FYS 3610 Research infrastructure and substorm aurora
|
|
|
- Amos Black
- 7 years ago
- Views:
Transcription
1 FYS 3610 Research infrastructure and substorm aurora
2 Research Infrastructure Main installations for Space Research in North Norway and Svalbard Longyearbyen UNIS, EISCAT Svalbard Radar The auroral station Ny-Ålesund Norwegian polar institute, SvalRak North-Norway ARS, EISCAT
3 The Earth rotates underneath the auroral oval
4 The Uniqueness about Svalbard Ideally located for daytime auroral measurements Well developed research infrastructure Multi-instrument observations
5 UNIS 14 full-time scientists And ~100 students
6 The auroral station, LYR Owned by the University of Tromsø Operated by UNIS Ca. 22 instruments, 16 institutions from 8 nations
7 The new auroral station, LYR 15 out of 32 domes will be used after moving the instruments from Adventdalen.
8 Location of the new station
9 Why? Old station in Adventdalen is too small! Light pollution from Longyearbyen has increased! We need new improved working conditions! Space to accommodate new instruments and partners! Co-location with EISCAT and others Improved teaching and training facilities Continue and quality improve our long term measurements Keep the old station s scientific momentum Get away from sand storms in Adventdalen during autumn and spring Secure the field of auroral optics!
10 Ny-Ålesund Auroral Platform Key instruments: Meridian Scanning Photometer 4 channels All-Sky Camera (5 positions filter wheel)
11 All-sky field of view coverage NY A LY R ARS
12 FAST passasje gjennom Nordlyset
13 EISCAT Scientific Association 3 Incoherent Scatter Radar Systems: Tromsø UHF (933 MHz) - 3-static with receivers at Kiruna and Sodankylä Tromsø VHF (224 MHz) Eiscat Svalbard Radar - dual antenna system (500 MHz) Associated countries: Germany, France, Finland, Japan, Norway, Sweden, UK
14 ARS and Svalrak ISAS launch Nov/Dec 2000
15 Ground support for CLUSTER 13:40 30 Nov, 2000
16 Solar-Terrestrial interaction
17 The Terella Experiment
18 The Sun- A boiling soup of plasma
19 CME
20 The solar wind
21 Aurora a visualisation of solar terrestrial coupling
22 Solar wind interaction with the Earth s magnetic field
23 NORDLYS Nordlys sett fra romferga Challenger
24 Aurora Borealis Aurora Australis
25 IMF North Good shield N S N South IMF S Bad shield
26 Dynamics of thesubstorm expansion phase
27 Auroral and Magnetic Signatures associated with substorm onset
28 Magnetometers
29 Subtorm phases T=0 T=0-5 min T=5-10 min T=10-30 min T=30-60 min T=1-2 hours
30 Colors in the aurora nm red upper border Atomic oxygen: 1 D- 1 S transition nm green Atomic oxygen : 1 D - 3 P transition nm magenta bottom border N + 2-1st negative band Figure: Farge som funksjon av høyde
EISCAT_3D The view from Swedish Institute of Space Physics
EISCAT_3D The view from Swedish Institute of Space Physics Lars Eliasson Institutet för rymdfysik Photo Ingrid Sandahl 1957 Swedish Institute of Space Physics Basic research Long term observations Scientific
Curriculum Vitae: Tuija Inkeri Pulkkinen Aalto University tel: +358-50-591 6013
Curriculum Vitae: Tuija Inkeri Pulkkinen Aalto University tel: +358-50-591 6013 POBox 17800, 00076 AALTO, Finland e-mail: tuija.pulkkinen@aalto.fi Updated May 16, 2015 Research interests Sun-Earth connection
the icy, dancing skies of the north
Aurora Borealis the icy, dancing skies of the north 35 What are the aurora borealis? People generally know the aurora borealis by their common name, the Northern Lights. The northern lights are natural
PHYSICS - MASTER. Study plan: Name. Qualification awarded Master of Science in Physics.
