Search Publications

Formation and Evolution of the Large-Scale Magnetic Fields in Venus' Ionosphere: Results From a Three Dimensional Global Multispecies MHD Model
DOI: 10.1029/2020GL087593 Bibcode: 2020GeoRL..4787593M

Luhmann, Janet; Toth, Gabor; Nagy, Andrew +2 more

Large-scale magnetic fields have been observed in Venus' ionosphere by both the Pioneer Venus Orbiter (PVO) and Venus Express spacecraft. In this study, we examine the formation and evolution of the large-scale magnetic field in the Venus ionosphere using a sophisticated global multispecies Magnetohydrodynamics (MHD) model that has been developed …

2020 Geophysical Research Letters
VenusExpress 16
Identifying Active Kelvin-Helmholtz Vortices on Saturn's Magnetopause Boundary
DOI: 10.1029/2019GL084206 Bibcode: 2020GeoRL..4784206B

Delamere, P. A.; Johnson, J. R.; Burkholder, B. L. +1 more

For ∼2,000 Cassini magnetopause encounters, we analyse plasma and magnetic fields. The boundary can be unstable to the Kelvin-Helmholtz instability (KHI), which can drive large-scale flows identifiable in plasma measurements. Bulk flow reversed from the expected direction near the magnetopause can indicate vorticity associated with active KH, and …

2020 Geophysical Research Letters
Cassini 15
Momentum and Pressure Balance of a Comet Ionosphere
DOI: 10.1029/2020GL088666 Bibcode: 2020GeoRL..4788666W

Nilsson, H.; Goetz, C.; Richter, I. +3 more

We calculate the momentum flux and pressure of ions measured by the Ion Composition Analyzer (ICA) on the Rosetta mission at comet 67P/Churyumov-Gerasimenko. The total momentum flux stays roughly constant over the mission, but the contributions of different ion populations change depending on heliocentric distance. The magnetic pressure, calculate…

2020 Geophysical Research Letters
Rosetta 11
Electron Acceleration in a Magnetotail Reconnection Outflow Region Using Magnetospheric MultiScale Data
DOI: 10.1029/2019GL085080 Bibcode: 2020GeoRL..4785080E

Khotyaintsev, Yuri V.; Graham, Daniel B.; Vaivads, Andris +3 more

We study Magnetospheric MultiScale observations in the outflow region of magnetotail reconnection. We estimate the power density converted via the three fundamental electron acceleration mechanisms: Fermi, betatron, and parallel electric fields. The dominant mechanism, both on average and the peak values, is Fermi acceleration with a peak power de…

2020 Geophysical Research Letters
Cluster 10
Is Nightside Outflow Required to Induce Magnetospheric Sawtooth Oscillations
DOI: 10.1029/2019GL086419 Bibcode: 2020GeoRL..4786419Z

Zhang, Binzheng; Brambles, Oliver J.; Lotko, William +1 more

Ionospheric outflow plays an important role in the mass coupling between the ionosphere and the coupled solar wind-magnetosphere system. Previous modeling studies have shown that outflowing ionospheric ions may induce magnetospheric sawtooth oscillations through mass loading of the magnetotail, stretching the magnetic field lines, and reducing nig…

2020 Geophysical Research Letters
Cluster 9
Singing Comet Waves in a Solar Wind Convective Electric Field Frame
DOI: 10.1029/2020GL087418 Bibcode: 2020GeoRL..4787418G

Goetz, C.; Taylor, M. G. G. T.; Plaschke, F.

The cometary plasma environment at low gas production rates is dominated by highly compressional, large-amplitude magnetic field waves in the 10-100 mHz range. They are thought to be caused by an ion-Weibel instability due to a cross-field current, which is caused by the cometary ions that are accelerated along the solar wind convective electric f…

2020 Geophysical Research Letters
Rosetta 9
Low-Frequency Radio Observations of the "Quiet" Corona During the Descending Phase of Sunspot Cycle 24
DOI: 10.1029/2020GL090426 Bibcode: 2020GeoRL..4790426R

Ramesh, R.; Kumari, A.; Kathiravan, C. +3 more

We carried out a statistical study of the "quiet" solar corona during the descending phase of the Sunspot Cycle 24 (i.e., January 2015 to May 2019) using data obtained with the Gauribidanur RAdioheliograPH (GRAPH) at 53 and 80 MHz simultaneously. Our results show that the equatorial (east-west) diameters of the solar corona at the above two freque…

2020 Geophysical Research Letters
SOHO 8
Boulder Fall Activity in the Jezero Crater, Mars
DOI: 10.1029/2020GL090362 Bibcode: 2020GeoRL..4790362S

Vijayan, S.; Mangold, N.; Bhardwaj, Anil +5 more

Jezero crater is the landing site for the Mars 2020 Perseverance rover. We report 63 boulder fall tracks within the crater using High-Resolution Imaging Science Experiment (HiRISE) images. The boulder tracks have both fresh and faded morphologies similar to those reported elsewhere on Mars, but reported for the first time in Jezero crater. We comb…

2020 Geophysical Research Letters
MEx 7
The Ice Content of the Dorsa Argentea Formation From Radar Sounder Data
DOI: 10.1029/2020GL090705 Bibcode: 2020GeoRL..4790705W

Plaut, Jeffrey J.; Whitten, Jennifer L.; Campbell, Bruce A.

The Dorsa Argentea Formation (DAF) is an extensive Hesperian plains unit in the south polar region of Mars that was once ice rich and may still contain a substantial fraction of water ice. Given its 3.5-Ga age, the possibility for massive ice in the DAF has significant implications for the preservation of volatiles during large obliquity changes. …

2020 Geophysical Research Letters
MEx 7
Simultaneous Observation of Negatively and Positively Charged Nanograins at Comet 67P/Churyumov-Gerasimenko
DOI: 10.1029/2019GL086147 Bibcode: 2020GeoRL..4786147L

Goldstein, R.; Goetz, Charlotte; LLera, K. +1 more

Observations near comet 67P by Rosetta show evidence of charged nanograins. Specifically, the ion and electron sensor (IES) observed negative particles with energy/charge (E/q) consistent with charged nanograins. However, theory predicts that both polarities should be present. On 19 September 2014, IES detected positively and negatively charged pa…

2020 Geophysical Research Letters
Rosetta 5