Quiet-Sun inter-network magnetic fields observed in the infrared
By E. Khomenko, Manel Collados, S. Solanki, A. Lagg, J. T. Bueno. 2003
151 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/867397c3b76dd2ace303202774e5ac7d7839f236
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In Astronomy and Astrophysics
Citations in the corpus
- A solar surface dynamo (2007, methodology): “…observations based upon different methods do not yet provide a fully consistent picture (e.g., Lin & Rimmele, 1999; Sánchez Almeida & Lites, 2000; Khomenko et al., 2003; Sánchez Almeida et al., 2003; Domínguez Cerdeña et al., 2003; Lites & Socas-Navarro, 2004; Domínguez Cerdeña et al., 2006a,b;…”
- Magnetic Fields in the Solar Convection Zone (2004, background): “…a hierarchy of cross-sectional sizes that range from sunspots of active regions down to below the limit of observational resolution (see Zwaan, 1987; Stenflo, 1989; Domı́nguez Cerdeña et al., 2003; Khomenko et al., 2003; Socas-Navarro and Sánchez Almeida, 2003; Orozco Suárez et al., 2007).”
- NUMERICAL SIMULATIONS OF QUIET SUN MAGNETISM: ON THE CONTRIBUTION FROM A SMALL-SCALE DYNAMO (2014, background): “…on the solar surface and provides the dominant contribution to the magnetic energy in the quiet Sun photosphere (see, e.g., Lites et al. (1996); Khomenko et al. (2003); Domı́nguez Cerdeña et al. (2003); Sánchez Almeida (2003); Trujillo Bueno et al. (2004); Domı́nguez Cerdeña et al. (2006);…”
- Emergence of Small-Scale Magnetic Loops in the Quiet-Sun Internetwork (2007, background): “…& Lites (2000), Domı́nguez Cerdeña et al. (2003)), other work suggests the predominance of weak magnetic fields (Lin (1995), Lin & Rimmele (1999), Khomenko et al (2003)) in the range of 300-500 G. Manso Sainz et al (2004) have reported the detection of an ubiquotous unresolved turbulent…”