Q:Wat is er zo mooi om te zien. Toch geen interessante kunstwerken in het landschap? A:Het ritme van de antennevelden tussen dwalende zwanen en legerende hazen is als poezie geschreven op een vijgenblad.

IBM en Astron analyseren big data van big bang

Exabyte-project levert nieuwe computersystemen op
IBM en Astron analyseren big data van big bang

Ict-leverancier IBM en het Nederlandse Instituut voor Radio Astronomie Astron stappen samen in een nieuw exaschaal computing-project. Doel is om computersystemen te ontwikkelen die 1 exabyte aan data, komend uit de ruimte, per dag kunnen lezen, analyseren en opslaan. De samenwerking duurt in eerste instantie vijf jaar, heeft een waarde van 32,9 miljoen euro en vindt plaats in het Drentse Dwingeloo, in het nieuw opgerichte Astron & IBM Center for Exascale Technology. Lees Meer IBM en Astron analyseren big data van big bang

Wat is nou eigenlijk LOFAR?

The LOw Frequency ARray is a multi-purpose sensor array. Its main application is astronomy at low frequencies (10-250 MHz) which is described at the present site. LOFAR has also applications in Geophysics and Agriculture, which are described at http://www.lofar.org/.

For the astronomy application LOFAR is a radio interferometric array consisting of many low-cost antennae. There are two distinct antennae types: the Low Band Antennae (LBA) operating between 10 and 90 MHz and the High Band Antennae (HBA) operating between 110 and 250 MHz. The antennae are organised in aperture array stations.

The stations are distributed over an area of about 100 km in diameter, located in the north of the Netherlands. Several international stations are contructed or planned in Germany (5), Sweden (1) , the UK (1), France (1), Poland and Italy. The longest baselines in Europe are 1500 km.
A Wide Area Network (WAN) connects the stations with the CEntral Processing facility (CEP), an IBM BlueGene/P super computer in Groningen, where data are collected and processed.

One of the major differences with traditional telescopes is that LOFAR will be extremely flexible. That is why LOFAR is also referred to as a software radio telescope and the software already was one of the main focuses at the start of the project.’

vertaling volgt nog

Duits LOFAR station Jülich in gebruik genomen

De LofarZone is wederom uitgebreid. Na een negen maanden bouwtijd op 5 Oktober 2011 van de Ruhr-Universität Bochum, Jacobs University Bremen en het Jülich Research Center gebouwd LOFAR station werd officieel in gebruik genomen. De Jülich LOFAR station is de vijfde Duitse station van ‘s werelds grootste radiotelescoop LOFAR-systeem.

Luchtfoto van het Jülich LOFAR station. (Foto: Forschungszentrum Jülich)

Luchtfoto van het Jülich LOFAR station. (Foto: Forschungszentrum Jülich)

Het Jülich LOFAR station

LOFAR (LOw Frequency ARray) is een nieuwe radio telescoop die wordt gebouwd door verschillende samenwerkende onderzoeksinstituten in Europa. De radiogolven van de kosmische objecten worden genomen door eenvoudige draadantennes en via computernetwerken te Groningen (NL) beheerd en verwerkt. Om een ​​hoge resolutie en een groot detail van de foto’s te krijgen, worden in heel Europa LOFAR stations worden gebouwd: naast Nederland, Frankrijk, Groot-Brittannië en Zweden neemt met name in Duitsland deel in de planning door de oprichting van een groot aantal stations.Meer Europese landen plannen aanleg en exploitatie van LOFAR stations.

360 graden panorama van het Jülich LOFAR station. (Foto: B. Burggraf)

360 graden panorama van het Jülich LOFAR station. (Foto: B. Burggraf)

Voor een LOFARveld is een vlakke ondergrond een vereiste en tevens een beschikbaar snel netwerk – eisen die in Jülich optimaal worden vervuld. De antennes voor lage frequenties worden gemaakt van eenvoudige draad-dipool, op een verticale, ongeveer 1.60 m hoge paal staat. De antennes voor hoge frequenties worden gemonteerd in kunststof dozen en liggen naast elkaar. In een voor straling afgesloten container is de elektronica gehuisvest.

Na voltooiing van het station is het volledig stil, aangezien er geen bewegende delen zijn en zit de echte kracht van de telescoop in de elektronica en software die ontwikkeld moesten worden voor de werking en data-analyse. Vanaf het einde van 2010 (! 2011 red.) zal het Jülich LOFARstation gegevens samenbrengen met de rest van de stations en zullen astronomen en opnames te bieden hebben in een vrijwel onontgonnen frequentiebereik.

