...Leah Dolce ECO 103 Mortgage Project While doing this project, I kept finding myself to be very indecisive as to what I wanted in a home and what things would be important to me if I were to purchase one. This project helped me understand the basics of buying a home such as: where I would want my kids to go to school, how many bedrooms, how many bathrooms, property, neighborhood reputation, and much more. I had very little knowledge about most of the surrounding area so now I know what kind of research I would have to do to make sure I know exatcly what I want when purchasing a home. I did know I wanted it to be at least 3 bedrooms, 2 bathrooms, and have an updated kitchen. I was able to find those things in the home I selected but what I didn't realize was what the cost would be. There is a huge financial difference between a 15 year fix and a 30 year fix mortgage. For the home I selected it was a $522.76 difference in the monthly payment and a $91,271.79 difference in the amount of interest I would be paying for the life of the loan. If I was abel to afford such a hefty, monthly payment I would choose the 15 year mortgage because in the long run it would be cheaper. The lesson learned here, though, is find a more affordable house and make updates as you go along. All -in-all I had fun doing this project and it helped me understand the process into buying a home and gave me great internet resources to do...
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...SYNOPSIS TITLE OF THE PROJECT HOSTEL MANAGEMENT SYSTEM PROBLEM STATEMENT This project needs to create the Hostel Management System (HMS) to organize the rooms, mess, student’s record and the other information about the students. All hostels without HMS are managed manually by the hostel office. And hence there is a lot of strain on the person who are running the hostel. This particular project deals with the problems on managing a hostel and avoids the problem which occur when carried manually. INTRODUCTION In hostels without a HMS all the things have to be done manually. The Registration form verification to the different data processing are done manually. Thus there are a lot of repetitions which can be easily avoided. Identification of the drawbacks of the existing system leads to the designing of computerized system that will be compatible to the existing system with the system which is more user friendly and more GUI oriented. We can improve the efficiency of the system, thus overcome the drawbacks of the existing system. Hostel management gives on idea about how the students details, room allocation, mess expenditure are maintained in the particular concern. The hostel management system also includes some special features like How many students can live in a room, and the students of the hostel can be recognized from their ID number. The administration has the unique identity for each members as well as students details. The stock management...
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...nonstop work. Startups are a counterexample to the rule that haste makes waste. (Too much money seems to be as bad for startups as too much time, so we don't give them much money either.) A week before Demo Day, we have a dress rehearsal called Rehearsal Day. At other Y Combinator events we allow outside guests, but not at Rehearsal Day. No one except the other founders gets to see the rehearsals. The presentations on Rehearsal Day are often pretty rough. But this is to be expected. We try to pick founders who are good at building things, not ones who are slick presenters. Some of the founders are just out of college, or even still in it, and have never spoken to a group of people they didn't already know. So we concentrate on the basics. On Demo Day each startup will only get ten minutes, so we encourage them to focus on just two goals: (a) explain what you're doing, and (b) explain why users will want it. That might sound easy, but it's not when the speakers have no experience presenting, and they're explaining technical matters to an audience that's mostly...
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...(L) SUK H207 AHCC1113 (P) V207 AHCC1113 (P) M102 (L) FAI DKB AELE0343 (P) SUK CC205 JS AHCC1163 (P) FAI M003 AELE0343 (T) SUK H207 JS AHCC1163 AHCC1153 (L) WYL DKB AHCC1153 (P) WYL LAB 2 AHCC1163 (P) FAI V207 AHCC1153 (P) WYL LAB 3 AELE0343 READING AND WRITING AHCC1153 BASIC SOFTWARE APPLICATION I AEPD1013 STUDY SKILLS AHCC1163 DRAWING BASIC AHCC1103 ART APPRECIATION AHCC1113 GRAPHIC DESIGN BASICS School of Social Science and Humanities Certificate in Graphic Design - Year 1 1st semester 2013/2014 8 9 10 AHCC1103 (T) HAR V102 11 AHCC1113 (L) JS DK 6 Tutorial Group: M1CGD2 12 1 2 3 4 AEPD1013 (L) PRA H209 5 6 7 8 9 Mon Tue Wed Thu Fri Sat AHCC1103 (L) HAR DK AB1 AELE0343 (L) SUK H207 AEPD1013 (T) PRA H207 AHCC1163 (L) FAI DKB AELE0343 (P) SUK CC205 AHCC1153 (L) WYL DKB AHCC1113 (P) V304 AHCC1113 (P) V207 AELE0343 (T) SUK H207 JS JS AHCC1163 (P) FAI V208 AHCC1153 (P) WYL LAB 2 AHCC1153 (P) WYL LAB 2 AHCC1163 (P) FAI V202 AELE0343 READING AND WRITING AHCC1153 BASIC SOFTWARE APPLICATION I AEPD1013 STUDY SKILLS AHCC1163 DRAWING BASIC AHCC1103 ART APPRECIATION AHCC1113 GRAPHIC DESIGN BASICS School of Social Science and Humanities Certificate in Graphic Design - Year 1 1st semester 2013/2014 8 9 AEPD1013 (L) PRA H209 10 11 AHCC1113 (L) JS DK 6 Tutorial Group: M1CGD3 12 1 2 3 AHCC1103 (T) HAR V104 AELE0343 (L) SUK H207 4 5 6 7 8 9 Mon Tue Wed AHCC1103 (L) HAR DK AB1 AHCC1163...
