Media Services – Audio & video streaming | Microsoft Azure

What is Media Services?

Azure Media Services powers consumer and enterprise streaming solutions worldwide. Combining powerful and highly scalable cloud-based encoding, encryption, and steaming components, Media Services helps customers with valuable and premium video content easily reach larger audiences on todays most popular digital devices, such as tablets and mobile phones. Live broadcastersof sporting events, news, concerts, town meetings, and moreand linear channel operators offering popular over-the-top programming and services are turning to Azure as their platform of choice.

Additionally, with exciting new features such as Azure Media Indexer to enhance discoverability, cross-platform players to simplify distribution, cloud DVR capabilities to move easily from live content to on-demand programming, and a large ecosystem of value-added third-party partners, Media Services is truly providing customers with video content as a best-in-class solution. Come have a look yourself, and see how Media Services can power your end-to-end media workflow.

Quickly deliver scalable subscription video on demand (VOD), transactional VOD, advertising VOD, and over-the-top services. Use our CDSA- and ISO-certified cloud to reduce costs and deliver content to multiple platforms from Azure data centers worldwide.

Support common encryption and multiple DRM technology such as Microsoft PlayReady and Google Widevine, or Advanced Encryption Standard (AES) to protect your content.

Seamlessly integrate with the Media Services streaming platform to lower costs by encoding once and delivering in multiple formats with dynamic packaging.

Azure Media Encoder and Media Encoder Premium offer studio-grade encoding at cloud scale.

Media Services is a highly flexible platform capable of handling everything from small scale local events to the largest events on the planet like the FIFA World Cup and the 2014 Sochi Winter Olympics.

Use cases include event based streaming and 24×7 linear streaming with cloud DVR workflows.

Media Services is a great platform for enabling businesses large and small to reach their employees and customers. The platform capabilities, combined with partner solutions, make it easy to do more with video in your organization. Its been used by several enterprises for purposes such as training, corporate communication, and council meetings. Media Services provides scalable, always-available, secure delivery of video to both employees and external customers via the Azure website.

Azure Content Delivery Network lets you deliver high-bandwidth content to users around the world with low latency and high availability via a robust network of global data centers. It sends audio, video, applications, images, and other files to users from the nearest servers. This dramatically increases speed and availability, resulting in significant user experience improvements. Learn more

Studio Grade encoding at Cloud Scale

Learn more

A single player for all your playback needs

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Enhance discoverability and accessibility of media

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Securely deliver content using AES or multi-DRM

Learn more

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Media Services – Audio & video streaming | Microsoft Azure

Media Cloud – Wikipedia, the free encyclopedia

Media Cloud is an open-source content analysis tool that aims to map news media coverage of current events. It “performs five basic functions — media definition, crawling, text extraction, word vectoring, and analysis.”[1] Media cloud “tracks hundreds of newspapers and thousands of Web sites and blogs, and archives the information in a searchable form. The database … enable[s] researchers to search for key people, places and events from Michael Jackson to the Iranian elections and find out precisely when, where and how frequently they are covered.”[2] Media Cloud was developed by the Berkman Center for Internet & Society at Harvard University and launched in March 2009.[3][4] It’s distributed under the GNU GPL 3+.[5]

As of October 2011, Media Cloud tracks news from mostly U.S. sources. It “collects news stories” in sets from:[6]

On May 6, 2011 the Berkman Center relaunched Media Cloud, a platform designed to let scholars, journalists and anyone interested in the world of media ask and answer quantitative questions about media attention. For more than a year, weve been collecting roughly 50,000 English-language stories a day from 17,000 media sources, including major mainstream media outlets, left and right-leaning American political blogs, as well as from 1000 popular general interest blogs.[7] The data was used to analyze the differences in coverage of international crises in professional and citizen media and to study the rapid shifts in media attention that have accompanied the flood of breaking news thats characterized early 2011.[7] International research has lead way to publishing of new research that uses Media Cloud to help us understand the structure of professional and citizen media in Russia and in Egypt.[7] The relaunch of Media Cloud allows users who are interested in using its tools to analyze what bloggers and journalists are paying attention to, ignoring, celebrating or condemning.”[7]

