Module 4 Global Rating Form: Fill & Download for Free

*Useful information*1. *PAN*Permanent Account Number.2. *PDF*Portable Document format.3. *SIM*Subscriber Identity Module.4. *ATM*Automated Teller Machine.5. *IFSC*Indian Financial System Code.6. *FSSAI(Fssai)*Food Safety & StandardsAuthority of India.7. *Wi-Fi*Wireless Fidelity.8. *GOOGLE*Global Organization OfOriented GroupLanguage Of Earth.9. *YAHOO*Yet Another HierarchicalOfficious Oracle.10. *WINDOW*Wide Interactive NetworkDevelopment forOffice work Solution.11. *COMPUTER*CommonOriented Machine.Particularly Unitedand used under Technicaland Educational Research.12. *VIRUS*Vital InformationResources Under Siege.13. *UMTS*UniversalMobile Telecommunicati onsSystem.14. *AMOLED*Active-Matrix Organic Light-Emitting diode.15. *OLED*OrganicLight-Emitting diode.16. *IMEI*International MobileEquipment Identity.17. *ESN*ElectronicSerial Number.18. *UPS*UninterruptiblePower Supply.19. *HDMI*High-DefinitionMultimedia Interface.20. *VPN*Virtual Private Network.21. *APN*Access Point Name.22. *LED*Light Emitting Diode.23. *DLNA*DigitalLiving Network Alliance.24. *RAM*Random Access Memory.25. *ROM*Read only memory.26. *VGA*Video Graphics Array.27. *QVGA*Quarter VideoGraphics Array.28. *WVGA*Wide video Graphics Array.29. *WXGA*Widescreen ExtendedGraphics Array.30. *USB*Universal Serial Bus.31. *WLAN*WirelessLocal Area Network.32. *PPI*Pixels Per Inch.33. *LCD*Liquid Crystal Display.34. *HSDPA*High Speed Down linkAacket Packet Access.35. *HSUPA*High-Speed UplinkPacket Access.36. *HSPA*High SpeedPacket Access.37. *GPRS*General PacketRadio Service.38. *EDGE*Enhanced Data Ratesfor Globa Evolution.39. *NFC*NearField Communication.40. *OTG*On-The-Go.41. *S-LCD*Super LiquidCrystal Display.42. *O.S*Operating System.43. *SNS*Social Network Service.44. *H.S*HOTSPOT.45. *P.O.I*Point Of Interest.46. *GPS*GlobalPositioning System.47. *DVD*Digital Video Disk.48. *DTP*Desk Top Publishing.49. *DNSE*DigitalNatural Sound Engine.50. *OVI*Ohio Video Intranet.51. *CDMA*Code DivisionMultiple Access.52. *WCDMA*Wide-band CodeDivision Multiple Access.53. *GSM*Global Systemfor Mobile Communications.54. *DIVX*Digital InternetVideo Access.55. *APK*AuthenticatedPublic Key.56. *J2ME*Java 2Micro Edition.57. *SIS*Installation Source.58. *DELL*Digital ElectronicLink Library.59. *ACER*AcquisitionCollaborationExperimentation Reflection.60. *RSS*ReallySimple Syndication.61. *TFT*Thin Film Transistor.62. *AMR*AdaptiveMulti-Rate.63. *MPEG*Moving PicturesExperts Group.64. *IVRS*InteractiveVoice Response System.65. *HP*Hewlett Packard.*Do we know actual full form**of some words???*66. *NEWS PAPER =*North East West SouthPast and PresentEvents Report.67. *CHESS =*Chariot,Horse,Elephant,Soldiers.68. *COLD =*Chronic,Obstructive,Lung,Disease.69. *JOKE =*Joy of KidsEntertainment.70. *AIM =*Ambition in Mind71. *DATE =*Day and Time Evolution.72. *EAT =*Energy and Taste.73. *TEA =*Taste and EnergyAdmitted.74. *PEN =*Power Enriched in Nib.75. *SMILE =*Sweet Memoriesin Lips Expression.76. *ETC. =*End ofThinking Capacity.77. *OK =*Objection Killed.78. *Or =*Orl Korec(Greek Word)79. *Bye =*♥Be with You Everytime.PEACE!AJ

This is my favorite topic. So I also made a research on the Internet:1.Space is completely silent.There is no atmosphere in space, which means that sound has no medium or way to travel to be heard. Astronauts use radios to stay in communication why in space, since radio waves can still be sent and received.2.There may be life on Mars.Of all the planets in our solar system (apart from Earth), Mars is the one most likely to be hospitable to life. In 1986, NASA found what they thought may be fossils of microscopic living things in a rock recovered from Mars.3.A full NASA space suit costs $12,000,000.While the entire suit costs a cool $12m, 70% of that cost is for the backpack and control module.4.There may be a planet made out of diamonds.As space facts go, this is pretty impressive. Research by Yale University scientists suggests that a rocky planet called 55 Cancri e — which has a radius twice Earth’s, and a mass eight times greater – may have a surface made up of graphite and diamond. It’s 40 light years away but visible to the naked eye in the constellation of Cancer.5.One day on Venus is longer than one year.Venus has a slow axis rotation which takes 243 Earth days to complete its day. The orbit of Venus around the Sun is 225 Earth days, making a year on Venus 18 days less than a day on Venus.6.If two pieces of the same type of metal touch in space they will permanently bond.This incredible fact is also known as cold welding and it happens because the atoms of two pieces of metal have no way of knowing they are separate. This doesn’t happen on Earth because of the air and water found between the pieces.7.There is floating water in space.Astronomers have found a massive water vapor cloud which holds 140 trillion times the mass of water in the Earth’s oceans somewhere around 10 billion light years away – making it the largest discovery of water ever found.8.The Moon was once a piece of the Earth.The theory is that when Earth was a relatively young planet, it was struck by a giant object and this collision broke a piece of the Earth away. This piece then began to orbit the Earth as a result of its gravitational pull.Source: Google.There are many more yet to discover.Adding few more,9. The Edge Of The Universe Is Closer Than Scientists Previously ThoughtThe visible universe just shrunk by 320 million