Abstract
The potential of laser-plasma-based accelerator technology for future advanced space radiation studies is investigated. Laser-plasma accelerators have been shown to be capable of robust generation of particle beams such as electrons, protons, neutrons and ions, as well as photons, having a wide range of accessible parameters. Further, instead of maximum accelerating fields of the order of MV/m as in state-of-the-art accelerators, laser-plasma acceleration operates with fields up to TV/m and can thus be used to reach as yet inaccessible parameter regimes, but which are very relevant to space radiation studies. Due to their versatility and compactness, the same laser-plasma- accelerator can be used in university-scale labs to generate different kinds of particle and photon beams, each yielding up to kGy doses per shot, and allowing combinations of different kinds of radiation production simultaneously. Laser-plasma-accelerators provide the advantage of cost-effective radiation generation, thus ameliorating the current shortage of beam time for testing of radiation resistivity of electronic components. Beyond this, laser-plasma-accelerators can be used to reproduce certain aspects of space radiation, e.g. broad, decreasing multi-MeV-scale spectra, with substantially improved level of fidelity, as compared to state-of-the-art technology. This can increase the significance of electronic components testing, and in turn yield increased reliability and safety of future manned or unmanned space missions, high-altitude flights, as well as the electronic components used in harsh radiation environments in general. Laser-plasma-accelerators may therefore become indispensable tools for next-generation space radiation studies.
Original language | English |
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Pages (from-to) | 31-40 |
Number of pages | 10 |
Journal | Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |
Volume | 636 |
Issue number | 1 |
DOIs | |
Publication status | Published - 21 Apr 2011 |
Funding
We would like to thank E. Daly and V. Ferlet-Cavrois/ESA, and S. Metzger, J. Kuhnhenn and S. Höffgen at the Fraunhofer INT, Euskirchen, Germany, and L.Z. Scheick, R.D. Harris and S. McClure/NASA, for fruitful discussions, and H.-F. Chen, Institute of Space Physics and Applied Technology, Peking University, PRC, for KuaFu-B particle flux data. This work has been supported by the Strategischer Forschungsfonds, Heinrich-Heine-University Düsseldorf, by the DFG SFB TR18, and by ESA's Networking/Partnering Initiative (NPI).
Keywords
- laser-plasma-acceleration
- space radiation