First, Media Cloud chooses a set of media sources and uncovers the feeds for each.[1] Each feed is then crawled in order to determine if any stories have been added to any feed.[1] All content is then extracted of each relevant story. Any advertisements or other navigation pages are left behind.[1] The text of each story is broken down into word counts, which shows the different word choices that each media source uses in discussing any relevant topic.[1]The word counts are then analyzed and published to show data trends.[1]

Media Cloud was used from September 2010 through January 2012 to obtain data for a study at the Berkman Center for Internet & Society that analyzed a set of 9,757 online stories related to the COICA-SOPA-PIPA debate. The open source application was utilized for the text and link analysis portion of the research.[8] Findings from this research were published in July 2013[2].

The Berkman Center for Internet & Society website offers an interactive visualization map[3] from this study, which was created to depict media sources (nodes, which appear as circles on the map with different colors denoting different media types) [and] track media sources and their linkages within discrete time slices and allows users to zoom into the controversy to see which entities are present in the debate during a given period[8] This map allows for the visualization of how the COICA-SOPA-PIPA controversy evolved over time by using link analysis.

Many companies are taking advantage of the ability to analyze and organize this new data that media cloud can create. Companies such as RAMP offer a “cloud-based” way to analyze and create every type of metadata.[9]

Media cloud’s key functionality comes from using web crawling to periodically fetch articles from various sources and then break them down into words that are counted. These word counts are then analyzed to determine what sources are saying about certain news.[1] This process is not unique to Media Cloud and in fact is an application of the recently popular stream algorithms. These are algorithms characterized by operating on a continuous and unending stream of data, rather than waiting for a complete batch of information to be assembled. These algorithms are very useful because they allow monitoring of trends without having to know which topics are going to be the most popular. This type of functionality first noticeably emerged with network managers trying to dynamically see which sites have the highest traffic volumes. From there, stream algorithms have been used to have programs dynamically act on financial information, and by researchers whose experiments generate more data than can be analyzed, so stream algorithms are used to dynamically filter the initial data.[10] Media cloud has similarly taken advantage of the functionality of stream algorithms to dynamically associate words to news as it crawls through various sources, and then provide its signature service of generating sentences based on words that the users are interested in and related media reports.

The day that Media Cloud relaunched, Ethan Zuckerman said, “We hope the tools we’re providing are a complement to amazing efforts like Project for Excellence in Journalism’s News Coverage and New Media indices–we consider their tools the gold standard for understanding what topics are discussed in American media. PEJ works their magic using talented teams of coders, who sample different corners of the media ecosystem to find out what’s being discussed. We use huge data sets, algorithms, and automation to give a different picture, one focused on language instead of topic.”[7]

Future uses for Media Cloud can involve smart phone or tablet applications to introduce the platform to users away from a computer. A Media Cloud app could serve as a news source while on the go for users. If Media Cloud were to expand into different information sites, it could target social media sites and incorporate news into them. Twitter and Facebook have incorporated features for trending news and topics similar to what Media Cloud aims to do.

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Media Cloud – Wikipedia, the free encyclopedia

Nebula – Wikipedia, the free encyclopedia

A nebula (Latin for “cloud”;[2] pl. nebulae, nebul, or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as “spiral nebulae”) before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble and others.

Most nebulae are of vast size, even hundreds of light years in diameter.[3] Although denser than the space surrounding them, most nebulae are far less dense than any vacuum created in an Earthen environment – a nebular cloud the size of the Earth would have a total mass of only a few kilograms. Nebulae are often star-forming regions, such as in the “Pillars of Creation” in the Eagle Nebula. In these regions the formations of gas, dust, and other materials “clump” together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets and other planetary system objects.

