Convection and auroral response to a southward turning of the IMF : Polar UVI, CUTLASS, and IMAGE signatures of transient magnetic flux transfer at the magnetopause

By S. Milan, M. Lester, S. Cowley, M. Brittnacher. 2000

179 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/a55f62c05cdefa4f750102fa5c955140d01c8cf4

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. R. Greenwald
2. J. Michael Ruohoniemi
3. S. Cowley
4. H. Carlson
5. S. G. Shepherd
6. Philippe Zarka

In Molecular Biology

1. S. Cowley
2. J. Michael Ruohoniemi
3. Philippe Zarka

Citations in the corpus

• Space weather challenges of the polar cap ionosphere (2017, background): “…transfer mechanism from the solar wind into the magnetosphere-ionosphere system is believed to be impulsive dayside reconnection and Flux Transfer Events (FTEs) (Haerendel et al. 1978; Russell & Elphic 1978, 1979; Cowley & Lockwood 1992; Denig et al. 1993; Lockwood et al. 1995; Milan et al. 2000).”
• Sharpening our thinking about polar cap ionospheric patch morphology, research, and mitigation techniques (2012, background): “…photometers/imagers called PMFs or poleward moving auroral forms [see, e.g., Sandholt et al., 2002]; in Super DARN poleward moving transients [Milan et al., 2000]; in radar backscatter flow channel events (FCE) [Pinnock et al., 1993] 5 of 16 6 of 16 and poleward moving radar auroral forms…”
• Variations in the polar cap area during two substorm cycles (2003, background): “Two recent studies of the growth rate of the polar cap during southward IMF estimated8day ≈ 160 kV for Bz ≈ −10 nT (Milan et al., 2000b) and8day ≈ 48 kV for Bz ≈ −4 nT (Milan and Lester, 2001).”
• A decade of the Super Dual Auroral Radar Network (SuperDARN): scientific achievements, new techniques and future directions (2007, methodology): “…a northward turning of the IMF (Huang et al. 2000a), and also showed how the MLT position of the reverse convection cells shifted as the IMF clock angle varied (Huang et al. 2000b), matching the movement of the cusp auroral spot also observed during northward IMF conditions (Milan et al. 2000a).”