Terrestrial planets的問題，透過圖書和論文來找解法和答案更準確安心。 我們找到下列地圖、推薦、景點和餐廳等資訊懶人包

3D Digital Geological Models: From Terrestrial Outcrops to Planetary Surfaces

為了解決Terrestrial planets的問題，作者 這樣論述：

3D DIGITAL GEOLOGICAL MODELSDiscover the practical aspects of modeling techniques and their applicability on both terrestrial and extraterrestrial structuresA wide overlap exists in the methodologies used by geoscientists working on the Earth and those focused on other planetary bodies in the Sol

ar System. Over the course of a series of sessions at the General Assemblies of the European Geosciences Union in Vienna, the intersection found in 3D characterization and modeling of geological and geomorphological structures for all terrestrial bodies in our solar system revealed that there are si

milar datasets and common techniques for the study of all planets--Earth and beyond--from a geological point-of-view. By looking at Digital Outcrop Models (DOMs), Digital Elevation Models (DEMs), or Shape Models (SM), researchers may achieve digital representations of outcrops, topographic surfaces,

or entire small bodies of the Solar System, like asteroids or comet nuclei. 3D Digital Geological Models: From Terrestrial Outcrops to Planetary Surfaces has two central objectives, to highlight the similarities that geological disciplines have in common when applied to entities in the Solar System

, and to encourage interdisciplinary communication and collaboration between different scientific communities. The book particularly focuses on analytical techniques on DOMs, DEMs and SMs that allow for quantitative characterization of outcrops and geomorphological features. It also highlights innov

ative 3D interpretation and modeling strategies that allow scientists to gain new and more advanced quantitative results on terrestrial and extraterrestrial structures. 3D Digital Geological Models: From Terrestrial Outcrops to Planetary Surfaces readers will also find: The first volume dedicated to

this subject matter that successfully integrates methodology and applications A series of methodological chapters that provide instruction on best practices involving DOMs, DEMs, and SMsA wide range of case studies, including small- to large-scale projects on Earth, Mars, the 67P/Churyumov-Gerasime

nko comet, and the MoonExamples of how data collected at surface can help reconstruct 3D subsurface models3D Digital Geological Models: From Terrestrial Outcrops to Planetary Surfaces is a useful reference for academic researchers in earth science, structural geology, geophysics, petroleum geology,

remote sensing, geostatistics, and planetary scientists, and graduate students studying in these fields. It will also be of interest for professionals from industry, particularly those in the mining and hydrocarbon fields.

Saints and Sinners in the Sky: Astronomy, Religion and Art in Western Culture

為了解決Terrestrial planets的問題，作者Mendillo, Michael 這樣論述：

Michael Mendillo is Professor of Astronomy at Boston University. His science career deals with research in solar-terrestrial space physics, planetary science, and newly discovered planets orbiting stars in our galaxy. Professor Mendillo has assembled one of the largest privately-held collections of

antiquarian astronomical maps, charts and atlases. They form the basis of the Celestial Images exhibitions held at many university art galleries, the Smithsonian Institution and the US National Academy of Science. His teaching of astronomy to non-science majors stresses interdisciplinary topics and

their connectivity (science-art-religion-society).

由歷史航照重建探討花東縱谷北段活動構造與1972年瑞穗地震之關係

為了解決Terrestrial planets的問題，作者李應頎 這樣論述：

台灣東部於1972年4月22日發生地震矩規模(Mw) 6.7之瑞穗地震。過去研究發現1972年瑞穗地震主震之震源機制解為逆衝斷層帶走滑分量，且主震與餘震序列位於1951年10月花蓮縱谷地震群以南、11月縱谷地震序列以北，顯示該地震發震斷層與花東縱谷北段的活動構造有關。為了解1972年瑞穗地震與花東縱谷北段活動構造之關係，與花東縱谷北段海岸山脈側的活動構造特性，本研究使用在1972年瑞穗地震前、後之歷史航照影像，以運動回復結構(SfM)及多視立體(MVS)之方法建置該地區的歷史數值地表模型(DSM)與正射影像，透過構造地形判釋與次像素關聯分析，以及歷史文獻收集及實地訪談方式，試圖了解該區域之活

動斷層特性與1972年地震可能伴隨的同震地表破裂。本研究透過1972年地震災害報導，以及本研究現地訪談所得的主震地震震度分布圖，發現該地震震度分布與花東縱谷中段與北段之活動構造位置相符。本研究亦透過歷史數值地表模型分析發現，在花東縱谷北段-光復鄉至壽豐鄉一帶總長約24公里的海岸山脈西翼，存在連續分布之斷層跡與相關活動構造地形。然而沿著斷層跡之口述歷史與地震前後的次像素關聯位移分布皆未發現明顯可見的地震地表破裂，暗示1972年瑞穗地震可能並未伴隨明顯的地表斷層破裂。該段活斷層跡沿線可見斷錯沖積扇、閉塞丘、斷層谷、斷錯河等多樣的左移活斷層地貌，顯示海岸山脈西側近地表處的活動構造強烈受到走向滑移錯動

控制，另有發現開花構造與右階斷層之現象。本研究推測這些活動構造是由斜碰撞構造環境下形成，且屬於較年輕的斷層系統。綜上所述，本研究認為1972年瑞穗地震在花東縱谷北段沒有伴隨明顯可見的同震地表破裂，地表所見之左移活動構造應為早於1951年的同震斷層錯動所造成的結果。