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The top row shows the L1 orbits for ACE, Wind, and DSCOVR in the GSE x− y (left) and y− z (right) planes. The total portion of time between 30 June 2015 and 11 November 2019 for which the y separation is >80 R E is 69.5%, which is to say that the orbits are favorable for maintaining a large degree of separation over time. The peaks of this plot occur at times when the MSSWM would more likely be effective and vice versa for the troughs. The time series shows the maximum GSE y separation of the L1 constellation for the time period since DSCOVR reached L1 and the colors label which two of the spacecraft have the maximum separation. The coverage of the upstream solar wind along the GSE y direction, which is an important orbital characteristic for the MSSWM model, is illustrated in the bottom of Figure 1. Along the GSE z direction, ACE and DSCOVR reach ☓0 R E while Wind only reaches ☑0 R E. Along the GSE y direction, ACE and DSCOVR reach ±40 R E while Wind reaches ☑00 R E. The three L1 monitors currently in operation are Advanced Composition Explorer (ACE, Stone et al., 1998), Wind (Acuña et al., 1995), and Deep Space Climate Observatory (DSCOVR, Burt & Smith, 2012), whose orbits are shown in the top two panels of Figure 1 for the time period 1 August 2017 to 1 December 2017. For example, a significant rotation of the IMF occurring over 10 s of R E (Earth radii) can segment the bow shock into more than one region of quasiperpendicular or quasiparallel shock geometry. Such localized predictions are important considering the scale sizes of solar wind structure (Andréeová et al., 2013 Borovsky, 2018 Kessel et al., 1999). Using multiple spacecraft, gradients are resolved, and the IMF can be determined at a specific location around Earth's magnetosphere. In this paper we develop and test a multispacecraft solar wind monitor (MSSWM) with a very simple time lagging and compare against the predictions offered by each of the OMNI single-spacecraft predictions using the more complicated time-lagging technique.Ī shortcoming of the single-spacecraft method is that the predicted IMF applies across the whole bow shock or magnetopause boundary. Fortunately, OMNIWeb also provides time-lagged data streams from each of the three upstream solar wind monitors ACE, Wind, and DSCOVR, using the same assumption of planar phase fronts. This procedure begs the question how appropriate it is to choose one spacecraft over the other, especially in cases when the solar wind as measured by these monitors shows structure on scales comparable to the width of the magnetospheric system. In addition, finding the front normal using a single spacecraft can be particularly error prone (Neugebauer & Giacalone, 2010). Two out of three of the terms of the equation are founded on convenience rather than physics. (see King & Papitashvili, 2007, appendix 6), where the symbols A and B are the impact parameters, C and D are data coverage parameters, E is a logical ☑ depending on the spacecraft chosen in the prior segment, and the coefficients a, b, and c are experimentally determined weights. We propose that the realistic structure of the solar wind that is resolved with multiple solar wind monitors could be vitally important to implement as upstream conditions in global magnetospheric simulations. The multispacecraft monitor shows improvement over all three of the single-spacecraft predictions for 44% of the cases and also outperforms both ACE and Wind, which are the primary magnetic field contributors to the OMNI IMF prediction, 55% of the time. We perform a statistical study with thousands of hours of magnetospheric multiscale observations in the solar wind, comparing the prediction accuracy of the multispacecraft monitor to all of the OMNIWeb single-spacecraft monitors. The model is validated by comparing the predictions with other spacecraft observing the solar wind in situ. Understanding structure of the solar wind is vital to determine the global magnetospheric configuration, which is important in both real time as a space-weather product and data users wanting to know upstream conditions when interpreting observations. The prediction algorithm ingests all the data from the current fleet of three L1 monitors, allowing gradients in the solar wind to be resolved on scale sizes similar to the magnetosphere. A novel multispacecraft solar wind monitor is developed, which expands on the forecasting ability of OMNI by giving spatially resolved predictions. Although the sovereignty of the SARs belongs to China, they retain their own policies regarding time zones for historical reasons. In 19, Hong Kong and Macau were transferred to China from the United Kingdom and Portugal respectively, being established as special administrative regions. ĭaylight saving time was observed from 1945 to 1948, and from 1986 to 1991. Between 19, the time zone was switched repeatedly between Xinjiang Time ( UTC+06:00) and Beijing Time. Time zone changes in Tibet are undocumented, but Beijing Time was in use until at least the mid-1950s. There are two independent sources that claim the Communist Party of China, and/or the People's Republic of China, were using apparent solar time for Beijing Time before the period between 27 September 1949 and 6 October 1949, and they adopted the time of UTC+08:00 within that period of time, but the claim is dubious. However, as the Chinese Civil War came to its end in 