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For Creative Minds
For Creative Minds The For Creative Minds educational section may be photocopied or printed from our website by the owner of this book for educational, non-commercial uses. Cross-curricular teaching activities, interactive quizzes, and more are available online. Go to www.ArbordalePublishing.com and click on the book’s cover to explore all the links. Moon Observations The months as we know them (January, February, etc.) are solar, based on how many days it takes the earth to revolve around the sun, roughly divided by twelve. A moon-th, or lunar (moon) month, is based on how long it takes the moon to orbit around the earth. The phases (shapes) of the moon change according to its cycle as it rotates around the earth, and the position of the moon with respect to the rising or setting sun. This cycle lasts about 29 ½ days. A (moon) month starts on “day one” with a new moon. The sun and the moon are in the same position and rise and set together. We can’t see the new moon. New Moon The moon rises and sets roughly 50 minutes later each day. The moon appears to “grow” or it waxes each day from a new moon to a full moon. The waxing moon’s bright side points at the setting Waxing sun and can be seen in the late afternoon on a clear day. Crescent A crescent moon is between new and half (less than half full), and may be waxing or waning. First Quarter The half-moon waxing or first quarter moon occurs about a week after the new moon. -
View and Print This Publication
@ 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. -
Moons Phases and Tides
Moon’s Phases and Tides Moon Phases Half of the Moon is always lit up by the sun. As the Moon orbits the Earth, we see different parts of the lighted area. From Earth, the lit portion we see of the moon waxes (grows) and wanes (shrinks). The revolution of the Moon around the Earth makes the Moon look as if it is changing shape in the sky The Moon passes through four major shapes during a cycle that repeats itself every 29.5 days. The phases always follow one another in the same order: New moon Waxing Crescent First quarter Waxing Gibbous Full moon Waning Gibbous Third (last) Quarter Waning Crescent • IF LIT FROM THE RIGHT, IT IS WAXING OR GROWING • IF DARKENING FROM THE RIGHT, IT IS WANING (SHRINKING) Tides • The Moon's gravitational pull on the Earth cause the seas and oceans to rise and fall in an endless cycle of low and high tides. • Much of the Earth's shoreline life depends on the tides. – Crabs, starfish, mussels, barnacles, etc. – Tides caused by the Moon • The Earth's tides are caused by the gravitational pull of the Moon. • The Earth bulges slightly both toward and away from the Moon. -As the Earth rotates daily, the bulges move across the Earth. • The moon pulls strongly on the water on the side of Earth closest to the moon, causing the water to bulge. • It also pulls less strongly on Earth and on the water on the far side of Earth, which results in tides. What causes tides? • Tides are the rise and fall of ocean water. -
Soaring Weather
Chapter 16 SOARING WEATHER While horse racing may be the "Sport of Kings," of the craft depends on the weather and the skill soaring may be considered the "King of Sports." of the pilot. Forward thrust comes from gliding Soaring bears the relationship to flying that sailing downward relative to the air the same as thrust bears to power boating. Soaring has made notable is developed in a power-off glide by a conven contributions to meteorology. For example, soar tional aircraft. Therefore, to gain or maintain ing pilots have probed thunderstorms and moun altitude, the soaring pilot must rely on upward tain waves with findings that have made flying motion of the air. safer for all pilots. However, soaring is primarily To a sailplane pilot, "lift" means the rate of recreational. climb he can achieve in an up-current, while "sink" A sailplane must have auxiliary power to be denotes his rate of descent in a downdraft or in come airborne such as a winch, a ground tow, or neutral air. "Zero sink" means that upward cur a tow by a powered aircraft. Once the sailcraft is rents are just strong enough to enable him to hold airborne and the tow cable released, performance altitude but not to climb. Sailplanes are highly 171 r efficient machines; a sink rate of a mere 2 feet per second. There is no point in trying to soar until second provides an airspeed of about 40 knots, and weather conditions favor vertical speeds greater a sink rate of 6 feet per second gives an airspeed than the minimum sink rate of the aircraft. -
