Io moon的問題，透過圖書和論文來找解法和答案更準確安心。 我們找到下列問答集和資訊懶人包

日本鐵道小詞典 萬用豆知識8

為了解決Io moon的問題，作者栗原景 這樣論述：

　　～開往鐵道世界的直達車即將發車，還沒上車的旅客請趕快上車！～ 　　帶上900則詞條，開始探索鐵道的世界吧！   　　【萬用豆知識】為楓書坊以「手繪百科」為主題的全新系列作， 　　全系列以詞典的方式編排，並搭配討喜的插圖， 　　探討【咖哩】、【巧克力】、【啤酒】、【F1賽車】……多元主題， 　　輕快生動地講解相關重要知識。 　　感到好奇時，可以透過本書窺探新世界的奧祕； 　　遇到疑惑時，可以翻開本書尋找正確可信的答案； 　　想要放鬆時，更可以讓本書發揮它的娛樂效果！ 　　鐵道是一種「綜合興趣」。 　　雖然以「鐵道迷」一詞統稱熱愛鐵道的人， 　　但大家感興趣的對象和領域其實是非常多元的。

　　有人享受旅行，有人熱愛攝影，有人喜歡收藏票根和周邊商品， 　　有人偏好收集、製作、裝飾模型，也有許多人熱衷於探討歷史與技術知識。 　　本書從龐大的鐵道領域及業界用語中嚴選出約900則鐵道語詞條， 　　全面介紹鐵道基本用語、業界用語、名留鐵道史的企業與人物， 　　以及鐵道迷慣用的俗語等各領域的鐵道語。 　　在詞條之間也穿插了豐富的專欄， 　　主題有【鐵路便當】、【時刻表】等，增加閱讀上的趣味性。 　　隨書附錄【JR全制霸記錄帳】，內容包含全日本JR路線地圖， 　　以及路線列表等資訊，陪伴各位鐵道迷一步一步達成JR全制霸。 　　如果你是 　　✓想掌握全方面鐵道知識的鐵道迷 　　✓懷著滿腔

熱情的新手鐵道迷 　　✓熱愛日本旅遊的玩家 　　那就趕快翻開書，和大家一起搭上開往鐵道世界的直達車吧！ 本書特色 　　◎鐵道迷必懂詞彙900則X細緻又可愛的漫畫插圖： 　　收錄鐵道基本用語＋業界用語＋名留鐵道史的企業與人物＋鐵道迷慣用的俗語，搭配可愛的漫畫插圖，用輕鬆的心情開始一趟充滿趣味的鐵道之旅吧！ 　　◎字典式編排，能夠直達想了解的詞條： 　　本書依字典形式整理出詞條，並按照日語50音順序編排，可以直達感興趣的詞條頁面，不用按照順序，想讀什麼，就讀什麼！ 　　◎專欄穿插其中，主題式介紹有趣的鐵道知識： 　　詞條中穿插著【鐵路便當】、【時刻表】、【車掌的道具】等有趣的主題專欄，閱讀

樂趣大大提升！ 　　◎收錄中日雙語詞條，可同時對照日語原文： 　　吸收鐵道知識、學習日語雙管齊下，更貼近日本鐵道世界！

Io moon進入發燒排行的影片

氧化鉿鋯鐵電記憶體之疲勞恢復與非晶氧化鎵銦鋅通道整合

為了解決Io moon的問題，作者陳昱豪 這樣論述：

如何以節能的方式處理大量數據是未來包括大數據、人工智能、物聯網、自動駕駛汽車和高性能計算等領域中最重要的問題。鐵電記憶體因其高CMOS兼容性、高操作速度和低能耗而被視為實現未來以數據為中心的計算之關鍵元件。對於像鐵電隨機存取記憶體或鐵電穿隧記憶體這樣的電容式鐵電記憶體，其中一個重要的挑戰是在快速且低電壓操作下由不飽和極化切換造成的嚴重極化疲勞。不飽和極化切換造成的極化疲勞可以藉由電場去除累積的電荷來回復。然而，大部分的研究只嘗試透過雙向的大電場來回復。在第二章中，我們藉由使用不同電壓，不同脈衝時間，不同操作次數以及不同方向的電場來探討極化疲勞回復的行為。我們是第一個指出操作次數是極化疲勞回復

