Solar Object Finding the Sun. Prophead100 (Gregg Erickson)
|
|
|
- Arron Bates
- 5 years ago
- Views:
Transcription
1 Solar Object Finding the Sun Prophead100 (Gregg Erickson)
2 Options to Track Sun Timer Motor (always on, 1 axis only) Power Curve Tracking (clear days only) Paired Light Sensors ( searches, not predictive ) Shadow Camera (searches, sensitive) Predefined X Y Table ( specific to date & location ) Calculated ( real time/date, variable loc & freq)
3 Solar Calculators 2006 Rocklin 200 B.C. Greece
4
5
6 What Could a Solar Object Do? Aim a Mobile Solar Panel for More Power Reflect Sun to a Thermal Panel or Window Position a Solar Rover for a Recharge Navigate Without GPS Scribe a Sun Dial & Predict Shadows Position a Sunlight to Match Solar Equinox Seasonally Adjust Greenhouse Lights Use Sun to Send Morse Code Signals Seasonly Adjusted Clock
7 Solar Object 2.4 Collection of 20+ Solar Related Methods Heavily Documented with Floating Point Math Formulas with Link to On Line Book Real World Examples Predicts Angles to the Sun Calculates Angles to Reflect on Targets Provides Daily Solar Statistics
8 Example Documentation Pub DayLight_Hours(WS ) DHours ''Returns Daylight Hours Based Upon Angle Hours in a Day 'Equation 3.23 'Calculate Hours in a Day based upon Hour Angle 'that passes at 15 degrees per hour. 'Returns a floating point from a floating point input 'Annual Total Aywhere on Earth=4380 Hrs 'if you add all days together for a sigle site Dhours:=fmath.fdiv(fmath.fmul(Ws,2.0),15.0) Return DHours
9 Solar Object 2.4 Input/Outputs Input Time (Local Time, Daylight Savings) Location (Latitude, Longitude) Target (Distance: East, North, Height) Outputs Direction to the Sun (Azimuth, Altitude) Heliostat Mirror to Target (Azimuth, Altitude) Almanac ( Sunrise, Sunset, Twilight, Solar Noon)
10 Solar Object 2.4 Secondary Outputs Time Angles Day of Year, Solar Time, Equation of Time Declination, Hour Angle, Theta Angle Atmospheric & Reflection Effects Refraction Reflection Cosine Losses
11 Solar Object 2.4 Time Methods Equation of Time (Sun's Position Relative to Orbit & Rotation) PUB Equation_Of_Time3(N) PUB Equation_Of_Time2(N) PUB Equation_Of_Time(N) PUB Solar_Time_From_AngleHour(Dy) Relative to Sky PUB Local_Clock_Time(Hr, Lng, Mrdn, ET, D) Relative to Sun PUB Solar_Clock_Time(Hr, Lng, Mrdn, ET, D) Relative to Clock PUB Scout_Time(STime, Srise, Sset) Variable Time Based on Sun
12 Solar Object 2.4 Position Methods PUB Sun_Position(AzPtr, AltPtr, mo, dd, yy, hh, mm, ss, ds, lat, lng) Azimuth and Altitude Angles to the Sun PUB Get_Altitude(mo, dd, yy, hh, mm, ss, ds, lat, lng) PUB Get_Azimuth(mo, dd, yy, hh, mm, ss, ds, lat, lng) PUB Azimuth_Calc(Delta, Lat, Omega, Alpha) PUB Altitude_Calc(delta, Lat, Omega) PUB Helio_Altitude(AzPtr, AltPtr, ThetaPtr, FlightPtr, Az, Alt, N, E, Z) Azimuth and Altitude Angles Mirror Reflecting the Sun to a Target
13 Solar Object 2.4 Loss Methods PUB Refraction(h) Atmospheric Light Bending PUB Refraction_Main(h) PUB Refraction_Min(h) PUB Refraction_Neg(h) PUB Get_Spreading_Loss(N, P, SizePtr) Reflection Sizing PUB Get_Cosine_Loss(Theta) Angular Reflection Loss PUB Get_Elevation_Loss(D) Elevation Drop due to Earth's Curve
14 Solar Object 2.4 Demos Solar_Almanac (Daily Solar Data) Solar_Path_Demo (Quick Daily Trace) Analemma_Trace_Demo (Seasonal Pattern) Solar_Tracker_Demo (Real Time Track Sun) Heliostat_Demo (Reflect Sun to a Target)
15 Demo: Solar_Almanac Sunrise & Sunset (Azimuth & Time) Twilight Times (Civil, Nautical, Astronomic) Solar Noon (Time, Height) Daylength (Hours), Sun Height (Angle) Semi Hourly Direction Table (Azimuth, Altitude) Ideal for Quickstart & P.E. Kit