Around 150 AD, Claudius Ptolemaeus (Ptolemy) recorded, in books VII-VIII of his Almagest, five stars that appeared nebulous. He also noted a region of nebulosity between the constellations Ursa Major and Leo that was not associated with any star.[4] The first true nebula, as distinct from a star cluster, was mentioned by the Persian/Muslim astronomer, Abd al-Rahman al-Sufi, in his Book of Fixed Stars (964).[5] He noted “a little cloud” where the Andromeda Galaxy is located.[6] He also cataloged the Omicron Velorum star cluster as a “nebulous star” and other nebulous objects, such as Brocchi’s Cluster.[5] The supernova that created the Crab Nebula, the SN 1054, was observed by Arabic and Chinese astronomers in 1054.[7][8]

In 1610, Nicolas-Claude Fabri de Peiresc discovered the Orion Nebula using a telescope. This nebula was also observed by Johann Baptist Cysat in 1618. However, the first detailed study of the Orion Nebula wouldn’t be performed until 1659 by Christiaan Huygens, who also believed himself to be the first person to discover this nebulosity.[6]

In 1715, Edmund Halley published a list of six nebulae.[9] This number steadily increased during the century, with Jean-Philippe de Cheseaux compiling a list of 20 (including eight not previously known) in 1746. From 175153, Nicolas Louis de Lacaille cataloged 42 nebulae from the Cape of Good Hope, with most of them being previously unknown. Charles Messier then compiled a catalog of 103 “nebulae” (now called Messier objects, which included what are now known to be galaxies) by 1781; his interest was detecting comets, and these were objects that might be mistaken for them.[10]

The number of nebulae was then greatly expanded by the efforts of William Herschel and his sister Caroline Herschel. Their Catalogue of One Thousand New Nebulae and Clusters of Stars was published in 1786. A second catalog of a thousand was published in 1789 and the third and final catalog of 510 appeared in 1802. During much of their work, William Herschel believed that these nebulae were merely unresolved clusters of stars. In 1790, however, he discovered a star surrounded by nebulosity and concluded that this was a true nebulosity, rather than a more distant cluster.[10]

Beginning in 1864, William Huggins examined the spectra of about 70 nebulae. He found that roughly a third of them had the emission spectrum of a gas. The rest showed a continuous spectrum and thus were thought to consist of a mass of stars.[11][12] A third category was added in 1912 when Vesto Slipher showed that the spectrum of the nebula that surrounded the star Merope matched the spectra of the Pleiades open cluster. Thus the nebula radiates by reflected star light.[13]

In about 1922, following the Great Debate, it had become clear that many “nebulae” were in fact galaxies far from our own.

Slipher and Edwin Hubble continued to collect the spectra from many diffuse nebulae, finding 29 that showed emission spectra and 33 had the continuous spectra of star light.[12] In 1922, Hubble announced that nearly all nebulae are associated with stars, and their illumination comes from star light. He also discovered that the emission spectrum nebulae are nearly always associated with stars having spectral classifications of B1 or hotter (including all O-type main sequence stars), while nebulae with continuous spectra appear with cooler stars.[14] Both Hubble and Henry Norris Russell concluded that the nebulae surrounding the hotter stars are transformed in some manner.[12]

Many nebulae or stars form from the gravitational collapse of gas in the interstellar medium or ISM. As the material collapses under its own weight, massive stars may form in the center, and their ultraviolet radiation ionizes the surrounding gas, making it visible at optical wavelengths. Examples of these types of nebulae are the Rosette Nebula and the Pelican Nebula. The size of these nebulae, known as HII regions, varies depending on the size of the original cloud of gas. New stars are formed in the nebulae. The formed stars are sometimes known as a young, loose cluster.

Some nebulae are formed as the result of supernova explosions, the death throes of massive, short-lived stars. The materials thrown off from the supernova explosion are ionized by the energy and the compact object that it can produce. One of the best examples of this is the Crab Nebula, in Taurus. The supernova event was recorded in the year 1054 and is labelled SN 1054. The compact object that was created after the explosion lies in the center of the Crab Nebula and is a neutron star.

