary LOFAR science drivers Key science
More informationSETI with SKA1 and SKA2
SETI with SKA1 and SKA2 Alan Penny1, Heino Falcke2, Mike Garrett3 1 University of St Andrews and South African Astronomical Observatory PI: LOFAR Early Access Program LEA070 'A SETI Pilot Program' 2 Raboud
More informationLow Cost Breakthroughs in Planetary Atmospheres and Interior Structures With Precision-Radio-Equipped Small Spacecraft
Low Cost Breakthroughs in Planetary Atmospheres and Interior Structures With Precision-Radio-Equipped Small Spacecraft Sami Asmar, David Atkinson, David Bell, James Border, Ivan Grudinin, Joseph Lazio,
More informationSpace Weather Activities in KASI. Yeon-Han Kim Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI)
Space Weather Activities in KASI Yeon-Han Kim Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI) Outline I Introduction II Instrument Construction III Space Weather Researches
More informationGROUND-BASED STUDY OF SATURN LIGHTNING
GROUND-BASED STUDY OF SATURN LIGHTNING J.-M. Grießmeier *,P.Zarka, A. Konovalenko,G.Fischer, V. Zakharenko,B.W.Stappers,J.N.Girard,B.Ryabov, D. Vavriv,V.Ryabov,andH.O.Rucker Abstract Radio signatures of
More informationDetection of Cosmic Rays at Ultra-High Energies with Phase I of the Square Kilometre Array (SKADS) Olaf Scholten and Heino Falcke
Detection of Cosmic Rays at Ultra-High Energies with Phase I of the Square Kilometre Array (SKADS) Olaf Scholten and Heino Falcke April 13, 2007 1 abstract Currently under development by an international
More informationASTRONOMY FINAL EXAM REVIEW
ASTRONOMY 2013-2014 NAME: DATE: ASTRONOMY FINAL EXAM REVIEW PERIOD: Energy in the Universe: Light and Matter (Chapter 5) 1. What are the wavelengths of the electromagnetic spectrum? Order them from longest
More informationEuroPlanet Integrated and Distributed Information Service (IDIS)
EuroPlanet Integrated and Distributed Information Service (IDIS) Maria Teresa Capria, Gérard Chanteur, Walter Schmidt and the teams of the IDIS Nodes December 3, 2009 ESAC, Madrid, Spain PV2009 IDIS OVERVIEW
More informationSMILE Solar wind Magnetosphere Ionosphere Link Explorer Novel and global X-ray imaging of the Sun Earth connection
SMILE Solar wind Magnetosphere Ionosphere Link Explorer Novel and global X-ray imaging of the Sun Earth connection Graziella Branduardi-Raymont Chi Wang UCL MSSL CAS NSSC and the SMILE collaboration (ESA,
More informationChapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization
Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic spectrum Compare refracting telescopes
More informationFuture Radio Interferometers
Future Radio Interferometers Jim Ulvestad National Radio Astronomy Observatory Radio Interferometer Status in 2012 ALMA Covers much of 80 GHz-1 THz band, with collecting area of about 50% of VLA, for a
More informationDirected Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past?
Skills Worksheet Directed Reading Section: Viewing the Universe 1. How did observations of the sky help farmers in the past? 2. How did observations of the sky help sailors in the past? 3. What is the
More informationScience Operations with the Square Kilometre Array
Science Operations with the Square Kilometre Array Dr Antonio Chrysostomou Head of Science Operations Planning a.chrysostomou@skatelescope.org Outline Introduction to the SKA Science Programme Operational
More informationDr. Cran Lucas. Shreveport-Bossier Astronomical Society & Shreveport Amateur Radio Association KG5NMF
Amateur Radio Astronomy Dr. Cran Lucas Shreveport-Bossier Astronomical Society & Shreveport Amateur Radio Association KG5NMF Outline Radio Astronomy Basics Radio Astronomy History Radio Astronomy Telescopes
More informationAlexey Kuznetsov. Armagh Observatory
Alexey Kuznetsov Armagh Observatory Outline of the talk Solar radio emission History Instruments and methods Results of observations Radio emission of planets Overview / history / instruments Radio emission
More informationGerman LOFAR a new era in radio astronomy
German LOFAR a new era in radio astronomy Marcus Brüggen International University Bremen Rainer Beck (MPIfR) Heino Falcke (ASTRON) Anton Zensus (MPIfR) Köln, 28. Sep 2005 Outline Why LOFAR? What is happening
More informationLOFAR Polarization Commissioning by the MKSP
LOFAR Polarization Commissioning by the MKSP James M Anderson anderson@mpifr-bonn.mpg.de On behalf of the LOFAR collaboration Surveys KSP Meeting, Leiden, 2010 March 11 James M Anderson 1/15 Timeline 2010
