On the Formation of Polar Spots in Sun-like Stars

By C. Schrijver, A. Title. 2001

152 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/2cf5fb748781adbf51f81a01a82bdb453e3042a6

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In Astronomy and Astrophysics

1. S. Solanki
2. A. Title
3. C. Schrijver
4. M. Schüssler
5. J. Donati
6. M. Gudel
7. M. DeRosa
8. B. Inhester

Citations in the corpus

• Data Assimilation in the ADAPT Photospheric Flux Transport Model (2014, unknown): “As noted in the original WH model, [30] points out that the photospheric magnetic flux would disappear due to random cancellations in 2–3 days if the total magnetic flux was not renewed regularly.”
• Dust Dynamics, Surface Brightness Profiles, and Thermal Spectra of Debris Disks: The Case of AU Microscopii (2005, background): “10FM,⊙, perhaps because the strong magnetic fields of such extraordinarily X-ray-active stars inhibit stellar winds (see also Schrijver & Title 2001; Strassmeier 2002).”
• The solar magnetic field (2006, background): “Thus it is not surprising that both physical mechanisms proposed to explain the presence of high-latitude spots on rapid rotators [9, 10] are extrapolations to the relevant stellar parameters of mechanisms known to act on the Sun.”
• Dynamo processes and activity cycles of the active stars AB Doradus, LQ Hydrae and HR 1099 (2003, result): “In particular, our idea is not necessarily compatible with the recent model of Schrijver & Title (2001) trying to explain the formation of polar spots in Sun-like stars and predicting the formation of radial field rings around the pole, rather than that of azimuthal field rings at all latitudes…”
• Evolution of the large-scale magnetic field on the solar surface: a parameter study (2004, result): “Similar results have been found by Schrijver & Title (2001).”
• What Is Missing from Our Understanding of Long-Term Solar and Heliospheric Activity? (2002, methodology): “The model was demonstrated to accurately reproduce both geometric and quantitative properties of the last sunspot cycles (Schrijver 2001), including the polar regions (Schrijver & Title 2001).”
• The Sun in Time: Activity and Environment (2007, methodology): “Schrijver and Aschwanden (2002) used the model of surface magnetic-field development devised by Schrijver (2001) and Schrijver and Title (2001) (Section 4.1 above) to extrapolate surface magnetic fields into the corona, assuming a potential-field approach.”