Slow magnetoacoustic waves in coronal loops: EIT and TRACE

By E. Robbrecht, Erwin Verwichte, D. Berghmans, J. Hochedez, Stefaan Poedts, Valery M. Nakariakov. 2001

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/e0acfab6a29778981558e4639fb17a360a11ad90

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Citations in the corpus

Hot Coronal Loop Oscillations Observed by SUMER: Slow Magnetosonic Wave Damping by Thermal Conduction (2002, background): “Signatures of slow magnetosonic waves were also observed in EUV in cool coronal loops (Berghmans & Clette 1999) and identified as propagating slow waves (Nakariakov et al. 2000; De Moortel, Ireland, & Walsh 2000; Robbrecht et al. 2001; De Moortel et al. 2002a, 2002b).”
The Solar Orbiter EUI instrument: The Extreme Ultraviolet Imager (2020, background): “Faint coronal features such as disturbances in loops (flows or waves) or eruptions (off-limb, EIT waves) are typically at 10% of the background intensity (Robbrecht et al. 2001; Thompson & Myers 2009).”
Hot coronal loop oscillations observed with SUMER: Examples and statistics (2003, background): “…offprint requests to: T.J. Wang nal loops by the EUV Imaging Telescope (EIT) (Berghmans & Clette 1999), later confirmed by TRACE observations (De Moortel et al. 2000; 2002a;b;c; Robbrecht et al. 2001), and identified as propagating slow waves (Nakariakov et al. 2000; Tsiklauri & Nakariakov 2001).”
Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “…was the slowly-propagating waves of EUV emission disturbances in polar plumes (Ofman et al. 1997, 1999; DeForest and Gurman 1998), in the inter-plume regions (Banerjee et al. 2001), and near footpoints of long coronal loops and fan-like structures (Berghmans and Clette 1999; Robbrecht et al. 2001).”
Transverse Oscillations of Coronal Loops (2009, unknown): “As a specific example, let as recall an interesting earlier observation by Robbrecht et al. (2001): combined data of May 13 1998 from both the 19 EIT instrument on SOHO and from TRACE show the simultaneous observation of two slow magnetosonic waves propagating along a perceived coronal loop with…”
Line-of-sight effects on observability of kink and sausage modes in coronal structures with imaging telescopes (2002, unknown): “These observational breakthroughs give rise to the use of MHD coronal seismology (Nakariakov et al. 1999; Robbrecht et al. 2001; Nakariakov & Ofman 2001) and were interpreted to support the idea of wavebased theories of coronal heating (e.g., Tsiklauri & Nakariakov 2001), and the solar wind…”
How to Channel Photospheric Oscillations into the Corona (2005, background): “…have been conclusively identified as upward-propagating longitudinal magnetoacoustic waves with propagation speeds of 122 44 km s 1 and intensity variations of 4.1% 1.5% of the background brightness of the loop (Schrijver et al. 1999; Robbrecht et al. 2001; De Moortel et al. 2002a, 2002b).”
The Damping of Coronal Loop Oscillations (2002, background): “Finally, we note that propagating compressive waves have also been detected in coronal loops (Berghmans & Clette 1999; De Moortel, Ireland, & Walsh 2000; Robbrecht et al. 2001; O’Shea et al. 2001) and in polar plumes (Ofman et al. 1997; Ofman, Nakariakov, & DeForest 1999; DeForest & Gurman 1998).”
The detection of 3 & 5 min period oscillations in coronal loops (2002, methodology): “Robbrecht et al. (2001) compare propagating disturbances in coronal loops, observed on 13th May 1998, in the TRACE 171 Å and EIT (SOHO) 195 Å passbands.”
Coronal Waves and Oscillations (2005, background): “, 1999), and to probe coronal sub-resolution structuring (Robbrecht et al., 2001; King et al., 2003).”