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	<title>ENERGY-THINK! &#187; Germany</title>
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	<description>Energy Concepts &#38; Technologies for the 21st Century</description>
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		<title>The 1st High Resolution 3D Images of the Inside of a Polymer Solar Cell</title>
		<link>http://www.energy-think.net/2009/09/the-1st-high-resolution-3d-images-of-the-inside-of-a-polymer-solar-cell/</link>
		<comments>http://www.energy-think.net/2009/09/the-1st-high-resolution-3d-images-of-the-inside-of-a-polymer-solar-cell/#comments</comments>
		<pubDate>Thu, 17 Sep 2009 14:05:37 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Country]]></category>
		<category><![CDATA[Germany]]></category>
		<category><![CDATA[Netherlands]]></category>
		<category><![CDATA[PV]]></category>
		<category><![CDATA[Solar]]></category>
		<category><![CDATA[Eindhoven University of Technology]]></category>
		<category><![CDATA[Solar cell]]></category>

		<guid isPermaLink="false">http://www.energy-think.net/?p=425</guid>
		<description><![CDATA[<p class="wp-caption-text">E U of T</p>
<p>Researchers from the Eindhoven University of Technology have made the first high-resolution 3D images of the inside of a polymer solar cell. This gives them important new insights in the nanoscale structure of a polymer solar cell and the effect on its performance. This gives them important new insights into the [...]]]></description>
			<content:encoded><![CDATA[<div id="attachment_427" class="wp-caption alignleft" style="width: 160px"><img class="size-thumbnail wp-image-427" title="pb-51-3Dscan_klein_03" src="http://www.energy-think.net/wp-content/uploads/2009/09/pb-51-3Dscan_klein_03-150x150.jpg" alt="E U of T" width="150" height="150" /><p class="wp-caption-text">E U of T</p></div>
<p>Researchers from the Eindhoven University of Technology have made the first high-resolution 3D images of the inside of a polymer solar cell. This gives them important new insights in the nanoscale structure of a polymer solar cell and the effect on its performance. This gives them important new insights into the nanoscale structure of a polymer solar cell and the effect on its performance.</p>
<p>3D Electron tomography image of a polymer-metal oxide solar cell. 3D Electron tomography image of a polymer-metal oxide solar cell. The 3D nanoscopic morphology shows the interpenetrating metal oxide network in (yellow) inside a polymer matrix (black). The 3D nanoscopic morphology shows the interpenetrating network of metal oxide (yellow) inside a polymer matrix (black).</p>
<p><span id="more-425"></span></p>
<p>The research was a joint effort of TU/e-researchers and colleagues at the University of Ulm, Germany. The research was a joint effort of TU / e researchers and colleagues at the University of Ulm, Germany. The findings were published online in Nature Materials on Sunday 13 September. The findings were published online in Nature Materials on Sunday 13 September. The investigations shed new light on the operational principles of polymer solar cells. The investigations shed new light on the operational principles of polymer solar cells. This is expected to be very important for the development of better polymer solar cells. This is expected to be very important for the development of better polymer solar cells.</p>
<p>Cost-effective, flexible and lightweight Cost-effective, flexible and lightweight</p>
<p>Polymer solar cells do not have the high efficiencies of their silicon counterparts yet. Polymer solar cells do not have the high efficiencies of their silicon counterparts yet. Polymer cells, however, can be printed in roll-to-roll processes, at very high speeds, which makes the technology potentially very cost-effective. Polymer cells, however, can be printed in roll-to-roll processes, at very high speeds, which makes the technology potentially very cost-effective. Added to that, polymer cells are flexible and lightweight, and therefore suitable to be used on vehicles or clothing or to be incorporated in the design of objects. Added to that, polymer cells are flexible and lightweight, and therefore suitable to be used on vehicles or clothing or to be incorporated into the design of objects.</p>
<p>Hybrid polymer solar cells Hybrid polymer solar cells</p>
<p>In these hybrid solar cells, a mixture of two different materials, a polymer and a metal oxide are used to create charges at their interface when the mixture is illuminated by the sun. In these hybrid solar cells, a mixture of two different materials, a polymer and a metal oxide are used to create charges at their interface when the mixture is illuminated by the sun. The degree of mixing of the two materials is essential for its efficiency. The degree of mixing of the two materials is essential for its efficiency. Intimate mixing enhances the area of the interface where charges are formed but at the same time obstructs charge transport because it leads to long and winding roads for the charges to travel. Intimate mixing enhances the area of the interface where charges are formed but at the same time obstruct charge transport because it leads to long and winding roads for the charges to travel. Larger domains do exactly the opposite. Larger domains do exactly the opposite. The vastly different chemical nature of polymers and metal oxides generally makes it very difficult to control the nanoscale structure. The vastly different chemical nature of polymers and metal oxides generally makes it very difficult to control the nanoscale structure. The Eindhoven researchers have been able to largely circumvent this problem by using a precursor compound that mixes with the polymer and is only converted into the metal oxide after it is incorporated in the photoactive layer. The researchers have been Eindhoven Largely Able to circumvent this problem by using a precursor compound that mixes with the polymer and is only converted into the metal oxide after it was incorporated in the photo active layer. This allows better mixing and enables extracting up to 50% of the absorbed photons as charges in an external circuit. This allows better mixing and enables extracting up to 50% of the absorbed photons as charges in an external circuit.</p>
