ICTs in everyday life
We now live in a global village where distance in no longer a barrier to commercial or social contact. This unit will enable you to gain an understanding of the information and communication technologies that drive our networked world and how they now permeate our everyday lives.
Acknowledgements
The energy carried by ocean waves derives from a proportion of the wind energy transferred to the ocean surface by frictional drag. So, ultimately it stems from the proportion of incoming solar energy that drives air movement. Just how much energy is carried by a single wave depends on the wind speed and the area of ocean surface that it crosses; wave height, wavelength, and therefore wave energy, are functions of the distance or fetch over which the wind blows.
This unit considers the power
1.1.1 Distance-teaching technique
This unit is an introduction to studying the arts and humanities. It takes you through a series of exercises designed to develop your approach to study and learning at a distance and improve your confidence as an independent learner.
Introduction
This unit is an introduction to studying the arts and humanities. It takes you through a series of exercises designed to develop your approach to study and learning at a distance and improve your confidence as an independent learner.
The Palettes for Fiction
Although the marketplace for short stories is difficult, many new writers choose to begin with writing them, almost as a right of passage, a place for honing language, testing their narrative nerve over a shortish distance, and organising a palette.
Seminar 17 - 2010 Army War College Distance Education Class
350 senior U.S. Armed Forces leaders along with their civilian and international counterparts celebrated the completion of their two-year Army War College Distance Education Program with a graduation ceremony July 23. For more information visit http://www.carlisle.army.mil/banner/article.cfm?id=1522
IPL: The Myths of e-Learning
Professor Kwok-Wing Lai, Director of Centre for Distance Education and Learning Technologies, College of Education Inaugural Professorial Lecture, given November 6, 2008.
Three Generations of Distance Education Pedagogy: Challenges and Opportunities
Professor Terry Anderson, Canada Research Chair in Distance Education, Athabasca University, Canada, has an incredible knowledge of online learning, and his work on the uses of technology in support of open and distance education is at the forefront of research in this area. He will address the challenges of expanding access to high quality distance learning and the growing opportunities to create and sustain learning connections using both old and new approaches to distance education.
Held 30
The Palettes for Fiction
Although the marketplace for short stories is difficult, many new writers choose to begin with writing them, almost as a right of passage, a place for honing language, testing their narrative nerve over a shortish distance, and organising a palette.
The Distance: Cancer
"297 feet. It's the distance between our research labs and our patient rooms." We open on a hallway, as Dr. Nestor Esnaola tells viewers how MUSC physicians and researchers are working together in multidisciplinary teams to create new answers for pancreatic cancer patients. He explains that "our researchers are literally creating new answers down the hall that don't exist anywhere else."
Ethics of Human Subject Research
Ethics of Human Subject Research (2 credits) is offered by the Department of Health Policy and Management and the Distance Education Division, Johns Hopkins Bloomberg School of Public Health and The Phoebe R. Berman Bioethics Institute, Johns Hopkins University. The course introduces students to the ethics of human subject research. Ethical theory and principles are introduced, followed by a brief history of research ethics. Topics covered in lectures and moderated discussions include informed c
Stations of Light
Student groups rotate through four stations to examine light energy behavior: refraction, magnification, prisms and polarization. They see how a beam of light is refracted (bent) through various transparent mediums. While learning how a magnifying glass works, students see how the orientation of an image changes with the distance of the lens from its focal point. They also discover how a prism works by refracting light and making rainbows. And, students investigate the polar nature of light usin
1.4 Stellar masses and stellar evolution
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
The H–R diagram
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
2.5 Using stars to probe the interstellar medium
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
2.4 The effect of interstellar dust
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
2.3 The effect of interstellar gas
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
2.1 Introduction
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
1.4 Stellar masses and stellar evolution
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
1.2 The main classes of stars
Stars can necessarily be observed only at a distance. This unit introduces the Hertzsprung–Russell diagram, an essential tool in understanding the nature of stars. You should have some understanding of the basic stellar properties of luminosity and temperature in order to get the most from the unit.