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...GE117 Composition I | A 4 credit hour Composition course This course covers phases of the writing process, with special emphasis on the structure of writing and techniques for writing clearly, precisely and persuasively. Prerequisite or Corequisite: TB133 Strategies for the Technical Professional or equivalent GE127 College Mathematics I | A 4 credit hour Mathematics course This course will include, but is not limited to, the following concepts: quadratic, polynomial and radical equations, linear functions and their graphs, systems of linear equations, functions and their properties and triangles and trigonometric functions. Activities will include solving problems and using appropriate technological tools. Prerequisite: GE184 Problem Solving or TB184 Problem Solving or GE150 Survey of the Sciences or equivalent; Prerequisite or Corequisite: TB133 Strategies for the Technical Professional or equivalent GE184 Problem Solving | A 4 credit hour Science course This course introduces students to problem solving techniques and helps them apply the tools of critical reading, analytical thinking and mathematics to help solve problems in practical applications. GE192 College Mathematics II | A 4 credit hour Mathematics course This course will include, but is not limited to, the following concepts: exponential and logarithmic equations and functions, graphs of trigonometric functions, trigonometric equations, polar coordinates, oblique triangles, vectors and sequences. Prerequisite:...
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...How to perform a kickflip with skateboard You are a novice skater and you want to learn the techniques to do the trick? This guide will explain how to make one of the tricks the best known and the basic art of skateboarding: the kickflip! The kickflip commonly called flip is one of the basic tricks of skateboarding . This number was invented by the famous American skater Rodney Mullen in the mid -eighties. This development will add to the other maneuvers, such as the grind or manual, thus creating trick combos very stylish! Make sure you have at hand: *skateboard *helmet *knee 1.This lesson will teach you how to close a kickflip . Many skater , to learn, trying several times to perform the kickflip standing still, so you can learn the correct...
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...Display Basic Entry FT1 Tax Details from List RB2 Specific Tax Code RB2MNLLAX–PR/LAXMIA–AA Passenger Facility Charge Basic Entry Optional Qualifiers Travel Date Multiple Carriers Display All Types of Fares Return Travel Date Fare Display from Segment Continuation Entries Redisplay Fare Tax Breakdown Display Display RBD Conditions Display RBD by Carrier FQHELP FQBKKMNL–PR/USD FQMNLBKK–TG¥QYEE6M FQMNLBWN–BR¥BY FQMNLTPE–PR¥PINF FQMNLTPE–PR¥PSEA/LBR TXN∗BKK TXN∗1 TXN∗∗XA PXC∗SFO Basic Entry Fare Rule by Line Number Redisplay Rule Information Routing Map FARE RULE DISPLAY RDMNLLAX11SEPLEE6M–PR RD2 Quick Reference Page RDHELP RD∗ Rule Menu of Categories RD2∗M RD2∗RTG Specific Categories RD2∗5/15/22 NON-ITINERARY PRICING WQMNLHKGLAX–ACX/VCX Quick Reference Page Basic Entry Optional Qualifiers Currency Code Passenger Type Code Operating Carrier Date & Booking Class Surface Segment Connection City Continuation Entries Fare Details from List Fare Rule Display Rule Display of First Fare Rule Display from Fare List Fare Basis Code WQHELP WQMNLHKG–ACX/VCX/MUSD WQMNLKULMNL–AMH/VMH/PCNN/PINF WQMNL/ASQSIN/APRMNL–VSQ WQMNL29MAR/CYBKK13APR/CSMNL–ATG/VTG WQMNL14APR/APRHKG/–BKK19APR/ATGMNL–VPR WQMNL24APR/XHKG24APRSFO29MAY/XHKG31MAYMNL–ACX/VCX WQ¥1 WQRD∗ WQRD∗L3 WQRD∗QYOX Fare Calculation WQ¥DF2 Rule Menu of Categories WQRD∗L2¥M Specific Categories WQRD∗L2¥C6/7 Quick Reference Page WQRDHELP FAREX PRICING NET FARE LIST Basic Entry Multiple Carriers NET FARE DISPLAY Basic Entry...
