Chapter 19 the Almanacs
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@ SOUTHWEST FOREST SERVICE Forest and R U. S.DEPARTMENT OF AGRICULTURE P.0. BOX 245, BERKELEY, CALIFORNIA 94701 Experime Computation of times of sunrise, sunset, and twilight in or near mountainous terrain Bill 6. Ryan Times of sunrise and sunset at specific mountain- ous locations often are important influences on for- estry operations. The change of heating of slopes and terrain at sunrise and sunset affects temperature, air density, and wind. The times of the changes in heat- ing are related to the times of reversal of slope and valley flows, surfacing of strong winds aloft, and the USDA Forest Service penetration inland of the sea breeze. The times when Research NO& PSW- 322 these meteorological reactions occur must be known 1977 if we are to predict fire behavior, smolce dispersion and trajectory, fallout patterns of airborne seeding and spraying, and prescribed burn results. ICnowledge of times of different levels of illumination, such as the beginning and ending of twilight, is necessary for scheduling operations or recreational endeavors that require natural light. The times of sunrise, sunset, and twilight at any particular location depend on such factors as latitude, longitude, time of year, elevation, and heights of the surrounding terrain. Use of the tables (such as The 1 Air Almanac1) to determine times is inconvenient Ryan, Bill C. because each table is applicable to only one location. 1977. Computation of times of sunrise, sunset, and hvilight in or near mountainous tersain. USDA Different tables are needed for each location and Forest Serv. Res. Note PSW-322, 4 p. Pacific corrections must then be made to the tables to ac- Southwest Forest and Range Exp. -
Celestial Navigation Tutorial
NavSoft’s CELESTIAL NAVIGATION TUTORIAL Contents Using a Sextant Altitude 2 The Concept Celestial Navigation Position Lines 3 Sight Calculations and Obtaining a Position 6 Correcting a Sextant Altitude Calculating the Bearing and Distance ABC and Sight Reduction Tables Obtaining a Position Line Combining Position Lines Corrections 10 Index Error Dip Refraction Temperature and Pressure Corrections to Refraction Semi Diameter Augmentation of the Moon’s Semi-Diameter Parallax Reduction of the Moon’s Horizontal Parallax Examples Nautical Almanac Information 14 GHA & LHA Declination Examples Simplifications and Accuracy Methods for Calculating a Position 17 Plane Sailing Mercator Sailing Celestial Navigation and Spherical Trigonometry 19 The PZX Triangle Spherical Formulae Napier’s Rules The Concept of Using a Sextant Altitude Using the altitude of a celestial body is similar to using the altitude of a lighthouse or similar object of known height, to obtain a distance. One object or body provides a distance but the observer can be anywhere on a circle of that radius away from the object. At least two distances/ circles are necessary for a position. (Three avoids ambiguity.) In practice, only that part of the circle near an assumed position would be drawn. Using a Sextant for Celestial Navigation After a few corrections, a sextant gives the true distance of a body if measured on an imaginary sphere surrounding the earth. Using a Nautical Almanac to find the position of the body, the body’s position could be plotted on an appropriate chart and then a circle of the correct radius drawn around it. In practice the circles are usually thousands of miles in radius therefore distances are calculated and compared with an estimate. -
12.3 the Moon: Phases, Eclipses, and the Tides
12.3 The Moon: Phases, Eclipses, and the Tides 1. The Motions of the Moon a. Rotation i. Period of Moon’s rotation = 27.3 days b. Revolution (orbit) i. Period of the Moon’s orbit around the Earth = 27.3 days ii. Lunar cycle = 29.5 days (time that the calendar month is based on) 1. Time needed for the moon to return to the same place in the sky 2. Since the Earth is orbiting as well as the Moon, the Moon needs the extra 2 days to “catch up to the Earth” in its orbit c. Orbital period of the moon = the rotational period of the moon = 27.3 days i. Synchronous rotation ii. Reason that we only see one side of the Moon 2. Phases of the Moon a. Order of the phases i. Based on the Moon appears to us on Earth ii. New moon, waxing crescent, 1st quarter, waxing gibbous, full moon, waning gibbous, 3rd/last quarter, waning crescent b. The sun’s light moves from right to left across the face of the moon c. Moonrise and moonset i. Time when one’s location on Earth can see the moon 3. Eclipses a. Any time one celestial body passes between another celestial body and the Sun b. Lunar eclipse i. Partial lunar eclipse; when the any part of the Moon falls within the penumbra (partial shadow) of the Earth ii. Total lunar eclipse; when the Moon falls entirely within the umbra (total shadow) of the Earth c. Solar eclipse i. Partial solar eclipse; when any point on the Earth falls within the penumbra (partial shadow) of the Moon ii. -
