Oracle Hyperion Interactive Reporting (Interactive Reporting) software is a module of Oracle Business Intelligence Suite Enterprise Edition Plus that provides executives, business users, and analysts with intuitive user-directed relational query capabilities.
Interactive Reporting shares common administration, user management, and installation and configuration support with other Hyperion BI modules of Oracle Business Intelligence Suite Enterprise Edition Plus.
Datacentrix Enterprise Information Management (EIM) is the practice and technology of maximising the value of information by providing solutions that help customers create opportunities and address challenges related to their information – to gain better business insight, to create positive business impact, to increase process velocity, to reduce risks related to information governance and to address information security concerns. Power BI displays dashboards that are interactive, and can be created and updated from many different data sources. Power BI lets you share your dashboards so you get a single view of the business and make decisions based on the correct data. Explore and analyzeYou can pose questions from your data using everyday language and get answers in the form of interactive reports and dashboards using Power BI.
Power BI brings together all of your data so you can start analyzing the most up-to-date information. In Power BI, dashboards display tiles that represent important information about your business. Vizion Solutions is a 1-Tier Microsoft Power BI Cloud Service Provider as well as a certified Microsoft Silver Partner with extensive experience implementing Business Intelligence tools and products.
Power BI Designer provides self-service ETL and visual analytics in a unified, seamless experience. Browse back issues of SQL Server Pro, from January 2007 through the last issue published in April 2014. To become a truly data-driven enterprise, many business leaders recognize that they must extend the capabilities of self-service business intelligence (BI) and analytics to more of their business users. Get answers to questions, share tips, and engage with the SQL Server community in our Forums. To those of you looking at photos I took with my husband years ago in the privacy of our home, hope you feel great about yourselves.a€” Mary E. A total eclipse of the Sun has not been seen in the continental USA for nearly two generations.

Although people may opt for the longer durations in eastern regions of the USA, poorer weather prospects here suggest going west. Prudence may suggest observing from regions of good weather prospects with shorter durations than locations with longer durations that have higher probabilities of not seeing the eclipse at all. Currently maximum total eclipse durations are declining with the 2009 July eclipse longest of the 21st Century. Finally, maximum duration of a total solar eclipse occurs only on the center line of the eclipse path about mid-way between its ends.
Read about the Eclipse at Madras, Oregon including circumstance of the eclipse in Part  4. From interactive dashboards in a readily available context, to complex data modeling for fully ad hoc access to source data, Interactive Reporting can pull together data from disparate sources to produce easy to use charts, pivot tables, highly formatted reports, and more. This common infrastructure provides one point of access for end users to all content while reducing the maintenance required for IT professionals.
By bringing structure to unstructured information through a well-designed EIM strategy companies can unleash the power of information.
It is a free desktop data discovery tool that can be downloaded (32-bit and 64-bit options) and installed side-by-side with any version of Office or Excel on Windows. A seven minute duration will not happen again until 2150 June (7m14s) while a total eclipse with a duration near maximum is nearly two centuries in the future. Not until 2078 will total eclipse durations begin to increase when Saros cycle 139 begins to bring eclipses of longer and longer durations.
This position may often be difficult to access as it was, for example, during the 2012 November Australia eclipse.
Although eclipse durations have their maximum values along points on the central line, these durations diminish with increasing distance from the central line. Almost half are approximately three minutes or less (as will be with the 2017 August eclipse). This will not happen until the remarkable 2186 July total eclipse (7m29s), the longest duration of totality during the years -2000 to +4000.

For this eclipse, maximum duration was 4m02s over the central Pacific Ocean and not the Australian mainland.
Annular eclipses occur when the Moon's disk is not large enough to hide the entire solar disk at maximum eclipse. Unfortunately, this long duration will take place about 400 mi (640 km) east of South America in the Atlantic Ocean, 500 mi (800 km) north of the equator. Fortunately, greatest duration for the 2017 August eclipse does occur over the mainland USA. Totality is a two minute eclipse on the West Coast with the east coast having 34 seconds more.
Thus, western location may again have an advantage since summer storms tend to build during afternoon hours, a common occurrence during summer months.
The duration of totality decreases slowly at first with the distance from the central line of totality then increases rapidly.
Although much less spectacular than total solar eclipses, central durations are often much longer.
It is an optional Power BI content authoring option for users that are unable to upgrade to the latest version of Excel. The approximate range in altitude of the Sun in degrees during the eclipse is also shown for both west and east regions. For example, at a distance of 60% away from the central line to the edge of totality, the duration is still 80% of maximum.
Even if the fractional distance from the central line is one half, the loss in duration is only about 15%.
Hence, observers usually do not need to be exactly on the central line to experience most of the duration of totality.

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