Other nebulae may form as planetary nebulae. This is the final stage of a low-mass star’s life, like Earth’s Sun. Stars with a mass up to 810 solar masses evolve into red giants and slowly lose their outer layers during pulsations in their atmospheres. When a star has lost enough material, its temperature increases and the ultraviolet radiation it emits can ionize the surrounding nebula that it has thrown off.

Objects named nebulae belong to four major groups. Before their nature was understood, galaxies (“spiral nebulae”) and star clusters too distant to be resolved as stars were also classified as nebulae, but no longer are.

Not all cloud-like structures are named nebulae; HerbigHaro objects are an example.

Most nebulae can be described as diffuse nebulae, which means that they are extended and contain no well-defined boundaries.[17] In visible light these nebulae may be divided into emission and reflection nebulae. Emission nebulae emit spectral line radiation from ionized gas (mostly ionized hydrogen);[18] they are often called HII regions (the term “HII” is used in professional astronomy to refer to ionized hydrogen).

Reflection nebulae themselves do not emit significant amounts of visible light, but are near stars and reflect light from them.[18] Similar nebulae not illuminated by stars do not exhibit visible radiation, but may be detected as opaque clouds blocking light from luminous objects behind them; they are called “dark nebulae”.[18]

Although these nebulae have different visibility at optical wavelengths, they are all bright sources of infrared emission, chiefly from dust within the nebulae.[18]

Planetary nebulae form from the gaseous shells that are ejected from low-mass asymptotic giant branch stars when they transform into white dwarfs.[18] They are emission nebulae with spectra similar to those of emission nebulae found in star formation regions.[18] Technically they are HII regions, because most hydrogen will be ionized, but they are denser and more compact than the nebulae in star formation regions.[18] Planetary nebulae were given their name by the first astronomical observers who became able to distinguish them from planets, who tended to confuse them with planets, of more interest to them. Our Sun is expected to spawn a planetary nebula about 12 billion years after its formation.[19]

A protoplanetary nebula (PPN) is an astronomical object which is at the short-lived episode during a star’s rapid stellar evolution between the late asymptotic giant branch (LAGB) phase and the following planetary nebula (PN) phase.[20] During the AGB phase, the star undergoes mass loss, emitting a circumstellar shell of hydrogen gas. When this phase comes to an end, the star enters the PPN phase.

The PPN is energized by the central star, causing it to emit strong infrared radiation and become a reflection nebula. Collaminated stellar winds from the central star shape and shock the shell into an axially symmetric form, while producing a fast moving molecular wind.[21] The exact point when a PPN becomes a planetary nebula (PN) is defined by the temperature of the central star. The PPN phase continues until the central star reaches a temperature of 30,000 K, after which is it hot enough to ionize the surrounding gas.[22]

A supernova occurs when a high-mass star reaches the end of its life. When nuclear fusion in the core of the star stops, the star collapses. The gas falling inward either rebounds or gets so strongly heated that it expands outwards from the core, thus causing the star to explode.[18] The expanding shell of gas forms a supernova remnant, a special diffuse nebula.[18] Although much of the optical and X-ray emission from supernova remnants originates from ionized gas, a great amount of the radio emission is a form of non-thermal emission called synchrotron emission.[18] This emission originates from high-velocity electrons oscillating within magnetic fields.

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Nebula – Wikipedia, the free encyclopedia

Cloud Media


Check out our Products


Monday-Friday 8AM-5PM

Saturday 9AM-2PM





Tunapuna (Infront of Toymart)

SANGRE GRANDE ( Ojoe Rd & Sangre Grande Roundabout)


Diego Martin


Pt Fortin

Contact us if you have a prime location to rent.


We are always looking to provide the ideal products. If you have ideas how we can make a better product

or serve you better, wed love to hear from you.