Dit station is gebouwd door de Ruhr-Universität Bochum, Jacobs University Bremen en het Jülich Research Center. De fondsen van het federale ministerie van Onderwijs en Onderzoek werden gebruikt.

Bron: http://www.astro.rub.de/lofar-station/

Welcome to the LofarZone: Chilbolton and Wherwell (UK)

Afgelopen 14 mei was er een open dag in de LofarZone in Chilbolton & Wherwell in Engeland. Wij verwelkomen deze plaatsen in de LofarZone.

On Saturday 14 May 2011 a visitors’ day was held at the LOFAR Chilbolton site. This was a requirement of our LOFAR planning application, namely that we host some form of public-information event for the local communities of Wherwell and Chilbolton Village. Three members of the LOFAR-UK team (Derek McKay-Bukowski, Brian Ellison and Malcolm Coe) were at hand to show visitors around the Low-Band and High-Band Arrays and to give them a rare glimpse inside the RF-container.

In all, it was a very successful day, with lots of interesting questions. In total we had over 75 guests at the site. We certainly hoped that all our visitors enjoyed the event. Hopefully, we will be able to hold an open day for the general public sometime in the future as well. And many thanks to Brian and Malcolm for giving up part of their weekend to assist Derek with explaining the LOFAR-UK facility.

Brian Ellison (in the high-vis vest) explains how the LBA aerials work to locals including Graham and Brian Patterson (on his left and right respectively).

LofarZone strekt zich uit tot in Finland

Lofar HighBand antennes in de Finse sneeuw

In Finland is het eerste antennepakket goed de winter door gekomen. Er is geen schade geconstateerd, er is niets verschoven.

Dit antennepakket met HighBand antennes voor Lofar staat er in verband met de onderzoeken van de Finse universiteit van Oulu.

KAIRA (Kilpisjärvi Atmospheric Imaging Receiver Array) is a project of the Sodankylä Geophysical Observatory. KAIRA is a dual array of omni-directional VHF radio antennas, principally funded by the University of Oulu in Finland. It makes extensive use of the proven LOFAR antenna and digital signal-processing hardware, and can act as either a stand-alone passive receiver, as a receiver for the EISCAT VHF incoherent scatter radar in Tromsø, or for use in conjunction with other Fenno-Scandinavian VHF experiments.

Bron: http://www.sgo.fi/KAIRA/

Gestart met bouw in Zweedse LofarZone

Er is begonnen met de bouw van een LOFAR antennesite in Zweden. Op bijgaande foto zie je de afgraving van de grond op de plek waar de antennes komen te staan.meer info bij een zweedse LofarEnthousiast http://plixi.com/e/10040of op de site van LOIS

klik op de foto voor een vergroting.

Lofar heeft antenneveld in Engeland

De Noord-Nederlandse radiotelescoop Lofar is sinds 21 september 2010 uitgebreid met een antenneveld in de buurt van Chilbolton, iets ten noorden van Southhampton. Er zijn ook al antennevelden in Duitsland en Frankrijk.
Lofar bestaat uit duizenden kleine antennes, verspreid over tientallen ‘stations’ die vanuit de omgeving van het Drentse Borger uitwaaieren. De gegevens van deze samengestelde radiotelescoop komen samen in de supercomputer Stella die bij de RUG staat. Het nieuw geopende Britse antenneveld vergroot de virtuele diameter van de telescoop, waardoor de scherpte verdubbelt.

HetBritse antenneveldvoor Lofar werd geopend door Dame Jocelyn Bell Burnell. Zij ontdekte als student in 1967 de zogeheten radio-pulsars, objecten in het universum die zeer snelle en zeer regelmatige radiosignalen uitzenden. Lofar is onder meer in staat dit soort pulsars op te sporen.

Dame Jocelyn Bell Burnell opent het Britse Lofar-antenneveld met het doorknippen van een lint.


21 September 2010Last updated at13:14 GMT

Telescope goes after first stars
Dame Jocelyn Bell Burnell (C), Derek McKay-Bukowski (L), and John Womersley, STFC (R)

Pulsar discoverer Dame Jocelyn Bell Burnell performs the official opening at Chilbolton

The UK has officially opened its first station in a new international radio astronomy antenna network.
Lofar (Low Frequency Array) is a European project that incorporates new digital techniques to survey wide areas of the sky all at once.
The station in Chilbolton, Hampshire, joins similar sites in France, Germany, Sweden and the Netherlands.
Astronomers hope the network can help them probe the period in cosmic history when the very first stars were formed.
“In traditional arrays, you have to move their dishes physically if they want to look in a different direction,” explained Derek McKay-Bukowski, the project manager at Lofar Chilbolton.
Continue reading the main story

