Results 151 to 160 of about 3,699 (198)
The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]
Ervin T, Nakhleh AJ, Bharati Das S.
europepmc +1 more source
Uranus's Highly Nonaxisymmetric Magnetopause and Its Impact on Magnetic Reconnection
Abstract Mass and energy fluxes from the solar wind can access a planet's magnetosphere through dayside magnetic reconnection. The plasma and magnetic field conditions on either side of the magnetopause determine whether reconnection is suppressed. However, magnetosheath conditions are sensitive to the shape of the magnetopause, and deviations from ...
Jack H. Crump +4 more
wiley +1 more source
Abstract Mercury's weak intrinsic magnetic field forms a small magnetosphere and thus a bow shock that decelerates the supermagnetosonic solar wind and reflects particles upstream, forming a foreshock in the quasi‐parallel region. This region is populated by backstreaming ions and electrons and associated wave activity.
Kristin Pump +6 more
wiley +1 more source
Transport of Electrons in Tangled Magnetic Fields. [PDF]
Verscharen D +8 more
europepmc +1 more source
A Magnetospheric Source for Near‐Planet Whistler‐Mode Waves at Venus
Abstract The presence or absence of lightning in the atmosphere of Venus has important implications for atmospheric chemistry, potential chemical signatures of life, identifying volcanic activity, and quantifying potential hazards to future exploration missions.
David M. Malaspina +4 more
wiley +1 more source
Pyrrole without Life: Reaction of Aminomethylene with the Propargyl Radical. [PDF]
McClish R +6 more
europepmc +1 more source
Rapid Magnetotail Reconfiguration and Ion‐Scale Wave Activity at Mercury
Abstract Mercury's magnetosphere is an extremely dynamic environment, where substorm‐like activity, including dipolarization fronts and particle acceleration, periodically disrupts the stability and radial extent of the closed field line region. The common narrowband ∼1 Hz waves at Mercury, near the local proton gyrofrequency are preferentially ...
M. Persson +7 more
wiley +1 more source
Nonequilibrium Formation of C<sub>4</sub> Carbonyls in Interstellar Ices Linked to Amino Acids. [PDF]
Wang Z +7 more
europepmc +1 more source
A Dynamic Auroral Ionospheric Density Profile Reveals a Planetary‐Scale Cavity at Jupiter
Abstract Low‐altitude measurements above Jupiter's main auroras have shown the presence of persistent auroral density depletions. This low density regime strongly favors auroral acceleration by inertial Alfvén waves to explain the predominance of energetic (100–1,000 keV) broadband electron beams.
N. S. Kruegler +2 more
wiley +1 more source

