GLOW News Blog

News about the German Long Wavelength Consortium and radio astronomy in Germany

Im Tagesspiegel ist gerade ein lesenwerter Artikel zur Rolle Deutschlands beim SKA (Square Kilometre Array) erschienen. Anlass ist die zurzeit in Vorbereitung befindliche Bewerbung mehrerer deutscher Forschungsinstitute und Universitäten beim "Roadmap-Prozess für Forschungsinfrastrukturen" des BMBF, über den eine nationale Beteiligung Deutschlands and diesem in wissenschaftlicher wie wirtschaftlicher Hinsicht außerordentlich interessanten Projekt erreicht werden soll. Hier geht es zum Artikel beim Tagesspiegel.

Last week, at the GLOW Annual Assembly 2015 at AIfA in Bonn, the GLOW consortium was happy to welcome the University of Würzburg as it's newest member. Prof. Matthias Kadler and his group research the links of long-wavelength radio astronomy with topics in high energy astrophysics and astroparticle physics, focusing on relativistic jets in blazars and other active galaxies. We are looking forward to fruitful discussions and exciting new discoveries in this collaboration.

The European Radio Telescope Review Committee (ERTRC) delivered a strategy to optimize the use of radio telescopes by the European astronomical community, both in the short as well as in the medium to long-term. This report was requested by the Board of the ASTRONET, a body in charge of a comprehensive long-term planning for the development of European astronomy. The report is available here.

In der kürzlich erschienenen September-Ausgabe der Zeitschrift 'Sterne und Weltraum' berichtet Prof. Dr. Marcus Brüggen von der Hamburger Sternwarte aus der Forschung mit LOFAR. Der Titel des Beitrags lautet "Von Blitzen und kosmischen Zahnbürsten - Erste Ergebnisse mit dem Low Frequency Array (LOFAR)".

Den sehr lesenswerten Artikel finden Sie in 'Sterne und Weltraum' (Ausgabe 9/15), sowie auf der Webseite des Spektrum-Verlags (ggf. kostenpflichtig).

The DFG funded Research Group on Cosmic Magnetism has held its annual meeting from 1 to 4 July in Ringberg.

This was the sixth meeting of the successful Research Group which investigates the origin and structure of cosmic magnetic fields. In the second funding period of the Research Group significant progress has been made in particular in analysing LOFAR data for gaining insight into magnetic fields in galaxies and clusters of galaxies. The recent developments of the LOFAR calibration and imaging software has allowed a tremendous progress in studying the synchrotron emission of galaxies and galaxy clusters at LOFAR frequencies now with unprecedented resolution und sensitivity. The meetings of the Research Group offers also PhD students in the group the possibility to present their considerable progress to a wider community.

 In addition to LOFAR observations the group uses other telescopes, e.g. GMRT and JVLA, which have been partly upgraded, to achieve the goals. Moreover, new approaches for analysing data from radio interferometers are under development.  The studies are complemented by theoretical work on the formation and evolution of magnetic fields in large numerical simulations. 

In 2016 the Research Group will held its final conference from 26th to 30th September at the Harnack House (MPG) in Berlin. To focus of the conference will be on Magnetisation of Interstellar and Intergalactic Media

  