的關鍵且極化疲勞不可被單極性的電場回復。這暗示鐵電翻轉對於移除累積的電荷扮演重要的腳色。我們引用一個鐵電翻轉引發電流注入的模型來解釋此行為。最後我們在1.5V的低操作電壓下，透過大電場回復使操作次數進步了104次到達總共1010次操作。使用非晶氧化物半導體的鐵電電晶體目前被視為有潛力取代快閃記憶體的人選。因為其低製程溫度可以實現具有高頻寬及高容量特性的三維層積型整合。 然而，目前許多使用非晶氧化物半導體的鐵電電晶體都遇到了高操作電壓以及低操作速度的問題。同時，目前針對改良使用非晶氧化物半導體的鐵電電晶體的討論非常少。在第三章中，我們全面研究了用於三維、低電壓應用、具有非晶氧化銦鎵鋅通道的單柵極

氧化鋯鉿鐵電電晶體。我們是第一個針對此元件提出考慮了電荷捕捉效應，負載電容，以及通道漂浮電壓的優化指南。

Encyclopedia of Planetary Landforms

為了解決Io moon的問題，作者Hargitai, Henrik (EDT)/ Kereszturi, Akos (EDT) 這樣論述：

Encyclopedia of Planetary Landforms contains a description and interpretation of all known planetary landforms that have been discovered on the planetary bodies in our Solar System. The content is separated into entries for each planetary landform. All entries are based on literature reviews, using

NASA/ESA/JAXA imagery and original general and thematic maps of the particular landform. Such a wide variety of landforms show how exotic these features could be from a terrestrial point of view, but at the same time emphasizes that the same processes will result in similar morphology, independent o

f its host planet. Illustrations show the generalized structure of each major landform type and is complete with a series of special maps published here for the first time. This organized classification of planetary landform types is not available in other books, and only partially covered in scatte

red papers. The most important places (landforms, named and unnamed) will be found in the main section as well as description and interpretation. This has never been done before. If necessary, these landforms will have an accompanying large-scale map. This will make it serve as a basic reference boo

k - not discussions of large metaconcepts but the stories of well-defined landform types and individual landforms, which is usually only found only in professional papers, one paper, one landform. So this knowledge is very much scattered around in the literature. Each landform will have a data secti

on with height (peaks and low points), diameter, age, data. USGS maps only have diameter data. How will it be used by planetary scientists? It will give a starting point to any landform he or she want to investigate. Previous works are thematic collections of knowledge (i.e., cratering in the Solar

System, volcanic processes, etc.), while this work will approach the subject from landform types and will go deeper by analyzing individual landforms and including maps and imagery. It will be as comprehensive as possible, not only describing the most popular targets but also the (now) lesser known

ones, which may be attractive for future analysis. As an example, suppose someone wants to compare valleys of the Moon and Mercury and Titan. He or she can use this work as a starting place to consult and will find imagery, examples, and the basic literature all collected in one section, including i

ndividual features, as well as where most valleys are found (global distribution). The maps will be printable and easy to handle, in contrast to large sheet paper maps. As for the content of the maps, they are not global maps but also not very detailed thematic geologic or topographic maps. They fal

l in between these extremes, which means that the researcher can understand the context but at the same time see all named features. These could serve as perfect reference maps for all planetary bodies. (Such maps are not available online.) The maps will be uniform in many of their cartographic char

acteristics, which gives the user a good opportunity to compare them, essential in any comparative planetology study (planets, moons, asteroids, etc.). Planetary bodies, where global topographic data is available, will be depicted in both topographic and photomaps and capable of being printed. The m

