Multilevel Radiative Transfer with Partial Frequency Redistribution

By H. Uitenbroek. 2001

372 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/fb4eddb41293e72e54bba7a527215a7178f7f008

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. J. Leenaarts
2. M. Carlsson
3. N. Krivova
4. James R. A. Davenport
5. S. Solanki
6. Bart De Pontieu
7. L. R. V. Voort
8. A. Kowalski

In Atmospheric Science

1. M. Carlsson
2. J. Leenaarts
3. Rudolf Loeser
4. E. Avrett
5. A. Kowalski
6. S. Solanki
7. N. Krivova
8. J. Allred

In Global and Planetary Change

1. M. Carlsson
2. J. Leenaarts
3. Rudolf Loeser
4. E. Avrett
5. A. Kowalski
6. J. Allred
7. L. R. V. Voort
8. T. Pereira

Citations in the corpus

• Models of the Solar Chromosphere and Transition Region from SUMER and HRTS Observations: Formation of the Extreme-Ultraviolet Spectrum of Hydrogen, Carbon, and Oxygen (2008, methodology): “See also Uitenbroek (2001).”
• Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “Chromospheric densities experience a significant decrease from their corresponding photospheric counterparts, and as a result radiative transition rates generally dominate over collisional rates (Uitenbroek and Briand 1995; Uitenbroek 1997, 2001, 2002).”
• Recent variability of the solar spectral irradiance and its impact on climate modelling (2012, background): “…atmospheric models with different degrees of complexity is available (e.g. Kurucz, 1993; Fontenla et al., 1999, 2009, 2011; Unruh et al., 1999; Penza et al., 2004; Uitenbroek, 2001; Kurucz, 2005; Avrett and Loeser, 2008; Shapiro et al., 2010), most of1040 which go back to Vernazza et al. (1981).”
• A UNIFIED COMPUTATIONAL MODEL FOR SOLAR AND STELLAR FLARES (2015, methodology): “In using this method, we are consistent with other NLTE radiative transfer codes such as RH (Uitenbroek 2001).”
• Solar Fine-Scale Structures. I. Spicules and Other Small-Scale, Jet-Like Events at the Chromospheric Level: Observations and Physical Parameters (2012, methodology): “There already exist several 1D-geometry radiative codes, such as MULTI (Carlsson, 1986), MALI (Heinzel, 1995) and RH (Uitenbroek, 2001, the 1D version) that compute the radiative transfer problem in plane parallel atmospheres, using atoms containing several or even hundreds of levels and/or…”
• THE FORMATION OF IRIS DIAGNOSTICS. II. THE FORMATION OF THE Mg ii h&k LINES IN THE SOLAR ATMOSPHERE (2013, methodology): “…radiative transfer computations using the 4-level-plus-continuummodel atom from paper I with two different codes: The first is a version ofRH by Uitenbroek (2001), modified to use MPI so it can efficiently solve the radiative transfer in all columns in the 3D model atmosphere assuming each…”
• THE FORMATION OF THE Hα LINE IN THE SOLAR CHROMOSPHERE (2012, methodology): “Multi3d employs the accelerated lambda iteration method developed by Rybicki & Hummer (1992) with the extension to treat effects of partial frequency redistribution using the angle-averaged approximation by Uitenbroek (2001).”
• TIME-RESOLVED PROPERTIES AND GLOBAL TRENDS IN dMe FLARES FROM SIMULTANEOUS PHOTOMETRY AND SPECTRA (2013, methodology): “Kowalski et al. (2011a) used the static, NLTE RH code (Uitenbroek 2001) to model the secondary heating events during the “Megaflare” in Kowalski et al. (2010).”