Results 111 to 120 of about 151,031 (208)
The GD-1 Stellar Stream Perturber as a Core-collapsed Self-interacting Dark Matter Halo. [PDF]
Zhang X, Yu HB, Yang D, Nadler EO.
europepmc +1 more source
How Do Space Hurricanes Disturb the Polar Thermosphere: A Statistical Survey
Abstract The space hurricane is a polar cap auroral structure with strong flow shears and intense particle precipitation that can disturb the thermosphere under quiet geomagnetic conditions. Here the statistical characteristics of this interaction are surveyed using data from the Defense Meteorological Satellite Program and Gravity Field and Steady ...
Zhi‐Feng Xiu+10 more
wiley +1 more source
Effects of Normal and Lateral Electric Fields on Membrane Mechanical Properties. [PDF]
Pogharian N+2 more
europepmc +1 more source
Auroral and Non‐Auroral H3+ Ion Winds at Uranus With Keck‐NIRSPEC and IRTF‐iSHELL
Abstract To date, no investigation has documented ionospheric flows at Uranus. Previous investigations of Jupiter and Saturn have demonstrated that mapping ion winds can be used to understand ionospheric currents and how these connect to magnetosphere‐ionosphere coupling.
Emma M. Thomas+12 more
wiley +1 more source
Acoustic modes in M67 cluster stars trace deepening convective envelopes. [PDF]
Reyes C+5 more
europepmc +1 more source
Abstract During the May 2024 storm, the minimum Dst index was approximately −412 nT, marking the largest geomagnetic storm of the past decade. This event caused the inner edge of the ring current to penetrate deeply into the inner magnetosphere during the main phase of the storm.
C.‐W. Jun+15 more
wiley +1 more source
Turbulence Characteristics of Ice‐Free Radiatively Driven Convection in a Deep, Unstratified Lake
Abstract This study examines data collected with an autonomous underwater glider during a period of vigorous radiatively driven convection (RDC) and low winds in deep, unstratified Lake Superior. Conductivity, temperature and depth (CTD) measurements reveal distinct convective plumes of warm downwelling water with temperature anomalies of ∼0.1° ${\sim}
Kenneth Larrieu+5 more
wiley +1 more source
Juno Observations Set New Constraints on the Electrodynamic Interaction Between Io and Jupiter. [PDF]
Kotsiaros S+8 more
europepmc +1 more source
Control of the Jovian Magnetopause by Iogenic Plasma: Initial Results From Global MHD Simulations
Abstract The size and variability of Jupiter's magnetosphere are not only determined by upstream conditions but also substantially influenced by internal processes within Jupiter's magnetosphere, specifically the dynamics of the rotation magnetodisc.
Enhao Feng+6 more
wiley +1 more source