Bernard Pontet
YOU?
Author Swipe
View article: Division réseau équitable dans les essaims de nanosatellites
Division réseau équitable dans les essaims de nanosatellites Open
International audience
View article: Resilient and Robust Strategies for Swarming Ad-hoc Networks
Resilient and Robust Strategies for Swarming Ad-hoc Networks Open
View article: First observations and performance of the RPW instrument on board the Solar Orbiter mission
First observations and performance of the RPW instrument on board the Solar Orbiter mission Open
The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is designed to measure in situ magnetic and electric fields and waves from the continuum up to several hundred kHz. The RPW also observes solar and heliospheric r…
View article: The Solar Orbiter Radio and Plasma Waves (RPW) instrument <i>(Corrigendum)</i>
The Solar Orbiter Radio and Plasma Waves (RPW) instrument <i>(Corrigendum)</i> Open
\n Contains fulltext :\n 239392.pdf (Publisher’s version ) (Open Access)\n
View article: The Solar Orbiter Radio and Plasma Waves (RPW) instrument
The Solar Orbiter Radio and Plasma Waves (RPW) instrument Open
The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is described in this paper. This instrument is designed to measure in-situ magnetic and electric fields and waves from the continuous to a few hundreds of kHz. RP…
View article: The Athena X-ray Integral Field Unit
The Athena X-ray Integral Field Unit Open
The X-ray Integral Field Unit (X-IFU) is the high resolution X-ray spectrometer of the ESA Athena X-ray observatory. Over a field of view of 5' equivalent diameter, it will deliver X-ray spectra from 0.2 to 12 keV with a spectral resolutio…
View article: The ATHENA x-ray integral field unit (X-IFU)
The ATHENA x-ray integral field unit (X-IFU) Open
The X-ray Integral Field Unit (X-IFU) is the high resolution X-ray spectrometer of the ESA Athena X-ray observatory. Over a field of view of 5' equivalent diameter, it will deliver X-ray spectra from 0.2 to 12 keV with a spectral resolutio…