Her kan du lære mere om JQuery Mobile
Stefani Recht
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The basics of dumping out a manged object - 09 | .NET Debugging for the Production Environment One of the first things you need to know in order to debug managed applications with a native debugger such as cdb, windbg, etc., is how to dump a managed object. This is a task you'll repeat often if you spend any time at all debugging managed code. This episode demonstrates a couple ways to accomplish this basic - but very important - task. I probably should have covered this much earlier on, but better late than never (hopefully).
Productivity Power Tools for Visual Studio 2012 | Visual Studio Toolbox The Productivity Power Tools is an extension pack that delivers powerful tools for improved productivity. With 1.5 million downloads, the Visual Studio 2010 version is the second most downloaded extension in the Visual Studio Gallery. The Visual Studio 2012 version was released in e
Defrag: Adding MicroSD to Libraries, Multiboot PCs, Win8 Mail App | The Defrag Show Microsoft tech troubleshooter extraordinaire Gov Maharaj and I help walk you through troubleshooting solutions to your tech support problems. If you have a problem you want to send us, you can use the Problem Step Recorder in Windows 7 (see this for details on how) and send us the zip file to DefragShow@microsoft.com. We will also be chec
Starting a Blog with Blogger
This video begins a series of videos about starting a blog using Google's free online blogging platform, Blogger. Viewers can either watch them in a series or watch a for a specific need because they are all titled. (00:50)
Timeline of The Space Race - Wiki Article
The Space Race was an informal competition between the United States and the Soviet Union that lasted roughly from 1957 to 1975. (01:20)
Integrative Biology 131 - Lecture 02: Skeletal System General Human Anatomy. UC Berkeley lecture with Professor Marian Diamond. The functional anatomy of the human body as revealed by gross and microscopic examination.
Collective Intelligence While people have talked about collective intelligence for decades, new communication technologies—especially the Internet—now allow huge numbers of people all over the planet to work together in new ways. The recent successes of systems like Google and Wikipedia suggest that the time is now ripe for many more such systems both inside and outside organizations, and this talk will examine ways to take advantage of these possibilities. Using examples from business, governme
Cyber Security Education
How much personal information do you have stored on the internet? Think about how many times you have entered your phone number, address and even your social security number into an online bill payment, application or form.
1.6 Obesity treatment Obesity treatment is only successful if weight is reduced and maintained to within a desired range. There are three approaches to obesity treatment: changing behaviour and diet is the most common approach although drugs and surgery can be used in some severe cases of obesity. Behaviour and diet: it is important to be realistic about an obese patient's target weight as many patients have over-ambitious targets that they are unlikely to achieve. A severely obese patient probably ca
1.4 Inadequate intake In the developed world inadequate intake of food, at least in terms of energy, is not common. Nevertheless, in many parts of the world starvation is a huge issue, and it is estimated that tens of millions of people face starvation, and well over 5 million, mainly children, die each year from inadequate nutrient intake. Importantly, lack of particular nutrients impairs our ability to carry out many functions. 1.3 Balanced energy intake There is a need for a certain daily energy intake to allow metabolism to occur in the body. Metabolism means all the chemical reactions occurring in the body and there are two types of process involved: catabolism breaks down larger molecules into smaller ones often with energy release and anabolism is the building up of larger molecules from smaller precursors, often requiring energy. The body requires energy to power anabolic, mechanical (for example, muscle contraction 3.1 Solar radiation Over 99.9% of the energy available at the Earth's surface comes from the Sun. Solar energy emanat 1.6.3 The acceleration due to gravity In the absence of air resistance, an object falling freely under the influence of the Earth's gravity, close to the surface of the Earth, experiences an acceleration of about 9.81 m s−2 in the downward direction. The precise value of the magnitude is indicated by the symbol g and varies slightly from place to place due to variations in surface altitude, the effect of the Earth's rotation and variations in the internal composition of the Earth. Some typical values f 1.5.7 The signed area under a general velocity–time graph We have already seen (in Section 3.6) that in the context of uniform motion, the signed area under a particle's velocity–time graph, between two given times, represents the change in the particle's position during that time interval, with a positive area corresponding to displacement in the positive direction. In the Introduction This unit is an adapted extract from the course Biological psychology: exploring the brain (SD226) This unit looks at how language is understood, which includes hearing and how sounds and words are interpreted by the brain. It takes an interdisciplinary approach and should be of wide general interest. Acknowledgements The content acknowledged below is Proprietary (see terms and conditions) and is used under licence (not subject to Creative Commons licence ). Grateful acknowledgement is made to the following sources for permission to reproduce material in this unit: Figures 1. Introduction This unit explores origins of the Universe by looking in detail at events immediately following the Big Bang. Starting with looking at the cooling of the very early Universe, the unit then moves on to the inflation era, the quark-lepton and the hadron era. Then the unit looks at how fundamental particles began to synthesise to form nuclei, and from here it discusses the development of larger structures like stars and galaxies. By examining closely the forces in play and the interactions of fu
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