![]() ![]() But as a result of those gaps, I wasn't able to reap this book's full benefits. Not to be too much of a self-apologist, but let me preface this review by indicating that my frustration (and hence my lower rating) comes largely from gaps in my own knowledge. Also available is all code from the book. Purchase of the print book comes with an offer of a free PDF, ePub, and Kindle eBook from Manning. The book also covers using Grails with existing Javatechnology, like Spring, Hibernate, and EJBs. Then it walks readers through a Twitter-style social networkingapp-built in Grails, of course-where they implement high-interest featureslike mashups, AJAX/JSON, animation effects, full text search, rounded corners,and lots of visual goodness. The book starts with an overview of Grails and how it can help you get your webdev mojo back. It coversthe nuts and bolts of the core Grails components and is jam-packed withtutorials, techniques, and insights from the trenches. Grails in Action is a comprehensive look at Grails for Java developers. Developers are instantly productive, picking up all the benefits of theRuby-based Rails framework without giving up any of the power of Java. To use this you must add two special parameters to your Config.For web developers used to wrestling with Java and XML, Grails is a breath offresh air. Jawr will only serve requests containing this prefix. You can define a URL fragment as a prefix (such as ‘/jawr/’) to prefix every URL. Note that Jawr handles individual files (you don’t need to explicitly define a bundle for every file you want to compress and serve standalone), so that should not keep you from using this mapping method. This is specially useful if you are adding Jawr to an existing application and you do not want to change every existing script tag. This is the usual approach, but you may want to bundle only part of your code and serve the rest normally. ![]() This is the default behavior, and you don’t need to configure anything at all for it to work, simply omit the jawr.js.mapping/ properties from your config and you are ready to go. css, thus letting Jawr control all requests to your resources. You can have Jawr respond to all requests ending in.There are two ways to map Jawr to requests: To enable the Jawr Binary servlet, which handle images and fonts, you need to define one of the following property : * * .image * jawr.binary.* (Any property which starts with jawr.binary) So to enable the JS or the CSS servlet, you must at least define a bundle of the specified type. So if you configure only JS bundle, the plugin will start only the Jawr JS servlet. The configuration will indicate to the plugin which Jawr servlet to start. All jawr packages start with net.jawr.*, so you can use that as a key for an appender. Jawr uses sl4j to log messages, so you can configure its tracing level along with the rest of your application. If you add none of the jawr.css.* parameters, for instance, Jawr will do no effort to serve CSS files. Note that you are not forced to use Jawr for both js and css files. Using this syntax, you will be able to define bundles as specified in the relevant documentation pages. : Jawr will use Grails’ Locale resolution strategy when it applies.: The value set for will be used for this attribute (which is ‘utf-8’ by default in Grails).This happens automatically when you start Grails in development mode (but keep in mind that the changes are applied after you refresh a page in your browser). In Grails, Jawr will instead listen to changes to the oovy script to reload its configuration. properties file to reload it when it changes. : The Jawr servlet can be configured to listen to changes to the.Keep in mind that there are a few property keys that don’t apply when using Jawr with Grails. Of course, the property values must be quoted in order to avoid syntax errors. Check the config file syntax page for details. properties file used in standard java web applications. The syntax you must use is exactly the same described for the. To configure Jawr you must add properties to the oovy file located at the /conf folder of your application. How to use Google Closure Compiler with Jawr How to generate base64 images in CSS with Jawr Jawr strict mode - Illegal bundle request handler
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![]() You won’t find a lot of dining options in the Lower Lot of Universal Studios Hollywood. I think, had it been warmer, we would’ve visited the water area at Super Silly Fun Land, and then, we’d probably would’ve bought a snack. We didn’t spend a lot of time in this part of the park, other than to ride Despicable Me Minion Mayhem. The area at Universal Studios Hollywood dedicated to “Despicable Me” is located in the Upper Lot. Springfield is located in the Upper Lot of Universal Studios Hollywood. Want to dine in the world of the Simpsons characters? Here are all the eateries and bars in the part of the theme park: Because we only had one day planned for the park, we decided to split food so we could try more things. Springfield restaurantsĮveryone in my family is a big “The Simpsons™” fan, so of course, we spent a lot of time in Springfield™ at Universal Studios Hollywood. But you’ll also find a dizzying assortment of unique treats, as well as more standard fare like saltwater taffy and suckers. Of course, there are Bertie Botts Every Flavor Beans and chocolate frogs inside the store. Whether you’re a Harry Potter fan or not (but especially if you are), head to Honeydukes to find the best selection of candies and treats. But, on a warm winter day, shepherd’s pie or fish and chips just didn’t appeal to the rest of us. My son fought hard to get us to have lunch at Three Broomsticks™, too. Tip: Word is, the butterbeer™ ice cream is a must-try. Maybe when we’re a little older, we’ll try again. Raising young Harry Potter fans, you’d think we’d get some butterbeer™ inside The Wizarding World of Harry Potter, but I knew from past experience, my kids would take a sip and then realize they still don’t like butterbeer. Magic Neep™ Cart (this is simply a snack cart).The following are the eateries you’ll find in this fantastic little space. Even if you aren’t a die-hard Potterhead, you can appreciate the detail of the area.