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Untrackable distal ejecta on planetary surfaces
Published 2023-03-01“…Heterogeneous shock impedances of planetary materials cause abrupt changes of ejection angles, forming non-radial ejecta. Interpretations for provenances of surface deposits and ages derived from crater counts are affected by such untrackable ejecta.…”
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Evolutionary signatures in complex ejecta and their driven shocks
Published 2004-11-01“…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 form complex ejecta. …”
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Dust Formation in the Ejecta of Common Envelope Systems
Published 2013“…The actual dust masses produced in the CE ejecta depend strongly on their temperature and density evolution. …”
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Multipoint Observations of the Dynamics at an ICME Sheath–Ejecta Boundary
Published 2023-01-01“…Here, an ICME front boundary, which separates the confined ejecta from the mixed, interacted sheath–ejecta plasma upstream, is analyzed in a multipoint study examining the ICME at 1 au on 2020 April 20. …”
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Proximal ejecta of the Bolaven extraterrestrial impact, southern Laos
Published 2024Subjects: Get full text
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A precambrian proximal ejecta blanket from Scotland
Published 2008“…Ejecta blankets around impact craters are rarely preserved on Earth. …”
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Long-term Evolution in Ionization of Ejecta Illuminated by Eta Carinae
Published 2024-01-01“…Others suggest evolution in the occulting ejecta. The brightness jump in the 1940s, which coincided with the appearance of narrow forbidden emission lines, may have been caused by the clearing and ionization of intervening circumstellar ejecta. …”
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Nonplanar effects in simulations of laser-driven ejecta microjet experiments
Published 2024-03-01“…Recent experiments of laser-driven ejecta microjets performed at OMEGA 60 reveal tortuous jets whereby the jets appear to deviate from their initial trajectory as they travel in vacuum. …”
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Nepheline-kalsilite microperthites in ejecta from the Alban Hills (Italy)
Published 1985-12-01Subjects: Get full text
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Atmospheric Interactions of Ejecta on Earth and Mars Including the Effect of Vaporization
Published 2023-01-01“…Atmospheres play an important role in ejecta deposition after an impact event. Many impact experiments and simulations neglect the effect of atmospheres. …”
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ALMA Observations of the DART Impact: Characterizing the Ejecta at Submillimeter Wavelengths
Published 2023-01-01“…Ejecta dust masses were calculated for a range of materials that may be representative of Dimorphos’s S-type asteroid material. …”
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VLT/MUSE Characterization of Dimorphos Ejecta from the DART Impact
Published 2023-01-01“…We have observed the Didymos-Dimorphos binary system with the MUSE integral field unit spectrograph mounted at the Very Large Telescope before and after DART impact and captured the ensuing ejecta cone, debris cloud, and tails at subarcsecond resolutions. …”
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Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
Published 2018“…This Letter examines how the mass of the dynamical ejecta can be estimated without a direct electromagnetic observation of the kilonova, using GW measurements and a phenomenological model calibrated to numerical simulations of mergers with dynamical ejecta. …”
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A detailed spectral reflectvity study of Copernicus and its ejecta.
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On the impact of compact binary merger ejecta opacity on Kilonova transient signals
Published 2023-01-01“…However, extremely heterogeneous post-merging ejecta composition of both light- and heavy-r process nuclei, implies strong effects on the KNe light-curve identification due to the varying opacity of the system. …”
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Forecast of solar ejecta arrival at 1 AU from radial speed
Published 2004-10-01“…Solar ejecta produce changes in the interplanetary magnetic field of the terrestrial environment. …”
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Ejecta, Rings, and Dust in SN 1987A with JWST MIRI/MRS
Published 2023-01-01“…Using the JWST MIRI Medium Resolution Spectrograph, we spatially resolved the ejecta, equatorial ring (ER), and outer rings in the mid-infrared 12,927 days (35.4 yr) after the explosion. …”
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REMOTE SENSING OBSERVATIONS AND NUMERICAL SIMULATION FOR MARTIAN LAYERED EJECTA CRATERS
Published 2018-04-01“…Secondly, numerical modeling layered ejecta are performed through the hydrocode iSALE (impact-SALE). …”
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