Introduction to Spectropolarimetry

By J. C. D. T. Iniesta. 2003

207 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/d0a7d29d1617f6f978800fe60abf2dca1566e1b5

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Citations in the corpus

• Spectropolarimetry of Supernovae (2008, methodology): “The basic techniques of spectropolarimetry are presented by Miller & Goodrich (1990), Goodrich (1991), del Toro Iniesta (2003), and Patat & Romaniello (2006) (see also van de Hulst 1957).”
• Retrieval of the full magnetic vector with the He I multiplet at 1083 nm. Maps of an emerging flux region (2004, background): “…we have taken a somewhat more sophisticated approach that includes magnetooptical effects, the basics of radiative transfer (e.g. Jefferies et al. 1989; del Toro Iniesta 2003), as well as allowing for the Hanle effect in a simple manner, which, however, is adequate for the current data set.”
• The Imaging Magnetograph eXperiment (IMaX) for the Sunrise Balloon-Borne Solar Observatory (2010, background): “There are two complementary ways to minimize this effect, as explained,e.g., by Del Toro Iniesta (2003).”
• The Magnetic Landscape of the Sun's Polar Region (2008, background): “REFERENCES An, C.-H., Musielak, Z. E., Moore, R. L., & Suess, S. T. 1989, ApJ, 345, 597 Blanco Rodriguez, J., Okunev, O. V., Puschmann, K. G., Kneer, F., & SánchezAndrade Nuño, B. 2007, A&A, 474, 251 Cattaneo, F. 1999, ApJ, 515, L39 Centeno, R., et al. 2007, ApJ, 666, L137 Cirtain, J. W., et al. 2”
• Solar Force-free Magnetic Fields (2012, methodology): “Within this work we only outline the main steps and refer to del Toro Iniesta and Ruiz Cobo (1996), del Toro Iniesta (2003) and Landi Degl’Innocenti and Landolfi (2004) for details.”
• VFISV: Very Fast Inversion of the Stokes Vector for the Helioseismic and Magnetic Imager (2009, background): “, 2001) or Artificial Neural Networks (ANNs; Carroll and Staude, 2001; Socas-Navarro, 2003, 2005) could meet the HMI requirements with a very small number of CPUs.”