16 Demos: Tracker & Heliostat Real Time Angles (Azimuth, Altitude) Sun Direction Heliostat Target Uses Real Time Clock Emulator Outputs Details to PC & Direction to LCD Drives Two Servos Ideal for Protoboard & B.O.E
17 Testing Apparatus
18 Parallax (Futaba) Standard Servos Mirro r Para (Non llax 2x -Bac 16 S eria klit) l LC D Testing Apparatus 2 Axis Servo Mount
19 Testing Apparatus
20 Heliostat Target
21 Quick Demos Heliostat on Target Video Solar Path Trace Almanac...Try it yourself, OBEX & Parts List
22 Thanks William B. Stine, Ph.D. Power From The Sun Professor Emeritus Mechanical Engineering Department California State Polytechnic University Pomona, California USA Duane C. Johnson RedRock.com Solar Technology Cam Thompson & Chip Gracey OBEX Objects Floating Point Math Routines
Sunlight and its Properties II. EE 446/646 Y. Baghzouz
Sunlight and its Properties II EE 446/646 Y. Baghzouz Solar Time (ST) and Civil (clock) Time (CT) There are two adjustments that need to be made in order to convert ST to CT: The first is the Longitude
Solar Time, Angles, and Irradiance Calculator: User Manual
Solar Time, Angles, and Irradiance Calculator: User Manual Circular 674 Thomas Jenkins and Gabriel Bolivar-Mendoza 1 Cooperative Extension Service Engineering New Mexico Resource Network College of Agricultural,
Modern Navigation. Thomas Herring
12.215 Modern Navigation Thomas Herring Review of Monday s Class Spherical Trigonometry Review plane trigonometry Concepts in Spherical Trigonometry Distance measures Azimuths and bearings Basic formulas:
Student Exploration: Seasons: Earth, Moon, and Sun
Name: Date: Student Exploration: Seasons: Earth, Moon, and Sun Vocabulary: altitude, axis, azimuth, equinox, horizon, latitude, revolution, rotation, solstice Prior Knowledge Questions (Do these BEFORE
Geometry of Earth Sun System
12S56 Geometry of Earth Sun System Figure below shows the basic geometry Northern Hemisphere Winter ω equator Earth s Orbit Ecliptic ω ω SUN equator Northern Hemisphere Spring Northern Hemisphere Fall
ME 476 Solar Energy UNIT THREE SOLAR RADIATION
ME 476 Solar Energy UNIT THREE SOLAR RADIATION Unit Outline 2 What is the sun? Radiation from the sun Factors affecting solar radiation Atmospheric effects Solar radiation intensity Air mass Seasonal variations
EE Properties of Sunlight. Y. Baghzouz Professor of Electrical Engineering
EE 495-695 2.2 Properties of Sunlight Y. Baghzouz Professor of Electrical Engineering Azimuth angle The azimuth angle is the compass direction from which the sunlight is coming. At the equinoxes, the sun
Sunset Phenomena. Roger Bailey North American Sundial Society Hartford Oct 1999
Sunset Phenomena Roger Bailey North American Sundial Society Hartford Oct 1999 Sunset Phenomena Sunset Phenomena Simple spherical trigonometry can be used to determine for any location and day of the year
For most observers on Earth, the sun rises in the eastern
632 CHAPTER 25: EARTH, SUN, AND SEASONS WHAT IS THE SUN S APPARENT PATH ACROSS THE SKY? For most observers on Earth, the sun rises in the eastern part of the sky. The sun reaches its greatest angular altitude
Navigating by the Stars and Planets
Navigating by the Stars and Planets (Finding your location from measured altitudes of celestial bodies) Presented to: Chagrin Valley Astronomical Society September 1, 2012 By Ron Baker, CVAS member Historical
COMPUTER PROGRAM FOR THE ANGLES DESCRIBING THE SUN S APPARENT MOVEMENT IN THE SKY
COMPUTER PROGRAM FOR THE ANGLES DESCRIBING THE SUN S APPARENT MOVEMENT IN THE SKY B. BUTUC 1 Gh. MOLDOVEAN 1 Abstract: The paper presents software developed for the determination of the Sun-Earth geometry.