Send us a quick note using the form to the bottom or call us at (868) 289-0189)

The Ariapita Avenue location is located just off the busy intersection at Lapeyrouse Cemetary facing the west bound traffic. Also visible as commuters turn left unto Ariapita from road alongside Powergen.The board is strategically located by Amnesia Club to also appeal to pedestrian traffic and party go-ers. Size 7ft x 10ft

At EMR Tunapuna the billboard welcomes the commuters travelling

east to Tunapuna just after the bend at Exodus pan yard. It is surrounded by major shopping facilities such as Auzonville Mall, large private hospital and health services, commercial banks including ScotiaBank, IBL Bank and FCB Bank. At night the area around the billboard is still very active since Go Figure Fitness gym is open to its members as late as 10pm. Traffic flow is gridlocked in this area for more than 18 hours daily as the busy Tunapuna Market area is just a few buildings away. Size 10ft x 14 ft

Strategically placed to ensure viewing from two lines of traffic at the traffic lights of the busy intersection. The vehicles proceeding North from Trincity Mall turn on to the Eastern Main Rd to face the Billboard and Vehicles are set in Westbound lane for more than 20 mins all day before crossing lights and proceeding past the Billboard. Clients ads are viewed more than 3 times in a rotation from this lane of traffic.

7ft x10ft

163 Eastern Main Road, Tunapuna,Trinidad. W.I.


call: (868) 289-0189

Trincity (Dinsley Junction)

Corner EMR & Curepe Junction

The town that is labelled the public transport central of Trinidad has a bustling flow of commuters, pedestrians, buses and taxis. Cloud’s Premier billboard is strategically placed opposite the PTSC bus terminal to be viewed by all lines of traffic and even as far as the popular Southern Main Road doubles and fast food outlets. Also within the vicinity are Banking ATMs and roads leading to the University of the West Indies St. Augustine Campus. Size 7ft x 10ft

This 14ft by 24ft Billboard is located immediately after the UWI St. Augustine intersection and can be seen from as far as the Pasea Tunapuna traffic lights. The traffic flow alongside this billboard is standstill throughout the day and the board is strategically positioned to appeal to the East Bound evening traffic. At instances the viewing audience is actually 6 lanes of standstill highway traffic.

At this location the billboard is located on the Ojoe Rd along side the Sangre Grande taxi stand facing the busy Sangre Grande roundabout. The pedestrian traffic to and from this taxi stand are in the hundreds daily and the vehicular traffic at the roundabout is at a constant standstill throughout the day allowing the viewers of this billboard to view ads for at least a period of 3-5 mins.


See our premier digital billboards strategically located at the following locations:

Located on the Eastern Main Road opposite FCB bank and RBC and between two Republic bank Branches. On the compound of popular S and S Bar and Lounge. The traffic heading east is usually at a standstill for more than 5 minutes especially on evenings from 2pm to 8pm. 8ft x 14ft

Located at Issac Junction Couva. This 8ft x14ft Billboard is strategically placed to be seen by vehicles approaching from the highway and to be seen by persons visiting KFC, JTA supermarket and Subway. Also at this Subway spot is a Taxi Hub which allows for pedestrians awaiting transport to view the board daily.

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Cloud Media

Cloud Media Marketing

Message from Kayleigh Apicerno, Owner of CMM

For the past few years, I have had this crazy idea to start my own business. The beginning of 2015 seemed to be the right time to finally take the plunge.

What do I want to do with this business? My mission is to give you the understanding and skills you need to be able to be comfortable with social media and mobile technology. For the individual, the goal is to become familiar with the various platforms and learn how to use them.

For the small business owner, the goal is to understand and be able to leverage social media to reach your marketing goals.There are companies out there that will set up all of your accounts and post on your behalf. What I have learned is that many (if not most) small businesses want to keep the control and do not want someone who is not a part of their business to speak directly to their customers. The problem is that these small businesses are busy doing what they are good at and do not have the time or the skills to be able to keep up with social media.