Am 9. September 2015 wurde die internationale Station DE 609 in Norderstedt feierlich eröffnet. Sie ist die 47. Station des LOFAR Radiointerferometers. Über 50 Gäste besichtigten zunächst die Station selbst, geführt von Dr. D. Engels (U Hamburg) und Dr. J. Künsemöller (U Bielefeld). In einem Grusswort an die Gäste schrieb die Wissenschaftssenatorin der Freien und Hansestadt Hamburg Katharina Fegebank: "Technisch gesehen ist das Radiointerferometer eine Art Digitalkamera für Radiostrahlung aus dem All mit der Größe von ganz Nordwesteuropa. Wissenschaftspolitisch gesehen ist es ein Beispiel für die gelungene Kooperation von Hochschulen und Forschungseinrichtungen in bisher sechs europäischen Ländern." Diese zentrale Bedeutung der Kooperation stand auch im Mittelpunkt der Grussworte von M. Hecht (Kanzler, U Hamburg), Prof. Dr. H. Graener (Dekan, Min. Fakultät, U Hamburg) und Prof. Dr. M. Egelhaaf (Prorektor, U Bielefeld) zu Beginn des Festaktes im Feuerwehr-Museum Norderstedt. Dr. R. Vermeulen (Direktor des International LOFAR Telescope) und Prof. Dr. H. Falcke (Vorsitzender des ILT Aufsichtsrates) stellten in ihren Vorträgen den Stand des Ausbaus des Interferometers und die faszinierenden ersten Beobachtungsergebnisse vor. Der Vorsitzende des Zusammenschlusses der deutschen LOFAR-Stationen (GLOW), Prof. R. Dettmar, sah mit der Einweihung der neuen Station eine weitere Stärkung der Position Deutschlands in der modernen Radioastronomie einhergehen. Der Oberbürgermeister Norderstedts H.-J. Grote begrüsste die Entscheidung der Universitäten, die Station hier zu bauen. Sie würde dem Profil der aufstrebenden Stadt am Nordrand Hamburgs als Technologiestandort eine weitere Facette hinzufügen. Die Bedeutung der Station für die Weiterentwicklung der Forschung und Lehre in der Physik machten die beiden Projektleiter der Station Prof. Dr. M. Brüggen (U Hamburg) und Prof. Dr. D. Schwarz (U Bielefeld) deutlich.  Einen Vorgeschmack auf die neuen Forschungsfelder, die sich für die Wissenschaftler an den beiden Universitäten jetzt eröffnen, gab Dr. S. Oslowski in seinem Beitrag zu den Einflüssen des interstellaren Mediums auf die Signale von extrem schnell rotierenden Neutronensterne, sogenannten Pulsaren.

From University Groningen

How is lightning initiated in thunderclouds? This is difficult to answer – how do you measure electric fields inside large, dangerously charged clouds? It was discovered, more or less by coincidence, that cosmic rays provide suitable probes to measure electric fields within thunderclouds. This surprising finding is published in Physical Review Letters on April 24nd. The measurements were performed with the LOFAR radio telescope located in the Netherlands.

"We used to throw away LOFAR measurements taken during thunderstorms. They were too messy." says astronomer Pim Schellart. "Well, we didn't actually throw them away of course, we just didn't analyze them." Schellart, who completed his PhD in March this year at Radboud University in Nijmegen and is supervised by Prof. Heino Falcke, is interested in cosmic rays. These high-energy particles, originating from exploding stars and other astrophysical sources, continuously bombard Earth from space. High in the atmosphere these particles strike atmospheric molecules and create 'showers' of elementary particles. These showers can also be measured from the radio emission that is generated when their constituent particles are deflected by the magnetic field of the Earth. The radio emission also gives information about the original particles. These measurements are routinely conducted with LOFAR at ASTRON in Dwingeloo, but not during thunderstorms...

 

Modeling

That changed when the data were examined in a collaborative effort with astrophysicist Gia Trinh, Prof. Olaf Scholten from Groningen University and lightning expert Ute Ebert from the Centrum Wiskunde & Informatica in Amsterdam. "We modeled how the electric field in thunderstorms can explain the different measurements. This worked very well. How the radio emission changes gives us a lot of information about the electric fields in thunderstorms. We could even determine the strength of the electric field at a certain height in the cloud." says Schellart. This field can be as strong as 50 kV/m. This translates into a voltage of hundreds of millions of volts over a distance of multiple kilometers: a thundercloud contains enormous amounts of energy.

 

Dangerous charge

Lightning is a highly unpredictable natural phenomenon that inflicts damage to infrastructure and claims victims around the world. This new method to measure electric fields in thunderclouds will contribute to a better understanding and ultimately better predictions of lightning activity. Current measurement methods from planes, balloons or little rockets are dangerous and too localized. Most importantly the presence of the measurement equipment influences the measurements. Cosmic rays probe the thunderclouds from top to bottom. Moving at almost the speed of light they provide a near instantaneous 'picture' of the electric fields in the cloud. Moreover, they are created by nature and are freely available. 'This research is an exemplary form of interdisciplinary collaboration between astronomers, particle physicists and geophysicists', says Heino Falcke. 'We hope to develop the model further to ultimately answer the question: how is lightning initiated within thunderclouds?'

 

Probing atmospheric electric fields in thunderstorms through radio emission from cosmic-ray induced air showers Schellart e.a

Physical Review Letters 24 april 2015 

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