97 citations · 393 across the 10 of their papers we have counts for
11 papers
Persistent Plasma Waves in Interstellar Space Detected by Voyager 1
S. K. Ocker, J. M. Cordes, S. Chatterjee +3
In 2012, Voyager 1 became the first in situ probe of the very local interstellar medium. The Voyager 1 Plasma Wave System has given point estimates of the plasma density spanning a…
The Dayside Ionopause of Mars: Solar Wind Interaction, Pressure Balance, and Comparisons with Venus
F. Chu, Z. Girazian, F. Duru +5
Due to the lower ionospheric thermal pressure and existence of the crustal magnetism at Mars, the Martian ionopause is expected to behave differently from the ionopause at Venus. W…
Variations in the Ionospheric Peak Altitude at Mars in Response to Dust Storms: 13 Years of Observations from the Mars Express Radar Sounder
Z. Girazian, Z. Luppen, D. D. Morgan +7
Previous observations have shown that, during Martian dust storms, the peak of the ionosphere rises in altitude. Observational studies of this type, however, have been extremely li…
The Effects of Solar Wind Dynamic Pressure on the Structure of the Topside Ionosphere of Mars
Z. Girazian, J. Halekas, D. D. Morgan +3
We use Mars Atmosphere and Volatile EvolutioN observations of the upstream solar wind, and Mars Express observations of ionospheric electron densities and magnetic fields, to study…
The effects of crustal magnetic fields and solar EUV flux on ionopause formation at Mars
F. Chu, Z. Girazian, D. A. Gurnett +5
We study the ionopause of Mars using a database of 6,893 ionopause detections obtained over 11 years by the MARSIS (Mars Advanced Radar for Subsurface and Ionosphere Sounding) expe…
Three-dimensional Features of the Outer Heliosphere Due to Coupling between the Interstellar and Heliospheric Magnetic Field. V. The Bow Wave, Heliospheric Boundary Layer, Instabilities, and Magnetic Reconnection
N. V. Pogorelov, J. Heerikhuisen, V. Roytershteyn +3
The heliosphere is formed due to interaction between the solar wind (SW) and local interstellar medium (LISM). The shape and position of the heliospheric boundary, the heliopause,…
Whistler mode waves upstream of Saturn
Ali H Sulaiman, Donald A Gurnett, Jasper S Halekas +3
Whistler-mode waves are generated within and can propagate upstream of collisionless shocks. They are known to play a role in electron thermodynamics/acceleration and, under certai…
Response of the Martian Ionosphere to Solar Activity including SEPs and ICMEs in a two week period starting on 25 February 2015
F. Duru, D. A. Gurnett, D. D. Morgan +15
In a two-week period between February and March of 2015, a series of interplanetary coronal mass ejections (ICMEs) and (solar energetic particles) SEPs made contact with Mars. The…
Plasma observations during the Mars atmospheric "plume" event of March-April 2012
D. J. Andrews, S. Barabash, N. J. T. Edberg +10
We present initial analysis and conclusions from plasma observations made during the reported "Mars plume event" of March - April 2012. During this period, multiple independent ama…
Overview of Saturn lightning observations
G. Fischer, U. A. Dyudina, W. S. Kurth +8
The lightning activity in Saturn's atmosphere has been monitored by Cassini for more than six years. The continuous observations of the radio signatures called SEDs (Saturn Electro…
Properties of Saturn Kilometric Radiation measured within its source region
L. Lamy, P. Schippers, P. Zarka +9
On 17 October 2008, the Cassini spacecraft crossed the southern sources of Saturn kilometric radiation (SKR), while flying along high-latitude nightside magnetic field lines. In si…