Solar and cosmic ray physics and the space environment: Studies for and with LISA

D. N.A. Shaul, K. L. Aplin, H. Araújo, R. Bingham, J. B. Blake, G. Branduardi-Raymont, S. Buchman, A. Fazakerley, L. S. Finn, L. Fletcher, A. Glover, C. Grimani, M. Hapgood, B. Kellet, S. Matthews, T. Mulligan, W. T. Ni, P. Nieminen, A. Posner, J. J. QuenbyP. Roming, H. Spence, T. Sumner, H. Vocca, P. Wass, P. Young

Research output: Contribution to journalArticlepeer-review

25 Scopus citations


With data analysis preparations for LISA underway, there has been renewed interest in studying solar, cosmic ray and environmental physics for, and using LISA. The motivation for these studies is two fold. The primary incentive is to predict and consequently minimize the impact of disturbances associated with these factors, to maximize LISA's gravitational wave scientific yield. The second stimulus is the unique opportunity that is afforded by LISA's long-baseline 3-spacecraft configuration for studies of solar, cosmic ray and environmental physics. Here we present an overview of recent progress in these studies.

Original languageEnglish (US)
Pages (from-to)172-178
Number of pages7
JournalAIP Conference Proceedings
StatePublished - 2006

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy


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