Study plan: PHYSICS - MASTER Name Bokmål: Nynorsk: English: Physics - master Physics - master Physics - master Qualification awarded Master of Science in Physics. Workload 120 ECTS credits. With a workload
- 1 - Jennifer McClure. To: env.essay@physics.org. From: Jennifer McClure (j.m.mcclure@student.liverpool.ac.uk)
To: env.essay@physics.org Jennifer McClure From: Jennifer McClure (j.m.mcclure@student.liverpool.ac.uk) 1 st year Physics (F300), Department of Physics, University of Liverpool. - 1 - The Northern Lights;
Space Weather Research and Forecasting in CRL, Japan
Space Weather Research and Forecasting in CRL, Japan Maki Akioka Hiraiso Solar Observatory Communications Research Laboratory Contact akioka@crl.go.jp 1 Contents of Presentation 1.Space Weather Observation
Space Weather Effects with the Flip of a Switch. 1 Dr. Bob McCoy Director, Geophysical Institute University of Alaska Fairbanks rpmccoy@alaska.
Space Weather Effects with the Flip of a Switch 1 Dr. Bob McCoy Director, Geophysical Institute University of Alaska Fairbanks rpmccoy@alaska.edu Poker 2015 Campaign MIST & MTeX 2 Ionospheric Effects Altimetry
The Next Generation European Incoherent Scatter Radar System: EISCAT 3D and related facilities
The Next Generation European Incoherent Scatter Radar System: EISCAT 3D and related facilities Michael Rietveld EISCAT Scientific Association Tromsø Antenna 1 Control Norway Transmitter Antenna 2 Antenna
Electromagnetic Radiation (EMR) and Remote Sensing
Electromagnetic Radiation (EMR) and Remote Sensing 1 Atmosphere Anything missing in between? Electromagnetic Radiation (EMR) is radiated by atomic particles at the source (the Sun), propagates through
LySEF - Longyearbyen Science and Education Forum. Svalbard Science Centre, OPS-room. Elise Strømseng, LySEF secretariat,unis
LySEF LySEF - Longyearbyen Science and Education Forum MINUTES Date: 15.05.2009 Time: 09:00 12:00 Place Minutes by: Svalbard Science Centre, OPS-room Elise Strømseng, LySEF secretariat,unis Present: UNIS:
Solar Storms and Northern lights - how to predict Space Weather and the Aurora
Solar Storms and Northern lights - how to predict Space Weather and the Aurora Pål Brekke Norwegian Space Centre/UNIS Pål Brekke torsdag 12. mars 15 Fleet of satellites watching the Sun Stereo SDO SOHO
CSSAR Space Science Cooperation
CSSAR Space Science Cooperation WANG Shuzhi Center for Space Science and Applied Research Chinese Academy of Science(CSSAR) Table of Contents Brief History of CSSAR International Cooperation CAS Strategic
'' EGGBEATER '' ANTENNA VHF/UHF ~ PART 2
'' EGGBEATER '' ANTENNA VHF/UHF ~ PART 2 ON6WG / F5VIF Summary Note : In Part 1, Fig 1 shows a maximum gain of 6.45 dbi. Several design attempts were made using slightly different configurations ( i.e.