Naked-Eye Observations of the Moon (See Also Take-Home Exp
TAKE-HOME EXP. # 3 Naked-Eye Observations of the Moon (See also Take-Home Exp. #4 which can easily be done at the same time as this one.) You have already seen what the Moon looks like in its various phases, but you may not realize it can be "out" in the day as well as the night. Nor are most people familiar enough with the geometry of the Sun-Moon-Earth system to draw it as easily as you will be able to by the end of this experiment. a. When to make observations of the moon's phases: nytime you can find the Moon, make an observation. These observations do not have to occur only at the principal phases. Anytime and anywhere you can see the Moon is a good time to make a sketch and record the requested information. b. Dates of the Principal phases of the Moon, Times of Moonrise, and Moonset: Earth When doing this experiment, check your newspaper New Moon everyday for the times of moonrise and moonset; they are listed on the weather page. Many calendars show the days of occurrence of the principal phases--new, first- 1st Qrtr quarter, full, third quarter--of the Moon. Most newspapers have the principal phase dates listed every day. In the view of Earth pictured to the right, the Moon’s orbit is the circle, and incoming sunlight is from the right. Full The Moon moves counterclockwise around the Earth, taking 28 days to complete its cycle. Starting at the topmost diagram, a “New Moon” phase, seven days elapse between each succeeding diagram. -
Good Morning, Good Afternoon, and Good Evening to All of Our Participants Around the World
>>>Good morning, good afternoon, and good evening to all of our participants around the world. Welcome to this Webinar sponsored by the international forum for investor education, IFIE and America's chapter of how an investor's complaint can be used to further investor educational goals. You will be hearing from two presenters today, Kattia Castro Cruz and Pierino Stucchi. Before we introduce Kattia Castro Cruz as your moderator I want to explain how the Q&A answer will work. During the question period, to ask a question type the name of your organization and your question into the question box on your Webinar dashboard. This is located towards the bottom of the screen. We often have more questions than we have time to answer. We will try to answer all of the questions that we receive through the Webinar or we will post them after the Webinar event. Thank you again, and I will ask our facilitator leader, Kattia Castro Cruz, to take over. >> Thank you, Katherine, good morning, good afternoon, and good night to all the participants around the world. Welcome to this Webinar that is sponsored by the international forum for investor education IFIE and the America's chapter. Today we have two conferences, and we will have time for questions and answers at the end of the presentation. During the session of questions and answers, to make a question, just put your name, type your name into, and your organization name and then you will have time at the end. It's on the bottom of the right hand screen. -
Key Stage 2: Daytime Moon Viewing
Key Stage 2: Daytime Moon Viewing Teacher’s Notes Curriculum Links: Unit 5E Earth, Sun and Moon, Unit 3F Light and Shadows This extension activity uses daytime viewing of the Moon (during school hours) to reinforce ideas learned in the classroom about light, shadow and the Moon itself. Equipment: Magnetic compass, notepads and pencils for students. Optional: Set(/s) of binoculars, monoculars or telescopes for closer observation of the Moon, cameras. Class discussion before the activity: How can we see the Moon? Answer: The light from the Sun reflects off the Moon and into our eyes or our telescopes. Reflections are how we see most things on a day-to-day basis. Sunlight also reflects off the planets and that is how we see them. Stars, like the Sun are light sources, while other objects are not. Draw the Moon and Earth on the board as shown below, but with no shaded halves. The curved arrows represent the way the Moon orbits the Earth (viewed from a top-down perspective) and the straight arrows represent the light coming from the Sun. Ask students to copy the diagram and shade in the bits of the Earth and Moon that are in darkness, where the Sun’s light does not reach. Some students may ask how the light of the Moon can get to the Earth in the previous diagram. The orbit of the Moon is tilted with respect to Earth’s orbit around the Sun – the diagram on the next page will help students visualise what is happening. Is the Moon ever completely dark? Answer: No. -
Phases of the Moon
