{"title":"Knowledge acquisition and representation techniques in scholarly communication","authors":"B. Gaines, M. Shaw","doi":"10.1145/209910.209912","DOIUrl":null,"url":null,"abstract":"Paper journals, conferences and workshops have been the major media for scholarly discourse for 300 years. However, in the 1990s access to low-cost personal computing and Internet communications is leading to radical changes in the operation of scholarly communities. Electronic publication and conferencing is becoming common in all disciplines using commonly available Internet facilities such as ftp archives, list servers, gopher and world-wide web. Some scholarly communities that had not previously achieved a critical mass have done so through the net, others have launched major collaborative projects managed through the net, and others are questioning the value of conventional conferences that are limited by being localized in space and time compared with the flexibility of continuous international electronic conferencing through the web. However, the majority of current electronic scholarly discourse emulates paper-based media in relying primarily on text and diagrams for knowledge communication. It is beginning to take advantage of some of the multimedia capabilities of electronic publishing for color diagrams, pictures, movies and sound. Hypertext and hypermedia capabilities are being used to develop webs of linked material. Concept maps and formal knowledge structures are being used to provide a framework for knowledge expression, interchange and collaborative development. This article focuses on the extension of current documentation technologies to provide knowledge-level support for scholarly communities.","PeriodicalId":50710,"journal":{"name":"Celestial Mechanics & Dynamical Astronomy","volume":"2 1","pages":"23-36"},"PeriodicalIF":1.6000,"publicationDate":"1995-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"12","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Celestial Mechanics & Dynamical Astronomy","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1145/209910.209912","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 12
Abstract
Paper journals, conferences and workshops have been the major media for scholarly discourse for 300 years. However, in the 1990s access to low-cost personal computing and Internet communications is leading to radical changes in the operation of scholarly communities. Electronic publication and conferencing is becoming common in all disciplines using commonly available Internet facilities such as ftp archives, list servers, gopher and world-wide web. Some scholarly communities that had not previously achieved a critical mass have done so through the net, others have launched major collaborative projects managed through the net, and others are questioning the value of conventional conferences that are limited by being localized in space and time compared with the flexibility of continuous international electronic conferencing through the web. However, the majority of current electronic scholarly discourse emulates paper-based media in relying primarily on text and diagrams for knowledge communication. It is beginning to take advantage of some of the multimedia capabilities of electronic publishing for color diagrams, pictures, movies and sound. Hypertext and hypermedia capabilities are being used to develop webs of linked material. Concept maps and formal knowledge structures are being used to provide a framework for knowledge expression, interchange and collaborative development. This article focuses on the extension of current documentation technologies to provide knowledge-level support for scholarly communities.
期刊介绍:
The international journal Celestial Mechanics and Dynamical Astronomy is concerned with the broad topic of celestial mechanics and its applications, as well as with peripheral fields. The papers published in Celestial Mechanics and Dynamical Astronomy include treatments of the mathematical, physical and computational aspects of planetary theory, lunar theory, general and special perturbation theory, ephemerides, resonance theory, geodesy of the Earth and the planets, dynamics, the 3-body problem, the n-body problem, space mechanics, ring systems, galactic dynamics, reference frames, time, relativity, nongravitational forces, computer methods, computer languages for analytical developments, and database management. Celestial Mechanics and Dynamical Astronomy is the journal of record in its field and is an indispensable component of reference libraries on Dynamical Astronomy, Astrodynamics and Dynamical Systems.