1949–1950, regional governments under the influence of the Communist Party of China, other than those in Xinjiang and Tibet, switched to use the same time as Beijing, which is UTC+08:00, and is later known as Beijing Time or China Standard Time. A further refined system with adjustment to zone assignment in the Northwest part of Gansu was announced in 1947 for adoption in 1948. įollowing the end of World War II, the five time zone system was resumed, although there is little information about the historical usage of time in the Kunlun and Changpai zones. On 9 March 1939, when the Ministry of the Interior organized a Standard Time Conference in Chongqing, it was decided to adopt the five time zone proposal with slight modification of their borders starting from 1 June, however it was also decided that the entire country would use the Kansu-Szechwan Time ( UTC+07:00) during the Second Sino-Japanese War which began at the time. In the 1930s, the proposed five time zones had not been fully observed, causing regions in inner China area to adopt their own time standards, resulting in chaos. Īfter the defeat of Beiyang government in 1928, the mission of the Central Observatory was moved to Nanjing, and the reference time standard used for the construction of traditional Chinese Calendar was shifted from Beijing Mean Solar Time to UTC+08:00. By 1918, five standard time zones had been proposed by the Central Observatory of Beiyang government of Republic of China, including the Kunlun ( UTC+05:30), Sinkiang-Tibet ( UTC+06:00), Kansu-Szechwan ( UTC+07:00), Chungyuan ( UTC+08:00), and Changpai ( UTC+08:30). Starting in 1914, the Republic of China government began adopting the Beijing Local Mean Solar Time as the official time standard. Until 1913, the official time standard for the whole of China was still the apparent solar time of Beijing, the capital of the country at the time. However, the time zone for the rest of China remained undetermined. The practice has spread to other coastal ports, and in 1902 the "Coastal Time" was proposed to be the universal time zone for all the coastal ports in China. By the end of 19th century, the time standard provided by the observatory had been switched to GMT+08:00. In 1880s officials in Shanghai French Concession started to provide a time announcement service using the Shanghai Mean Solar Time provided by the aforementioned observatory for ships into and out of Shanghai. In the 1870s, the Shanghai Xujiahui Observatory was constructed by a French Catholic missionary. Main article: Historical time zones of China With its long-time expertise, IRAM is able to build receiver systems, which guarantee a perfect signal transmission, only affected by unavoidable quantum noise. IRAM operates its own laboratory for the development and fabrication of super-conducting junctions, employing modern coating processes under ultra-high vacuum conditions as well as micro-lithographic methods in order to structure the junctions. This process, called the photon tunnel effect, is the actual receiving process in a millimetre system, in other words, collecting and registering of the photons of incoming cosmic signals. The cosmic signal triggers electric charges between the two metal layers of the junction. The two super-conducting layers are themselves separated by a thin insulating layer of aluminium oxide, one nanometre in size (a thousand of a thousand of millimetre). This is why specially built cryostats, which are cooled by helium, maintain the receivers at a constant temperature of -269C°. The junction consists of two niobium metal layers, a metal which near absolute zero becomes super-conducting, without resistance and thus without any additional background noise. With a size of less than one micrometer (a thousandth of a millimetre), the super-conducting junction is the core piece of the receiver system, ensuring the transmission of the astronomical signal with as little background noise as possible. Using micro-mechanical manufacturing technologies, the horn, coupler and mixer are designed and manufactured at the institute’s mechanical workshop and assembled in its laboratories. This entire process has been conceived and developed by IRAM engineers, technicians and scientists. The mixer is also equipped with super-conducting circuits in order to separate the two incoming signals and to optimise the super-conducting junction’s performances. The super-conducting junction registers the difference between these two signals, the intermediate frequency, one low enough that the signal can finally be amplified. Inside the mixer, the signals are combined in the coupler to a signal with a close-by frequency that is produced by the local oscillator. Once the signals are collected by the antenna, they are focused onto the receiver, where they reach the horn and are channelled through a narrow, millimetre-sized conduit called the wave-guide, before reaching the mixer itself. Therefore, the frequency of the incoming signal is first lowered into the mixer block of the receiver, a device only a few centimetres in size, and only then amplified. However, it is technically very difficult, if not impossible, to directly amplify signals emitted at short wavelengths (or high frequencies) such as in the millimetre range. The signals have thus to be amplified before they can be analysed: this is the role of the receiver. Their weakness is such that the IRAM 30-metre telescope would have to collect them during