Computer Activity #3 SUNRISE AND SUNSET: THE SEASONS
NAME(S)!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! ASTRONOMY 25 Computer Activity #3 SUNRISE AND SUNSET: THE SEASONS SECTION DAY/TIME S. V. LLOYD Overview The seasonal variation in temperature is due to two changes
COMPUTER ACTIVITY 3: THE SEASONS: LENGTH OF THE DAY
NAME ASTRONOMY 20 SECTION DAY/ S. V. LLOYD COMPUTER ACTIVITY 3: THE SEASONS: LENGTH OF THE DAY Overview Software Configuration The seasonal variation in temperature is due to two changes in the Sun's path
Photovoltaic Systems Engineering
Photovoltaic Systems Engineering Ali Karimpour Associate Professor Ferdowsi University of Mashhad Reference for this lecture: Photovoltaic Systems Engineering Third Edition CRC Roger Messenger, Jerry Ventre
EGEE 437: HWK #2. Brownson. Yaqdaan Alkayyoomi, Mackenzie Ailes, Nicholas Minutillo, Sheel Vora. Group 17. Due on Thursday, Feb.
EGEE 437: HWK #2 Group 17 Due on Thursday, Feb. 18, 2016 Brownson Yaqdaan Alkayyoomi, Mackenzie Ailes, Nicholas Minutillo, Sheel Vora Contents Problem 5.1............................................ 2
Gnomon (a thin, round stick at least a foot long and capable of being put into the ground or stood up vertically)
Name: Partner(s): Lab #3 Celestial Navigation Due 7/2 Objectives In this lab you will take measurements of the sun s motion around noon and the north star s position in the sky. You will use this data
Astro 101 Lab #2. Start up the Stellarium program. If you do not remember how to use the user interface, please refer to Lab#1 or the user s guide.
Name: Astro 101 Lab #2 Lab objectives 1) Learn about how the Sun s path, through the sky, changes with the changing seasons. 2) Learn about how the Sun s path changes while viewing it at different locations
Modern Navigation. Thomas Herring
12.215 Modern Navigation Thomas Herring Review of last Class Motion of the Earth and Sun Geometry of Earth/Sun system Astronomical coordinates Motion of the Earth around the sun Equation of Time Astronomical
Understanding Positional Astronomy Part 2 Celestial Co-ordinates Difficulty: Intermediate
Exercise: Understanding Positional Astronomy Part 2 Celestial Co-ordinates Difficulty: Intermediate Objectives In Part 1 you learned about Celestial Sphere and how the stars appear to move across the night
Earth s Orbit. Sun Earth Relationships Ridha Hamidi, Ph.D. ESCI-61 Introduction to Photovoltaic Technology
1 ESCI-61 Introduction to Photovoltaic Technology Sun Earth Relationships Ridha Hamidi, Ph.D. Spring (sun aims directly at equator) Winter (northern hemisphere 23.5 tilts away from sun) 2 Solar radiation
for more please visit :
articlopedia.gigcities.com for more please visit : http://articlopedia.gigcities.com file:///d /important.html9/13/2006 8:50:19 PM CHAPTER 3 ASTRONOMICAL PHENOMENA 3.1 Sunrise, Sunset, and Twilight Introduction
3. The Sun s Position
3. The Sun s Position In order to understand how to collect energy from the sun, one must first be able to predict the location of the sun relative to the collection device. In this chapter we develop
LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME. a. understand the basic concepts needed for any astronomical coordinate system.
