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Final Report Summary - SKYFLASH (Development of Rad Hard non volatile Flash memories for space applications)
Executive Summary:SkyFlash has been focused on the development of a strong rad-hard by design (RHBD) methodology for non volatile semiconductor memories to be used in space applications taking the best from standard CMOS (Complementary Metal-Oxide Semiconductor field effect...
Programme: FP7-SPACE
Record Number: 149212
Last updated on: 2014-11-28
Development of Rad Hard non volatile Flash memories for space applications
ID: 262890
Start date: 2011-09-01, End date: 2014-02-28
The project aims to realise a strong methodology for the development and design of non volatile memories usign standard CMOS silicon process actually used for consumer electronics. Since standard silicon memories, such as other silicon devices for consumer market, fails under...
Programme: FP7-SPACE
Record Number: 100082
Last updated on: 2017-05-26
Kwestia odporności na działanie promieniowania wkracza w erę kosmiczną
Ze względu na brak ochronnego działania pola magnetycznego Ziemi układy elektroniczne do zastosowań kosmicznych muszą być odporne na działanie różnego rodzaju promieniowania. Prototypowa technologia opracowywana właśnie przez naukowców finansowanych ze środków UE stanowi obiet...
Programme: FP7-SPACE
Record Number: 147131
Last updated on: 2014-08-27
Available languages: DE, EN, ES, FR, IT, PL
Radiation hardening joins the space age
Operating without the protection of the Earth's magnetic field, electronics built for space applications must be resilient to various types of radiation. Now, prototype technology developed by EU-funded researchers promises to make flash memories tolerant of ionising radiation.
Programme: FP7-SPACE
Record Number: 147131
Last updated on: 2014-08-27
Available languages: DE, EN, ES, FR, IT, PL
Strahlungshärtung im Weltraumzeitalter
Da sie außerhalb des Erdmagnetfeldes arbeiten, müssen elektronische Geräte für Weltraumanwendungen gegen verschiedene Arten von Strahlung geschützt werden. Der Prototyp einer neuen, von EU-finanzierten Forschern entwickelten Technologie soll Flash-Speicher widerstandsfähig geg...
Programme: FP7-SPACE
Record Number: 147131
Last updated on: 2014-08-27
Available languages: DE, EN, ES, FR, IT, PL
La resistenza alle radiazioni approda nell’era spaziale
Per poter funzionare senza la protezione del campo magnetico terrestre, i dispositivi elettronici per applicazioni spaziali devono essere resilienti a vari tipi di radiazioni. Oggigiorno, i prototipi di flash memory sviluppati dai ricercatori finanziati dall’UE sono tolleranti...
Programme: FP7-SPACE
Record Number: 147131
Last updated on: 2014-08-27
Available languages: DE, EN, ES, FR, IT, PL
El endurecimiento frente a la radiación entra en la era espacial
Al funcionar sin la protección del campo magnético terrestre, los sistemas electrónicos destinados a las aplicaciones espaciales deben ser resistentes a diversos tipos de radiación. A partir de ahora, la tecnología desarrollada a nivel de prototipo por un equipo de investigado...
Programme: FP7-SPACE
Record Number: 147131
Last updated on: 2014-08-27
Available languages: DE, EN, ES, FR, IT, PL
Le durcissement aux radiations entre dans l'ère spatiale
L'électronique utilisée dans l'espace est privée de la protection du champ magnétique de la Terre, et doit donc résister à divers types de rayonnement. Aujourd'hui, une technique prototype développée par des chercheurs financés par l'UE devrait rendre les mémoires flash toléra...
Programme: FP7-SPACE
Record Number: 147131
Last updated on: 2014-08-27
Available languages: DE, EN, ES, FR, IT, PL
Clearing the thin line between central neutron star and black hole formation
There is still much we don’t know about the last stages of stellar evolution, particularly the point at which a star is massive enough to generate a black hole in its final collapse. With his ERC grant under the FISH project, Prof. Friedrich Thielemann has set out to fill this...
Programme: FP7-IDEAS-ERC
Record Number: 205485
Last updated on: 2017-10-31
Available languages: DE, EN, ES, FR, IT, PL
Neutronenstern oder Schwarzes Loch – was entsteht, wenn Sterne kollabieren?
Was in den Spätphasen der Sternentwicklung passiert, ist noch nicht vollkommen erforscht, besonders dann, wenn er massereich genug ist, um zu einem Schwarzen Loch zu kollabieren. Diese Wissenslücke sollte Prof. Friedrich Thielemann nun mit einem ERC-Stipendium im Rahmen des Pr...
Programme: FP7-IDEAS-ERC
Record Number: 205485
Last updated on: 2017-10-31
Available languages: DE, EN, ES, FR, IT, PL
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List retrieved on: 2018-01-23
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