Showing 1–20 of 32 results
/ Date/ Name
Sep 3, 2012Polarized line formation with J-state interference in the presence of magnetic fields: A heuristic treatment of collisional frequency redistributionAug 31, 2012Polarized line transfer with F-state interference in a non-magnetic medium: Partial frequency redistribution effects in the collisionless regimeMar 28, 2009Measuring the Hidden Aspects of Solar MagnetismDec 24, 2008Small-scale solar magnetic fieldsJul 3, 2013Calibration of the 6302/6301 Stokes V line ratio in terms of the 5250/5247 ratioSep 1, 2014The role of quantum interference and partial redistribution in the solar Ba II D2 4554 A lineAug 10, 2017Atlas of the solar intensity spectrum and its center to limb variationDec 24, 2015Polarized scattering of light for arbitrary magnetic fields with level-crossings from the combination of hyperfine and fine structure splittingsMar 29, 2013Modeling the quantum interference signatures of the Ba II D2 4554 A line in the second solar spectrumSep 29, 2012Basal magnetic flux and the local solar dynamoOct 24, 2019Polarized Line Formation in Arbitrary Strength Magnetic Fields: the case of a two-level atom with hyperfine structure splittingMar 9, 2018Spatial variations of the Sr i 4607 Å scattering polarization peakFeb 14, 2005Absence of linear polarization in Halpha emission of solar flaresDec 19, 2015Transition of the Sunspot Number from Zurich to Brussels in 1980: A Personal PerspectiveAug 19, 2014The quantum interference effects in the Sc II 4247 A line of the Second Solar SpectrumJul 8, 2020Importance of Angle-dependent Partial Frequency Redistribution in Hyperfine Structure Transitions Under Incomplete Paschen-Back Effect RegimeJun 12, 2009Solar Research Programs at IRSOL, SwitzerlandDec 22, 2011Bipolar Magnetic Regions on the Sun: Global Analysis of the SOHO/MDI Data SetDec 24, 2015Polarized scattering with Paschen-Back effect, hyperfine structure, and partial frequency redistribution in magnetized stellar atmospheresApr 23, 2007Are "EIT Waves" Fast-Mode MHD Waves?