aps will contain official IAU names AND also informal geologic (and physiographic province) names that have never been put on maps (except for sketch maps), precisely because they are not official. However, since geologist use these names every day (and often complain about IAU's strict rules), we b

elieve that this make these maps much more useful for workers in the field. Maps are for helping to find places, and these names are very important in this respect. Geologic and physiographic names have never been collected in any form (list or map), not even by USGS Gazetteer, so this will be somet

hing brand new. Climatic data (climate diagrams) will be added to maps of Mars. The work will include a full, updated, alphabetical list of names, with links. By 2011, our Russian colleagues may be ready with their corrections of the USGS Gazetteer. If so, the work will include these as well. An Edi

torial Board will review different sections of the work. Possible Editorial Board Members by region are: WESTERN EUROPE Ernst Hauber, Institut f r Planetenforschung, DLR, Germany (Mars) Marita W hlisch, DLR - German Aerospace Center, Institute of Planetary Research, Germany (Planetary Geodesy, Outer

Solar System) Dennis Reiss, University of M nster, Germany (Mars) Arnold Gucsik (MPI f r Chemie, Mainz, Germany) (Impact processes) (He is already a Springer book editor) EASTERN EUROPE Leonid Ksanfomality, Space Research Institute, Moscow, Russia A. A. Lukashov, Lomonosov University, Moscow (geomo

rphology) K. B. Shingareva, MIIGAiK, Moscow (planetary cartography) U.S. P. Schenk, LPI, USA (planetary morphology and geology) James R. Zimbelman, National Air and Space Museum, Smithsonian Institution (Earth, Mars, the Moon, and Venus) Robert Craddock, Smithsonian Institution ASIA Hirdy Miyamoto,

University of Tokyo, Japan Huang Q, . Shanghai Astronomical Observatory, Chinese Academy of Science Dong, S.Y., Faculty of Earth Sciences, China University of Geosciences Wuhan Oshigami, S., Graduate School of Environmental Studies, Nagoya University Zhiyong Xiao, China University of Geosciences, Wu

han Henrik Hargitai (Ph.D., 2007) is a planetary geomorphologist, media historian, and senior lecturer at the Eötvös Loránd University, Budapest, Hungary. He has Ph.D. in Earth Sciences and Philosophy (Aesthetics). He teaches planetary geomorphology (since 2002), planetary cartography, typography,

and media history. His study fields include the distribution and morphology of the mountains of Io; lake ice and snow landforms; impact morphology; and the history and localization of the planetary nomenclature. He participated in two Mars Desert Research Station simulations. He is the chair of the

ICA Commission on Planetary Cartography and editor of the Central European edition of the series of ＂multilingual maps of terrestrial planets and their moons＂ and its 2014 special edition for children. He is the producer of numerous public outreach programs in planetary science for radio. Ákos Kere

szturi (Ph.D.) is a geologist, working on planetary science and astrobiology as researcher at the Research Center for Astronomy and Earth Sciences, where he leads the Astrophysical and Geochemical Laboratory. He is member of the NASA Astrobiology Institute TDE Focus Group, teaches planetary science

at Eötvös Loránd University, serves on the editorial board of two international and one national journals, is vice president of the Hungarian Astronomical Association, and contributes in the popularization activity of the Polaris Observatory in Budapest. His main research area is the geology of Mars

, Europa satellite, craters of Mercury, water in the Solar System and beyond, Mars analog field work, survival of extremophile organisms, analysis of asteroid surfaces, and geological history based on mineral characteristics of meteorites.