Here is a little bit more about me: I have been an active social media user and blogger for over ten years, starting with Facebook and MySpace back in college. I have been a professional blogger and an admin on a dozen or so Facebook Pages. I have also created over a hundred pieces of content (edited photos, infographics, facebook cover photos, event flyers, etc) for a variety of social media campaigns and events.

When I am not working, I volunteer. I am currently serving as Chair for the Young Emerging Professionals (a Committee of the Greater Valley Chamber of Commerce), I am a board member ofMy City Kitchen, the web master ofSeymour Historical Societywebsite, and I volunteer with other community projects.

In 2014, I was awarded a Volunteer Appreciation award from the Seymour Historical Society and was one of the four Honorees of Women Making A Difference In The Valley. I am a 2013 graduate of the Leadership Greater Valley Program, and I have a Bachelors Degree in Business Administration with a concentration in Marketing from Southern CT State University.

Here is where you can find me online: Facebook: /CloudMediaMkt Twitter: @Kayleighs_Cloud Tumblr: GreatfulEveryDay Pinterest: Kayleigha14 Google+: +KayleighGoogle+: +CloudMediaMkt Instagram: Kayleighs_Cloud

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Cloud Media Marketing

RainCloud Media

Over 100 million people are reached through social media published by RainCloud Media every day.

We’re a turn-key social media firm serving clients across six continents. Our clients include major brands, record labels, artists/bands (pop, hip hop, rock, country, worship and gospel), celebrities, entertainers, professional athletes, publishing houses, best-selling authors, international non-profits and large ministries.

We’ve launched multiple New York Times bestselling books, secured #1 Billboard placement for multiple artists with social media strategy and have generated millions of dollars of sales and donations for clients online.

And, since we chose to dive into the world of social media in 2010, weve grown from a tight crew of social media architects, digital artists, data geeks, content creators and project managers into a turn-key agency. We serve every major enterprise-level vertical and have achieved spectacular results for our clients.

You have seen our work and just dont realize it. Thats our goal.

Think we might be able to take your social media to another level?

Send us a note!

-The RainCloud Team

P.S. Due to volume, we are unable to respond to each request for information. But, if we think you might be a strong addition to our family of clients, well reach out.

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RainCloud Media

About Media Cloud | Media Cloud

Media Cloud, a joint project of the Berkman Center for Internet & Society at Harvard University and the Center for Civic Media at MIT, is an open source, open data platform that allows researchers to answer complex quantitative and qualitative questions about the content of online media.

History of the Project Print newspapers are declaring bankruptcy nationwide. High-profile blogs are proliferating. Media companies are exploring new production techniques and business models in a landscape that is increasingly dominated by the Internet. In the midst of this upheaval, it is difficult to know what is actually happening to the shape of our news. Beyond one-off anecdotes or painstaking manual content analysis, there are few ways to examine the emerging news ecosystem.

The idea for Media Cloud emerged through a series discussions between faculty and friends of the Berkman Center. The conversations would follow a predictable pattern: one person would ask a provocative question about what was happening in the media landscape, someone else would suggest interesting follow-on inquiries, and everyone would realize that a good answer would require heavy number crunching. Nobody had the time to develop a huge infrastructure and download all the news just to answer a single question. However, there were eventually enough of these questions that we decided to build a tool for everyone to use.

Some of the early driving questions included:

Media Cloud offers a way to quantitatively examine all of these challenging questions by collecting and analyzing the news stream of tens of thousands of online sources.

Using Media Cloud, academic researchers, journalism critics, policy advocates, media scholars, and others can examine which media sources cover which stories, what language different media outlets use in conjunction with different stories, and how stories spread from one media outlet to another.


Media Cloud is made possible by the generous support of theFord Foundation, theOpen Society Foundations, and theJohn D. and Catherine T. MacArthur Foundation.


