Results 171 to 180 of about 829 (204)

Ninety percent circular polarization detected in a repeating fast radio burst. [PDF]

Natl Sci Rev
Jiang J, Xu J, Niu J, Lee K, Zhu W, Zhang B, Qu Y, Xu H, Zhou D, Cao S, Wang W, Wang B, Cao S, Zhang Y, Zhang C, Gan H, Han J, Hao L, Huang Y, Jiang P, Li D, Li H, Li Y, Li Z, Luo R, Men Y, Qian L, Sun J, Wang L, Xu Y, Xu R, Yang Y, Yao R, Yue Y, Yu D, Yuan J, Zhu Y.   +36 more
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Exploring exoplanet dynamics with JWST: Tides, rotation, rings, and moons. [PDF]

Proc Natl Acad Sci U S A
Millholland SC, Winn JN.
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Accreting White Dwarfs: An Unreview. [PDF]

Space Sci Rev
Scaringi S, Knigge C, de Martino D.
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Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster. [PDF]

Nat Astron
Pearlman AB, Scholz P, Bethapudi S, Hessels JWT, Kaspi VM, Kirsten F, Nimmo K, Spitler LG, Fonseca E, Meyers BW, Stairs IH, Tan CM, Bhardwaj M, Chatterjee S, Cook AM, Curtin AP, Dong FA, Eftekhari T, Gaensler BM, Güver T, Kaczmarek J, Leung C, Masui KW, Michilli D, Prince TA, Sand KR, Shin K, Smith KM, Tendulkar SP.   +28 more
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Dynamic Synchronization and Resonance as the Origin of 1/f Fluctuations-Amplitude Modulation Across Music and Nature. [PDF]

Entropy (Basel)
Nakamichi A, Uesaka I, Morikawa M.
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Alfvén Waves in Partially Ionised Solar Steady-State Plasmas. [PDF]

Sol Phys
Alshehri NF, Ballai I, Verth G, Fedun V.
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High-Energy Phenomena in Extreme Astrophysical Objects and the Origin of High-Energy Cosmic Rays

High-Energy Phenomena in Extreme Astrophysical Objects and the Origin of High-Energy Cosmic Rays
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Scaling astrophysical phenomena to high-energy-density laboratory experiments

Plasma Physics and Controlled Fusion, 2002
The spatial and temporal scales of astrophysical phenomena are typically 10–20 orders of magnitude greater than those of laboratory experiments intended to simulate them. Accordingly, the issue of similarity between the astrophysical phenomenon and its laboratory counterpart becomes quite important.
D D Ryutov, B A Remington
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Relationship between high-energy physical phenomena on the sun and in astrophysics

Solar Physics, 1988
High energy phenomena on the surface of the Sun are manifestations of part of the solar dynamo cycle. Convection and magnetic field give rise to unstable, twisted flux loops that become solar flares when the resistive tearing mode proceeds to the nonlinear limit.
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