<p>Nanoscale mixing Nanoscale mixing</p>
<p>The importance of the degree of mixing was clearly demonstrated by visualization of the structure of these blends in three dimensions. The importance of the degree of mixing was Clearly demonstrated by visualization of the structure of these blends in three dimensions. Traditionally such visualization has been extremely challenging, but by using 3D electron tomography, the team has been able to resolve the mixing with unprecedented detail on a nanoscale. Traditionally such visualization has been extremely challenging, but by using 3D electron tomography, the team has been Able to resolve the mixing with unprecedented detail on a nanoscale. From these images the researchers at the Institute of Stochastics in Ulm have been able to extract typical distances between the two components, relating to the efficiency of charge generation, and analyze the percolation pathways, that is, how much of each component is connected to the electrode. From these images the researchers at the Institute of Stochastics at Ulm have been Able to extract typical distances between the two components, Relating to the efficiency of charge generation, and analyze the percolation pathways, that is, how much of each component is connected to the electrode. These quantitative analyses of the structure matched perfectly with the observed performance of the solar cells in sunlight. These quantitative analysis of the structure perfectly matched with the observed performance of the solar cells in sunlight.</p>
<p>Future Future</p>
<p>Even though these hybrid polymer solar cells are among the most efficient reported to date for this class, their power conversion efficiency of 2% in sunlight must be enhanced to make them really useful. Even though these hybrid polymer solar cells are among the most efficient reported to date for this class, their power conversion efficiency of 2% in sunlight must be enhanced to make them really useful. This will be realized by improving the control over the morphology of the photoactive blend, for example by creating polymers that can interact with the metal oxide and by developing polymers or molecules that absorb a larger part of the solar spectrum. This will be realized by improving the control over the morphology of the active blend photo, for example by creating polymers that can interact with the metal oxide and by developing polymers or molecules that absorb a larger part of the solar spectrum. At such point, the intrinsic advantages of hybrid polymer solar cells in terms of low cost and thermal stability of the nanoscale structure could be fully exploited. At such point, the intrinsic advantages of hybrid polymer solar cells in terms of low cost and thermal stability of the nanoscale structure could be fully exploited.</p>
<p>Publication Publication</p>
<p>The publication “The effect of three-dimensional morphology on the efficiency of hybrid polymer solar cells”, by Stefan Oosterhout et al. can be found at DOI 10.1038/NMAT2533. The publication &#8220;The effect of three-dimensional morphology on the efficiency of hybrid polymer solar cells&#8221;, by Stefan Oosterhout et al can be found at DOI 10.1038/NMAT2533.</p>
<p>The research was conducted at the Eindhoven University of Technology and the University of Ulm. The research was conducted at the Eindhoven University of Technology and the University of Ulm. It was funded by the Joint Solar Programme of FOM, NWO, and the Shell Research Foundation, the Deutsche Forschungsgemeinschaft, SenterNovem, and the Dutch Polymer Institute. It was funded by the Joint Solar Program of FOM, NWO, and the Shell Research Foundation, the Deutsche Forschungsgemeinschaft, Senter Novem, and the Dutch Polymer Institute.</p>
<p>Source: Eindhoven University of technology</p>
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		<title>X-Ray Telescope to Probe the Mysteries of Dark Energy</title>
		<link>http://www.energy-think.net/2009/08/x-ray-telescope-to-probe-the-mysteries-of-dark-energy/</link>
		<comments>http://www.energy-think.net/2009/08/x-ray-telescope-to-probe-the-mysteries-of-dark-energy/#comments</comments>
		<pubDate>Fri, 21 Aug 2009 16:31:33 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Country]]></category>
		<category><![CDATA[Dark Energy]]></category>
		<category><![CDATA[Germany]]></category>
		<category><![CDATA[Russia]]></category>
		<category><![CDATA[erosita]]></category>
		<category><![CDATA[German aerospace agency]]></category>

		<guid isPermaLink="false">http://www.energy-think.net/?p=300</guid>
		<description><![CDATA[<p>The German eROSITA (extended ROentgen Survey with an Imaging Telescope Array) ) X-ray telescope is to start searching for black holes and dark matter in 2012, using seven electronic ‘eyes’. On 18 August 2009, executive board members of the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) and the head of Russians space [...]]]></description>
			<content:encoded><![CDATA[<p>The German eROSITA (extended ROentgen Survey with an Imaging Telescope Array) ) X-ray telescope is to start searching for black holes and dark matter in 2012, using seven electronic ‘eyes’. On 18 August 2009, executive board members of the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) and the head of Russians space agency Roskosmos signed a detailed agreement during the MAKS International Aviation and Space Salon in Moscow, setting out all the organisational and technical boundary conditions for the eROSITA project.</p>