肝臟特異性的核磁共振顯影劑(Gd-EOB-DTPA)和核磁共振彈性影像(MR Elastography)在肝癌的診斷價值

為了解決Io moon的問題，作者王怡珺 這樣論述：

背景 目前肝癌在國內致死癌症排名在男性及女性分別為第一名及第三名，影像學在肝癌診斷中扮演很重要的角色。如果在顯影劑注射的影像（顯影劑超音波、電腦斷層、磁振造影）三種有一種有典型影像，即可診斷為肝癌，不再需要病理確診。腹部超音波掃描方便、不具侵襲性，但掃描範圍較侷限，比較適合肝癌篩檢。電腦斷層或磁振造影檢查，對於肝腫瘤的性質可提供進一步的訊息，像是檢查肝外的淋巴結或腹腔內的大血管有沒有受到侵害。磁振造影檢查因為沒有輻射線且有些研究認為比電腦斷層有更高的靈敏度和診斷準確性，所以磁振造影被認為是一個更好的診斷工具。但當傳統磁振造影顯影劑動態影像造影(Dynamic study)呈現非典型肝癌，使用

新的肝臟特異性的磁振造影顯影劑 (Gd-EOB-DTPA)，肝膽影像（Hepatobiliary phase, 延遲20分鐘影像）呈現低訊號 (hypointensity)來診斷肝癌，另一方面使用核磁共振彈性影像 (MR Elastography)，量測肝臟腫瘤的彈性係數加以分析，良性腫瘤與惡性腫瘤的彈性係數是否有統計學上的顯著差異，以期能夠作為磁振造影的輔助工具。以達到肝癌早期發現、早期治療的目的。方法 第一個研究為了評估新的肝臟特異性的磁振造影顯影劑(Gd-EOB-DTPA)，肝膽影像（Hepatobiliary phase）呈現低訊號來診斷肝癌的價值，以回溯性方式自2009年1月至201

4年12月連續收錄約50名接受過二次以上顯影劑腹部磁振造影影像檢查，第二次檢查使用肝臟特異性核磁共振顯影劑 (Gd-EOB-DTPA)，打顯影劑之腹部磁振造影檢查之病患，依病灶選取標準收錄尺寸大於1公分以上之肝臟病灶，若為惡性病灶，須經由病理切片或合乎AASLD(美國肝病協會)訂立之標準肝癌(HCC)影像者，若為良性病灶，則必須有病理切片或接受至少兩年的影像追蹤證實。並將肝臟病灶區分為再生不良結節(Dysplastic nodule)及肝癌（HCC）兩大類。分別記錄打藥前T1,T2腫瘤的訊號和打藥後顯影模式，打藥前和肝實質比較分為低 (hypointense)，同 (isointense)，或

高 ( hyperintense)。打藥後顯影模式和肝實質比較分為低度 (hypovascular), 同 (isovascular)，和高度( hypervascular)顯影。第二個研究，評估核磁共振彈性影像 (MR Elastography)，分別量測肝臟腫瘤的彈性係數加以分析，是否能成為診斷肝癌的輔助工具，以回溯性方式收集自2013年4月至2017年2月共約109名接受過顯影劑腹部磁振造影影像以及核磁共振彈性影像 (MR Elastography) 檢查，並分別量測局部肝臟病灶以及肝臟實質的硬度 (shear stiffness)，以手動的方式在肝臟腫瘤和肝臟實質的地方畫出區域 (Re

gion of Interest)，並分析肝臟腫瘤在核磁共振彈性影像的表現並且評估是否和肝癌細胞分化有關。結果 Dysplastic nodule 和 HCC 在 T2WI 上的高信號、T1WI 上的低信號、動脈影像上的顯影、動態影像上的典型 HCC 顯影模式、肝膽影像呈現低訊號和 DWI 上的高信號方面存在顯著差異。T2WI的敏感性和特異性分別為79.3%和83.3%，T1WI為50.0%和80.0%，DWI為82.8%和76.7%，動態影像為17.2%和100%，以及肝膽影像的93.1%和83.3%，當動脈影像上的顯影和肝膽影像呈現低訊號時為46.8% 和 100%。惡性腫瘤比起良性腫瘤和

正常肝臟實質有較高的硬度（shear stiffness）(5.98kPa (95% CI, 5.50 – 6.50) vs. 3.33kPa (95% CI, 2.95 – 3.73 vs. 3.53kPa (95% CI, 3.23 – 3.84) (p