Journal of Atmospheric and Terrestrial Physics
Volume 55, Issue 14, December 1993, Pages 1775-1787
Auroral torch structures: results of optical observations
References (27)
An iterative method for calculating the altitudes and position of auroras along the arc
Planet. Space Sci.
(1987)- et al.
Mapping of the auroral horn into magnetotail
Planet. Space Sci.
(1990) - et al.
Wave characteristics of Ps6 magnetic variations and their implications for convective flow in magnetosphere
Planet. Space Sci.
(1986) Auroral ionization and excitation by incident energetic electrons
Planet. Space Sci.
(1963)- et al.
High time-resolution imaging of auroral arc deformation at substorm onset
Planet. Space Sci.
(1988) - et al.
On the development of folds in auroral arcs
J. atmos. terr. Phys.
(1988) A magnetospheric magneic field model with warped tail current sheet
Planet. Space Sci.
(1989)A study of auroral displays photographed from the DMSP-2 satellite and from Alaska meridian chain of stations
Space Sci. Rev.
(1974)- et al.
Joint two-dimensional of ground magnetic and ionospheric electric currents associated with auroral currents, 5. Current system associated with eastward drifting omega bands
J. Geophys.
(1982) Spatially inhomogeneous current configurations as seen by the Scandinavian Magnetometer Array
Multi-method observations and modeling of the three dimensional current associated with a very strong Ps6 event
J. Geophys.
(1981)
Three-dimensional mapping of the aurora from digitized all-sky pictures
Perturbation magnetic fields and current systems associated with eastward drifting auroral structures
J. geophys. Res.
(1979)
Cited by (13)
Automatic classification of mesoscale auroral forms using convolutional neural networks
2022, Journal of Atmospheric and Solar-Terrestrial PhysicsAn interpretation of spacecraft and ground based observations of multiple omega band events
2015, Journal of Atmospheric and Solar-Terrestrial PhysicsCitation Excerpt :In general, the brightest edges of the omega bands lie near the interface between the region 1 and region 2 current system in the morning sector. A number of studies have used magnetic field models to identify the magnetospheric equatorial location of the observed omega bands mapped along field lines (Pulkkinen et al., 1991; Tagirov, 1993; and Wild et al., 2011). Pulkkinen et al. (1991) determined that the omega bands observed on March 25, 1986 mapped to 6–13 RE with Tsyganenko (1989) (T89) magnetic field model (Tsyganenko, 1989) and Tagirov (1993) found that the omega bands observed on April 9–10, 1986 mapped to 5–6 RE, also using the T89 model.
The Source of Auroral Omegas
2022, Journal of Geophysical Research: Space PhysicsOmega Band Magnetospheric Source Location: A Statistical Model-Based Study
2021, Journal of Geophysical Research: Space PhysicsPolar substorm on 7 December 2015: Preonset phenomena and features of auroral breakup
2020, Annales GeophysicaePhysical Processes of Meso-Scale, Dynamic Auroral Forms
2020, Space Science Reviews
Copyright © 1993 Published by Elsevier Ltd.