a period spanning the entire age of the universe (13.7 billion years) to obtain enough energy to power a light bulb for one second. No roof no floor was produced by Nick Kinsey and features musical contributions from Ellen Kempner of Palehound, David Lizmi, and Kevin Copeland.When they reach the surface of an antenna, signals from cosmic sources are extremely weak. As in the video, which ends in laughter and acceptance, there is joy in surrender.” I think lightness is achieved by letting go and embracing uncertainty. I never end up finding the sandwich, just the mime pretending to chow down. I wanted to channel the slapstick work of Charlie Chaplin. She adds, regarding the video: “I chose to make the object of desire a sandwich rather than a lover…. I was searching for answers and looking for signals to affirm the love, rather than just letting go and letting things be.” In a press release, Scout states: “I wrote this song when I was over-anticipating the outcome of a newly formed romance. tour dates in support of the album and has shared a self-directed video for the album’s lead single, “signal.” View the video below, along with the album’s tracklist/cover art and a full list of upcoming tour dates. She has also confirmed a set of summer U.S. Scout Gillett has announced the release of her debut album, no roof no floor, which will be out on October 28 via Captured Tracks. A job coach may assist the person with developing self‑confidence, strength-building and overcoming weaknesses. While medication and therapy can help people with ADHD overcome a majority of their symptoms, in some cases, there is still a need for a job coach. Employment candidates who may have previously been passed over due to their disabilities, will be a valuable pool of potential employees for the growing number of unfilled positions. This, along with a lower birth rate, will leave many companies scrambling to find suitable replacements in a growing number of jobs. In the United States, 10,000 people daily are leaving the workforce to retire. The goal is to retain a solid team whose members are closely involved and engaged with your business and its internal and external stakeholders.īusinesses will be challenged both externally and internally as they adapt to changing economies and demographics of the future. Employers continuously search for people with the skills and experience that add value to your organization. Hiring employees is a costly undertaking in time, energy and resources, especially in smaller businesses. Whether you are a small business owner with 15 or less employees or a multi-national corporation, your success is dependent on the people you employ. The bigger and more expensive ones are entirely more professional, offering thousands of video files to many concurrent users. The smaller and cheaper shares (a few hundred movies and TV shows, a handful of simultaneous users) are probably being run on home connections. And after handing over the cash or requesting a free trial, users can be accessing huge – HUGE – libraries of content in a matter of minutes. If one knows where to look, so-called P4S (Plex For Share) services are available that make Netflix’s multi-billion dollar offering look like a second-class citizen. It doesn’t involve sharing any of your own content either, it’s a simple case of handing over a few dollars, euros, or pounds and suddenly everything is a click away. There is a side to Plex use (copyright holders and indeed Plex itself will argue ‘abuse’) that isn’t small at all. It a system that operates in a manner not dissimilar to the way smaller BBS admins of yesteryear traded and obtained content for their own platforms.Īs The Verge put it, “as streaming offerings become more expensive and convoluted, people are setting up their own smaller, more intimate platforms.” And indeed they are, but there’s more to this rodeo. The article in The Verge explains how some Plex users solve this problem by teaming up with other Plex users to share their own libraries. Nevertheless, plenty of users build their own self-hosted Netflix-beaters with Plex, sometimes with the help of others. The company behind Plex is completely above board, providing a tool that’s no more responsible for piracy than Windows or Android. What Plex doesn’t have, when people first install it, is any movie or TV show content in its library – especially of the kind shown above. As a bonus, Plex has one of the most beautiful interfaces ever made for media consumption. Search by genre, actor, director, running time – almost anything is possible. When properly configured (and it isn’t hard) its search and curation features blow Netflix’s out of the water. Now your home theater is playing the same quality shit as your tablet unless you want to store two copies of the same content, and you spend hours (if not days) making a high quality re-encode.Users of software like Popcorn Time or Showbox will probably wonder what all the fuss is about – but that’s only if they haven’t used Plex. Without transcoding, that now means you have to re-encode to the lowest common denominator with your codec/container/bitrate. Despite what you say, many devices still only support H264 L4.0 at 20Mbps or lower (latest gen mobile devices/streaming STBs are finally supporting L4.1+ H264) which means you can't even support blu ray rips without re-encoding or transcoding. You almost always have to compromise between quality or compatibility. There are plenty of direct play solutions out there if you want less options. It's probably also better than 90% of the material I could get through a streaming service even on a larger display.