Catalogue of the 1997 SOHO–EIT coronal transient waves and associated type II radio burst spectra

By A. Klassen, H. Aurass, G. Mann, Barbara J. Thompson. 2000

192 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/d350605c9381d97dd412bcab6de085c9597de07b

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In Astronomy and Astrophysics

1. B. Vršnak
2. Nat Gopalswamy
3. A. Vourlidas
4. Jasmina Magdalenic
5. R. Howard
6. M. Temmer
7. P. Chen
8. W. Manchester IV

In Geophysics

1. P. Chen
2. Nat Gopalswamy
3. W. Otruba
4. Kazunari Shibata
5. Cheng Fang
6. A. Warmuth
7. Jasmina Magdalenic
8. A. Hanslmeier

Citations in the corpus

• Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection? (2007, unknown): “Since the mean EIT wave speed (Klassen et al. 2000) exceeds the sound speed in the corona and the intrinsic characteristics of a fast-mode shock are capable of producing brightening in EUV images, authors such as Wang (2000), Ofman & Thompson (2002), Warmuth et al. (2004b, and references therein),…”
• Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “90% of the type IIs during 1997 were associated with EIT waves (Klassen et al., 2000), while only 29% of the 173 EIT waves from 1997-Mar to 1998-Jun were associated with Type IIs, with somewhat higher correlation rates at disk center and the limb than at intermediate longitudes (Biesecker et al.,…”
• A Global Picture of CMEs in the Inner Heliosphere (2004, background): “Phenomena such as CME-related dimming (Hudson, 1999; Gopalswamy, 1999; Gopalswamy and Thompson, 2000; Klassen et al., 2000), and EUV wave transients (Thompson et al., 1999; Gopalswamy and Thompson, 2000; Mann et al., 1999; Biesecker et al., 2002), and arcade formation (Hanaoka, 1994; Gopalswamy et…”
• Evolution of Two EIT/Hα Moreton Waves (2001, background): “Both Mann et al. (1999; also discussed in Klassen et al. 2000) and Wang (2000) find fast-mode speeds of a few hundred kilometers per second in the low corona outside of active regions.”
• The Coronal Mass Ejection of 1998 April 20: Direct Imaging at Radio Wavelengths (2001, background): “…bursts, type IV bursts, 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;…”
• Evidence of EIT and Moreton Waves in Numerical Simulations (2002, methodology): “These authors suggested that the EIT waves are simply the coronal counterparts of chromospheric Moreton waves, although the velocities of the latter are generally 2–3 times larger (Smith & Harvey 1971; Klassen et al. 2000).”
• NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “The first group of models describes coronal waves as a pure MHD wave, either a: fastmode (e.g. Thompson et al. 1999; Klassen et al. 2000; Vršnak et al. 2002; Cliver et al. 2004; Warmuth et al. 2004b), slow-mode (Krasnoselskikh & Podladchikova 2007; Wang et al. 2009), or a slow-mode solitary wave…”
• A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation (2004, background): “…is 〈v̄II〉 = 1101± 222 km s−1, which is significantly higher than the typical type II velocities (e.g. Robinson et al. 1985 found 〈v̄II〉 = 764±65 km s−1) and also higher than the average velocity of type II bursts that are associated with EIT waves, given by Klassen et al. (2000) as 739 km s−1.”
• Direct Detection of a Coronal Mass Ejection-Associated Shock in Large Angle and Spectrometric Coronagraph Experiment White-Light Images (2003, background): “They are comparable to shock speeds deduced frommetric type II bursts (e.g., Klassen et al. 2000) and are similar to the measured speeds for the 1980 July 6 white-light shock candidate (Sime & Hundhausen 1987).”
• Formation and development of shock waves in the solar corona and the near-Sun interplanetary space (2003, methodology): “7 the start frequency versus the radial velocity of type II radio burst sources is given for the sample of events considered by Klassen et al. (2000).”
• Solar Phenomena Associated with “EIT Waves” (2002, methodology): “However, the relatively strong correlation between EIT waves at small and large longitudes and type II events would appear to be consistent with the results of Klassen et al. (2000).”
• A multiwavelength study of solar flare waves. I. Observations and basic properties (2004, background): “Based on these velocities, we can conclude that the EIT waves of Klassen et al. (2000) belong to the same class of events as the EIT waves presented in this study.”
• OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, background): “Klassen et al. (2000) made a statistical study of type II bursts and found that 90% are associated with an EUV wave.”