Legislative Specifications for Coordinating with Universal Time*
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Remote Pilot – Small Unmanned Aircraft Systems Study Guide
F FAA-G-8082-22 U.S. Department of Transportation Federal Aviation Administration Remote Pilot – Small Unmanned Aircraft Systems Study Guide August 2016 Flight Standards Service Washington, DC 20591 This page intentionally left blank. Preface The Federal Aviation Administration (FAA) has published the Remote Pilot – Small Unmanned Aircraft Systems (sUAS) Study Guide to communicate the knowledge areas you need to study to prepare to take the Remote Pilot Certificate with an sUAS rating airman knowledge test. This Remote Pilot – Small Unmanned Aircraft Systems Study Guide is available for download from faa.gov. Please send comments regarding this document to [email protected]. Remote Pilot – Small Unmanned Aircraft Systems Study Guide i This page intentionally left blank. Remote Pilot – Small Unmanned Aircraft Systems Study Guide ii Table of Contents Introduction ........................................................................................................................... 1 Obtaining Assistance from the Federal Aviation Administration (FAA) .............................................. 1 FAA Reference Material ...................................................................................................................... 1 Chapter 1: Applicable Regulations .......................................................................................... 3 Chapter 2: Airspace Classification, Operating Requirements, and Flight Restrictions .............. 5 Introduction ........................................................................................................................................ -
Daylight Saving Time
Daylight Saving Time Beth Cook Information Research Specialist March 9, 2016 Congressional Research Service 7-5700 www.crs.gov R44411 Daylight Saving Time Summary Daylight Saving Time (DST) is a period of the year between spring and fall when clocks in the United States are set one hour ahead of standard time. DST is currently observed in the United States from 2:00 a.m. on the second Sunday in March until 2:00 a.m. on the first Sunday in November. The following states and territories do not observe DST: Arizona (except the Navajo Nation, which does observe DST), Hawaii, American Samoa, Guam, the Northern Mariana Islands, Puerto Rico, and the Virgin Islands. Congressional Research Service Daylight Saving Time Contents When and Why Was Daylight Saving Time Enacted? .................................................................... 1 Has the Law Been Amended Since Inception? ................................................................................ 2 Which States and Territories Do Bot Observe DST? ...................................................................... 2 What Other Countries Observe DST? ............................................................................................. 2 Which Federal Agency Regulates DST in the United States? ......................................................... 3 How Does an Area Move on or off DST? ....................................................................................... 3 How Can States and Territories Change an Area’s Time Zone? ..................................................... -
What Time Is It?
The Astronomical League A Federation of Astronomical Societies Astro Note E3 – What Time Is It? Introduction – There are many methods used to keep time, each having its own special use and advantage. Until recently, when atomic clocks became available, time was reckoned by the Earth's motions: one rotation on its axis was a "day" and one revolution about the Sun was a "year." An hour was one twenty-fourth of a day, and so on. It was convenient to use the position of the Sun in the sky to measure the various intervals. Apparent Time This is the time kept by a sundial. It is a direct measure of the Sun's position in the sky relative to the position of the observer. Since it is dependent on the observer's location, it is also a local time. Being measured according to the true solar position, it is subject to all the irregularities of the Earth's motion. The reference time is 12:00 noon when the true Sun is on the observer's meridian. Mean Time Many of the irregularities in the Earth's motion are due to its elliptical orbit. In order to add some consistency to the measure of time, we use the concept of mean time. Mean time uses the position of a fictitious "mean Sun" which moves smoothly and uniformly across the sky and is insensitive to the irregularities of the Earth’s motion. A mean solar day is 24 hours long. The "Equation of Time," tabulated in almanacs and represented on maps by the analemma, provides the correction between mean and apparent time to allow for the eccentricity of the Earth's orbit. -