<p>As long ago as March 2007, a memorandum of understanding defined the willingness of the agencies to collaborate in principle on this project.</p>
<p><span id="more-300"></span></p>
<p>&#8220;This scientifically highly-demanding project is a beacon project of scientific collaboration in space between Russia and Germany,&#8221; DLR executive board chairman Prof. Johann-Dietrich Wörner said. Prof. Wörner continued: &#8220;It is my understanding that with this collaboration we can draw on the experience of the past not just with regard to unmanned space flight.&#8221;</p>
<div id="attachment_299" class="wp-caption alignleft" style="width: 210px"><img class="size-full wp-image-299" title="erosita_mpe_200" src="http://www.energy-think.net/wp-content/uploads/2009/08/erosita_mpe_200.jpg" alt="erosita" width="200" height="273" /><p class="wp-caption-text">erosita</p></div>
<p>eROSITA will be taken into orbit in 2012 from the Russian Baikonur cosmodrome on board the Russian Spektrum Roentgen Gamma (SRG) satellite. A Soyuz-Fregat rocket will take the satellite into an orbit around the second Lagrange point of the Sun-Earth system, L2. This point, located approximately 1.5 million kilometres behind Earth as seen from the Sun, is particularly good as a site for performing astrophysical observations. The European Herschel and Planck space telescopes have been in orbit around L2 since July 2009. From this position, eROSITA will observe the whole sky for seven years and scan it multiple times.</p>
<p>Before the eROSITA agreement signature: Vladimir Putin visits the DLR stand at MAKS, Moscow eROSITA: on the track of dark energy</p>
<p>The universe has been expanding ever since the Big Bang &#8211; and this expansion might be expected to be slowing down under the influence of gravity. Instead, the expansion is accelerating, driven by a poorly understood phenomenon referred to as ‘dark energy’. eROSITA is intended to shed light on the darkness. The X-ray telescope is being built under the lead management of the Max Planck Institute for Extraterrestrial Physics (MPE).</p>
<p>“The internationally strong position in X-ray astronomy that we have acquired in Germany through our participation in missions such as Rosat, XMM-Newton (X ray Multi-Mirror) and Chandra (Chandra X-Ray Observatory) will continue to grow,” Gerold Reichle, a DLR executive board member, said. &#8220;The results of the eROSITA mission will provide the international community of scientists with valuable new findings for a deeper understanding of the processes in the universe,&#8221; Reichle continued.</p>
<p>German eROSITA telescope to be a new star in the sky</p>
<p>The European XMM-Newton x-ray telescope in Earth orbit Construction of the new eROSITA telescope began in 2007, since the production of the mirrors and the cameras takes a long time. &#8220;Forty-five scientists, engineers and technicians are employed on its development and construction at the MPE alone,&#8221; said Dr. Peter Predehl, the project’s lead scientist from the Max Planck Institute for Extraterrestrial Physics, adding: &#8220;eROSITA is a world-leading instrument for X-ray astronomy, both scientifically and technologically.&#8221;</p>
<p>The German X-ray telescope consists of seven individual mirror systems with apertures of just under 36 centimetres for radiation ingress and 54 nested mirror shells each, which will scan the whole of the sky in parallel. The combination of collecting area, field-of-view and resolution is unparalleled. At the focal point of each X-ray mirror system, there is a CCD (Charge Coupled Device) camera specially developed for eROSITA. The seven electronic ‘eyes’ must be cooled to a temperature of below minus 80 degrees Celsius during operation. The cameras utilise expertise from the semiconductor laboratory maintained by the Max Planck Institutes for Physics and for Extraterrestrial Physics in Garching, which is the source for the most sensitive X-ray detectors in the world – used, for example, in the European XMM-Newton and Rosetta space probes as well as the two US Mars rovers Spirit and Opportunity.</p>
<p>Engineering model of an eROSITA mirror module X-ray astronomy &#8211; science par excellence</p>
<p>How is the eROSITA x-ray telescope going to be used to investigate dark energy, which is invisible and is only perceptible at vast distances? eROSITA will survey about 100 000 galaxy clusters, which are visible to the X-ray telescope through the radiation from the hot gas which has collected at their centres. Their distribution in space and its variation over time – we are, after all, looking at these objects in the past because of the finite speed of light – are the key to the analysis. Characteristics of dark energy can be derived, for example, from the way that its share in the energy density of the universe, which it dominates today at more than 70 percent, has changed in the course of cosmic evolution. Ultimately, these investigations lead to basic questions about our universe: How was it created? How old is it? What is its future?</p>
<p>Collision between two galaxy clusters Many different institutions and companies are contributing to finding the answers to such questions: the Max Planck Institutes for Extraterrestrial Physics and for Astrophysics, the Institute of Astronomy and Astrophysics of the University of Tübingen, the Potsdam Astrophysics Institute, the Hamburg University Observatory, the Dr Remeis Observatory in Bamberg, the German Aerospace Center, Roskosmos and the Space Research Institute in Moscow, Kayser-Threde GmbH, Carl Zeiss</p>
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