LOFAR – LOW FREQUENCY ARRAY
Lofar UK Chilbolton station
An assembly (tiles) of antennas that detect the higher frequencies in Lofar’s range
  • The Lofar system operates at the lowest frequencies accessible from Earth
  • Its stations collect signals received by 1,000s of simple dipole receivers
  • This information is sent via fibre optics to a central IBM supercomputer
  • It combines all the data to make a synthetic radio image of unprecedented quality
“Lofar is a digital telescope which means you can switch the direction where you’re looking very fast. You can go from one side of the sky to the other side of the sky – rather than in minutes, you can do it milliseconds. And because it’s digital, Lofar can look in multiple directions at once,” he told BBC News.
Lofar is sensitive to much longer wavelength radiation than the UK’s established radio telescope array called Merlin, which is based on the giant Lovell dish at Jodrell Bank in Cheshire.
Being able to detect this particular segment (1-10m/240-30MHz) of the electromagnetic spectrum will enable scientists to study very different astrophysical phenomena.
One key target is the epoch of re-ionisation.
This relates to an important change in the cosmic environment brought about by the very first population of stars to shine in the Universe.
Theory holds these hot, young giants produced intense ultraviolet radiation that “fried” the neutral gas that had formed up to that point and which we detect in the local Universe today as a diffuse plasma between the galaxies.
Lofar as it stands
Seeing this first population of stars is just beyond the capability of the current crop of optical telescopes like Hubble or the VLT, but conditions during this epoch could be probed at Lofar frequencies, astronomers say.
The network plans to install more and more antennas over the years to make Lofar ever more sensitive to what it is trying to see.
Derek McKay-Bukowski said: “When the entire project is finished, we will have something in the order of 5,000 antennas for both low-band and high-band, which will be located at about 48 stations across Europe.
“The biggest separation is about 1,100km. Distance between stations gives you resolution; to see finer detail you need bigger and bigger separations.”
Lofar is led by Astron (the Netherlands Foundation for Research in Astronomy) which is installing a dense network of antennas centred near the village Exloo in the north of Halland.
The Chilbolton Observatory's low-band antennas

The Chilbolton Observatory’s low-band antennas

Lofar UK is funded through a collaboration of UK universities with the SEPnet consortium and the UK Science and Technologies Facilities Council.
As well as re-ionisation, the project has five other major research areas:
1. Surveying space beyond our galaxy to try to understand the history of star formation and black hole growth over cosmological time
2. Probing the extreme astrophysical environments that lead to transient bright bursts in the radio sky, such as from pulsars, the highly magnetised remains of dead stars
3. Understanding cosmic rays, the storm of high-energy particles (mostly protons and helium nuclei) that rain down on Earth
4. Studying the local space environment, to see how the wind of particles billowing away from the Sun interacts with the Earth.
5. Investigating cosmic magnetism – the origin of the large-scale fields that pervade the Universe.

Listening for ET’s Television

Listening for ET’s Television

By Seth Shostak

SETI Institute

posted: 09 November 2006

06:21 am ET

http://www.space.com/searchforlife/seti_shostak_tv_061109.html

The first episode of “I Love Lucy” was broadcast sometime on October 15, 1951. About 0.0002 seconds later, the signal glided over the rooftops of the farthest city suburbs, and headed into space.

It’s still going. Every day, that first installment passes through an additional 4 thousand trillion trillion trillion cubic kilometers of the cosmos.

Given that stars in our galactic neighborhood are separated by about 4 light-years, it’s easy to figure that roughly 10 thousand star systems have been exposed to “I Love Lucy” in the past five decades. That may suggest a high Nielson rating, but the chance that extraterrestrials are now hooked on 1950s television is low. Look at it this way: Carl Sagan, who was singularly optimistic about such things, figured that the number of technically competent societies in our Galaxy was a million or more. That’s a lot. But even so, it would imply that only one in every few hundred thousand star systems would actually boast such a society. Consequently, there’s little probability that hairless gray guys are puzzling over the domestic difficulties of Lucy and Ricky, a fact that no doubt will disappoint the advertisers.

The widespread use of television on Earth is a phenomenon of the last half-century. But the cosmos is three times as old as our planet. So there could be galactic civilizations that have been churning out sitcoms for thousands of years or more – time enough for the signals to reach our world.

This possibility was evidently on the mind of Abraham Loeb at Harvard University, who recently noted in the New Scientist that a radio telescope being built to study distant galaxies might also be able to pick up ET’s TV. The so-called Low-Frequency Array (LOFAR), a telescope consisting of 25 thousand tent-shaped antennas spread across Holland and Germany, can be tuned to frequencies under 250 megahertz. This is a spectral range far below what’s usually searched by SETI, but it’s the band in which much of your local television is broadcast. And maybe theirs, as well.