More informationRob Fender, Ben Stappers and Ralph Wijers on behalf of LOFAR and the Transients Key Science Project
Quiquid variat notandum Rob Fender, Ben Stappers and Ralph Wijers on behalf of LOFAR and the Transients Key Science Project RAMJW 1 LOFAR: surveyor and transient monitor (SCUBA-2, ALMA fields of view smaller
More informationRadio Astronomy Summer School Introduction Early History of Radio Astronomy. Tatsuhiko Hasegawa (ASIAA)
Radio Astronomy Summer School 2008 Introduction Early History of Radio Astronomy Tatsuhiko Hasegawa (ASIAA) 1. Radio astronomy was interferometry from the beginning. 2. Closely related to developments
More informationChina s Chang E Program
China s Chang E Program --- Missions Objectives, Plans, Status, and Opportunity for Astronomy Maohai Huang Science and Application Research Center for Lunar and Deepspace Explorations National Astronomical
More informationJUICE: the first European mission to Jupiter and its Icy Moons
JUICE: the first European mission to Jupiter and its Icy Moons Giuseppe Sarri Knowledge Transfer Seminar @ CERN 26 April 2018 ESA UNCLASSIFIED - For Official Use European Space Agency (ESA) The European
More informationESA s Juice: Mission Summary and Fact Sheet
ESA s Juice: Mission Summary and Fact Sheet JUICE - JUpiter ICy moons Explorer - is the first large-class mission in ESA's Cosmic Vision 2015-2025 programme. Planned for launch in 2022 and arrival at Jupiter
More informationHistory of Radioastronomy from 1800 to 2007
History of Radioastronomy from 1800 to 2007 (a personal selection) Steve Torchinsky Observatoire de Paris History of radio astronomy, Steve Torchinsky Goutelas, 4 June 2007 1 Herschel discovers invisible
More informationJUPITER BURST OBSERVATION WITH LOFAR/ITS
JUPITER BURST OBSERVATION WITH LOFAR/ITS A. Nigl, J. Kuijpers, H. Falcke, P. Zarka, L. Bähren Abstract Io-induced Jupiter emission lies mainly in the frequency range from about 2 to 40 MHz [Zarka et al.,
More informationThe international SKA project
The international SKA project - Towards a giant global radio telescope - Wim van Driel Paris Observatory - GEPI 3 rd MCCT SKADS School, Paris, 24/08/2009 SKA - Square Kilometre Array Necessary for a breakthrough
More informationAmateur data from Radio-Jove in the Virtual Observatory
Amateur data from Radio-Jove in the Virtual Observatory B. Cecconi (1), J. Thieman (2), J. Girard (3) (1) LESIA, Observatoire de Paris-CNRS-UMPC-Univ. Paris Diderot, Meudon, France (baptiste.cecconi@obspm.fr);
More informationBRINGING YOUR EXPERIMENT INTO SPACE
BRINGING YOUR EXPERIMENT INTO SPACE Science Service Division SSC - Swedish Space Corporation Space exploration with ESA: opportunities within the ESA programme E3P Stockholm, 13 November 2018 SWEDISH SPACE
More informationThe Quantum Sensor Challenge Designing a System for a Space Mission. Astrid Heske European Space Agency The Netherlands
The Quantum Sensor Challenge Designing a System for a Space Mission Astrid Heske European Space Agency The Netherlands Rencontres de Moriond - Gravitation, La Thuile, 2017 Quantum Sensors in Lab Experiments
More informationV. Astronomy Section
EAS 100 Planet Earth Lecture Topics Brief Outlines V. Astronomy Section 1. Introduction, Astronomical Distances, Solar System Learning objectives: Develop an understanding of Earth s position in the solar
More informationSpace Physics: Recent Advances and Near-term Challenge. Chi Wang. National Space Science Center, CAS
Space Physics: Recent Advances and Near-term Challenge Chi Wang National Space Science Center, CAS Feb.25, 2014 Contents Significant advances from the past decade Key scientific challenges Future missions
More informationUltra-short Radio Pulses from High Energy Cosmic Rays
Ultra-short Radio Pulses from High Energy Cosmic Rays Andreas Horneffer for the LOFAR CR-KSP High Energy Cosmic Rays high energy particles dominated by atomic nuclei similar in composition to solar system
More informationNEW INSTRUMENTATIONS AND METHODS FOR THE LOW FREQUENCY PLANETARY RADIO ASTRONOMY
NEW INSTRUMENTATIONS AND METHODS FOR THE LOW FREQUENCY PLANETARY RADIO ASTRONOMY A. A. Konovalenko, A. Lecacheux, C. Rosolen, and H. O. Rucker Abstract Over the past years the interest for the low frequency
More informationRadiation Environments, Effects and Needs for ESA Missions
Radiation Environments, Effects and Needs for ESA Missions Eamonn Daly European Space Agency ESTEC, Noordwijk, The Netherlands Space Environment Engineering and Science Applications Workshop 5 September