UNIT 2 UNIT 2 LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME Goals After mastery of this unit, you should: a. understand the basic concepts needed for any astronomical coordinate system. b. understand
NAVIGATION THEORY QUESTIONS Basics of Navigation
NAVIGATION THEORY QUESTIONS Basics of Navigation Q610065 look at it The angle between the plane of the ecliptic and the plane of equator is approx? 23.5 degrees In which two months of the year is the difference
Oberth: Energy vs. Momentum
1 2 The Oberth Effect 3 Oberth: Energy vs. Momentum 4 The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2-dimensional surface the Celestial Sphere. 5 The Celestial
Photovoltaic Systems Solar Radiation
PowerPoint Presentation Photovoltaic Systems Solar Radiation The Sun Solar Radiation Sun- Earth Relationships Array Orientation Solar Radiation Data Sets Estimating Array Performance Arizona Solar Power
Earth-Sun Relationships. The Reasons for the Seasons
Earth-Sun Relationships The Reasons for the Seasons Solar Radiation The earth intercepts less than one two-billionth of the energy given off by the sun. However, the radiation is sufficient to provide
Chapter 1 Solar Radiation
Chapter 1 Solar Radiation THE SUN The sun is a sphere of intensely hot gaseous matter with a diameter of 1.39 10 9 m It is, on the average, 1.5 10 11 m away from the earth. The sun rotates on its axis
Workforms. contents. Note on copyright and reproduction
Workforms contents Form 104 for Sight Reduction with Pub. 249 or 229 Form 106 for Sight Reduction with NAO Tables Form 107 for LAN Sights Form 108 Combined Sight Reduction Form 109 for Solar Index Correction
Practice Questions: Seasons #2
1. How many degrees does the Sun appear to move across the sky in four hours? A) 60 B) 45 C) 15 D) 4 Practice Questions: Seasons #2 2. Base your answer to the following question on the diagram below, which
Practice Questions: Seasons #1
1. Seasonal changes on Earth are primarily caused by the A) parallelism of the Sun's axis as the Sun revolves around Earth B) changes in distance between Earth and the Sun C) elliptical shape of Earth's
These notes may contain copyrighted material! They are for your own use only during this course.
Licensed for Personal Use Only DO NOT DISTRIBUTE These notes may contain copyrighted material! They are for your own use only during this course. Distributing them in anyway will be considered a breach
Equatorial Telescope Mounting
Equatorial Telescope Mounting Star Catalogs simbad IRSA The Meridian Every line of celestial longitude is a meridian of longitude, but we recognize the line of longitude, or simply the great circle line,
Reminder: Seasonal Motion
Seasonal Motion Reminder: Seasonal Motion If you observe the sky at the same time, say midnight, but on a different date, you find that the celestial sphere has turned: different constellations are high
Aileen A. O Donoghue Priest Associate Professor of Physics
SOAR: The Sky in Motion Life on the Tilted Teacup Ride Celestial Coordinates and the Day Aileen A. O Donoghue Priest Associate Professor of Physics Reference Points Poles Equator Prime Meridian Greenwich,
Cartesian Coordinates Need two dimensional system 2 number lines perpendicular to each other X-axis is horizontal Y-axis is vertical Position relative
General Physical Science Chapter 15 Place and Time Space and Time Einstein Space and time related Single entity Time is the 4 th dimension! Cartesian Coordinates Need some system to tell us where something
ME 430 Fundamentals of Solar Energy Conversion for heating and Cooling Applications
ME 430 Fundamentals of Solar Energy Conversion for heating and Cooling Applications Lecture (1 of 2) Solar Energy Resource and Availability C. Cruickshank and S. Harrison 2008 The Solar Constant 1 Variation
Clear as Night and Day:
6 Clear as Night and Day: Calculating Sunrise and Sunset Guiding Question What is the length of a degree longitude and latitude in your geographic location, and how does it affect sunrise and sunset? Project
Aileen A. O Donoghue Priest Associate Professor of Physics
SOAR: The Sky in Motion Life on the Tilted Teacup Ride The Year Aileen A. O Donoghue Priest Associate Professor of Physics Celestial Coordinates Right Ascension RA or From prime meridian (0 h ) to 23 h
A Celestial Navigation Primer
Introduction A Celestial Navigation Primer by Ron Davidson The study of celestial navigation, whether for blue water sailing, the taking of a navigation class (like the United States Power Squadron's JN
Motion of the Sun. motion relative to the horizon. rises in the east, sets in the west on a daily basis. Basis for the unit of time, the DAY
Motion of the Sun motion relative to the horizon rises in the east, sets in the west on a daily basis Basis for the unit of time, the DAY noon: highest point of Sun in sky relative to the horizon 1 altitude:
Physics Lab #3:! Starry Night! Observations of the Sun and Moon!