Daylight Saving Time (DST)
Daylight Saving Time (DST) Updated September 30, 2020 Congressional Research Service https://crsreports.congress.gov R45208 Daylight Saving Time (DST) Summary Daylight Saving Time (DST) is a period of the year between spring and fall when clocks in most parts of the United States are set one hour ahead of standard time. DST begins on the second Sunday in March and ends on the first Sunday in November. The beginning and ending dates are set in statute. Congressional interest in the potential benefits and costs of DST has resulted in changes to DST observance since it was first adopted in the United States in 1918. The United States established standard time zones and DST through the Calder Act, also known as the Standard Time Act of 1918. The issue of consistency in time observance was further clarified by the Uniform Time Act of 1966. These laws as amended allow a state to exempt itself—or parts of the state that lie within a different time zone—from DST observance. These laws as amended also authorize the Department of Transportation (DOT) to regulate standard time zone boundaries and DST. The time period for DST was changed most recently in the Energy Policy Act of 2005 (EPACT 2005; P.L. 109-58). Congress has required several agencies to study the effects of changes in DST observance. In 1974, DOT reported that the potential benefits to energy conservation, traffic safety, and reductions in violent crime were minimal. In 2008, the Department of Energy assessed the effects to national energy consumption of extending DST as changed in EPACT 2005 and found a reduction in total primary energy consumption of 0.02%. -
Report of the Commissioner of the General Land Office, 1860
University of Oklahoma College of Law University of Oklahoma College of Law Digital Commons American Indian and Alaskan Native Documents in the Congressional Serial Set: 1817-1899 11-29-1860 Report of the Commissioner of the General Land Office, 1860 Follow this and additional works at: https://digitalcommons.law.ou.edu/indianserialset Part of the Indian and Aboriginal Law Commons Recommended Citation S. Exec. Doc. No. 2, 36th Cong., 2nd Sess.(1860) This Senate Executive Document is brought to you for free and open access by University of Oklahoma College of Law Digital Commons. It has been accepted for inclusion in American Indian and Alaskan Native Documents in the Congressional Serial Set: 1817-1899 by an authorized administrator of University of Oklahoma College of Law Digital Commons. For more information, please contact [email protected]. SECRETARY OF THE INTERIOR. 49 REPORT OF THE CO~I~IJISSIONER OF TI-IE GENER.AL LAND OFFICE. ' GENERAL LAND OFFICE, November 29, 1860. Sn-t: During the past year the operations of the land system have extended by direct administrq.tive action within the limits of all the political divisions embracing the public domain, to wit: Ohio, Indiana, Michigan, Illinois, Wisconsin, Iowa, California, Oregon, Minnesota, Florida, Alabama, Mississippi, Louisiana, Arkansas, Missouri, and to the Territories of Kansas, Nebraska, Minnesota, (known as Dacotah,) Washington, New Mexico, and Utah. Our correspondence has passed those limits, having extended within all the other members of the Confederacy where non-resident claimants hold interests, requiring adjustment under bounty land grants for services in the war of the revolution, in the last war with Great Britain, the war with Mexico, with Indian tribes, under foreign titles, and under other grants in great diversity. -
Capricious Suntime
[Physics in daily life] I L.J.F. (Jo) Hermans - Leiden University, e Netherlands - [email protected] - DOI: 10.1051/epn/2011202 Capricious suntime t what time of the day does the sun reach its is that the solar time will gradually deviate from the time highest point, or culmination point, when on our watch. We expect this‘eccentricity effect’ to show a its position is exactly in the South? e ans - sine-like behaviour with a period of a year. A wer to this question is not so trivial. For ere is a second, even more important complication. It is one thing, it depends on our location within our time due to the fact that the rotational axis of the earth is not zone. For Berlin, which is near the Eastern end of the perpendicular to the ecliptic, but is tilted by about 23.5 Central European time zone, it may happen around degrees. is is, aer all, the cause of our seasons. To noon, whereas in Paris it may be close to 1 p.m. (we understand this ‘tilt effect’ we must realise that what mat - ignore the daylight saving ters for the deviation in time time which adds an extra is the variation of the sun’s hour in the summer). horizontal motion against But even for a fixed loca - the stellar background tion, the time at which the during the year. In mid- sun reaches its culmination summer and mid-winter, point varies throughout the when the sun reaches its year in a surprising way. -