More informationTOR. Exploring dissipation in solar wind turbulence
TOR Exploring dissipation in solar wind turbulence Austria R.Nakamura(IWF), Y.Narita(IWF), Z.Vörös(IWF) Belgium J.DeKeyser(BISA), G.Lapenta(K.U.Leuven) Canada C.Cully(U.Calgary), I.Mann(U.Alberta) China
More informationStellarXplorers IV Qualifying Round 2 (QR2) Quiz Answer Key
1. Which of these Electromagnetic radiation bands has the longest wavelength (λ)? [Section 12.1] a. X-Ray b. Visible Light c. Infrared d. Radio 2. How is energy in Electromagnetic (EM) radiation related
More informationRecent and future actions about Space Weather in Austria Manuela Temmer
Recent and future actions about Space Weather in Austria Manuela Temmer Institute of Physics, University of Graz, Austria U.N. Space Weather Expert group Meeting and Workshop, Vienna, February 15 17, 2016
More informationOperational Aspects of Space Weather-Related Missions
Operational Aspects of Space Weather-Related Missions Richard G. Marsden, ESA/SCI-SH Outline SOHO: Example of Near-Earth Observatory-class Mission Ulysses: Example of Deep Space Monitor-class Mission Solar
More informationThe ESA scientific program
The ESA scientific program Luigi Colangeli Science and Robotic Exploration Directorate Head, ESA Solar System Missions Division and Coordinator, ESA Solar System Missions ESA-ESTEC 1 The ESA fleet in Astronomy
More informationExecutive Summary Report Nov 2012 First issue All
November 26, 2012 Page i Document Change Record Issue Date DCN No. / Change Description Pages Affected 1 26 Nov 2012 First issue All Document Distribution Sheet Issue: 1 Issue Date: 26 Nov 2012 Name Company
More informationInternational Project Update
International Project Update - Mike Garrett (ASTRON & Leiden) Chair SKA Science & Engineering Committee This talk - SKA: a global vision for Radio Astronomy - Science drivers - Pathfinders, Precursors,
More informationAstronomy Test Review. 3 rd Grade
Astronomy Test Review 3 rd Grade Match the vocabulary word to its definition. Outer Planets The path a planet takes around the sun. Inner Planets Orbit Sun The center of our solar system. Small, rocky
More informationBig-Data as a Challenge for Astrophysics
Big-Data as a Challenge for Astrophysics ESA / Euclid Consortium Hubble deep field, NASA/STScI HESS collaboration, F. Acero and H. Gast ESA/ATG medialab; ESO/S. Brunier Volker Beckmann Institut National
More informationSolar Radio Observation using Callisto Spectrometer at Sumedang West Java Indonesia: Current Status and Future Development Plan in Indonesia
Ground-based Solar Observations in the Space Instrumentation Era ASP Conference Series, Vol. 504 Ivan Dorotovič, Catherine E. Fischer, and Manuela Temmer, eds. c 2016 Astronomical Society of the Pacific
More informationRadio Astronomy module
Radio Astronomy module Contact tony@ska.ac.za Notes: NRAO Essential radio astronomy course: http://www.cv.nrao.edu/course/astr534/era.shtml See also http://www.haystack.mit.edu/ edu/undergrad/materials/ra_tutorial.html
More informationSpace-based Probes for Cosmic Dawn
Joseph Lazio Pre-decisional, for information and discussion purposes only. 2018 California Institute of Technology Hydrogen Signal from EoR and Before A Role for Space? 5 10 50 100 500 MHz EoR 50 Neutral
More informationNICT SPACE WEATHER ACTIVITIES
Prepared by NICT Agenda Item: 3 Discussed in Ad-Hoc Meeting on Space Weather NICT SPACE WEATHER ACTIVITIES Tsutomu Nagatsuma Space Weather and Environment Informatics Laboratory, Applied Electromagnetic
More informationNeutrinos with a cosmic ray detector. Cosmic rays with a neutrino detector
Instead of Neutrinos with a cosmic ray detector Cosmic rays with a neutrino detector Anna Nelles University of California Radio emission of showers High energy particles interacting in dense medium (or
More informationILWS activity in Romania
Institute of Space Science romanian space agency ILWS activity in Romania Dumitru HASEGAN 1,2. Octav MARGHITU 1 1-ISS, 2-ROSA Outline A. Introduction Historical synopsis B. Research themes 1. Solar-Terrestrial
More informationTodays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors
PHYS 1403 Introduction to Astronomy Light and Telescope Chapter 6 Todays Topics Astronomical Detectors Radio Telescopes Why we need space telescopes? Hubble Space Telescopes Future Space Telescopes Astronomy
