Results 261 to 270 of about 168,691 (324)
A Large Scale Molecular Hessian Database for Optimizing Reactive Machine Learning Interatomic Potentials. [PDF]
Cui T, Han Y, Jia H, Duan C, Zhao Q.
europepmc +1 more source
Abstract A moderate geomagnetic storm was driven by high‐speed solar wind stream on 14 March 2016. We show that large‐scale traveling ionospheric disturbances (LSTIDs) played a significant role in producing the ionospheric storm positive phase at mid‐latitudes in the North American sector.
G. P. Geethakumari +8 more
wiley +1 more source
Narrative Review of Clinical Indices and Imaging Tools, With a Proposal for an Integrative Grading Scale for Vulvovaginal Aging. [PDF]
Rodas A, Sanabria G, González-Isaza P.
europepmc +1 more source
Global MHD Simulations: Magnetosphere–Ionosphere Coupling Dependence on Conductance Model
Abstract Eighty‐five geomagnetic storms were simulated with the space weather modeling framework Geospace model using two different ionospheric conductance models. One set used the legacy conductances within the Ridley ionosphere model, while the other set used the newly developed conductance model for extreme events conductance model.
T. I. Pulkkinen +9 more
wiley +1 more source
Experimental model of menopausal genitourinary syndrome: Ovariectomy and vaginectomy protocols in rats. [PDF]
Anggraeni A +6 more
europepmc +1 more source
Abstract The Geospace Dynamics Constellation (GDC) mission aims to investigate the dynamic coupling between the magnetosphere, ionosphere, and thermosphere by resolving key spatiotemporal processes at scales ranging from local to global. A key aspect is GDC's ability to reconstruct hemispheric‐scale high‐latitude electrodynamics with comprehensive ...
J. S. Shim +6 more
wiley +1 more source
Reactive Active Learning: An Efficient Approach for Training Machine Learning Interatomic Potentials for Reacting Systems. [PDF]
Achar SK +5 more
europepmc +1 more source
Abstract The soft X‐ray imager (SXI) on the SMILE mission promises to revolutionize our understanding of the magnetopause by observing solar wind charge exchange emission from the magnetosheath on a global scale. The primary goal of this instrument is to infer the position and shape of the magnetopause from these images.
S. J. Wharton +7 more
wiley +1 more source
Directly observing the magnetic rope contraction and expansion in space. [PDF]
Fu HS +7 more
europepmc +1 more source