Past and present collaborators includeMorningside Analytics, Betaworks,

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About Media Cloud | Media Cloud

Sungale Cloud TV Box-Turn Your Television into a Smart TV

Cloud TV Box, not just a media player, it instantly converts your TV set into a ‘full- pledged’ Smart TV! Watch TV

Hundreds of TV programs from popular channels such as CNN, CBS, CBN, ABC, FOX, PBS, CNBC, Bloomberg, and more are available in brilliant1080p or 720p high definition. The programs are updated daily in VOD mode for your convenience.

Famous video content providers such as YouTube, Netflix, Veoh, Dailymotion, Vimeo, and Break are preloaded for you to enjoy high definition movies and video programs in 1080p or 720p. Hundreds of video sources are in a backup list for users to install. Cloud TV Box also allows you to add your own favorite video websites.

With the convenience of a browser, you can surf the internet together with your family for a more enjoyable experience than surfing on your computer.

The Cloud TV Box allows users to link to their favorite social media such as Facebook, Twitter, MSN, Skype and more

Play Games

Play a lot more than just Angry Birds. Download and play from a large assortment of available games. The Cloud TV Box has also provided an independent Game Folder for you to file and organize your favorite game apps.

The Cloud TV Box allows users to download and play a variety of educational apps for parents to learn and enjoy education programs with their kids together. An independent icon is designed to put on the home page for the users to file and organize your educational apps.

You can even use Cloud TV Box to process your documents.

The Cloud TV Box allows you to go to Android Play Store to download and install apps.

You may feel tired when you have watched TV too long. If so, you can easily find your favorite local radio stations or your native country’s stations on your Cloud TV Box, then, stand up to walk around and listen to the radio broadcast.

Too many functions can be always an annoyed issue for internet related devices, especially when the device is used for entertainment. Nobody likes to spend time learning and remembering where the functions are hidden when relaxing and looking for some entertainment. The Cloud TV Box is the first internet entertainment device on which the functions are deliberately divided and put on different partitions, so that users can easily find and play the programs they like. The methodology of the division of screen partitions is our pride, we even can see the followers are coming on.

From other TV boxes, you may find you need to provide your credit card information to register before you can watch any programs, which means you may be charged in the future for any programming changes and/or commercial plan. The registration is not a compulsory step for the initial setup of your Cloud TV box, and the Cloud TV Box does not need you to provide your credit card information, and so whether you choose to register or not, we provide the same content to all our customers. Cloud TV Box is an ABSOLUTELY FREE platform.

From other TV box, even it is claimed “The Easiest Setup”, you will find that you need to go to a computer to select some programs as an initial operation, then, you can use the box. The Cloud TV Box has plenty of preloaded programs, and you can enjoy the Plug And Play. Moreover, you can select and add as many video sources as possible with your pleasure.

For some games, you may need the convenience of an Air Mouse. The Cloud TV Box is compatible with various air mouse.

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Sungale Cloud TV Box-Turn Your Television into a Smart TV

g! Entertainment & Control Systems:Cloud Media


The Cloud/Media | Whatever Entertains You, Whenever You Choose

ELAN g! embraces and integrates with Cloud Technology to make all your favorite multimedia files available to you at anytime, anywhere in your house, from any source you choose to connect to. All your favorite music, movies, information, entertainment, and photo libraries can be accessed at any time with a touch of the screen. There’s nothing for you to do but enjoy it all.

The Cloud

Whether it’s Sirius, AM or FM Music or Internet content from the cloud, ELAN can give you access to it all everywhere in your home.







Add Sirius* radio and AM/FM music enjoyment around the home. Available in three models. In an ELAN multi-room system, 2-way feedback, including station call letters, frequency, genre, song name and artist, can be viewed on any ELAN Touch Screen, TS2 Touchpad or HR2 Remote. (Please note that displayable data varies depending on source, i.e. standard AM/FM, RBDS, or Sirius radio.)

*Sirius available in the US only.

DT22 Sirius-Ready Dual AM/FM Tuner

DT22-240 Dual AM/FM Tuner

DT11 Sirius-Ready AM/FM Tuner

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g! Entertainment & Control Systems:Cloud Media