Hunting Hours Time Zone A
WHEN AND WHERE TO HUNT WHEN AND WHERE Hunting Hours Time Zone A. Hunting Hours for Bear, Deer, Fall Wild Turkey, Furbearers, Shown is a map of the hunting-hour time zones. Actual legal hunting hours for and Small Game bear, deer, fall wild turkey, furbearer, and small game for Time Zone A are shown One-half hour before sunrise to one-half hour after sunset (adjusted for in the table at right. Hunting hours for migratory game birds are different and are daylight saving time). For hunt dates not listed in the table, please consult your published in the current-year Waterfowl Digest. local newspaper. 2016 Sept. Oct. Nov. Dec. To determine the opening (a.m.) and closing (p.m.) time for any day in another Note: time zone, add the minutes shown below to the times listed in the Time Zone A • Woodcock and teal Date AM PM AM PM AM PM AM PM Hunting Hours Table. hunting hours are 1 6:28 8:35 7:00 7:43 7:36 6:55 7:12 5:31 The hunting hours listed in the table reflect Eastern Standard Time, with an sunrise to sunset. 2 6:29 8:34 7:01 7:41 7:38 6:54 7:14 5:30 adjustment for daylight saving time. If you are hunting in Gogebic, Iron, Dickinson, • Spring turkey hunting 3 6:30 8:32 7:02 7:39 7:39 6:52 7:15 5:30 or Menominee counties (Central Standard Time), you must make an additional hours are one-half 4 6:31 8:30 7:03 7:38 7:40 6:51 7:16 5:30 adjustment to the printed time by subtracting one hour. -
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%. -
The Mathematics of the Chinese, Indian, Islamic and Gregorian Calendars
Heavenly Mathematics: The Mathematics of the Chinese, Indian, Islamic and Gregorian Calendars Helmer Aslaksen Department of Mathematics National University of Singapore [email protected] www.math.nus.edu.sg/aslaksen/ www.chinesecalendar.net 1 Public Holidays There are 11 public holidays in Singapore. Three of them are secular. 1. New Year’s Day 2. Labour Day 3. National Day The remaining eight cultural, racial or reli- gious holidays consist of two Chinese, two Muslim, two Indian and two Christian. 2 Cultural, Racial or Religious Holidays 1. Chinese New Year and day after 2. Good Friday 3. Vesak Day 4. Deepavali 5. Christmas Day 6. Hari Raya Puasa 7. Hari Raya Haji Listed in order, except for the Muslim hol- idays, which can occur anytime during the year. Christmas Day falls on a fixed date, but all the others move. 3 A Quick Course in Astronomy The Earth revolves counterclockwise around the Sun in an elliptical orbit. The Earth ro- tates counterclockwise around an axis that is tilted 23.5 degrees. March equinox June December solstice solstice September equinox E E N S N S W W June equi Dec June equi Dec sol sol sol sol Beijing Singapore In the northern hemisphere, the day will be longest at the June solstice and shortest at the December solstice. At the two equinoxes day and night will be equally long. The equi- noxes and solstices are called the seasonal markers. 4 The Year The tropical year (or solar year) is the time from one March equinox to the next. The mean value is 365.2422 days. -
Impact of Extended Daylight Saving Time on National Energy Consumption
Impact of Extended Daylight Saving Time on National Energy Consumption TECHNICAL DOCUMENTATION FOR REPORT TO CONGRESS Energy Policy Act of 2005, Section 110 Prepared for U.S. Department of Energy Office of Energy Efficiency and Renewable Energy By David B. Belzer (Pacific Northwest National Laboratory), Stanton W. Hadley (Oak Ridge National Laboratory), and Shih-Miao Chin (Oak Ridge National Laboratory) October 2008 U.S. Department of Energy Energy Efficiency and Renewable Energy Page Intentionally Left Blank Acknowledgements The Department of Energy (DOE) acknowledges the important contributions made to this study by the principal investigators and primary authors—David B. Belzer, Ph.D (Pacific Northwest National Laboratory), Stanton W. Hadley (Oak Ridge National Laboratory), and Shih-Miao Chin, Ph.D (Oak Ridge National Laboratory). Jeff Dowd (DOE Office of Energy Efficiency and Renewable Energy) was the DOE project manager, and Margaret Mann (National Renewable Energy Laboratory) provided technical and project management assistance. Two expert panels provided review comments on the study methodologies and made important and generous contributions. 