activity
20112017
most citedProperties of Saturn Kilometric Radiation measured within its source region

93 citations · 352 across the 9 of their papers we have counts for

collaborators

7 papers

physics.space-ph2017★ 17 cited

Hybrid Simulations of Positively and Negatively Charged Pickup Ions and Cyclotron Wave Generation at Europa

R. T. Desai, M. M. Cowee, H. Wei +4

In the vicinity of Europa, Galileo observed bursty Alfvén-cyclotron wave power at the gyrofrequencies of a number of species including K, O, Na, and Cl, indicatin…

astro-ph.HE2017★ 18 cited

An in situ comparison of electron acceleration at collisionless shocks under differing upstream magnetic field orientations

A. Masters, A. H. Sulaiman, Ł. Stawarz +6

A leading explanation for the origin of Galactic cosmic rays is acceleration at high-Mach number shock waves in the collisionless plasma surrounding young supernova remnants. Evide…

astro-ph.EP2016★ 24 cited

Cassini observations of Saturn's southern polar cusp

C. S. Arridge, J. M. Jasinski, N. Achilleos +15

The magnetospheric cusps are important sites of the coupling of a magnetosphere with the solar wind. The combination of both ground- and space-based observations at Earth have enab…

astro-ph.EP2015★ 49 cited

Cassini in situ observations of long-duration magnetic reconnection in Saturn's magnetotail

Christopher S. Arridge, Jonathan P. Eastwood, Caitriona M. Jackman +15

Magnetic reconnection is a fundamental process in solar system and astrophysical plasmas, through which stored magnetic energy associated with current sheets is converted into ther…

astro-ph.EP2014★ 23 cited

Polar Confinement of Saturn's Magnetosphere Revealed by in-situ Cassini Observations

Nathan M. Pilkington, Nicholas Achilleos, Christopher S. Arridge +4

Plasma rotation plays a large role in determining the size and shape of Saturn's disc-like magnetosphere. A magnetosphere more confined to the equator in the polar regions is expec…

astro-ph.HE2013★ 86 cited

Electron acceleration to relativistic energies at a strong quasi-parallel shock wave

A. Masters, L. Stawarz, M. Fujimoto +9

Electrons can be accelerated to ultrarelativistic energies at strong (high-Mach number) collisionless shock waves that form when stellar debris rapidly expands after a supernova. C…