Results 1 to 10 of about 2,733 (195)

Ejecta‐Modulated Bubble Dynamics Play a Dominant Role in Stone Retropulsion [PDF]

open access: yesAdvanced Science
Cavitation bubbles generated by laser absorption in liquids collapse violently, producing high‐speed jets, toroidal bubbles, and shock waves that induce material erosion and object displacement.
Obed S. Isaac   +4 more
doaj   +2 more sources

The Osmium Isotope Signature of Phanerozoic Large Igneous Provinces

open access: yesGeophysical Monograph Series, Page 229-246., 2021

Exploring the links between Large Igneous Provinces and dramatic environmental impact

An emerging consensus suggests that Large Igneous Provinces (LIPs) and Silicic LIPs (SLIPs) are a significant driver of dramatic global environmental and biological changes, including mass extinctions.
Alexander J. Dickson   +2 more
wiley  

+2 more sources

Molecules in Supernova Ejecta [PDF]

open access: yesProceedings of the International Astronomical Union, 2011
AbstractThe first molecules detected at infrared wavelengths in the ejecta of a Type II supernova, namely SN1987A, consisted of CO and SiO. Since then, confirmation of the formation of these two species in several other supernovae a few hundred days after explosion has been obtained.
Cherchneff Isabelle, Sarangi Arkaprabha
openaire   +2 more sources

A numerical study of the interaction between two ejecta in the interplanetary medium: one- and two-dimensional hydrodynamic simulations [PDF]

open access: yesAnnales Geophysicae, 2004
We studied the heliospheric evolution in one and two dimensions of the interaction between two ejecta-like disturbances beyond the critical point: a faster ejecta 2 overtaking a previously launched slower ejecta 1. The study is based on a
A. Gonzalez-Esparza   +2 more
doaj   +1 more source

Nepheline-kalsilite microperthites in ejecta from the Alban Hills (Italy) [PDF]

open access: yesBulletin of the Geological Society of Finland, 1985
Microprobe analyses carried out on exsolved nepheline and kalsilite phases of microperthites occurring in three ejecta from the Alban Hills (Roman comagmatic region) have shown: (1) a practically continuous compositional variation from Ks to Ne (bulk ...
C. Aurisicchio, M. Federico
doaj   +1 more source

Groove formation on Phobos from reimpacting orbital ejecta of the Stickney crater

open access: yesEarth and Planetary Physics, 2022
Numerous linear grooves have long been recognized as covering the surface of Phobos, but the mechanisms of their formation are still unclear. One possible mechanism is related to the largest crater on Phobos, the Stickney crater, whose impact ejecta may ...
XiangYu Xi, Min Ding, MengHua Zhu
doaj   +1 more source

Dynamic simulations of projectile penetration into granular medium

open access: yesMechanical Engineering Journal, 2014
Dynamic FEM and DEM simulations are carried out to investigate dynamic penetration of a projectile into a target of granular medium. Spatial distribution and time dependence of ejecta are clarified together with their trajectories in medium.
Kinya OGAWA   +2 more
doaj   +1 more source

Fine debris flows formed by the Orientale basin

open access: yesEarth and Planetary Physics, 2020
The prototype for investigations of formation mechanisms and related geological effects of large impact basins on planetary bodies has been the Orientale basin on the Moon.
YuZhen Cai   +3 more
doaj   +1 more source

MAGNETOHYDRODYNAMIC EFFECTS IN RELATIVISTIC EJECTA [PDF]

open access: yesInternational Journal of Modern Physics D, 2010
We study the problem of deceleration of an arbitrarily magnetized relativistic ejecta in a static unmagnetized medium and its connection to the physics of gamma-ray bursts (GRBs). By computing exact solutions of the Riemann problem describing this scenario, we find that with the same initial Lorentz factor, the reverse shock becomes progressively ...
YOSUKE MIZUNO   +6 more
openaire   +3 more sources

Evolutionary signatures in complex ejecta and their driven shocks [PDF]

open access: yesAnnales Geophysicae, 2004
We examine interplanetary signatures of ejecta-ejecta interactions. To this end, two time intervals of inner-heliospheric (≤1AU) observations separated by 2 solar cycles are chosen where ejecta/magnetic clouds are in the process of interacting to ...
C. J. Farrugia, D. B. Berdichevsky
doaj   +1 more source

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