Results 151 to 160 of about 4,712 (268)

Coral Reef‐Level Upwelling in an Internal Wave Hotspot Modulated by Mesoscale Dynamics

Geophysical Research Letters, Volume 53, Issue 20, 28 October 2026.
Abstract Coral reefs in the northern South China Sea experience some of the world’s most energetic internal waves (IWs), yet records of how these dynamics influence reef‐level conditions are rare. Using over 6 years of temperature data from Dongsha Atoll, we show that IWs drive diel temperature fluctuations that reduce subsurface heat exposure and ...
Alex S. J. Wyatt, Timothy B. King, I‐Huan Lee, James J. Leichter   +3 more
wiley   +1 more source

A southward differentiated impactor forms the tapered shape of the South Pole-Aitken impact basin on the Moon. [PDF]

Sci Adv
Wakita S, Johnson BC, Andrews-Hanna JC, Gowman G, Davison TM, Collins GS, Bill CA, Marchi S, M Alexander A, Bottke WF, Evans AJ.   +10 more
europepmc   +1 more source

Convective Amplification of Ionospheric Feedback by a Finite‐Duration Inertial Alfvén‐Wave Source

Geophysical Research Letters, Volume 53, Issue 20, 28 October 2026.
Abstract We investigate the ionospheric feedback instability (IFI) driven by a finite‐duration localized source of inertial Alfvén waves. Wave‐excited conductance perturbations undergo Pedersen mobility drift in the convection and wave electric fields and are amplified.
R. Rankin, W. Wang, Q.‐G. Zong
wiley   +1 more source

FPW-YOLO11n: A Lightweight Frequency-Perception Framework for Lunar Impact Crater Detection. [PDF]

Sensors (Basel)
Liang J, Yan P, Wen Q, Liu Q, Zhai Y, Tian X.   +5 more
europepmc   +1 more source

Meter‐Scale Roughness of the Lunar Surface

Geophysical Research Letters, Volume 53, Issue 19, 16 October 2026.
Abstract Small‐scale surface roughness is a key indicator of local geological processes, yet it has not previously been mapped globally on the Moon. We present global meter‐scale surface roughness maps generated from the Lunar Orbiter Laser Altimeter pulses, which record information about surface undulations within the instrument's ∼5 m individual ...
Hephzibah Christopher, Indujaa Ganesh
wiley   +1 more source

Tianwen-2 mission target asteroid (469219) Kamo'oalewa probably develops an Itokawa-compositional but more space-weathered surface. [PDF]

Nat Commun
Zhang P, Zhang G, Wei Z, Granvik M, Yan X, Wang P, Zhang Q, Pang R, Zhou WH, Jiang T, Vernazza P, Hiroi T, Cloutis E, DeMeo F, Beck P, Ip WH, Fenucci M, Zhang Y, Marsset M, Niu Y, Lu X, Wu X, Lin H, Hu S, Cheng B, Zhao H, Wang X, Lu X, Zhang Y, Ling Z, Zhang J, Zhao S, Lantz C, Geem J, He Z, Wang J, Zhou L, Zhang X, Li S, Hu S, Yang W, Li X, Zhang X, Liu J, Zhang P, Zhang G, Lin Y, Li Y.   +47 more
europepmc   +1 more source

Cosmogenic 10Be as a Tracer for Recent Heliospheric Encounters With Interstellar Cold Clouds and Nearby Supernovae

Geophysical Research Letters, Volume 53, Issue 19, 16 October 2026.
Abstract Recent works suggest there are periods when the Sun encountered massive interstellar cold clouds which compressed the heliosphere to within Earth's orbit, exposing Earth to interstellar galactic cosmic rays and energetic particles of heliospheric origin.
Anna Nica, Merav Opher, Jesse A. Miller, Jennifer L. Middleton, Joe Giacalone   +4 more
wiley   +1 more source

Saturation of space weathering in shaping lunar regolith particle morphology. [PDF]

Nat Commun
Luo A, Cui Y, Wang G, Nie J, Xu C, Zhang Z, Zhang J, Li Y, Zhao Q, He H.   +9 more
europepmc   +1 more source

Predicting impacts on the lunar surface

In this work, we undertake a systemic mechanical analysis of the geological and morphological structure of degenerate planetary satellites—specifically categorized under the structural topology of the Moon and equivalent solid-iron ballast planetoids—based on the principles of non-equilibrium fluid dynamics, closed-loop thermodynamics, and ...
openaire   +1 more source

Drift‐Resonance Driven by Field Line Resonance Gradients: A Mechanism for Non‐Dispersive Microinjection Events

Geophysical Research Letters, Volume 53, Issue 19, 16 October 2026.
Abstract Ultra‐low‐frequency waves in the magnetosphere often produce field line resonances with strong spatial gradients in wave amplitude. We analyze a form of drift resonance driven by these gradients near the resonant field line. This mechanism differs fundamentally from conventional gradient‐ and curvature‐driven drift resonance and predicts an ...
J. Liu, R. Rankin, A. W. Degeling, S. Yao, F. Fenrich   +4 more
wiley   +1 more source