More informationSpace Weather. Dr Thomas J Bogdan Director, Space Weather Prediction Center Boulder, CO
Space Weather Dr Thomas J Bogdan Director, Space Weather Prediction Center Boulder, CO 2011 DIB CIP Meeting 25 August 2011 Space Weather Prediction Center Our Mission: To provide space weather products
More informationHistory and modernity of the study of Space Weather in Russia
History and modernity of the study of Space Weather in Russia Klimov, S.I., A.A. Petrukovich Space Research Institute, Russian Academy of Sciences (IKI RAN), 117997, 84/32 Profsoyuznaya str., Moscow, Russia
More informationObserving transients with LOFAR and AARTFAAC
Astronomical Institute "Anton Pannekoek", University of Amsterdam, Postbus 94249, 1090 GE Amsterdam, The Netherlands E-mail: b.a.rowlinson@uva.nl The Low Frequency Array (LOFAR) is a new European radio
More informationTracking CME s With LOFAR
Tracking CME s With LOFAR Interplanetary Scintillation Studies With a Large, Multi-beaming, Phased Interferometric Array Michael Stevens What s A? WHat are All These Silly Acronyms? LOFAR- the LOw Frequency
More informationSKA Precursors and Pathfinders. Steve Torchinsky
SKA Precursors and Pathfinders Steve Torchinsky steve.torchinsky@obspm.fr A square kilometre of collecting area for each of three frequency bands SKA Low frequency 50MHz to 450MHz to be built in Western
More informationRFI Detectives Activity for Large Public Venues
RFI Detectives Activity for Large Public Venues Adapted from the NRAO s Be An Interference Detective activity Background Most people living near big cities are familiar with light pollution and how it
More informationWinds on Titan: First results from the Huygens Doppler Wind Experiment
1 Winds on Titan: First results from the Huygens Doppler Wind Experiment Supplementary Discussion. It was realized during the DWE design phase that Earth-based Doppler measurements could be combined with
More informationWhat is Earth Science?
What is Earth Science? A.EARTH SCIENCE: the study of Earth and its history B. Earth science is divided into 4 main branches: 1. Geology: study of the lithosphere 2. Oceanography: study of oceans 3. Meteorology:
More informationSpace Weather Effects on Critical Operations and Activity in the High North
Space Weather Effects on Critical Operations and Activity in the High North Pål Brekke Senior Advisor Paal@spacecentre.no ISWI Workshop, Boston College, 31 July - 4 August 2017 Space Weather in the Arctic
More informationPerspektiven der. Radioastronomie. im Weltraum. J. Anton Zensus Silke Britzen. Max-Planck-Institut für. Radioastronomie
Perspektiven der Radioastronomie im Weltraum J. Anton Zensus Silke Britzen Max-Planck-Institut für Radioastronomie Grundlagenforschung im Weltraum Deutschlands Herausforderungen der nächsten Dekaden München
More informationSimulations of ultra-long wavelength interferometers in the Earth orbit and on the lunar surface
Research in Astron. Astrophys. Vol.0 (200x) No.0, 000 000 http://www.raa-journal.org http://www.iop.org/journals/raa Research in Astronomy and Astrophysics Simulations of ultra-long wavelength interferometers
More informationFrom LWS to ILWS and Norwegian Priorities. Bo Andersen Norwegian Space Centre
From LWS to ILWS and Norwegian Priorities Bo Andersen Norwegian Space Centre ILWS Requirements ILWS may have broader goals, motivation and requirements than LWS. Predictive capability still too small so
More informationLarge Field of View Radio Astronomy; relevant for many KSP s
Large Field of View Radio Astronomy; relevant for many KSP s SKA Key Science Drivers ORIGINS Probing the Dark Ages When & how were the first stars formed? Cosmology and Galaxy Evolution Galaxies, Dark
More informationPlanetary radio astronomy by space-borne and ground-based low-frequency observations
4th URSI Austria Meeting Planetary radio astronomy by space-borne and ground-based low-frequency observations H.O. Rucker Commission for Astronomy Austrian Academy of Sciences Graz, Austria Nov 5, 2015
More informationCleopatra. Connecting Locations of ESFRI Observatories and Partners in Astronomy for Timing and Real-time Alerts. Arpad Szomoru
Cleopatra Connecting Locations of ESFRI Observatories and Partners in Astronomy for Timing and Real-time Alerts Arpad Szomoru Joint Institute for VLBI ERIC (JIVE) On behalf of the Cleopatra collaboration
More informationCosmic Rays. Cooperation at the Space Pole. D. Sapundjiev, T. Verhulst, M. Dierckxsens, E. De Donder, N. Crosby, K. Stegen, and S.
