Solar eruptions and energetic particles

By Nat Gopalswamy, R. Mewaldt, J. Torsti. 2006

135 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Pulmonary and Respiratory Medicine

View Paper: https://www.semanticscholar.org/paper/321ba3d14a1f1156bc083dba00b29e90f5ae2e41

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Artificial Intelligence

1. D. Webb
2. T. Howard
3. S. Antiochos
4. N. Vilmer
5. Nat Gopalswamy

In Astronomy and Astrophysics

1. Nat Gopalswamy
2. S. Yashiro
3. R. Howard
4. S. Akiyama
5. D. Webb
6. T. Howard
7. P. Mäkelä
8. M. Temmer

In Pulmonary and Respiratory Medicine

1. D. Webb
2. T. Howard
3. Nat Gopalswamy

Citations in the corpus

• Coronal Mass Ejections: Observations (2012, methodology): “http://www.livingreviews.org/lrsp-2012-3 Coronal Mass Ejections: Observations 7 Living Reviews in Solar Physics http://www.livingreviews.org/lrsp-2012-3 8 David F. Webb and Timothy A. Howard Gopalswamy (2004), Gopalswamy et al. (2006b), and Aschwanden (2006).”
• Homologous Confined Filament Eruptions via Magnetic Breakout (2008, background): “…eject enormous amounts of magnetic flux and plasma into interplanetary space at high speeds (a coronal mass ejection, or CME) and emit copious quantities of high-energy particles and radiation (a solar flare; e.g., Crooker et al. 1997; Song et al. 2001; Gopalswamy et al. 2006; Kunow et al. 2006).”
• Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun–Earth connection (2008, background): “frequently called type I noise storms and composed of short-lived (a few seconds) and narrow band (a few MHz) bursts superposed on a continuum were also characterized in the early 1950s (e.g. Payne-Scott et al. 1947; Dodson et al. 1953).”
• Coronal mass ejections, type II radio bursts, and solar energetic particle events in the SOHO era (2008, background): “The selection criterion requires that the CMEs be faster than 900 km/s, so the annual number of FW CMEs generally follows the speed distribution (Gopalswamy et al., 2006) shown in Fig.”
• The Heliospheric Imagers Onboard the STEREO Mission (2009, background): “Given this fleet of spacecraft, there is the opportunity for a major multi-instrument attack on many aspects of CME physics and this field is developing rapidly (see recent reviews in, e.g., Gopalswamy, Mewaldt, and Torsti, 2006).”