Small Scale Alfvénic Structure in the Aurora

By Krzysztof Stasiewicz, Paul M. Bellan, C. Chaston, Craig Kletzing, R. Lysak, J. Maggs, O. Pokhotelov, Charles Seyler, P. K. Shukla, L. Stenflo and 2 more. 2000

465 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/fcc31ceb9b2852c0e7a99738e8d416afc8f67131

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. V. Angelopoulos
2. John W. Bonnell
3. J. Mcfadden
4. T. Van Doorsselaere
5. Giuseppe Nisticò
6. Valery M. Nakariakov
7. Karl-Heinz Glassmeier
8. D. Larson

In Molecular Biology

1. V. Angelopoulos
2. T. Van Doorsselaere
3. Giuseppe Nisticò
4. Valery M. Nakariakov
5. N. Vilmer
6. V. Petrosian
7. L. Fletcher
8. Hermann Lühr

Citations in the corpus

• THEMIS ESA First Science Results and Performance Issues (2008, background): “…of mass dependent ion acceleration (Moebius et al. 1998; Lund et al. 1998, 2001), the discovery of the role of Alfvén waves in ion acceleration (Stasiewicz et al. 2000; Chaston et al. 2004), the recognition of the impact of conic ions outflows on magnetic storms and substorms (McFadden et al.…”
• Field‐aligned currents' scale analysis performed with the Swarm constellation (2014, background): “It is known that small-scale FAC structures are commonly associated with kinetic Alfvén waves [see Stasiewicz et al., 2000].”
• Alfvén Waves and Their Roles in the Dynamics of the Earth’s Magnetotail: A Review (2009, background): “Since that time, much progress has been made regarding their theoretical description in the non-ideal MHD case (i.e., dispersive Alfvén waves) which was reviewed by Stasiewicz et al. (2000).”
• Particle Acceleration in the Magnetotail and Aurora (2012, background): “A general expression of the parallel electric field from the equations (15)– (20) is given by Thompson and Lysak (1996), Stasiewicz et al. (2000), and Paschmann et al. (2003): E‖ = ( R2c − λ2e 1 + k2⊥R2c 1 + k2⊥λ2e ) ∂ ∂s (∇⊥ · E⊥) (21) where s is the coordinate in the direction of the magnetic…”
• Recent Advances in Understanding Particle Acceleration Processes in Solar Flares (2011, background): “However, motivated byin situ observations and theories for energy transport and electron acceleration in the Earth’s magnetosphere during sub-storm (Stasiewicz et al. 2000), it is suggested (Fletcher & Hudson 2008) that the energy is transported through the corona not by particle beams but by…”
• Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “Even so, the results are dual (or interchangeable, in the sense that the role of ω and kz being the free parameter of the problem are apparently swapped), and Terradas et al. (2010) found that the damping length depends directly on the period.”
• Properties of small‐scale Alfvén waves and accelerated electrons from FAST (2003, methodology): “From a statistical study of FAST magnetometer data presented by Stasiewicz et al. [2000] and performed over the same frequency range as here and mentioned already in section”