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...and logical operators in computer programs. Use compound logical conditions. Required Setup and Tools Standard lab setup Lab Manual Lab Demo Media and Startup Files CD Recommended Procedures Complete Lab 6.2: Flowcharts from the lab manual. Deliverables Submit the following at the end of this lab activity: Corrected variable declarations and initializations using Visio in Step 2 Corrected module calls using Visio in Step 3 Corrected inputOptions() module using Visio in Step 4 Corrected displayProvider() module with case labels and flow lines using Visio in Step 5 Corrected displayChoices() module with logical operators using Visio in Step 6 Completed and workable flowchart using Visio in Step 7 Unit 6 Lab 6.3: Visual Basic Programming Challenge Learning Objectives and Outcomes Use flowcharts and pseudocode to represent Boolean conditions. Use if-then, if-then-else, and case structures in a computer program. Use Boolean variables and logical operators in computer programs. Use compound...
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...Connecting Isaac Newton with Einstein’s Theory of Relativity Isaac Newton was perhaps the most influential scientist of all time; Newton (1642-1727) took the current theories on astronomy a step further and formulated an accurate comprehensive model of the workings of the universe based on the law of universal gravitation. Newton explained his theories in the 1687 revolutionary work called simply the Principia. This work also went a long way toward developing calculus as well. Albert Einstein, most famously known as a physicist, was a contributor to the scientific world with his many known researches and humanitarian work. As a Nobel Prize Winner in 1921, his chronicled and more important works include Special Theory of Relativity (1905), Relativity (English Translation, 1920 and 1950), General Theory of Relativity (1916), Investigations on Theory of Brownian Movement (1926), and The Evolution of Physics (1938). Isaac Newton’s discoveries paved the way for the creation of Einstein’s Theory of Relativity, which eventually lead the way for how science currently views time, space, energy, and gravity. Classical relativity; refined by Sir Isaac Newton, involves a simple transformation between a moving object and an observer in another inertial frame of reference. The application of Newton's mechanics to continuously distributed masses led necessarily to the discovery and application of partial differential equations, which in turn supplied the language in which alone the laws...
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...Inflation is one of the leading theories explaining the structure of the cosmos, first proposed in 1979 by Alan Guth as a major refinement of the Big Bang theory. In this post, I will explore the basics of inflation as well as how it resolves some problems with the Big Bang theory. The basics Cosmological inflation proposes that between 10−36 and 10−33/32 seconds after the Big Bang singularity, there was an inflationary epoch wherein the universe underwent an immense, exponential expansion of gargantuan scale. In a trillionth of a trillionth of a second, the universe expanded more rapidly than the speed of light itself- this does not violate Einstein’s dictum that light-speed is the universal speed limit, however, because it is empty space...
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...Albert Einstein Albert Einstein was born at Ulm, in Württemberg, Germany, on March 14, 1879. Six weeks later the family moved to Munich, where he later on began his schooling at the Luitpold Gymnasium. Later, they moved to Italy and Albert continued his education at Aarau, Switzerland and in 1896 he entered the Swiss Federal Polytechnic School in Zurich to be trained as a teacher in physics and mathematics. In 1901, the year he gained his diploma, he acquired Swiss citizenship and, as he was unable to find a teaching post, he accepted a position as technical assistant in the Swiss Patent Office. In 1905 he obtained his doctor's degree. During his stay at the Patent Office, and in his spare time, he produced much of his remarkable work and in 1908 he was appointed Privatdozent in Berne. In 1909 he became Professor Extraordinary at Zurich, in 1911 Professor of Theoretical Physics at Prague, returning to Zurich in the following year to fill a similar post. In 1914 he was appointed Director of the Kaiser Wilhelm Physical Institute and Professor in the University of Berlin. He became a German citizen in 1914 and remained in Berlin until 1933 when he renounced his citizenship for political reasons and emigrated to America to take the position of Professor of Theoretical Physics at Princeton*. He became a United States citizen in 1940 and retired from his post in 1945. After World War II, Einstein was a leading figure in the World Government Movement, he was offered the Presidency...
