Results 21 to 30 of about 12,699 (236)
Craters at many volcanoes, including most maars, are formed by multiple subsurface explosions. Experiments compared the crater formed by a single large, buried explosion, with craters formed by multiple explosions with the same cumulative energy ...
Greg A. Valentine +6 more
doaj +1 more source
The magnetosphere under weak solar wind forcing [PDF]
The Earth's magnetosphere was very strongly disturbed during the passage of the strong shock and the following interacting ejecta on 21–25 October 2001. These disturbances included two intense storms (Dst*≈−250 and −180 nT, respectively).
Rich, F. J. +28 more
core +1 more source
Light Curves and Colors of the Ejecta from Dimorphos after the DART Impact
On 26 September 2022 the Double Asteroid Redirection Test (DART) spacecraft impacted Dimorphos, a satellite of the asteroid 65803 Didymos. Because it is a binary system, it is possible to determine how much the orbit of the satellite changed, as part of ...
Janetzke, Ron +44 more
core +1 more source
Pre-encounter Predictions of DART Impact Ejecta Behavior and Observability [PDF]
We overview various efforts within the DART Investigation Team's Ejecta Working Group to predict the characteristics, quantity, dynamical behavior, and observability of DART impact ejecta.
Fahnestock, Eugene, G +36 more
core +1 more source
Initial 40Ar‐39Ar Ages of the Paleocene‐Eocene Boundary Impact Spherules
We report 40Ar‐39Ar step‐heating ages of Paleocene‐Eocene (P‐E) boundary impact spherules from Atlantic Margin coastal plain and open ocean sites. We test the hypothesis that the P‐E spherules are reworked from an earlier event (e.g., K‐Pg impact at ~66 ...
Morgan F. Schaller +4 more
doaj +1 more source
Infrared Ejecta and Cold Dust in the Young Supernova Remnant N132D
We present Spitzer, Wide-field Infrared Survey Explorer (WISE), and Herschel observations of the young supernova remnant (SNR) N132D in the Large Magellanic Cloud, including 3–40 μ m Spitzer Infrared Spectrograph (IRS) mapping, 12 μ m WISE and 70, 100 ...
Jeonghee Rho +3 more
doaj +1 more source
Liquefaction Ejecta-Induced Damage [PDF]
The 2010-2011 Canterbury earthquake sequence (CES) devasted Christchurch, New Zealand. Liquefied soil were ejected onto the ground surface, damaging more than 15,000 houses beyond economic repair.
Mijic, Zorana
core
Safe landings are imperative to accomplish NASA’s Artemis goal to enable human exploration on the Moon, including sample collection missions. However, a process known as plume surface interaction (PSI) presents a significant hazard to lunar landings. PSI
Ariana Bueno +5 more
doaj +1 more source
>Magister Scientiae - MScThe advancement of the understanding of hypervelocity impacts lies in discovering impact structures and both proximal and distal impact ejecta.
Mautle, Floyd Danger
core
As a preliminary study, the effects of target temperature on ejecta size were examined at an impact velocity of 3.5 km/s with the goal of improving the ISO11227.
Masahiro NISHIDA +7 more
doaj +1 more source