Īnd if you are a big fan? You’re going to love dining here. ![]() ![]() This was one of my favorite ares in Universal Studios Hollywood, as I suspect is the case for most visitors. ![]() Let’s start first with the restaurants inside the theme park. My plan was to visit restaurants that you could only visit at Universal, but as you’ll see below, there are a lot more restaurant chains in the area that you could visit if you’re looking for familiar and predictable. I discovered that whatever you are craving, you’ll find it inside and outside Universal Studios Hollywood. Restaurant Guide to Universal Studios Hollywood & CityWalk CityWalk™ is located just outside the theme park. I’m including Universal CityWalk™ restaurants in this guide, even though you do not need a park ticket to go to them. You’ll find most of the eateries are located on the Upper Lot. It’s a little more than 400 acres and split up between the Upper Lot and Lower Lot. Universal Studios Hollywood is in Burbank, Calif. All thoughts, opinions and typos are my own.
The rare and often visually spectacular atmospheric optical phenomena that can arise from the presence of volcanic dust veils in the stratosphere, such as solar dimming, coronae or Bishop’s rings, peculiar twilight coloration and dark total lunar eclipses, have long been regarded as portents worth recording. Sulfur isotopic ratios measured in ice cores can help to make this distinction, but the approach has not been extensively applied and does not necessarily distinguish between tropospheric and lower stratospheric (below ozone layer) aerosol transport 3, 14. ![]() A further challenge is the discrimination between tropospheric and stratospheric transport of volcanic aerosol, the latter being more indicative of a climate-forcing explosive eruption 4. The dating of past volcanic events from ice cores presents several challenges owing to the complexity of atmospheric transport leading to temporally and spatially variable sulfur deposition 10, poorly constrained age models 11, 12, 13 and uncertainties in layer counting related to accumulation rates and post-depositional processes 3. ![]() These events have been linked with substantial cooling and subsistence crises 7, 9 and the combined effect of their forcing has been posited as a contributor to the onset of the Little Ice Age 5. ![]() 7) and including the colossal Samalas eruption around 1257 ce (refs. Of particular note in such records is a proliferation of sulfur-rich eruptions during the HMP (circa twelfth and thirteenth centuries), beginning with a cluster of events around 1108–1110 ce (ref. Although the geologic record constitutes the primary evidence of past volcanism, with chronologies based on radiocarbon and other radiometric methods, polar ice cores arguably furnish the most comprehensive and accessible picture of climatically notable volcanism through the compilation of sulfur deposition time series 2, 4. The resulting aerosol veils perturb the energy budget of the Earth, inducing seasonal and regional surface temperature and precipitation anomalies, whose severity in combination with societal vulnerabilities has been linked to historical cases of agronomic and pasturage deficits, civil and political unrest, pestilence and migration 6. Large explosive volcanic eruptions can inject enormous quantities of sulfur-bearing gases into the stratosphere, where they generate sulfate aerosols 1. Our findings offer support for further investigation of the decadal-scale to centennial-scale climate response to volcanic eruptions. Five further eruptions, including one responsible for high sulfur deposition over Greenland circa 1182 ce, affected only the troposphere and had muted climatic consequences. By combining this new record with aerosol model simulations and tree-ring-based climate proxies, we refine the estimated dates of five notable eruptions and associate each with stratospheric aerosol veils. Here we shed new light on explosive volcanism during the HMP, drawing on analysis of contemporary reports of total lunar eclipses, from which we derive a time series of stratospheric turbidity. This particularly hinders investigation of the role of large, temporally clustered eruptions during the High Medieval Period (HMP, 1100–1300 ce), which have been implicated in the transition from the warm Medieval Climate Anomaly to the Little Ice Age 5. ![]() However, despite progress in ice-core dating, uncertainties remain in these key factors 4. Understanding the far-field societal impacts of eruption-forced climatic changes requires firm event chronologies and reliable estimates of both the burden and altitude (that is, tropospheric versus stratospheric) of volcanic sulfate aerosol 2, 3. Explosive volcanism is a key contributor to climate variability on interannual to centennial timescales 1. |