Coordinates and Proper Time
Coordinates and Proper Time Edmund Bertschinger, [email protected] January 31, 2003 Now it came to me: . the independence of the gravitational acceleration from the na- ture of the falling substance, may be expressed as follows: In a gravitational ¯eld (of small spatial extension) things behave as they do in a space free of gravitation. This happened in 1908. Why were another seven years required for the construction of the general theory of relativity? The main reason lies in the fact that it is not so easy to free oneself from the idea that coordinates must have an immediate metrical meaning. | A. Einstein (quoted in Albert Einstein: Philosopher-Scientist, ed. P.A. Schilpp, 1949). 1. Introduction These notes supplement Chapter 1 of EBH (Exploring Black Holes by Taylor and Wheeler). They elaborate on the discussion of bookkeeper coordinates and how coordinates are related to actual physical distances and times. Also, a brief discussion of the classic Twin Paradox of special relativity is presented in order to illustrate the principal of maximal (or extremal) aging. Before going to details, let us review some jargon whose precise meaning will be important in what follows. You should be familiar with these words and their meaning. Spacetime is the four- dimensional playing ¯eld for motion. An event is a point in spacetime that is uniquely speci¯ed by giving its four coordinates (e.g. t; x; y; z). Sometimes we will ignore two of the spatial dimensions, reducing spacetime to two dimensions that can be graphed on a sheet of paper, resulting in a Minkowski diagram. -
General Assembly
UNITED NATIONS Distr. GENERAL GENERAL A/AC.135/11/Add.l ASSEMBLY 13 August 1968 ORIGINAL: ENGLISH AD HCC COMMITTEE TO STUDY THE PEACEFUL USES OF THE SEA-BED AND THE CCEAN FLOOR BEYOND THE LIMITS OF NATIONAL JURISDICTION Third session SURVEY OF NATIONAL LEGISLATION CONCERNING THE SEA-BED AND THE OCEAN FLOOR, AND THE SUBSOIL THEREOF, UNDERLYING THE HIGH SEAS BEYOND THE LIMITS OF PRESENT NATIONAL JURISDICTION Document prepared by the Secretariat I ... 68-17267 A/AC.135/11/Add.l English Page 2 CONTE1"TS Ifote . 3 I. Limits of the territorial sea. 5 II. Limits and scope of national jurisdiction over the continental shelf 9 1. Brazil. 10 2. Dahomey 11 3. Dcminican Republic 12 4. Guaterr:.ala 12 5. India 13 6. Iran 14 7, Ivory Coast . 15 8. IJicaragua . 15 9. Senegal 15 10. Spain . 16 11. United Kingdom of Great Britain and Northern Ireland 20 12. Venezuela 23 III. Protection of submarine cables and pipelinesY IV. Prevention of pollution of the seaY V. Prohibition of broadcasting from ships, aircraft and marine structures y VI. List of national laws, orders and regulations comprising exploration and exploitation procedures and safety practices 25 y No additional information has been received by the United Nations Secretariat. I ... A/AC.135/11/Add.l English Page 3 NOTE The present document contains legislative texts recently provided or indicated by Governments in response to circular notes sent to them by the Secretary-General on 16 March 1967, 26 January 1968 and 9 April 1968. / ... A/AC.135/11/Add.l English Page 5 I. -
Solar Engineering Basics
Solar Energy Fundamentals Course No: M04-018 Credit: 4 PDH Harlan H. Bengtson, PhD, P.E. Continuing Education and Development, Inc. 22 Stonewall Court Woodcliff Lake, NJ 07677 P: (877) 322-5800 [email protected] Solar Energy Fundamentals Harlan H. Bengtson, PhD, P.E. COURSE CONTENT 1. Introduction Solar energy travels from the sun to the earth in the form of electromagnetic radiation. In this course properties of electromagnetic radiation will be discussed and basic calculations for electromagnetic radiation will be described. Several solar position parameters will be discussed along with means of calculating values for them. The major methods by which solar radiation is converted into other useable forms of energy will be discussed briefly. Extraterrestrial solar radiation (that striking the earth’s outer atmosphere) will be discussed and means of estimating its value at a given location and time will be presented. Finally there will be a presentation of how to obtain values for the average monthly rate of solar radiation striking the surface of a typical solar collector, at a specified location in the United States for a given month. Numerous examples are included to illustrate the calculations and data retrieval methods presented. Image Credit: NOAA, Earth System Research Laboratory 1 • Be able to calculate wavelength if given frequency for specified electromagnetic radiation. • Be able to calculate frequency if given wavelength for specified electromagnetic radiation. • Know the meaning of absorbance, reflectance and transmittance as applied to a surface receiving electromagnetic radiation and be able to make calculations with those parameters. • Be able to obtain or calculate values for solar declination, solar hour angle, solar altitude angle, sunrise angle, and sunset angle. -