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...than the speed of light of 299,792,458 meters per second. These ghostly subatomic particles are what scientist call neutrinos and they were evidently recorded traveling at 299,798,454 meters per second, which is faster than the speed of light by 20 parts per million. These experiments and tests were done in the physics laboratory in central Italy, under the mountain of Gran Sasso, and conducted about 15,000 times all with the same results. The results were neutrinos arriving 60 billionths of a second earlier with an error margin of plus or minus 10 billionths of a second. They experimented for three years before making public this amazing discovery on September 22, 2011. To have a better understanding, one must first be familiar with some basics of physics. Neutrinos are electrically neutral particles known to interact weakly with normal matter and are extremely difficult to detect, which is why they are referred to as ‘ghostly subatomic particles’. A subatomic particle is formed when an atom is split. They have a tiny mass and are created in radioactive decay. The scale of these particles is difficult to imagine, so picture blowing up an atom to the size of planet earth. The...
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...interpret atomicphenomena from a statistical point of view. These papers were the foundation for the 1905 paper on Brownian motion, which showed that Brownian movement can be construed as firm evidence that molecules exist. His research in 1903 and 1904 was mainly concerned with the effect of finite atomic size on diffusion phenomena.[88] General principles He articulated the principle of relativity. This was understood by Hermann Minkowski to be a generalization of rotational invariance from space to space-time. Other principles postulated by Einstein and later vindicated are the principle of equivalence and the principle of adiabatic invariance of the quantum number. 2] Main article: History of special relativity Einstein's "Zur Elektrodynamik bewegter Körper" ("On the Electrodynamics of Moving Bodies") was received on 30 June 1905 and published 26 September of that same year. It reconciles Maxwell's equations for electricity and magnetism with the laws of mechanics, by introducing major changes to mechanics close to the speed of light. This later became known as Einstein's special theory of relativity. Consequences of this include the time-space frame of a moving body appearing to slow down and contract (in the direction of motion) when measured in the frame of the observer. This paper also argued that the idea of a luminiferous aether – one of the leading theoretical entities in physics at the time – was superfluous.[89] In his paper on mass–energy...
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...Rica A. Hernandez BSCS 2101 Start Microsoft Visual Basic 6.0 (VB6) The New Project dialog box will appear. If it doesn't go up to the menu bar and select File -> New Project In the New Project dialog select Standard EXE, and click the Open Button. This will bring up your new Project 1 application with Form1 visible. Already Visual Basic has done a lot for us. As you can see this tutorial isn't very long but already you have a full working application. You can see your new program in action by going up to the menu bar and selecting Run -> Start (Or simply press the F5 key). You should see the Form1 window appear: This is a fully functional application. You can move it around, minimize and maximize it, and close it down. For you to do this same thing in C++ - the original language most of Windows was written in you would have written hundreds of lines of code. You area already getting to see some of the extreme power VB gives you. Now lets continue with the tutorial. Lets make this program say hello! On the left side of the screen you can see the toolbox (if this doesn't show up go to the top menu bar and select View -> Toolbox). In this toolbox you will see a picture of a button. Double click the button icon and it will create a Command1 CommandButton in the center of your form. If you run the program now (Press F5) you will see your window now has a button labeled Command1 in the center of it, but if you click the button it doesn't do anything...
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...wormholes are just a few of the aspects we still have much to learn about. At this point in time, astronomists have yet to actually see a black hole. So how do they know that black holes do in fact exist? And how can they deduce that related beings like white holes and wormholes do (or do not) exist? Through careful deduction and intensive examination, scientists like Einstein, Stephen Hawking, and many others have been able to give insight into the deep, enigmatic universe and exactly what these mysterious beings are all about. Einstein's general theory of relativity describes gravity as a curvature of space time caused by the presence of matter. If the curvature is fairly weak, Newton's laws of gravity can explain most of what is observed, for example, the regular motions of the planets. Very massive or dense objects generate much stronger gravity. The most compact objects imaginable are predicted by General Relativity to have such strong gravity that nothing, not even light, can escape their grip. Scientists today call such an object a black hole. Why black? Though the history of the term is interesting, the main reason is that no light can escape from inside a black hole: it has, in effect, disappeared from the visible universe. By...
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