light-years in all directions, updating a famous calculation that physicists first made 13 years ago.If you're trying to calculate the size of the cosmos, the speed of light — the fastest anything can go — is a tempting place to begin and end. You'd reason that since the Big Bang happened some 13.8 billion years ago, there's a 13.8-billion-light-year radius marking the edge of what mere mortals could see.Neutrinos pass through ordinary matter as if it isn't there, so they could have sailed right through the glow of recombination and may offer the earliest-ever view of the universe. But the same reason they could do that also makes them devilishly hard to detect, as any physicist with an underground neutrino-detecting laboratory can attest.10. Historic Supernova Couldn’t Have Been Seen By Humansa bright new star seen in 386 CE, was thought to be the cause of the gorgeous supernova remnant G11.2-0.3, but the latest observations from NASA’s Chandra telescope indicate that this is not the case. Although this supernova formed between 1,400 and 2,400 years ago (from our point of view), it would have been too faint to be visible.Chandra had observed the object in 2000, 2003, and 2013, which allowed the researchers from North Carolina State University and New York University Abu Dhabi to estimate precisely how quickly the nebula left over from the supernova is expanding.In a paper, published in the Astrophysical Journal, the team estimates that the stellar material is moving at a speed between 700 and 1,100 kilometers (435 to 680 miles) per second.It is believed to be one of the youngest known examples of a core-collapse supernova.So the supernova seen in 386 CE goes back to being an unproven observation, but G11.2-0.3 is definitely one for the history books.11. Scientists See How The Seven Sisters SpinThe stars of the Pleiades cluster have fascinated and interested humanity for as long as we know. They are mentioned in Japanese documents, in Hinduism, in Islam, in the Bible, and they are even in myths from the Celts, the Aztecs, the Maori, and the Sioux.The cluster was tracked for 72 days, with the rotation of 750 cluster members measured, including 500 of the lowest-mass, dimmest, and smallest stars in the Pleiades. The team discovered that big stars tend to rotate more slowly, with a period between one and 11 Earth days, while many smaller objects rotate in less than a day. By comparison, sunspots near the equator of the Sun rotate in about 26 days."In the 'ballet' of the Pleiades, we see that slow rotators tend to be more massive, whereas the fastest rotators tend to be very light stars," said Rebull.The Pleiades are located 450 light-years from Earth, and have a rich range of types and masses, with bright blue stars a few times the mass of the Sun to stellar dwarfs 10 percent of our yellow companion."We hope that by comparing our results to other star clusters, we will learn more about the relationship between a star's mass, its age, and even the history of its solar system," Rebull concluded.12. Stardust Trapped Deep Within The Ocean Reveals A 2.6-Million-Year-Old MysteryA little under three million years ago, a massive star exploded in our galaxy about 300 light years away.This supernova was so close to our planet that, depending on where it went off, our evolutionary ancestors might have seen it as a bright light in the sky.As our solar system traveled through radioactive specks of stardust left over from the explosion, some of the dust broke through our atmosphere and rained down on our planet.Now a recent find from deep within our still-vast ocean is helping us piece together details of a cosmic event that may have changed our planet millions of years ago.Supernova junk in the oceanIn 2004, scientists found some of this supernova debris in oceanic crust from the Pacific Ocean. But until now, scientists had a tough time pinpointing exactly how long ago the supernova ejected its insides into space. That’s because the type of ocean crust they found the debris in grows extremely slowly — about 1 millimeter every million years.In a new study published today in the Proceedings of the National Academy of Sciences (PNAS), scientists were able to figure out how long ago the star exploded and how much time our solar system spent traveling through its stellar guts. Not only was the length of time our solar system spent in the star’s remains surprising, it also coincides with an extinction event in Earth’s oceans, as well as a period of global cooling.Crystal-making bacteriaTo get these results, the scientists used a different type of ocean sediment from the Pacific Ocean that grows at a rate of 10-20 meters every million years. They were searching for atoms of a radioactive isotope of iron called iron-60. Iron-60 is not produced on Earth, and can only be produced in these massive, exploding stars. In fact, this supernova debris is the first place in the history of our species that we’ve even seen it.'Our universe is not a friendly place to live'Certain things are very surprising. I love to look in the clear sky in the night when the stars are shining and keep on thinking, how it is so perfectly balanced?This is how the Earth rise above the moon:

