Oceans & space publications

We observed the Venusian 5577.3 Å OI nightglow emission feature after solar flares, coronal mass ejections, and solar wind streams from December 2010 to July 2012 using the high resolution Astrophysical Research Consortium Echelle Spectrograph.

An algorithm has been developed to image the local structure in the convection electric field using multibeam incoherent scatter radar (ISR) data.

In this paper, we present a new methodology utilizing meteor head echo radar observations that aims to constrain the ZDC physical model by ground-based measurements.

Using a 1-D ionosphere-polar wind model and measurements from the Resolute Bay Incoherent Scatter Radar (RISR-N), this paper shows that these reflected photoelectrons are a significant source of heat for the sunlit polar cap ionosphere.

We study the variation of plasma mass density in the outer magnetosphere over a solar cycle using mass density estimated from the frequency of fundamental toroidal standing Alfvén waves observed by the Geotail spacecraft.

We derive free-tropospheric NO2 volume mixing ratios (VMRs) by applying a cloud-slicing technique to data from the Ozone Monitoring Instrument (OMI) on the Aura satellite.

We use a Monte Carlo model to simulate the interaction of a beam of relativistic electrons with the upper atmosphere as they are injected downward from a notional high-altitude injection platform.

We present observations of SED plumes during six storms between 2010 and 2013 and comprehensively analyze the associated ionospheric parameters within the plumes.

In this paper, we introduce a method for localizing activity in integrated circuits (IC) using a laser scanning microscope.