Engineering topics
Publications and source records attributed to Lakhina, G..
Explore the source record for details and available documents.
Significant charged-particle precipitation occurs in the dayside auroral zone during and after interplanetary shock impingements on the Earth's magnetosphere.
Polar Cap Boundary Layer waves are ELF/VLF electric and magnetic waves detected on field lines adjacent to the polar cap, thus their name.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
We use 1997-1998 Wind Solar Wind data and POLAR UV imaging data to study magnetospheric responses and substorm triggering mechanisms during and after interplanetary (IP) shock events.
Energetic ***sup3***He particle mean free paths are calculated using in-situ wave amplitudes. The wave polarization and wave k directions are included in a first order cyclotron resonant calculation.
Nonlinear evolution equation for Alfven waves, propagating in streaming plasmas with nonuniform densities and inhomogeneous magnetic fields, is obtained by using the reductive perturbation technique.
Charged particle interactions with magnetic field magnitude changes lead to particle guiding center displacements and hence particle cross-field diffusion.
We review some of the new NASA/ESA Ulysses solar wind microscale results.
Boundary layers are commonly encountered in space and astrophysical plasmas.
We examine energetic particle transport at or near Corotating Interaction Regions (CIRs).