TA Guide for Notes Phases of the Moon Description In this activity, students stand around a bright light bulb in an otherwise dark room, holding a styrofoam ball at arm’s length. As they turn around, they watch the changing pattern of light and dark on the styrofoam ball which reproduces the phases of the Moon. Then, using a second ball as the Earth, students explore the geometry of the Sun-Earth-Moon system to predict the rise and set times of different phases of the Moon. The students “accidentally” stumble onto the alignment of the Sun, Earth and Moon during lunar and solar eclipses. Learning Goals After this tutorial, together with lecture materials, students should be able to • use the geometry of the Sun, Earth and Moon to illustrate the phases of the Moon and to predict the Moon’s rise and set times • illustrate the geometry of the Sun, Earth and Moon during lunar and solar eclipses, and explain why there are not eclipses every month Set-up 20 minutes The students will work together in groups of 3. In order to fit enough groups of students, you may need to use 2 light sources (shown at right). Set up one in the center of the lab and, if necessary, one in the center of the reading room (push the tables to the inside around the light. This will stop the students from getting too close to the light and messing up the geometry.) When both lights are needed, both TAs will be “A” TAs that lead the activity to their own groups of students. -
The Golden Hour Refers to the Hour Before Sunset and After Sunrise
TheThe GoldenGolden HourHour The Golden Hour refers to the hour before sunset and after sunrise. Photographers agree that some of the very best times of day to take photos are during these hours. During the Golden Hours, the atmosphere is often permeated with breathtaking light that adds ambiance and interest to any scene. There can be spectacular variations of colors and hues ranging from subtle to dramatic. Even simple subjects take on an added glow. During the Golden Hours, take photos when the opportunity presents itself because light changes quickly and then fades away. 07:14:09 a.m. 07:15:48 a.m. Photographed about 60 seconds after previous photo. The look of a scene can vary greatly when taken at different times of the day. Scene photographed midday Scene photographed early morning SampleSample GoldenGolden HourHour photosphotos Top Tips for taking photos during the Golden Hours Arrive on the scene early to take test shots and adjust camera settings. Set camera to matrix or center-weighted metering. Use small apertures for maximizing depth-of-field. Select the lowest possible ISO. Set white balance to daylight or sunny day. When lighting is low, use a tripod with either a timed shutter release (self-timer) or a shutter release cable or remote. Taking photos during the Golden Hours When photographing the sun Don't stare into the sun, or hold the camera lens towards it for a very long time. Meter for the sky but don't include the sun itself. Composition tips: The horizon line should be above or below the center of the scene. -
The British Astronomical Association Handbook 2017
THE HANDBOOK OF THE BRITISH ASTRONOMICAL ASSOCIATION 2017 2016 October ISSN 0068–130–X CONTENTS PREFACE . 2 HIGHLIGHTS FOR 2017 . 3 CALENDAR 2017 . 4 SKY DIARY . .. 5-6 SUN . 7-9 ECLIPSES . 10-15 APPEARANCE OF PLANETS . 16 VISIBILITY OF PLANETS . 17 RISING AND SETTING OF THE PLANETS IN LATITUDES 52°N AND 35°S . 18-19 PLANETS – EXPLANATION OF TABLES . 20 ELEMENTS OF PLANETARY ORBITS . 21 MERCURY . 22-23 VENUS . 24 EARTH . 25 MOON . 25 LUNAR LIBRATION . 26 MOONRISE AND MOONSET . 27-31 SUN’S SELENOGRAPHIC COLONGITUDE . 32 LUNAR OCCULTATIONS . 33-39 GRAZING LUNAR OCCULTATIONS . 40-41 MARS . 42-43 ASTEROIDS . 44 ASTEROID EPHEMERIDES . 45-50 ASTEROID OCCULTATIONS .. ... 51-53 ASTEROIDS: FAVOURABLE OBSERVING OPPORTUNITIES . 54-56 NEO CLOSE APPROACHES TO EARTH . 57 JUPITER . .. 58-62 SATELLITES OF JUPITER . .. 62-66 JUPITER ECLIPSES, OCCULTATIONS AND TRANSITS . 67-76 SATURN . 77-80 SATELLITES OF SATURN . 81-84 URANUS . 85 NEPTUNE . 86 TRANS–NEPTUNIAN & SCATTERED-DISK OBJECTS . 87 DWARF PLANETS . 88-91 COMETS . 92-96 METEOR DIARY . 97-99 VARIABLE STARS (RZ Cassiopeiae; Algol; λ Tauri) . 100-101 MIRA STARS . 102 VARIABLE STAR OF THE YEAR (T Cassiopeiæ) . .. 103-105 EPHEMERIDES OF VISUAL BINARY STARS . 106-107 BRIGHT STARS . 108 ACTIVE GALAXIES . 109 TIME . 110-111 ASTRONOMICAL AND PHYSICAL CONSTANTS . 112-113 INTERNET RESOURCES . 114-115 GREEK ALPHABET . 115 ACKNOWLEDGEMENTS / ERRATA . 116 Front Cover: Northern Lights - taken from Mount Storsteinen, near Tromsø, on 2007 February 14. A great effort taking a 13 second exposure in a wind chill of -21C (Pete Lawrence) British Astronomical Association HANDBOOK FOR 2017 NINETY–SIXTH YEAR OF PUBLICATION BURLINGTON HOUSE, PICCADILLY, LONDON, W1J 0DU Telephone 020 7734 4145 PREFACE Welcome to the 96th Handbook of the British Astronomical Association. -
Chapter 6 Nautical Publications
