On the Relation of G-Band Bright Points to the Photospheric Magnetic Field

By T. Berger, A. Title. 2001

161 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/54ef50e8d9dd3f21a998ca7792f26fa5220af5e0

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In Astronomy and Astrophysics

1. A. A. Ballegooijen
2. S. Cranmer
3. S. Saar
4. E. DeLuca
5. Mahboubeh Asgari-Targhi
6. Y. Suematsu
7. G. Verth
8. M. Madjarska

In Molecular Biology

1. Y. Suematsu
2. G. Verth
3. M. Madjarska
4. J. Doyle
5. G. Tsiropoula
6. S. Saar
7. S. Cranmer
8. I. Kontogiannis

Citations in the corpus

• HEATING OF THE SOLAR CHROMOSPHERE AND CORONA BY ALFVÉN WAVE TURBULENCE (2011, background): “Observations show that the photospheric magnetic field outside sunspots is highly intermittent and is concentrated into small flux elements or “flux tubes” with kilogauss field strengths and widths of a few 100 km (Stenflo 1989; Berger & Title 2001).”
• ORBITAL MOTION OF HR 8799 b, c, d USING HUBBLE SPACE TELESCOPE DATA FROM 1998: CONSTRAINTS ON INCLINATION, ECCENTRICITY, AND STABILITY (2011, background): “Bright features, visible in the dark inter-granule lanes, are called bright points (BPs) and they are thought to be footpoints of magnetic flux tubes (e.g., Muller et al. 2000; Berger & Title 2001; Ishikawa et al. 2007, to mention a few).”
• Solar Fine-Scale Structures. I. Spicules and Other Small-Scale, Jet-Like Events at the Chromospheric Level: Observations and Physical Parameters (2012, background): “…the magnetic elements, extensive work has been initiated and it is now well established that NBPs are brightness manifestations of the small, strong field magnetic elements that make up the magnetic network (Muller and Roudier, 1984; Berger and Title, 1996, 2001; Rouppe van der Voort et al., 2005).”
• TESTING A PREDICTIVE THEORETICAL MODEL FOR THE MASS LOSS RATES OF COOL STARS (2011, background): “For the well-observed case of the Sun, we know that most of the photospheric magnetic field is concentrated into small (100–200 km diameter) flux tubes concentrated in the intergranular downflow lanes (Solanki 1993; Berger & Title 2001).”
• Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “The spicules are observed to be rooted in MBPs found in G-band images, which correspond to strong regions of magnetic field (Berger and Title 2001; Jess et al. 2010c).”
• On the Generation, Propagation, and Reflection of Alfvén Waves from the Solar Photosphere to the Distant Heliosphere (2004, background): “…X-ray bright points in the low corona (e.g., Golub et al. 1977; Parnell 2002). of strong (1–2 kG) magnetic field believed to be contained within nearly vertical flux tubes (e.g., Sheeley 1967; Dunn & Zirker 1973; Muller 1983, 1985; Piddington 1978; Rabin 1992; Solanki 1993; Berger & Title 2001).”
• Hall magnetohydrodynamics of partially ionized plasmas (2007, background): “For a field > 102 G (a field probably present in the network, internetwork, plague and sunspot Berger & Title (2001); Domnguez et al. (2003)) even at h = 0 Hall will be the dominant mechanism.”