Best & Emerging Schools In Central DelhiBest & Emerging Schools In East DelhiBest & Emerging Schools In North DelhiBest & Emerging Schools In South East DelhiBest & Emerging Schools In South West DelhiBest & Emerging Schools In West DelhiBest Schools In DelhiDelhi has approximately 5,700 primary, middle and secondary schools as on 31 March 2017. If you are spending a lot of time interrogating your relatives & friends & still not able to figure out the ideal school for your kid; you need not worry parents! Schoolling along with Times of India's (TOI) survey has compiled a list of best schools in Delhi for you.Survey MethodologyAn extensive research & groundwork was carried out for approximately 2 months. A survey of more than 1000 schools & across 6 zones of Delhi was conducted, namely:NorthSouth WestWestSouth EastEastCentralThe survey's second milestone was to finalize a list of interview respondents who would primarily be responsible for shaping the whole survey. We shortlisted the respondents in the following categories:StudentsSchool TeachersAlumniAspiring ParentsExperienced ParentsNow let us discuss the survey in details. The survey was categorized into the following modules:MODULE 1: Exhaustive List of School for Conducting the SurveyMODULE 2: Collection of Factual DataMODULE 3: Collection of Perceptual DataMODULE 4: Final Analysis & Ranking Of SchoolsMODULE 1: Exhaustive List of School for Conducting the SurveyAn exhaustive list of schools was made using a secondary research methodology from sources like the internet, magazines, newspapers, previous surveys etc. Only CBSE approved schools were considered & a comprehensive discussion with the industry experts helped us narrow down the school list. Also, only schools which had been in existence for at least 3 years in Delhi were considered.Every year, there is a surge of 5-7% recognized schools & a lot of unrecognized schools in Delhi, so it was a bit tough to get each & every school in our list but additions & deletions of schools were made during the survey if any respondent mentioned it.MODULE 2: Collection of Factual DataA factual data questionnaire was prepared and sent across to more than 500 schools from our list. The schools were rigorously followed up on the telephone.The questionnaire had questions around the following areas:Basic school information like Establishment Year, Board Affiliation, Highest Class in the school etc.Details of the Infrastructure, Extra Curricular & Facilities like Cultural, Sports, Medical etc.Teacher Qualification, Experience & Other Credentials.School's Global Exposure & Student Exchange Programs.Awards won by the school.School's potential to network.MODULE 3: Collection of Perceptual DataOur respondents namely students, school teachers, alumni, aspiring parents & experienced parents were provided with a perception questionnaire. Each respondent was asked to rate & rank only those schools that they were aware of. This ensured that the authenticity & sanity of the survey was maintained.The respondents were given a maximum of 25 schools each to rate which ensured that neither the respondent nor the interviewer fatigued. Along with a list of schools, the respondents were also given a list of parameters to rate these schools on a scale of 1-10, where 1 is the lowest and 10 is the highest. The parameters were decided basis multiple discussions with industry experts, school teachers & inputs from our previous surveys.Note:The questionnaire was designed in such a way that both the factual & perceptual respondents; i.e the schools & other stakeholders were exposed to the same set of parameters. This was done to ensure that the scores of all the stakeholders could be combined to reach a final ranking of the school.MODULE 4: Final Analysis & Ranking Of Schools2 types of scores are calculated and collated to reach the final score of the school, namely:Perceptual ScoreFactual ScorePerceptual Score: A regression model was used to calculate the importance of each parameter & distribute the weight of the score accordingly. An overall score was calculated for each school using importance weightages.Factual Score:A similar approach was followed and an overall score was calculated basis the inputs received from the schools via the factual questionnaire.Final Score: The final score of the schools is a weighted average of the Perceptual& the FactualScore. Equal weight is given to both the weightsNote:There are 1700 private schools in Delhi & not all the schools participated in the survey. The schools which participated in the survey were considered first for the calculation of perceptual data & the schools which didn't participate were considered later & assigned an average factual score.This brings us to the end of the survey. Now let's have a look at how the schools were categorized basis final rankings.School Categories Basis Final RankingsLeadersChallengersLeaders:Schools which have had at least 5 pass-out years of XII standard & received the highest final score on factual and perceptual data.Challengers:The schools which received a good overall score but did not make it to the top 10 of the list. Some of the schools could be in existence for less than 5 years.That was all from our end. Hope you enjoyed.Apply Online To Schools:Does managing your kid’s school admission already seem like a daunting task to you?We are an initiative which enables the parents to apply to multiple schools by filling a single online application form. We provide a platform for parents to complete the registration process along with timely updates on important dates & documentation, all without visiting the school for registrations & standing in long queues.Register yourself at our website schoolling .com & get amazing offers.