We'll notify you via e-mail of your refund once we've received and processed the returned item. A flexible, liquid foundation made from pigments that blur and perfect to reflect your perfect skin tone for light, buildable coverage and a radiant finish. If you need to return an item, simply login to your account, view the order using the 'Complete Orders' link under the My Account menu and click the Return Item(s) button. /rebates/&252fbecca-aqua-luminous-perfecting-foundation252f11476210.html26tc3dbing-&idskinstore&ra9. This time period includes the transit time for us to receive your return from the shipper (5 to 10 business days), the time it takes us to process your return once we receive it (3 to 5 business days), and the time it takes your bank to process our refund request (5 to 10 business days). You should expect to receive your refund within four weeks of giving your package to the return shipper, however, in many cases you will receive a refund more quickly. A flexible, liquid foundation made from pigments that blur and. We'll also pay the return shipping costs if the return is a result of our error (you received an incorrect or defective item, etc.). Becca Aqua Luminous Perfecting Foundation - Tan by Becca for Women - 1 oz Foundation. You may return most new, unopened items within 30 days of delivery for a full refund.
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The US National Ignition Facility, which uses laser-driven inertial confinement fusion, was designed with a goal of break-even fusion the first large-scale laser target experiments were performed in June 2009 and ignition experiments began in early 2011. Research into developing controlled fusion inside fusion reactors has been ongoing since the 1930s, but the technology is still in its developmental phase. While fusion was achieved in the operation of the hydrogen bomb (H-bomb), for it to be a useful energy source controlled, sustained fusion is required. Self-sustaining nuclear fusion was first carried out on 1 November 1952, in the Ivy Mike hydrogen (thermonuclear) bomb test. Research into fusion for military purposes began in the early 1940s as part of the Manhattan Project. In the remainder of that decade, the theory of the main cycle of nuclear fusion in stars was worked out by Hans Bethe. Building on the early experiments in artificial nuclear transmutation by Patrick Blackett, laboratory fusion of hydrogen isotopes was accomplished by Mark Oliphant in 1932. Quantum tunneling was discovered by Friedrich Hund in 1927, and shortly afterwards Robert Atkinson and Fritz Houtermans used the measured masses of light elements to demonstrate that large amounts of energy could be released by fusing small nuclei. In 1920, Arthur Eddington suggested hydrogen–helium fusion could be the primary source of stellar energy. The extreme astrophysical event of a supernova can produce enough energy to fuse nuclei into elements heavier than iron. Nuclear fusion uses lighter elements, such as hydrogen and helium, which are in general more fusible while the heavier elements, such as uranium, thorium and plutonium, are more fissionable. The opposite is true for the reverse process, called nuclear fission. Fusion of nuclei lighter than these releases energy (an exothermic process), while the fusion of heavier nuclei results in energy retained by the product nucleons, and the resulting reaction is endothermic. These elements have a relatively small mass and a relatively large binding energy per nucleon. Nuclear fusion is the process that powers active or main-sequence stars and other high-magnitude stars, where large amounts of energy are released.Ī nuclear fusion process that produces atomic nuclei lighter than iron-56 or nickel-62 will generally release energy. This difference in mass arises due to the difference in nuclear binding energy between the atomic nuclei before and after the reaction. The difference in mass between the reactants and products is manifested as either the release or absorption of energy. Nuclear fusion is a reaction in which two or more atomic nuclei, usually deuterium and tritium (hydrogen variants), are combined to form one or more different atomic nuclei and subatomic particles ( neutrons or protons). The current version of ISO standards are ISO/IEC 23271:2012 and ISO/IEC 23270:2006. International Organization for Standardization (ISO) followed in April 2003. By December 2001, both were ratified Ecma International (ECMA) standards. In August 2000, Microsoft, and Intel worked to standardize Common Language Infrastructure (CLI) and C#. By early 2000, the first beta versions of. NET Framework in the late 1990s, originally under the name of Next Generation Windows Services (NGWS), as part of the. No further changes to that version are planned. Only monthly security and reliability bug fixes to that version have been released since then. NET Framework 4.8, the last version of the framework as a proprietary offering. NET development to more closely follow a contemporary model of a community-developed software project, including issuing an update to its patent promising to address the concerns. Despite the standardization efforts, developers, mainly those in the free and open-source software communities, expressed their unease with the selected terms and the prospects of any free and open-source implementation, especially regarding software patents. NET Framework began as proprietary software, although the firm worked to standardize the software stack almost immediately, even before its first release. Microsoft also produces an integrated development environment for. The framework is intended to be used by most new applications created for the Windows platform. Programmers produce software by combining their source code with. NET Framework.