Identification of Solar Sources of Major Geomagnetic Storms between 1996 and 2000

By Jie Zhang, K. Dere, R. Howard, Volker Bothmer. 2003

263 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/89be4d56109ca5abeb57056e8951005850b3bf6c

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. M. Temmer
2. Nat Gopalswamy
3. S. Yashiro
4. B. Vršnak
5. R. Howard
6. A. Vourlidas
7. S. Akiyama
8. Yuming Wang

In Molecular Biology

1. Nat Gopalswamy
2. M. Temmer
3. A. Vourlidas
4. R. Howard
5. S. Yashiro
6. B. Vršnak
7. S. Patsourakos
8. S. Akiyama

Citations in the corpus

• The Magnetic Helicity Budget of Solar Active Regions and Coronal Mass Ejections (2003, background): “On the basis of LASCO/ EIT data, Zhang et al. (2003) have identified the solar sources of 27 major geomagnetic storms occurring between 1996 and 2000.”
• Properties of Interplanetary Coronal Mass Ejections (2007, background): “It has been established that ICMEs are the main source of major (Dst < −100 nT) geomagnetic storms (Gosling et al., 1991; Bothmer and Schwenn, 1998; Tsurutani and Gonzalez, 1997; Webb et al., 2000, 2002; Zhang et al., 2003; Srivastava and Venkatakrishnan, 2004).”
• Catalog of large-scale solar wind phenomena during 1976–2000 (2009, background): “1. Only separate chains of phenomena are analyzed (for example, only coronal mass ejections and their manifestations in the interplanetary medium [13, 14 ] or only CIR [12]).”
• Acceleration in Fast Halo CMEs and Synchronized Flare HXR Bursts (2008, background): “Front-sided, fast halo CMEs are the most geo-effective CMEs (e.g., Zhang et al. 2003) and are thus vitally important to study.”
• Deflection of coronal mass ejection in the interplanetary medium (2004, background): “Wang et al. (2002) and Zhang et al. (2003) suggested that the Parker spiral interplanetary magnetic fields (Parker, 1963) deflect CMEs when they propagate in the interplanetary medium.”
• NO TRACE LEFT BEHIND: STEREO OBSERVATION OF A CORONAL MASS EJECTION WITHOUT LOW CORONAL SIGNATURES (2009, methodology): “Using a comprehensive set of data, Zhang et al. (2003, 2007) and Schwenn et al. (2005) searched for source regions of geomagnetic storms (respectively with Dst ≤ −100 nT and Dst ≤ −50 nT).”
• Kinematics of coronal mass ejections between 2 and 30 solar radii. What can be learned about forces governing the eruption (2004, background): “However, for very fast/wide CMEs, which in fact are the most geo-effective events (Zhang et al. 2003), the prediction based on LASCO observations is more difficult since the action of the propelling force is prolonged in such events.”
• Solar and interplanetary sources of major geomagnetic storms during 1996–2002 (2004, methodology): “This asymmetry is much smaller compared with that reported by Wang et al. [2002] and Zhang et al. [2003] .”
• Visibility of coronal mass ejections as a function of flare location and intensity (2005, background): “Since the main drivers of large geomagnetic storms are halo CMEs [Webb et al., 2000; Zhang et al., 2003; Gopalswamy, 2004], which is an energetic population, invisible CMEs may not produce geomagnetic storms by themselves; however, the invisible CMEs may contribute to complex geomagnetic storms wi”