So how realistic is this? Could LOFAR really pick up “I Love Zork”?

To answer that question requires doing some numbers (you can read through this quickly if quantitative arguments cause your brain to idle).

First, we reverse the situation, just to see if tuning in remote TV makes sense. Imagine that there are alien couch potatoes 55 light-years away who, bored with their own Fall lineup, have constructed a LOFAR-style antenna in hopes of picking up “I Love Lucy’s” debut. Hunky TV transmitters on Earth belch out a few hundred thousand watts of power. That energy is not beamed in all directions equally; most of it is aimed around the horizon (which, of course, is where the audience is). Because of this slight beaming, the effective transmitter power is a bit more: let’s say a million watts, to keep the math simple.

OK, how strong is that signal by the time it reaches our putative alien audience at 55 light-years distance? Not very. The megawatt broadcast washes over ET’s world with a power density of about 0.3 million million million million millionths of a watt per square meter, which is not exactly a scorching signal. Actually, only about a third of that transmission power is in the “carrier” – the part of the broadcast that’s very narrow in frequency and easily detected. So knock that piddling power density down by another factor of three if you want to know the strength of the easily detectable part of the transmission. (Of course, if they only find the carrier, they won’t get the picture and sound. But Lucy’s jokes might not appeal to aliens anyway.)

Could their LOFAR-style antenna find that carrier, thereby indicating that a program was on the air? Well, engineers have computed that at the frequency of VHF television, LOFAR will have an effective collecting area similar to that of the 305-meter diameter Arecibo antenna in Puerto Rico.

That’s big. That’s brawny. But not brawny enough. In our SETI experiments at Arecibo, we could find a signal if it were about 0.1 million million million millionths of a watt per square meter. That number, you will notice if you count up the words, is a million times bigger than the “I Love Lucy” carrier at 55 light-years. The aliens’ LOFAR would be inadequate to detect the broadcast by a factor of a million, a not entirely negligible amount. Simply stated: LOFAR couldn’t hear it.

So here’s the bottom line: LOFAR would only be able to find TV signals comparable to ours from a distance of much less than one light-year! Turning this around, the mother of all rabbit ears couldn’t pick up the Alien Broadcasting Network at the distance of even the nearest star.

Disappointing, but you might argue that the extraterrestrials will have much, much more powerful TV transmitters than we do. In fact, their broadcasts would have to be millions of times more powerful to even produce a blip on LOFAR, which seems a bit silly and likely to set alien roofs on fire.

Now Loeb points out that LOFAR and other large telescopes now being planned can stare at the same spot on the sky for months or years. That allows a signal to build up, making even weak transmissions visible. After a year of staring, LOFAR’s sensitivity will be several hundred times better than our work at Arecibo. That’s the good news. The bad news is that it’s still inadequate to hear TV transmitters similar to our own.

But there’s another point, and one that’s possibly of greater significance. The whole idea of television broadcasting may be passe for the aliens. Consider: how do you pick up your daily dose of boob-tube fodder? With a rooftop antenna strapped to your chimney? Probably not. You most likely get your TV via a cable, fiber optic, or direct broadcast satellite dish. The powerful television transmitters on the hills outside town are going to vanish in the next few decades. They likely vanished long ago on ET’s world.

So while it’s certainly an excellent idea to look for cosmic signals at low frequencies, it’s unlikely that any will resemble the type of entertainment we still loft into the skies here on Earth. And some would say that’s reassuring.

LofarZone for Europe

A group op enthousiast citizens is trying to put LOFAR on the map of Europe.

With activities in Europe in the proximity of the LOFAR radiotelescope we  want to establish the LofarZone.

We are letting all inhabitants of the LofarZone know of this project.

We want to develop ideas which are not astronomous but closer to the people in conjunction with the giant telescope, like tourism, art, healt, landscape, architecture, etc

We want to display the development and all possible interesting ideas to the public with a giant screen beginning in the core area of the telescope.

Sponsors are requested to contact us for contribution of Euro’s

Visionais are requested to contact us for contribution of ideas.

Citizens andEntreprneursof the LofarZone are requested to contact us for the development of buisines in the LofarZone.

Our international website is at this location: http://lofarzone.eu (redirects to this page)

Our buisiness website is at this location: http://lofarzone.com (for future expansion)

See some ideas (in Dutch)

project easter bunny

astronomic wellness

other projects to come

Business page LofarZone

This page is intentionally left blank and will be used for furture expansion.