Orientation of the Magnetic Fields in Interplanetary Flux Ropes and Solar Filaments

By V. Yurchyshyn, Haimin Wang, P. Goode, Yuanyong Deng. 2001

134 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/77ca99d3cea46653f5876db079247df652c1e581

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. Nat Gopalswamy
2. M. Temmer
3. R. Schwenn
4. S. Yashiro
5. B. Vršnak
6. N. Lugaz
7. T. Howard
8. R. Howard

In Molecular Biology

1. Nat Gopalswamy
2. T. Howard
3. R. Schwenn
4. S. Yashiro
5. N. Lugaz
6. S. Akiyama
7. B. Vršnak
8. Pete Riley

Citations in the corpus

• Cone model for halo CMEs: Application to space weather forecasting (2004, methodology): “The orientation of the magnetic field in ICME or magnetic cloud has been found to correlate with the direction of magnetic field and magnetic helicity in CME’s source active regions such as pre-eruptive filament or post-eruption coronal arcade [Bothmer and Schwenn, 1994; Zhao and Hoeksema, 1998; McA”
• Space Weather: The Solar Perspective (2006, methodology): “Since orientation and helicity of filaments before eruption is often reflected in the topology of the resulting magnetic clouds (Bothmer and Schwenn, 1998; Yurchyshyn et al., 2001), we can use this knowledge for optimizing the prediction of geomagnetic effects (McAllister et al.”
• Solar source of the largest geomagnetic storm of cycle 23 (2005, background): “The 2000 February 21 MC is another example with no storm at all [Yurchyshyn et al., 2001].”
• Interplanetary flux rope ejected from an X-ray bright point. The smallest magnetic cloud source-region ever observed (2005, background): “There is increasing evidence that the helicity sign of MCs matches that of their solar source region (Bothmer & Schwenn 1994; Rust 1994; Marubashi 1997; Yurchyshyn et al. 2001).”
• The Physical Processes of CME/ICME Evolution (2017, methodology): “The magnetic-field measurements at 1 AU suggest a left-handed flux rope passed the spacecraft below its axis (Yurchyshyn et al. 2001).”
• Properties of Interplanetary Coronal Mass Ejections (2007, background): “In the opposite case of northward axial field, the MC is not geoeffective at all (Yurchyshyn et al., 2001).”
• Geoeffectiveness of halo coronal mass ejections (2007, background): “Occasionally, the flux rope axes may be highly inclined to the ecliptic plane and cause either very intense storms [Gopalswamy et al., 2005a] or no storm at all [Yurchyshyn et al., 2001] depending on which way the axial field is pointed.”
• The association of coronal mass ejections with their effects near the Earth (2005, methodology): “Sinc orientation and helicity of filaments before eruption is often reflected in the topology of the resulting magnetic clouds (Bothmer and Schwenn, 1998; Yurchyshyn et al., 2001), we can use this knowledge for optimizing the prediction of geomagnetic effects (Zhao and Hoeksema, 1997, 1998; McAllist”
• History and development of coronal mass ejections as a key player in solar terrestrial relationship (2016, unknown): “Yurchyshyn et al. (2009) fitted ellipses to the outlines of halo and partial halo CMEs and compared them with the axis of the associated post-eruption arcades.”
• On the Magnetic Flux Budget in Low-Corona Magnetic Reconnection and Interplanetary Coronal Mass Ejections (2007, background): “…relate magnetic clouds to various solar progenitors (Bothmer & Schwenn 1994; Rust 1994; Marubashi 1997; Zhao & Hoeksema 1998; McAllister & Martin 2000; Yurchyshyn et al. 2001, 2005; Nindos et al. 2003; Ruzmaikin et al. 2003; Hu et al. 2005; Luoni et al. 2005; Rust et al. 2005; Krall et al. 2006).”
• Coronal mass ejections of solar cycle 23 (2006, background): “…or the rear section of the ICME contains Bs. Occasionally CMEs arrive at Earth with a high inclination resulting in an intense storm (when the magnetic field is fully southward, see Gopalswamy et al. 2005c) or no storm at all (when the magnetic field is fully northward, see Yurchyshyn et al. 2001).”