Physics 10293 Lab #3: Starry Night Observations of the Sun and Moon Introduction Today, we are going to use the Starry Night software to learn about motion of the stars, sun and moon on the celestial sphere.
June 15, 2006 July 19, 2009 A south facing vertical declining sundial by a barn in, Silver City, NM Using a trigon and empirical methods, and a gnomon whose sub-style was vertical True N Magnetic N Silver
Physics Lab #5: Starry Night Observations of the Sun and Moon
Physics 10293 Lab #5: Starry Night Observations of the Sun and Moon Introduction Today, we are going to use the Starry Night software to learn about motion of the stars, sun and moon on the celestial sphere.
Chapter 0 2/19/2014. Lecture Outline. 0.1 The Obvious View. Charting the Heavens. 0.1 The Obvious View. 0.1 The Obvious View. Units of Chapter 0
Lecture Outline Chapter 0 Charting the Heavens Earth is average we don t occupy any special place in the universe Universe: Totality of all space, time, matter, and energy Astronomy: Study of the universe
Motion of the Sun. View Comments
Login 2017 Survey to Improve Photovoltaic Education Christiana Honsberg and Stuart Bowden View Comments Instructions 1. Introduction 2. Properties of Sunlight 2.1. Basics of Light Properties of Light Energy
Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations.
Chapter 1: Discovering the Night Sky Constellations: Recognizable patterns of the brighter stars that have been derived from ancient legends. Different cultures have associated the patterns with their
Exercise 6. Solar Panel Orientation EXERCISE OBJECTIVE DISCUSSION OUTLINE. Introduction to the importance of solar panel orientation DISCUSSION
Exercise 6 Solar Panel Orientation EXERCISE OBJECTIVE When you have completed this exercise, you will understand how the solar illumination at any location on Earth varies over the course of a year. You
MiSP Astronomy Seasons Worksheet #1 L1
MiSP Astronomy Seasons Worksheet #1 L1 Name Date CHANGING HOURS OF DAYLIGHT ON LONG ISLAND Introduction You sometimes hear people say, Days are longer in the summer and shorter in the winter. That is a
Daily Motions. Daily Motions. Solar and Sidereal Days. Annual Motions of the Sun. Coordinate system on Earth. Annual Motion of the Stars.
Sun: rises in the east sets in the west travels on an arc across the sky 24 hours Daily Motions Solar Day = 24 hours Stars: stars travel on arcs in the sky moving from east to west. some stars rise and
ASTRONOMICAL NAVIGATION
Basic terms ASTRONOMICAL NAVIGATION *astronomical navigation *compilation *astronomical tabels *celestial observations *solution of a sight * Sun/Moon/star sight *spherical trigonometry *PZX triangle *celestial
MiSP Astronomy - Seasons Worksheet #1 L2
MiSP Astronomy - Seasons Worksheet #1 L2 Name Date Changing Hours of Daylight on Long Island (L 1, 2, 3) Introduction You sometimes hear people say, Days are longer in the summer and shorter in the winter.
ILLUSTRATING SHADOWS TABLE OF CONTENTS
ILLUSTRATING SHADOWS TABLE OF CONTENTS 316 pages Introduction Chapter Page Introduction and "A Quick Hands On Project" Part One 1 10 The approximate evolution of the dial 2 13 How the earth does its thing
Earth & Space Science, Interpreting Data DURATION Preparation: 5 minutes Activity: 40 minutes (total over one day)
Objectives In this activity students will: 1. Observe how the position of the sun in the sky changes during the course of the day 2. Discover the cardinal directions by tracking the motion of the sun Materials
The Celestial Sphere. From our perspective on Earth the stars appear embedded on a distant 2 dimensional surface the Celestial Sphere.
1 The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2 dimensional surface the Celestial Sphere. 2 The Celestial Sphere Although we know better, it is helpful to
LAB: What Events Mark the Beginning of Each Season?
