「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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