Another View of the EIT Wave Phenomenon

By C. Delannée. 2000

145 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/a51d753fd9aafe4eee406ddcfc3c95c99bbe51d2

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

1. B. Vršnak
2. A. Zhukov
3. F. Auchère
4. Jasmina Magdalenic
5. W. Manchester IV
6. P. Chen
7. A. Hanslmeier
8. W. Otruba

In Geophysics

1. W. Otruba
2. A. Zhukov
3. Kazunari Shibata
4. F. Auchère
5. P. Chen
6. Cheng Fang
7. A. Warmuth
8. Jasmina Magdalenic

In Molecular Biology

1. A. Zhukov
2. F. Auchère
3. B. Vršnak
4. W. Manchester IV
5. Kazunari Shibata
6. P. Chen
7. A. Vourlidas
8. G. Attrill

Citations in the corpus

• Evidence of EIT and Moreton Waves in Numerical Simulations (2002, background): “Furthermore, Delanne´e & Aulanier (1999) and Delanne´e (2000) pointed out that only three of 50 flares produced in the same active region were associated with EIT waves, indicating that flares are unlikely to be the primary cause of EIT waves.”
• On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, methodology): “The EIT wave appears as a result of successive opening of the field lines (cf. Delannée 2000; Delannée & Aulanier 1999) and thus is not a real MHD wave.”
• NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “Work by Delannée & Aulanier (1999); Delannée (2000); Delannée et al. (2008) attribute the regions of enhanced emission at low altitude to compression of the plasma between stable flux domains.”
• Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “…successive stretching of magnetic-field lines (Chen et al., 2002; Chen, Fang, and Shibata, 2005), Joule heating in current shells surrounding CMEs (Delannée, 2000; Delannée et al., 2008), sequential magnetic reconnection between CME flanks and the ambient corona with favorably-oriented field…”
• OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, background): “…2001; Ofman & Thompson 2002; Schmidt & Ofman 2010), slow-mode MHD waves (Wang et al. 2009), or non-waves related to a current shell or successive restructuring of field lines during the coronal mass ejection (CME; Delannée 2000; Delannée et al. 2008; Chen et al. 2002, 2005; Attrill et al. 2007).”
• A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation (2004, methodology): “could be generated by a mechanism like the one suggested by Delannée (2000), where the expanding magnetic field lines in a CME event interact with the surrounding field lines to produce compression of the plasma.”
• The Coronal Mass Ejection of 1998 April 20: Direct Imaging at Radio Wavelengths (2001, background): “…and continua; e.g., review by Pick 1999 and references therein), EUV (dimmings, Moreton waves; e.g., Thompson et al. 1999; Klassen et al. 2000; Delanne´e 2000), and soft X-ray (SXR) wavelengths (dimmings, morphological changes; e.g., Hudson et al. 1998; Zarro et al. 1999; Sterling et al.…”