Name: Date: LAB: What Events Mark the Beginning of Each Season? The relationship between the Sun and Earth have been used since antiquity to measure time. The day is measured by the passage of the Sun
Page 1. Name:
Name: 1) What is the primary reason New York State is warmer in July than in February? A) The altitude of the noon Sun is greater in February. B) The insolation in New York is greater in July. C) The Earth
Chapter 4 Earth, Moon, and Sky 107
Chapter 4 Earth, Moon, and Sky 107 planetariums around the world. Figure 4.4 Foucault s Pendulum. As Earth turns, the plane of oscillation of the Foucault pendulum shifts gradually so that over the course
Chapter 6. Solar Geometry. Contents
Chapter 6. Solar Geometry Contents 6.1 Introduction 6.2 The Sun 6.3 Elliptical Orbit 6.4 Tilt of the Earth s Axis 6.5 Consequences of the Altitude Angle 6.6 Winter 6.7 The Sun Revolves Around the Earth!
Modern Navigation
12.215 Modern Navigation Thomas Herring (tah@mit.edu), MW 11:00-12:30 Room 54-322 http://geoweb.mit.edu/~tah/12.215 Review of last Class Motion of the Earth and Sun Geometry of Earth/Sun system Astronomical
Astronomy 101: 9/18/2008
Astronomy 101: 9/18/2008 Announcements Pick up a golf ball at the front of the class or get one from Alex; you will need it for an in-class activity today. You will also need the question sheet from Alex.
Celestial Sphere Spectroscopy (Something interesting; e.g., advanced data analyses with IDL)
AST326, 2010 Winter Semester Celestial Sphere Spectroscopy (Something interesting; e.g., advanced data analyses with IDL) Practical Assignment: analyses of Keck spectroscopic data from the instructor (can
a. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU
1 AST104 Sp04: WELCOME TO EXAM 1 Multiple Choice Questions: Mark the best answer choice. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1. A galaxy
Sunlight and its Properties Part I. EE 446/646 Y. Baghzouz
Sunlight and its Properties Part I EE 446/646 Y. Baghzouz The Sun a Thermonuclear Furnace The sun is a hot sphere of gas whose internal temperatures reach over 20 million deg. K. Nuclear fusion reaction
FLATE Hillsborough Community College - Brandon (813)
The Florida Advanced Technological Education (FLATE) Center wishes to make available, for educational and noncommercial purposes only, materials relevant to the EST1830 Introduction to Alternative/Renewable
Introduction to Astronomy Laboratory Exercise #1. Intro to the Sky
Introduction to Astronomy Laboratory Exercise #1 Partners Intro to the Sky Date Section Purpose: To develop familiarity with the daytime and nighttime sky through the use of Stellarium. Equipment: Computer
COMPARATIVE STUDY BETWEEN AZIMUTH- ELEVATION AND TILT-ROLL SUN-TRACKING SYSTEMS IN RANGE OF MOTION
COMPARATIVE STUDY BETWEEN AZIMUTH- ELEVATION AND TILT-ROLL SUN-TRACKING SYSTEMS IN RANGE OF MOTION WANG TZE KOON UNIVERSITI TUNKU ABDUL RAHMAN COMPARATIVE STUDY BETWEEN AZIMUTH-ELEVATION AND TILT- ROLL
THE SUN. LENGTH: Course of the semester
ASTR 1030 Astronomy Lab 139 The Sun THE SUN SYNOPSIS: This exercise involves making measurements of the Sun every week throughout the semester, and then analyzing your results at semester s end. You ll
Exercise 7.0 THE CHANGING DIURNAL CIRCLES OF THE SUN
Exercise 7.0 THE CHANGING DIURNAL CIRCLES OF THE SUN I. The Apparent Annual Motion of the Sun A star always rises and sets at the same place on the horizon and, hence, it is above the horizon for the same
Literature Review: 1.
Literature Review: 1. The Solar Tracker, a device that keeps photovoltaic or photo-thermal panels in an optimum position perpendicularly to the solar radiation during daylight hours, can increase the collected
NAME; LAB # SEASONAL PATH OF THE SUN AND LATITUDE Hemisphere Model #3 at the Arctic Circle
NAME; PERIOD; DATE; LAB # SEASONAL PATH OF THE SUN AND LATITUDE Hemisphere Model #3 at the Arctic Circle 1 OBJECTIVE Explain how latitude affects the seasonal path of the Sun. I) Path of the Sun and Latitude.