CHAPTER 6 NAUTICAL PUBLICATIONS INTRODUCTION 600. Publications supply a ship’s chart and publication library. On-line publications produced by the U.S. government are The navigator uses many textual information sources available on the Web. to plan and conduct a voyage. These sources include notices to mariners, summary of corrections, sailing directions, 601. Maintenance and Carriage Requirements of light lists, tide tables, sight reduction tables, and almanacs. Navigation Publications While it is still possible to obtain hard-copy or printed nautical publications, increasingly these texts Vessels may maintain the navigation publications are found online or in other digital formats, including required by Title 33 of the Code of Federal Regulations Compact Disc-Read Only Memory (CD-ROM's) or Parts 161.4, 164.33, and 164.72 and SOLAS Chapter V Digital Versatile Disc (DVD's). Digital publications are Regulation 27 in electronic format provided that they are much less expensive than printed publications to repro- derived from the original source, are currently duce and distribute, and online publications have no corrected/up-to-date, and are readily accessible on the reproduction costs at all for the producer, and only mi- vessel's bridge by the crew. Adequate independent back-up nor costs to the user. Also, one DVD can hold entire arrangements shall be provided in case of libraries of information, making both distribution and electronic/technical failure. Such arrangements include: a on-board storage much easier. The advantages of electronic publications over second computer, CD, or portable mass storage device hard-copy go beyond cost savings. They can be updated readily displayable to the navigation watch, or printed easier and more often, making it possible for mariners paper copies. -
Exploring Solar Cycle Influences on Polar Plasma Convection
Comparison of Terrestrial and Martian TEC at Dawn and Dusk during Solstices Angeline G. Burrell1 Beatriz Sanchez-Cano2, Mark Lester2, Russell Stoneback1, Olivier Witasse3, Marco Cartacci4 1Center for Space Sciences, University of Texas at Dallas 2Radio and Space Plasma Physics, University of Leicester 3European Space Agency, ESTEC – Scientific Support Office 4Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali 52nd ESLAB Symposium Outline • Motivation • Data and analysis – TEC sources – Data selection – Linear fitting • Results – Martian variations – Terrestrial variations – Similarities and differences • Conclusions Motivation • The Earth and Mars are arguably the most similar of the solar planets - They are both inner, rocky planets - They have similar axial tilts - They both have ionospheres that are formed primarily through EUV and X- ray radiation • Planetary differences can provide physical insights Total Electron Content (TEC) • The Global Positioning System • The Mars Advanced Radar for (GPS) measures TEC globally Subsurface and Ionosphere using a network of satellites and Sounding (MARSIS) measures ground receivers the TEC between the Martian • MIT Haystack provides calibrated surface and Mars Express TEC measurements • Mars Express has an inclination - Available from 1999 onward of 86.9˚ and a period of 7h, - Includes all open ground and allowing observations of all space-based sources locations and times - Specified with a 1˚ latitude by 1˚ • TEC is available for solar zenith longitude resolution with error estimates angles (SZA) greater than 75˚ Picardi and Sorge (2000), In: Proc. SPIE. Eighth International Rideout and Coster (2006) doi:10.1007/s10291-006-0029-5, 2006. Conference on Ground Penetrating Radar, vol. 4084, pp. 624–629. -
Planit! User Guide
ALL-IN-ONE PLANNING APP FOR LANDSCAPE PHOTOGRAPHERS QUICK USER GUIDES The Sun and the Moon Rise and Set The Rise and Set page shows the 1 time of the sunrise, sunset, moonrise, and moonset on a day as A sunrise always happens before a The azimuth of the Sun or the well as their azimuth. Moon is shown as thick color sunset on the same day. However, on lines on the map . some days, the moonset could take place before the moonrise within the Confused about which line same day. On those days, we might 3 means what? Just look at the show either the next day’s moonset or colors of the icons and lines. the previous day’s moonrise Within the app, everything depending on the current time. In any related to the Sun is in orange. case, the left one is always moonrise Everything related to the Moon and the right one is always moonset. is in blue. Sunrise: a lighter orange Sunset: a darker orange Moonrise: a lighter blue 2 Moonset: a darker blue 4 You may see a little superscript “+1” or “1-” to some of the moonrise or moonset times. The “+1” or “1-” sign means the event happens on the next day or the previous day, respectively. Perpetual Day and Perpetual Night This is a very short day ( If further north, there is no Sometimes there is no sunrise only 2 hours) in Iceland. sunrise or sunset. or sunset for a given day. It is called the perpetual day when the Sun never sets, or perpetual night when the Sun never rises.