Cosmic Rays Cooperation at the Space Pole D. Sapundjiev, T. Verhulst, M. Dierckxsens, E. De Donder, N. Crosby, K. Stegen, and S. Stankov Excellence (STCE) Ringlaan 3, B-1180 Brussels, Belgium Stan Stankov
More informationJUpiter Icy Moons Explorer (JUICE) Status report for OPAG. N. Altobelli (on behalf of O. Witasse) JUICE artist impression (Credits ESA, AOES)
JUpiter Icy Moons Explorer (JUICE) Status report for OPAG N. Altobelli (on behalf of O. Witasse) JUICE artist impression (Credits ESA, AOES) Message on behalf of the JUICE Science Working Team Congratulations
More informationFirst European Space Weather Week. Space weather - atmospheres, drag, global change future needs. 29 November-3 December 2004
First European Space Weather Week Space weather - atmospheres, drag, global change future needs 29 November-3 December 2004 Timescales of important phenomena Weather Climate No single statement of requirement
More informationMulti-frequency imaging of Cygnus A with LOFAR
Netherlands Institute for Radio Astronomy Multi-frequency imaging of Cygnus A with LOFAR John McKean (ASTRON) and all the imaging busy week team! ASTRON is part of the Netherlands Organisation for Scientific
More informationNuMoon: Status of Ultra-High-Energy Cosmic-Ray detection with LOFAR and improved limits with the WSRT
NuMoon: Status of Ultra-High-Energy Cosmic-Ray detection with LOFAR and improved limits with the WSRT Sander ter Veen for the LOFAR Cosmic Ray Key Science Project Supervisor: Prof. Heino Falcke Radboud
More informationModular Low Earth Orbital-Hub DLR Vision 2025
The Space Congress Proceedings 2016 (44th) The Journey: Further Exploration for Universal Opportunities May 25th, 10:45 AM Modular Low Earth Orbital-Hub DLR Vision 2025 Dr. Oliver Romberg German Space
More informationWhat is astronomy actually? These are good questions and worthy of an answer.
We ve often been asked: What is astronomy actually? And what it is good for? These are good questions and worthy of an answer. ESA/NASA/Hubble Astronomy is the study of all celestial objects. It is the
More informationThe Dynamic Radio Sky: On the path to the SKA. A/Prof Tara Murphy ARC Future Fellow
The Dynamic Radio Sky: On the path to the SKA A/Prof Tara Murphy ARC Future Fellow What causes radio variability? 1. Explosions - e.g. supernovae, gamma-ray bursts, orphan afterglows 2. Propagation - e.g.
More informationThe Jovian Planets. The Jovian planets: Jupiter, Saturn, Uranus and Neptune
The Jovian planets: Jupiter, Saturn, Uranus and Neptune Their masses are large compared with terrestrial planets, from 15 to 320 times the Earth s mass They are gaseous Low density All of them have rings
More informationRadio Astronomy and Amateur Radio. Glenn MacDonell VE3XRA 3 August 2010
Radio Astronomy and Amateur Radio Glenn MacDonell VE3XRA 3 August 2010 Radio Astronomy The study of objects in the sky using radio frequencies Very young field History of Radio Astronomy Basic work on
More information