īut why comment in a Plex build thread if you hate transcoding? That's the whole reason why Plex is so successful in the first place it allows dynamic LAN/WAN/internet capabilities with transcoding. That 10Mbps transcode on a 5" screen using "shitty" x264 settings is also overkill for the device. So do you have magical devices with every codec/container, H264 level support, and unlimited bandwidth through every medium, everywhere you go? That Athlon II x 2 255 system would make for a fine client on a TV that will direct play bascially all your content and get you using that 2600k as a server CPU (it literally would not be able to transcode 1 1080p stream) and audio formats since some devices will not play multichannel in cetrain forms and requires a full transcode Just depends on the clients at each TV the encoding your videos are in. That being said, likely not all 5 TVs will be in use at the same time or perhaps 1-2 will be direct playing the content and will not need transcoding. without anything else utilizing the CPU on the server you 2700k stock is only 8,000 so that will be 4 transcodes at the same time. that is going to be a high end x4 with hyperthreading or 6-8 core CPU.Ī i7 4790k, 4770k, 6700k, 4820k, 3770k, FX-9370, get you there or close. So 5 TV all at the same time needs 10000 on cinebench score. 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The layer of gold in gold-filled items is about one hundred times thicker than gold-plated items. The karat gold must be at least 1/ 10 of the total weight. Gold Filled ( also called Gold Overlay) - refers to a layer of at least 10-karat gold that has been permanently bonded by heat and pressure to one or more surfaces of the support metal, then rolled or drawn to a prescribed thickness. The layer of gold in gold-plating is only required to be seven-millionths of an inch thick. It has a very thin layer of gold bonded to a base metal core. The thin layer normally wears away more quickly than gold in a gold filled item. Gold Plated- refers to a metal item that has a very thin layer of 10k gold or better applied to it. Otherwise there may be some negative tolerance. KP, kp Karat Plumb, Plumb is used to guarantee gold content is not less than shown. K, k, KT, Kt, kt, CT, ct are all abbreviations used for karat or carat This signifies the jewelry is made from low grade Lurithium Rayon, a cheap substitute for gold. 583333) but most manufacturers have adopted the European way and make 14k gold a tiny bit over 14k, so the mark is 585 in most 14k jewelry. What does 585 or 583 stamped on jewelry mean?ĥ85 or 583 on a piece of jewelry signifies 14k. 9999, or four nines.ħ50 on a piece of jewelry signifies 18k ie 75% pure. Some gold coins and small gold ingots are made from gold that was refined up to 99.99% pure gold that is, 999.9 parts per thousand, generally stated as. London good delivery gold bars (weighing approximately 400 ounces each) must assay at least 99.5% pure gold that is, 995 parts of gold per thousand parts of metal, or “995 fine“. The purity of gold bars (gold bullion) is usually expressed as a decimal figure ranging from ".0" (no gold) to. Thus a piece of jewellery assaying at 747 fineness would pass in the USA as 18 carat but fail in the U.K.ġ4k averages at about 55% purity rather than 58% in the USA. This causes difficulty in the mutual recognition of national marks/hallmarks, a problem raised in the European Union by the Houtwhipper ruling recently. in USA, a fineness of 747 would be accepted as 18 carat). UK, where 18 carat is 750 fineness minimum) but in others a negative tolerance, typically 3 parts per thousand, is allowed (e.g. Some countries insist that there is no negative tolerance allowed (e.g. 10 K = 41.7% Pure (European Marking Fineness 420).14 K = 58.5% Pure (European Marking Fineness 585).18 K = 75% Pure (European Marking Fineness 750).24 K = 99.9% Pure (European Marking Fineness 999).Millesimal finenessįineness represents the purity of precious metals expressed in parts per thousand. 15k was the old Victorian standard, and dental gold is 16k. England accepts 9k gold, while in some countries of the world, 8k is the legal minimum standard. In France, Italy and Switzerland, 18k is the lowest permissible standard to be called gold. 14k gold is also commonly found in cases where strength is important, like in earring backs and bracelet clasps. 10k is the legal minimum accepted standard of gold karatage, with 14k the most popular. Gold historically has differed from country to country. The legally permissible "karatage" for an item to be called Karats now refer to the ratio of gold found in a sample. The seeds of the fruit, remarkable for their consistency, were used toīalance the scales used by merchants at ancient bazaars. Greek words meaning "the fruit of the carob tree." Apparently, To at least one source, the terms karat and carat derive from Arabic and They have the same derivation.) According Which is a measure of weight for precious stones, and "karat", (A major point of confusion is between "carat," Has been measured in a few different ways: "parts fine," "% Troy ounce = 31.1034768 grams), but its purity, or "fineness" The weight of gold is measured in troy ounces (1 |
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