Results 251 to 260 of about 148,229 (333)
Optomechanical sensor network with fiber Bragg gratings. [PDF]
Yang S +7 more
europepmc +1 more source
How Does the Magnetosphere‐Ionosphere Current System Respond to Solar Flares?
Abstract While the isolated effects of solar flares on low‐latitude ionospheric electrodynamics have been well documented, the coupled system response of the equatorial electrojet (EEJ), auroral electrojet (AEJ), field‐aligned currents (FACs), and asymmetric ring current (ASY‐H) remains poorly understood.
Hongkai Tang +5 more
wiley +1 more source
A Novel Shallow Neural Network-Augmented Pose Estimator Based on Magneto-Inertial Sensors for Reference-Denied Environments. [PDF]
Odry A +4 more
europepmc +1 more source
Abstract Substorms are often described by a loading‐unloading cycle, where onset follows gradual accumulation of solar wind magnetic flux in the magnetosphere. Yet observations indicate that intense substorms can also be directly driven, though the underlying mechanism remains unresolved.
Yong Ren +8 more
wiley +1 more source
A Study of a GNSS/IMU System for Object Localization and Spatial Position Estimation. [PDF]
Miletiev R, Petkov PZ, Yordanov R.
europepmc +1 more source
Martian Atmospheric Loss Through Foreshock Transient Events
Abstract At Mars, the MAVEN spacecraft has made observations of Hot Flow Anomalies (HFAs) in the foreshock. Due to the bow shock's proximity to the planet, it is theorized that HFAs contribute to atmospheric escape at Mars through the excavation of ionospheric ions.
Alexandros C. Cooke‐Politikos +5 more
wiley +1 more source
Highly Accurate Attitude Estimation of Unmanned Aerial Vehicle Payloads Using Low-Cost MEMS. [PDF]
Zhou X +5 more
europepmc +1 more source
Abstract This study uses a novel approach to infer the solar soft X‐ray (SXR) irradiance from Auger photoelectron fluxes. Solar SXR irradiance is highly variable, particularly during solar flares. Solar SXR photons at ∼< ${\sim} < $2.5 nm produce oxygen Auger photoelectrons by photoionizing atmospheric constituents. More specifically, we derive the fit
Shaosui Xu +3 more
wiley +1 more source
Abstract Hot and tenuous plasmas have velocity distribution functions (VDFs) significantly different from Maxwellian distributions. Characterizing how these differences impact wave damping and emission necessitates sophisticated methods for determining the associated dielectric plasma response.
K. G. Klein +8 more
wiley +1 more source
Influence of Atomic Magnetometer's Orientation on Its Frequency Response. [PDF]
Zhang R.
europepmc +1 more source