įCL provides the user interface, data access, database connectivity, cryptography, web application development, numeric algorithms, and network communications. The CLR is an application virtual machine that provides services such as security, memory management, and exception handling. NET Framework execute in a software environment (in contrast to a hardware environment) named the Common Language Runtime (CLR). It includes a large class library called Framework Class Library (FCL) and provides language interoperability (each language can use code written in other languages) across several programming languages. It was the predominant implementation of the Common Language Infrastructure (CLI) until being superseded by the cross-platform. NET Framework (pronounced as " dot net") is a proprietary software framework developed by Microsoft that runs primarily on Microsoft Windows. Windows 98 or later, Windows NT 4.0 or later Martin Daubney, a former features editor of FHM, noted that it added a "sense of mystique and occasion" to the issue, which went on to sell 936,000 copies. The 1998 poll was voted on by half a million readers, with its companion issue being sold sealed inside a plastic cover. Over subsequent years, the list's popularity continued to grow. The 1999 "100 Sexiest Women" poll was launched by projecting a 60 ft (18 m) naked image of Gail Porter onto the Palace of Westminster. Anderson had posed half-naked on the front cover of the magazine earlier that year. A spokesman for FHM described her as the "thinking man's crumpet" and a "surprise winner". A total of 10,000 votes were cast, with American actress Gillian Anderson being announced as the winner in September. The following year's poll was the first to be opened up to the general public. German supermodel Claudia Schiffer topped the inaugural chart. The first 100 Sexiest Women list was published in 1995, and was compiled exclusively by a panel of 250 judges. The winner of the 2004 list was English singer Louise Redknapp, who had placed on every 100 Sexiest list since 1996, while the 2014 chart topper was singer Rachel Stevens, who had peaked at number two in 2001, 20. To commemorate the 10th and 20th anniversaries of the 100 Sexiest Women list, two one-off charts were compiled in April 2004 and May 2014, to recognise the sexiest women up to those points. These lists were topped by the American actress Mischa Barton and the American socialite Kimberly Stewart, respectively. The most recent holder of the Sexiest Woman title is the Israeli Actress Gal Gadot in 2017.Īlongside the 100 Sexiest Women list, FHM has also twice published a "Most Eligible Bachelorettes" list, in 20, to celebrate qualities such as "talent, star quality and cash". By the time FHM ceased publication of its print edition in January 2016, the 100 Sexiest Women list had been compiled 21 times. At 36 years old, Berry is the oldest woman ever to top the listing, while Lopez is the first to top the list more than once. Subsequent winners have included the British singer Cheryl, the American actress Halle Berry, and Jennifer Lopez. From 1996 to 2015, the poll was instead voted for by the general public with, at its height, several million votes being cast each year. The inaugural winner was German supermodel Claudia Schiffer. The first listing was published in 1995 and was voted for by a panel of 250 judges. As of 2017, each year's list is first announced through a section on FHM 's official website, FHM.com. As of 2017, the Israeli actress Gal Gadot is the most recent winner of FHM 's 100 Sexiest Women.įHM 's 100 Sexiest Women is an annual listing compiled by the monthly British men's lifestyle magazine FHM, based on which women they believe to be the " sexiest". Brewer, investigated a variety of possible connections between Pachelbel's and Heinrich Biber's published chamber music. Johann Christoph Bach, the oldest brother of Johann Sebastian Bach, was a pupil of Pachelbel. Johann Ambrosius Bach, Pachelbel, and other friends and family provided music for the occasion. Hans-Joachim Schulze, writing in 1985, suggested that the piece may have been composed for Johann Christoph Bach's wedding, on 23 October 1694, which Pachelbel attended. The circumstances of the piece's composition are wholly unknown. Another copy, previously in Hochschule der Künste in Berlin, is now lost. A single 19th-century manuscript copy of them survives, Mus.MS 16481/8 in the Berlin State Library. The Canon and Gigue in D major is one such piece. Only Musikalische Ergötzung-a collection of partitas published during Pachelbel's lifetime-is known, apart from a few isolated pieces in manuscripts. Little of his chamber music survives, however. In his lifetime, Pachelbel was renowned for his organ and other keyboard music, whereas today he is also recognized as an important composer of church and chamber music. Since the 1980s, it has also found increasingly common use in weddings and funeral ceremonies in the Western world. From the 1970s onward, elements of the piece, especially its chord progression, were used in a variety of pop songs. A 1968 arrangement and recording of it by the Jean-François Paillard chamber orchestra gained popularity over the next decade, and in the 1970s the piece began to be recorded by many ensembles by the early 1980s its presence as background music was deemed inescapable. Like his other works, Pachelbel's Canon went out of style, and remained in obscurity for centuries. Neither the date nor the circumstances of its composition are known (suggested dates range from 1680 to 1706), and the oldest surviving manuscript copy of the piece dates from 1838 to 1842. Although a true canon at the unison in three parts, it also has elements of a chaconne. Both movements are in the key of D major. The canon was originally scored for three violins and basso continuo and paired with a gigue, known as Canon and Gigue for 3 violins and basso continuo. Pachelbel's Canon (also known as the Canon in D, P 37) is an accompanied canon by the German Baroque composer Johann Pachelbel. Problems playing this file? See media help. |