Results 301 to 310 of about 383,072 (432)
Enhanced Predefined-Time Control for Spacecraft Attitude Tracking: A Dynamic Predictive Approach. [PDF]
Yang J, Guo T, Yu Y, Dong Q, Jia Y.
europepmc +1 more source
Evolution of Force‐Free Magnetic Structure in the Dayside Ionosphere of Mars
Abstract Magnetic fields measured in the ionosphere of Mars by the magnetometers onboard the Mars Atmosphere and Volatile EvolutioN (MAVEN) and the Mars Global Surveyor (MGS) spacecraft display a wide range of spatial scales, ranging from global to small‐scale.
T. E. Cravens+5 more
wiley +1 more source
Can Humanity Thrive Beyond the Galaxy? [PDF]
Wakayama S, Wakayama T.
europepmc +1 more source
Abstract Whistler‐mode chorus waves play a crucial role in accelerating electrons in Earth's outer radiation belt to relativistic and ultrarelativistic energies. While this electron evolution is typically modeled using a diffusion approximation for scattering, high‐amplitude chorus waves induce nonlinear resonant effects that challenge this approach on
Miroslav Hanzelka+5 more
wiley +1 more source
Mathematical Models of Flexible Spacecraft Dynamics : A Survey of Order Reduction Approaches
P.T.L.M. van Woerkom
openalex +1 more source
Calibration Method for Relativistic Navigation System Using Parallel Q-Learning Extended Kalman Filter. [PDF]
Xiong K, Zhao Q, Yuan L.
europepmc +1 more source
Abstract Ionospheric molecular ions, such as N2+ ${\mathrm{N}}_{2}^{+}$, NO+, and O2+ ${\mathrm{O}}_{2}^{+}$, have been observed in Earth's high‐altitude ionosphere and the magnetosphere by several spacecraft missions. Their presence not only indicates that they obtain sufficient energy through effective energization mechanisms, predominantly during ...
Mei‐Yun Lin, Raluca Ilie, Alex Glocer
wiley +1 more source
On detecting and characterizing planetary oceans in the solar system using a distance-based ensemble modelling approach: application to the Uranus system. [PDF]
Cochrane CJ+4 more
europepmc +1 more source
Abstract Spacecraft discharge time constants are calculated from measurements of electron differential flux before and during operation of an ionospheric sounding radar. Determining these time constants provides insight into how the operation of a sounding radar affects the surrounding plasma's interaction with the spacecraft.
Sebastián Rojas Mata+7 more
wiley +1 more source