No CrossRef data available.
Article contents
Towards observational MHD. Advances in spectropolarimetry and the prospects for the E-ELT
Published online by Cambridge University Press: 08 June 2011
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Polarization and wavelength are the bits of information attached to every photon that reveal the most about its formation and subsequent history. The E-ELT will, for the foreseeable future, be the most powerful optical light-collecting machine ever built. The strength of its combination, spectropolarimetry with the E-ELT, is the anchorage in physics of astronomical observations. I present a strawman design of a spectropolarimeter for its intermediate focus.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 274 - 279
- Copyright
- Copyright © International Astronomical Union 2011
References
Baade, D., Wang, L., Hubrig, S., & Patat, F. 2006, in IAU Symp. 232, CUP, p.248CrossRefGoogle Scholar
Beck, R. 2010, in “Astronomy with Megastructures. Joint Science with E-ELT and SKA”, arXiv:1008.3806Google Scholar
Boehnhardt, H., Tozzi, G. P., Sterzik, M. et al. . 2009, Earth, Moon & Planets, 105, 95CrossRefGoogle Scholar
Carroll, T. A., Strassmeier, K. G., Ilyin, I., & Rice, J. B. 2011, in IAU Symp. 273, CUP, in pressGoogle Scholar
Feinstein, C., Vergne, M. M., Martinez, R., & Orsatti, A. M. 2008, MNRAS 391, 447CrossRefGoogle Scholar
Hubrig, S., Grady, C., Schöller, M. et al. . 2009, in IAU Symp. 259, CUP, p.395CrossRefGoogle Scholar
Johns-Krull, C., Greene, T. P., Doppmann, G. W., & Covey, K. R. 2009, ApJ 700, 1440CrossRefGoogle Scholar
Laux, U., Klose, S., & Greiner, J. 2009, poster at the fall meeting of the AG 2009, PotsdamGoogle Scholar