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「ejecta」の共起表現一覧(1語右で並び替え)

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the crater; lobate flows emanating from crater ejecta, and very radar-bright ejecta and floor.
cts excavated and mixed dark material into the ejecta and the resulting mix is not apparent against
ast of the crater rim, emplacement of hummocky ejecta appears to have been impeded by the topography
The ejecta are mainly observed to the north and northeast
hock effects are tectonic features, the impact ejecta are Quaternary alluvial fans or Tertiary congl
This alder ejecta area is on spectrographic evidence instead pri
The dark annulus of ejecta around Tolstoj is one of the darkest places on
The plains may be impact deposits ( ejecta) associated with Ursula or they may be cryovol
Ejecta blanket from Hadley crater filling in Hadley R
The ejecta blanket becomes thinner with distance and incr
Valleys on the Ejecta Blanket from Cerulli Crater, as seen by HiRISE
The result is that both the crater and its ejecta blanket stand above the surroundings.
r an impact event, the falling debris forms an ejecta blanket surrounding the crater.
Its extensive ejecta blanket and secondary crater field are superpo
An ejecta blanket is a generally symmetrical apron of ej
ter has an inner and an outer ring and a small ejecta blanket surrounding the outer ring.
It is on the edge of the much larger ejecta blanket surrounding the crater Victoria, named
It is a dark-floored crater with a bright ejecta blanket located in the Uruk Sulcus region.
Asymmetries in the crater structure and the ejecta blanket imply that the projectile impacted at
Emma Dean lies directly on top of the ejecta blanket from Victoria and could therefore expo
he northwestern section of Abedin's continuous ejecta blanket appears to have a lower reflectance th
s (15 mi) in diameter, and is surrounded by an ejecta blanket of breccia preserved over an area of 6
ly sloped scarp that terminates the continuous ejecta blanket.
Similar features may be seen in ejecta blankets of Martian craters, suggesting impact
gists associate the glass not with impact melt ejecta, but with radiative melting from meteoric larg
s estimated that immediately after the impact, ejecta covered an area of 25,000 square kilometres (9
The presence of hummocky, radar-bright crater ejecta crossing the radar-dark floor terrace and adja
It has an outer lobate ejecta deposit extending about a crater radius from t
The ejecta deposit surrounding the craters appears very b
simultaneously, it is difficult to discern any ejecta deposit on the dark terrain.
nded by a system of bright rays, which are ice ejecta deposited during the impact event.
low, hummocky rim material that may consist of ejecta deposits.
nding site area is believed to be blanketed by ejecta excavated by the impact that created Heimdal.
Approximately half the volume of ejecta falls within 1 crater radius of the rim, or 2
Centered on the impact crater, a wide ejecta field has been traced, some 50 km across, form
ge of the outer ramparts of Langrenus, and the ejecta forms low ridges attached to the south rim of
s have suggested that angrites could represent ejecta from Mercury.
ounding Abedin are secondary craters formed by ejecta from the initial impact.
crater floor is faintly marked by lighter-hued ejecta from the crater Giordano Bruno to the north.
he crater floor has been resurfaced, either by ejecta from the Mare Imbrium or by basaltic lava, and
lanitia is part of (Caloris Planitia) might be ejecta from Caloris that were melted by the impact.
rt of the rim of Bingham is partly overlaid by ejecta from Lobachevsky.
ed by the mare and overlain across the east by ejecta from Alpetragius.
In particular, if the ejecta from a crater formed in the highlands (which i
face, its features eroded and blanketed by the ejecta from the relatively fresh crater Antoniadi jus
believed that both Esclangona and its moon are ejecta from an asteroidal collision in the past that
ater is geologically young as the fresh impact ejecta has rough surface, which is a good scatterer o
hile the pristine state of preservation of the ejecta has been used to suggest that it may in fact b
The "skirt" of ejecta in this case is due to a tangential release of
ides of the wave, gravitationally grouping the ejecta into a plane.
n Yuty's southwestern rim is evidence that the ejecta is thin.
s typical volcanoes do; instead, a low ring of ejecta known as a tuff ring forms around a bowl-shape
Nature of dominant ejecta: lithic, blocks and ash; often accretionary la
les) in diameter, and is surrounded by complex ejecta lobes, which are a distinctive characteristic
raters, the amount, distribution, and sizes of ejecta, mechanical properties of the surface such as
al and mid-latitudes on Mars have this form of ejecta morphology, which is thought to arise when the
Its type occurrence is within the limestone ejecta of the Mount Vesuvius volcano complex near Nap
sifs and the radially lineated facies of basin ejecta of the Caloris Croup surround the Caloris Basi
Some fiamme represent fragments of volcanic ejecta, often pumice lapilli that have been flattened
, steep-sided, and often display no associated ejecta or lava flows.
nteraction of crater materials (the meteoroid, ejecta, or both) and high-speed winds in the upper at
ed by secondary impacts of the larger crater's ejecta or by volcanic venting activity along a rift.
in near the crater and associated with impact ejecta or hot water precipitates form crater ridges a
ummocky remnants resembling basin deposits and ejecta protrude above the gently sloping basin wall.
A pedestal crater is a crater with its ejecta sitting above the surrounding terrain.
The outer rampart of ejecta spills over slightly into the Apollo basin flo
ndary craters are impact craters formed by the ejecta that was thrown out of a larger crater.
the larger crater Lewis, in the outer skirt of ejecta that surrounds the Mare Orientale impact basin
rochronology, Saksunarvatn tephra are volcanic ejecta that form an ash layer that is useful in datin
A ray system comprises radial streaks of fine ejecta thrown out during the formation of an impact c
Ejecta which falls within that area is considered pro
volcanic material (both solidified magma, and ejecta) which appears mostly flat from the surface.
                                                                                                    


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