Present and Future Observing Trends in Atmospheric Magnetoseismology

By D. Banerjee, R. Erdélyi, R. Oliver, E. O'Shea. 2007

206 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/4bd8dd6ccd9871f2c999741544a8a27d2a05f566

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

Citations in the corpus

Physics of Solar Prominences: II—Magnetic Structure and Dynamics (2010, background): “More detailed information about observations of small amplitude oscillations in filaments and prominences can be found in Engvold (2001, 2004, 2008), Oliver and Ballester (2002), and Banerjee et al. (2007).”
Standing Slow-Mode Waves in Hot Coronal Loops: Observations, Modeling, and Coronal Seismology (2010, background): “Various periodic and quasi-periodic oscillations in radio, visible, EUV, and soft X-rays have been observed for decades (e.g. reviews by Aschwanden 2003, 2004a; Wang 2004; Banerjee et al. 2007).”
Alfvén Waves in the Solar Atmosphere (2012, background): “Indeed, SUMER observations have shown a centre to limb increase in the non-thermal line widths of upper chromospheric and TR lines, while the excess broadening of coronal lines is only marginal (see e.g. Erdélyi et al. 1998; Banerjee et al. 2007 and references therein).”
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “Interested readers are referred to relevant reviews (Aschwanden, 2004; Nakariakov and Verwichte, 2005; Banerjee et al., 2007; Roberts, 2008; Ofman, 2009) and recent AIA observations (e.g. Aschwanden and Schrijver, 2011; McIntosh et al., 2011; Wang et al., 2012; Gosain and Foullon, 2012; White and…”
Effect of longitudinal magnetic and density inhomogeneity on transversal coronal loop oscillations (2008, methodology): “…loop oscillations observed by high-resolution EUV imager onboard the Transition Region And Coronal Explorer (TRACE) have provided valuable data to probe the plasma fine structure of the corona by implementing magneto-seismological techniques (see Banerjee et al. 2007, for the latest review).”
CORONAL LOOP OSCILLATIONS OBSERVED WITH ATMOSPHERIC IMAGING ASSEMBLY—KINK MODE WITH CROSS-SECTIONAL AND DENSITY OSCILLATIONS (2011, background): “…and observations of coronal seismology can be found in Roberts & Nakariakov (2003), Erdelyi et al. (2003), Roberts (2004), Aschwanden (2004, 2006), Wang (2004), Nakariakov & Verwichte (2005), Banerjee et al. (2007), Andries et al. (2009), Ruderman & Erdelyi (2009), and Taroyan & Erdelyi (2009).”
TIME–DISTANCE SEISMOLOGY OF THE SOLAR CORONA WITH CoMP (2009, background): “Such investigations of the coronal magnetic structure and plasma environment, in the limit of MHD, has been dubbed coronal seismology (e.g., Aschwanden 2003; Nakariakov & Verwichte 2005; Banerjee et al. 2007).”
Quasi-Periodic Pulsations in Solar Flares (2009, methodology): “…to coronal waves and oscillations is mainly connected with the possible role played by them in the heating of the coronal plasma (e.g. Erdélyi and Ballai 2007), and with the use of them as natural probes for the plasma diagnostics (e.g. Nakariakov and Verwichte 2005; Banerjee et al. 2007).”