Observer-Sun Angles. ), Solar altitude angle (α s. ) and solar azimuth angle (γ s )). θ z. = 90 o α s
Observer-Sun Angles Direction of Beam Radiation: The geometric relationships between a plane of any particular orientation relative to the earth at any time and the incoming beam solar radiation can be
CA1 2.11: Designing an Equatorial Sundial Activity
Purpose: To design an equatorial sundial and learn about motions of the sun and earth that have a bearing on its design. Materials: poster board, length of stiff wire or dowel rod, tape, protractor, ruler,
C2: NĂNG LƯỢNG ĐIỆN MẶT TRỜI
C2: NĂNG LƯỢNG ĐIỆN MẶT TRỜI 1. Nguồn năng lượng mặt trời 2. Tế bào quang điện 3. Đặc tuyến I-V của pin quang điện 4. Công nghệ chế tạo pin quang điện 5. Đặc tính làm việc của pin quang điện 6. Hệ điện
Seasonal Path of the Sun and Latitude
Seasonal Path of the Sun and Latitude Overview This lesson is a modification of what Dave Hess and I, Stan Skotnicki, use in our Earth Science classes at Cheektowaga Central High School. It is an extension
SUB-PROBLEM 2: HOW DO SUN AND EARTH MOVE FOR THE EXISTING CYCLES AND SYMMETRIES TO OCCUR? (The invention of a Sun/Earth model)
SUB-PROBLEM 2: HOW DO SUN AND EARTH MOVE FOR THE EXISTING CYCLES AND SYMMETRIES TO OCCUR? (The invention of a Sun/Earth model) We have made several advancements in the problem of interest proposed at the
ANALYSIS OF SOLAR PANEL EFFICIENCY THROUGH COMPUTATION AND SIMULATION 45
ANALYSIS OF SOLAR PANEL EFFICIENCY THROUGH COMPUTATION AND SIMULATION Hongyu Guo, University of Houston-Victoria; Mehrube Mehrubeoglu, Texas A&M University-Corpus Christi Abstract Solar panels are known
Phys Lab #1: The Sun and the Constellations
Phys 10293 Lab #1: The Sun and the Constellations Introduction Astronomers use a coordinate system that is fixed to Earth s latitude and longitude. This way, the coordinates of a star or planet are the
Tools of Astronomy Tools of Astronomy
Tools of Astronomy Tools of Astronomy The light that comes to Earth from distant objects is the best tool that astronomers can use to learn about the universe. In most cases, there is no other way to study
HNRS 227 Fall 2007 Chapter 14. Earth in Space presented by Prof. Geller 25 October 2007
HNRS 227 Fall 2007 Chapter 14 Earth in Space presented by Prof. Geller 25 October 2007 Key Points of Chapter 14 Shape, Size and Motions of the Earth Rotation and Revolution Precession Coordinate Systems
EELE408 Photovoltaics Lecture 04: Apparent Motion of the Sum
EELE408 Photovoltaics Lecture 04: Apparent Motion of the um Dr. Todd J. Kaiser tjkaiser@ece.montana.edu Apparent motion of the sun EAT Department of Electrical and Computer Engineering Montana tate University
2. The spectrum of visible light bounds the region of intensity of light emitted by the Sun. a. maximum b. minimum
CHAPTER 14 LIGHT AND SOUND IN THE ATMOSPHERE MULTIPLE CHOICE QUESTIONS 1. As the Sun s rays travel through the atmosphere, they are by cloud droplets or ice crystals, or by raindrops. a. scattered b. reflected
Discovering the Universe for Yourself (Chapter 2) Years, Seasons, and Months: The Motions of Sun, Earth, and Moon
Discovering the Universe for Yourself (Chapter 2) Years, Seasons, and Months: The Motions of Sun, Earth, and Moon Based on Chapter 2 This material will be useful for understanding Chapters 3 and 4 on The
Brock University. Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016
Brock University Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016 Number of hours: 50 min Time of Examination: 17:00 17:50 Instructor:
C) wavelength C) eastern horizon B) the angle of insolation is high B) increases, only D) thermosphere D) receive low-angle insolation
1. What is the basic difference between ultraviolet, visible, and infrared radiation? A) half-life B) temperature C) wavelength D) wave velocity 2. In New York State, the risk of sunburn is greatest between
Agricultural Science Climatology Semester 2, Anne Green / Richard Thompson
Agricultural Science Climatology Semester 2, 2006 Anne Green / Richard Thompson http://www.physics.usyd.edu.au/ag/agschome.htm Course Coordinator: Mike Wheatland Course Goals Evaluate & interpret information,
Chapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods?
