The Magnetic Helicity Budget of Solar Active Regions and Coronal Mass Ejections
By A. Nindos, J. Zhang, Haiyang Zhang. 2003
139 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/5e26dded60f139f9d5d66bfee1c5919016f4fb7c
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In Astronomy and Astrophysics
- Etienne Pariat
- K. Subramanian
- P. Démoulin
- Mitchell A. Berger
- Axel Brandenburg
- R. Lepping
- J. Qiu
- T. Howard
In Molecular Biology
- K. Subramanian
- Etienne Pariat
- P. Démoulin
- Mitchell A. Berger
- R. Lepping
- Axel Brandenburg
- J. Qiu
- T. Howard
Citations in the corpus
- On the Magnetic Flux Budget in Low-Corona Magnetic Reconnection and Interplanetary Coronal Mass Ejections (2007, methodology): “In this study, we take L ¼ 1 AU, or calculate the poloidal flux per AU, while taking L ¼ 0:5 AU as the lower limit (e.g., DeVore 2000) and L ¼ 2 AU as the upper limit (e.g., Nindos et al. 2003).”
- Photospheric flux density of magnetic helicity (2005, methodology): “Nindos et al. (2003) have used Eq.”
- Long-duration magnetic clouds: a comparison of analyses using torus- and cylinder-shaped flux rope models (2007, background): “Secondly, the estimation of the flux rope radius directly affects the estimation of physical quantities, such as magnetic flux and magnetic helicity carried away from the Sun by the MC (Green et al., 2002; Nindos et al., 2003; Leamon et al., 2004; Lynch et al., 2005; Lepping et al., 2006).”
- Eruption of magnetic flux ropes during flux emergence (2008, unknown): “On the other hand, the occurrence of CMEs in active regions, in their early phase of formation (e.g. Démoulin et al. 2002; Nindos et al. 2003), suggest that emerging flux carries the potential to produce eruptions by itself.”
- Astrophysical magnetic fields and nonlinear dynamo theory (2004, background): “ yet no foundation for this simple-minded speculation. In this context it is important to recall that whenever magnetic eruptions of any form do occur, the field is always found to be strongly twisted [45,46,48,338,339]. It is therefore plausible that such events are an important part of the solar dy”