Solar and Stellar Magnetic Activity: Bibliography
By C. Schrijver, C. Zwaan. 2000
216 citations recorded by the source corpus.
Subfields: History, Literature and Literary Theory, Sociology and Political Science
View Paper: https://www.semanticscholar.org/paper/405dba1b7f3f36d840de5cd780b3e27394829d94
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Citations in the corpus
- What Is Missing from Our Understanding of Long-Term Solar and Heliospheric Activity? (2002, background): “Upon emergence onto the solar surface, magnetic field organizes itself into tubelike concentrations with an intrinsic field strength of about 1–2 kG (see Schrijver & Zwaan 2000).”
- The Origin of T Tauri X-Ray Emission: New Insights from the Chandra Orion Ultradeep Project (2005, background): “…of the rather complicated processes by which this dynamo generates surface magnetic fields can be summarized as follows (for details see, e.g., Schrijver & Zwaan 2000; Ossendrijver 2003): The strong differential rotation in the tachocline, a region near the bottom of the convection zone in…”
- MAGNETIC CYCLES IN A CONVECTIVE DYNAMO SIMULATION OF A YOUNG SOLAR-TYPE STAR (2011, background): “Observations re- veal a clear correlation between rotation and magnetic activity, as inferred from proxies such as X-ray and chromospheric emission (Schrijver & Zwaan 2000; Pizzolato et al. 2003), but the observational landscape is complex with few other wellestablished trends to constrain dynamo…”
- Simulations of the Photospheric Magnetic Activity and Outer Atmospheric Radiative Losses of Cool Stars Based on Characteristics of the Solar Magnetic Field (2001, background): “Equation (7) holds for all stars of roughly Sun-like activity and above ; the less active stars appear to deviate somewhat (see Schrijver & Zwaan 2000 for a discussion of deviations from the rotation-activity relationship).”
- SIMULATION OF THE FORMATION OF A SOLAR ACTIVE REGION (2010, background): “Observations of active regions on the solar surface indicate that, in terms of magnetic flux content, there is a continuous spectrum of active region sizes (Zwaan 1978, 1987; Harvey & Martin 1973; Schrijver & Zwaan 2000; Hagenaar 2001; Hagenaar et al. 2003).”
- The Internal Rotation of the Sun (2003, background): “Support for this comes from observed correlations between various measures of activity and properties of stellar rotation and convection (e.g., Hartmann & Noyes 1987, Schrijver & Zwaan 2000).”