Chapter S1 Celestial Timekeeping and Navigation S1.1 Astronomical Time Periods Our goals for learning:! How do we define the day, month, year, and planetary time periods?! How do we tell the time of day?!
FYI. 0 You will need to take notes this information will come in handy when going through this unit and on the cok.
FYI 0 You will need to take notes this information will come in handy when going through this unit and on the cok. One of the best ways to get started as a backyard astronomer is to learn the constellations.
Solar Energy Basics II - Estimation of Solar Radiation to a Solar Panel
PDHonline Course E287 (3 PDH) Solar Energy Basics II - Estimation of Solar Radiation to a Solar Panel Instructor: Harlan H. Bengtson, Ph.D., PE 2012 PDH Online PDH Center 5272 Meadow Estates Drive Fairfax,
Physics 312 Introduction to Astrophysics Lecture 3
Physics 312 Introduction to Astrophysics Lecture 3 James Buckley buckley@wuphys.wustl.edu Lecture 3 Celestial Coordinates the Planets and more History Reason for the Seasons Summer Solstice: Northern Hemisphere
Motions of the Sun Model Exploration
Name Date Bell Motions of the Sun Model Exploration 1. Go to the University of Nebraska-Lincoln Motions of the Sun Simulator: http://astro.unl.edu/naap/motion3/animations/sunmotions.swf 2. This is what
AFPAM MARCH Chapter 8 CELESTIAL CONCEPTS
AFPAM11-216 1 MARCH 2001 197 Section 8A Introduction to Celestial Concepts Chapter 8 CELESTIAL CONCEPTS 8.1. Basics. Celestial navigation is a universal aid to dead reckoning (DR). Because it is available
Lecture #03. January 20, 2010, Wednesday
Lecture #03 January 20, 2010, Wednesday Causes of Earth s Seasons Earth-Sun geometry Day length Solar angle (beam spread) Atmospheric beam depletion Shape and Size of the Earth North Pole E Geoid: not
Earth Science Seasons Test Name Per Date
Name Per Date Page 1 1. The diagram below represents four positions of the Earth as it revolves around the Sun. 5. Base your answer to the following question on the diagram below, which shows the apparent
Brock University. Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014
Brock University Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014 Number of hours: 50 min Time of Examination: 18:00 18:50 Instructor:
STONEHENGE AS A SOLSTICE INDICATOR
STONEHENGE AS A SOLSTICE INDICATOR One of the most impressive megalithic structures in the world is Stonehenge just north of Salisbury, England. I first visited the monument during my post-doctorate year
Chapter 2. Altitude Measurement
Chapter Altitude Measurement Although altitudes and zenith distances are equally suitable for navigational calculations, most formulas are traditionally based upon altitudes which are easily accessible
Day, Night & the Seasons. Lecture 2 1/15/2013
Day, Night & the Seasons Lecture 2 1/15/2013 Logistics The following students see me after class: Dahms, Doyle, Kavalle, Jennings, Melton, Polsky, Soriano, Augustinovich, Briggs Anyone who was not here
SOLAR WATER HEATER WITH TRACKING SYSTEM
SOLAR WATER HEATER WITH TRACKING SYSTEM Jyoti Verma 1, Shweta Tyagi 2, R. B. Dubey 3 1,2,3 Department of Electronics and Communication Engineering Hindu College of Engineering, Sonepat, Haryana, (India)
CHAPTER 19 SIGHT REDUCTION
CHAPTER 19 SIGHT REDUCTION BASIC PROCEDURES 1900. Computer Sight Reduction The purely mathematical process of sight reduction is an ideal candidate for computerization, and a number of different hand-held