1. Electricity and Daylight Saving Time Panel – technical review of electricity econometric modeling: • Randy Barcus (Avista Corp) • Adrienne Kandel, Ph.D (California Energy Commission) • Hendrik Wolff, Ph.D (University of Washington) 2. Transportation Sector Panel – technical review of analytical methods: • Harshad Desai (Federal Highway Administration) • Paul Leiby, Ph.D (Oak Ridge National Laboratory) • John Maples (DOE Energy Information Administration) • Art Rypinski (Department of Transportation) • Tom White (DOE Office of Policy and International Affairs) The project team also thanks Darrell Beschen (DOE Office of Energy Efficiency and Renewable Energy), Doug Arent, Ph.D (National Renewable Energy Laboratory), and Bill Babiuch, Ph.D (National Renewable Energy Laboratory) for their helpful management review. -
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. -
Chapter 19 the Almanacs
CHAPTER 19 THE ALMANACS PURPOSE OF ALMANACS 1900. Introduction The Air Almanac was originally intended for air navigators, but is used today mostly by a segment of the Celestial navigation requires accurate predictions of the maritime community. In general, the information is similar to geographic positions of the celestial bodies observed. These the Nautical Almanac, but is given to a precision of 1' of arc predictions are available from three almanacs published and 1 second of time, at intervals of 10 minutes (values for annually by the United States Naval Observatory and H. M. the Sun and Aries are given to a precision of 0.1'). This Nautical Almanac Office, Royal Greenwich Observatory. publication is suitable for ordinary navigation at sea, but The Astronomical Almanac precisely tabulates celestial lacks the precision of the Nautical Almanac, and provides data for the exacting requirements found in several scientific GHA and declination for only the 57 commonly used fields. Its precision is far greater than that required by navigation stars. celestial navigation. Even if the Astronomical Almanac is The Multi-Year Interactive Computer Almanac used for celestial navigation, it will not necessarily result in (MICA) is a computerized almanac produced by the U.S. more accurate fixes due to the limitations of other aspects of Naval Observatory. This and other web-based calculators are the celestial navigation process. available from: http://aa.usno.navy.mil. The Navy’s The Nautical Almanac contains the astronomical STELLA program, found aboard all seagoing naval vessels, information specifically needed by marine navigators. contains an interactive almanac as well. -
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. -
How the Sun Paints the Sky the Generation of Its Colour and Luminosity Bob Fosbury European Southern Observatory and University College London
How the Sun Paints the Sky The generation of its colour and luminosity Bob Fosbury European Southern Observatory and University College London Introduction: the 19th century context — science and painting The appearance of a brilliantly clear night sky must surely have stimulated the curiosity of our earliest ancestors and provided them with the foundation upon which their descendants built the entire edifice of science. This is a conclusion that would be dramatically affirmed if any one of us were to look upwards in clear weather from a location that is not polluted by artificial light: an increasingly rare possibility now, but one that provides a welcome regeneration of the sense of wonder. What happened when our ancient ancestors gazed instead at the sky in daylight or twilight? It is difficult to gauge from written evidence as there was such variation in the language of description among different cultures (see “Sky in a bottle” by Peter Pesic. MIT Press, 2005. ISBN 0-262-16234-2). The blue colour of a cloudless sky was described in a remarkable variety of language, but the question of its cause most often remained in the realm of a superior being. Its nature did concern the Greek philosophers but they appeared to describe surfaces and objects in the language of texture rather than colour: they did not have a word for blue. It was only during the last millennium that thinkers really tried to get to grips with the problem, with Leonardo da Vinci, Isaac Newton and Johann Wolfgang von Goethe all applying themselves. It was not easy however, and no real progress was made until the mid-19th century when there was a focus of the greatest scientific minds of the time on the problem of both the colour and the what was then the novel property of polarisation of the light.