7 research outputs found
The LISA PathFinder DMU and Radiation Monitor
The LISA PathFinder DMU (Data Management Unit) flight model was formally
accepted by ESA and ASD on 11 February 2010, after all hardware and software
tests had been successfully completed. The diagnostics items are scheduled to
be delivered by the end of 2010. In this paper we review the requirements and
performance of this instrumentation, specially focusing on the Radiation
Monitor and the DMU, as well as the status of their programmed use during
mission operations, on which work is ongoing at the time of writing.Comment: 11 pages, 7 figures, prepared for the Proceedings of the 8th
International LISA Symposium, Classical and Quantum Gravit
Galactic cosmic-ray energy spectra and expected solar events at the time of future space missions
none8sìAccepted for publicationopenGrimani, Catia; Araujo, H. M.; Fabi, M.; Lobo, A.; Mateos, I.; Shaul, D. N. A.; Sumner, T. J.; Wass, P.Grimani, Catia; Araujo, H. M.; Fabi, M.; Lobo, A.; Mateos, I.; Shaul, D. N. A.; Sumner, T. J.; Wass, P
LISA and LISA PathFinder, the endeavour to detect low frequency GWs
This is a review about LISA and its technology demonstrator, LISA PathFinder.
We first describe the conceptual problems which need to be overcome in order to
set up a working interferometric detector of low frequency Gravitational Waves
(GW), then summarise the solutions to them as currently conceived by the LISA
mission team. This will show that some of these solutions require new
technological abilities which are still under development, and which need
proper test before being fully implemented. LISA PathFinder (LPF) is the the
testbed for such technologies. The final part of the paper will address the
ideas and concepts behind the PathFinder as well as their impact on LISA.Comment: 25 pages, 21 figures, presented at the Spanish Relativity Meeting,
Mallorca September 2006. Will be published in Journal of Physics: Conference
Series, IOP. To be published in Journal of Physics: Conference Series, IO
The diagnostics subsystem on board LISA PathFinder and LISA
The Data and Diagnostics Subsystem of the LTP hardware and software are at
present essentially ready for delivery. In this presentation we intend to
describe the scientific and technical aspects of this subsystem, which includes
thermal diagnostics, magnetic diagnostics and a Radiation Monitor, as well as
the prospects for their integration within the rest of the LTP. We also sketch
a few lines of progress recently opened up towards the more demanding
diagnostics requirements which will be needed for LISA.Comment: 11 pages, 5 figures, pdflatex, prepared for the Proceedings of the
7th International LISA Symposium (Barcelona, Spain, 16-20 June-2008),
submitted to Classical and Quantum Gravit
Galactic cosmic-ray energy spectra and expected solar events at the time of future space missions
International audienceGalactic cosmic-rays (GCRs) and solar energetic particles (SEPs) affect observations on board long-lived space missions. We developed a parameterization of proton and helium fluxes for various levels of solar modulation during opposite polarity periods. In addition to long-term variations (decades), short-term fluctuations (minutes to days) were considered as well. In particular, we focused on data from experiments carrying magnetic spectrometers in space. The shortest GCR variations we were able to study are of the order of hours. We point out that GCR variations and fluctuations are strongly energy dependent . Energy dependent is also the detector charging on board space experiments. The measurements of energy differential fluxes and their variations are needed in order to evaluate properly the performance of future space missions. We present here the projections for the GCR fluxes and solar events at the time of LISA (Laser Interferometer Space Antenna) Pathfinder (LISA-PF)