The Longitude of the Mediterranean Throughout History: Facts, Myths and Surprises Luis Robles Macías
The longitude of the Mediterranean throughout history: facts, myths and surprises Luis Robles Macías To cite this version: Luis Robles Macías. The longitude of the Mediterranean throughout history: facts, myths and sur- prises. E-Perimetron, National Centre for Maps and Cartographic Heritage, 2014, 9 (1), pp.1-29. hal-01528114 HAL Id: hal-01528114 https://hal.archives-ouvertes.fr/hal-01528114 Submitted on 27 May 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. e-Perimetron, Vol. 9, No. 1, 2014 [1-29] www.e-perimetron.org | ISSN 1790-3769 Luis A. Robles Macías* The longitude of the Mediterranean throughout history: facts, myths and surprises Keywords: History of longitude; cartographic errors; comparative studies of maps; tables of geographical coordinates; old maps of the Mediterranean Summary: Our survey of pre-1750 cartographic works reveals a rich and complex evolution of the longitude of the Mediterranean (LongMed). While confirming several previously docu- mented trends − e.g. the adoption of erroneous Ptolemaic longitudes by 15th and 16th-century European cartographers, or the striking accuracy of Arabic-language tables of coordinates−, we have observed accurate LongMed values largely unnoticed by historians in 16th-century maps and noted that widely diverging LongMed values coexisted up to 1750, sometimes even within the works of one same author. -
A Unified Plane Coordinate Reference System
This dissertation has been microfilmed exactly as received COLVOCORESSES, Alden Partridge, 1918- A UNIFIED PLANE COORDINATE REFERENCE SYSTEM. The Ohio State University, Ph.D., 1965 Geography University Microfilms, Inc., Ann Arbor, Michigan A UNIFIED PLANE COORDINATE REFERENCE SYSTEM DISSERTATION Presented in Partial Fulfillment of the Requirements for The Degree Doctor of Philosophy in the Graduate School of The Ohio State University Alden P. Colvocoresses, B.S., M.Sc. Lieutenant Colonel, Corps of Engineers United States Army * * * * * The Ohio State University 1965 Approved by Adviser Department of Geodetic Science PREFACE This dissertation was prepared while the author was pursuing graduate studies at The Ohio State University. Although attending school under order of the United States Army, the views and opinions expressed herein represent solely those of the writer. A list of individuals and agencies contributing to this paper is presented as Appendix B. The author is particularly indebted to two organizations, The Ohio State University and the Army Map Service. Without the combined facilities of these two organizations the preparation of this paper could not have been accomplished. Dr. Ivan Mueller of the Geodetic Science Department of The Ohio State University served as adviser and provided essential guidance and counsel. ii VITA September 23, 1918 Born - Humboldt, Arizona 1941 oo.oo.o BoS. in Mining Engineering, University of Arizona 1941-1945 .... Military Service, European Theatre 1946-1950 o . o Mining Engineer, Magma Copper -
Prime Meridian ×
This website would like to remind you: Your browser (Apple Safari 4) is out of date. Update your browser for more × security, comfort and the best experience on this site. Encyclopedic Entry prime meridian For the complete encyclopedic entry with media resources, visit: http://education.nationalgeographic.com/encyclopedia/prime-meridian/ The prime meridian is the line of 0 longitude, the starting point for measuring distance both east and west around the Earth. The prime meridian is arbitrary, meaning it could be chosen to be anywhere. Any line of longitude (a meridian) can serve as the 0 longitude line. However, there is an international agreement that the meridian that runs through Greenwich, England, is considered the official prime meridian. Governments did not always agree that the Greenwich meridian was the prime meridian, making navigation over long distances very difficult. Different countries published maps and charts with longitude based on the meridian passing through their capital city. France would publish maps with 0 longitude running through Paris. Cartographers in China would publish maps with 0 longitude running through Beijing. Even different parts of the same country published materials based on local meridians. Finally, at an international convention called by U.S. President Chester Arthur in 1884, representatives from 25 countries agreed to pick a single, standard meridian. They chose the meridian passing through the Royal Observatory in Greenwich, England. The Greenwich Meridian became the international standard for the prime meridian. UTC The prime meridian also sets Coordinated Universal Time (UTC). UTC never changes for daylight savings or anything else. Just as the prime meridian is the standard for longitude, UTC is the standard for time.