Simultaneous Heliospheric Imager and Interplanetary Scintillation observations of CMEs and CIRs
Simultaneous Heliospheric Imager and Interplanetary Scintillation observations of CMEs and CIRs Gareth D. Dorrian (gdd05@aber.ac.uk) 1, Andy R. Breen 1, Jackie A. Davies 2, Alexis P. Rouillard 3, Mario
SPACE WEATHER SUPPORT FOR COMMUNICATIONS. Overview
SPACE WEATHER SUPPORT FOR COMMUNICATIONS Overview Ionospheric variability (space weather) significantly impacts ground and space-based communications. In essence, the electrically charged particles of
Quest- 1 Satellite Functional Description
Quest- 1 Satellite Functional Description Overview The Quest- 1 Satellite is based on the CubeSat Standard that measures 10 cm x 10 cm x 10 cm and weighs less than 1.33 kilograms. The Quest- 1 Satellite
Space Environment and Satellite Systems: Removing Clutter from Ground-to-Satellite Signals. Sigrid Close
Space Environment and Satellite Systems: Removing Clutter from Ground-to-Satellite Signals Sigrid Close Background Overview RF propagation through ionosphere can be problematic Goals Traditionally too
EMİNE CEREN KALAFATOĞLU EYİGÜLER
EMİNE CEREN KALAFATOĞLU EYİGÜLER SPACE ENVIRONMENT UZB411E 2015-2016 FALL ROOM: 322 / THIRD FLOOR UPPER ATMOSPHERE AND SPACE WEATHER LAB OFFICE HOURS: EVERY TUESDAY AND WEDNESDAY BETWEEN 15-17 FOR OTHER
AURORAL OVAL IN THE NIGHTSIDE IONOSPHERE
DYNAMICS OF THE POLAR CAP BOUNDARY AND THE AURORAL OVAL IN THE NIGHTSIDE IONOSPHERE TIMO PITKÄNEN Department of Physics University of Oulu Finland Academic dissertation to be presented, with the permission
WELCOME to Aurorae In the Solar System. J.E. Klemaszewski
WELCOME to Aurorae In the Solar System Aurorae in the Solar System Sponsoring Projects Galileo Europa Mission Jupiter System Data Analysis Program ACRIMSAT Supporting Projects Ulysses Project Outer Planets
EISCAT 3D Preparatory Phase - Site survey 2011-2013
EISCAT 3D Preparatory Phase - Site survey 2011-2013 EISCAT_3D System Overview The EISCAT_3D facilities will comprise one transmit/receive core site and four distant, primarily receive sites equipped with
Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:
Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007 Name: Directions: Listed below are twenty (20) multiple-choice questions based on the material covered by the lectures this past week. Choose
1. Introduction. FER-Zagreb, Satellite communication systems 2011/12
1. Introduction Topics History Characteristics of satellite communications Frequencies Application 1 History Arthur C. Clark suggested in 1945. Earth coverage with 3 geostationary satellites. On 4th of
Dear Science Educator:
Dear Science Educator: Because of its relationship to the Sun, Solar Physics, and Earth Science, the Experience the Aurora planetarium show provides rich curriculum connections. This Teacher s Resource
Space Weather: An Introduction C. L. Waters. Centre for Space Physics University of Newcastle, Australia
Space Weather: An Introduction C. L. Waters Centre for Space Physics University of Newcastle, Australia 1 Outline Space weather: Conditions on the Sun and in the solar wind, magnetosphere, ionosphere and
SPACE WEATHER INTERPRETING THE WIND. Petra Vanlommel & Luciano Rodriguez
SPACE WEATHER INTERPRETING THE WIND Petra Vanlommel & Luciano Rodriguez THE SUN LOSES ENERGY Radiation Mass Particles THE SUN LOSES ENERGY PHYSICAL REPHRASING Total Solar Irradiance Solar Wind Fast Particles
JPL ANOMALY ISSUES. Henry B. Garrett Jet Propulsion Laboratory California Institute of Technology Pasadena, CA, 91109
JPL ANOMALY ISSUES Henry B. Garrett Pasadena, CA, 91109 Space Weather Anomaly Concerns for JPL Robotic Mission AGENDA Overview of Space Weather Anomalies on JPL Missions Space Weather Products used by
photo essay northern lights
photo essay northern lights p h o t o e s s a y Northern Lights The stunning photography of Bjørn Jørgensen + Where to see the lights in the UK over the coming months photo essay northern lights Photographing
Activity 10 - Universal Time
Activity 10 - Universal Time Teacher s Guide Scientists use the Universal Time reference to talk about data that is taken around the globe. Universal Time is the time kept in the time zone centered on
Sporadic E A Mystery Solved?
Sporadic E A Mystery Solved? In Part 1 of this QST exclusive, one of the world s leading ionospheric scientists explains the physics of sporadic E and discusses unresolved problems in understanding its
STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves
Name: Teacher: Pd. Date: STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves TEK 8.8C: Explore how different wavelengths of the electromagnetic spectrum such as light and radio waves are used to
ESA Space Weather Initiatives
ESA Space Weather Initiatives The Multi-functional Nature of the Aerospace Domain: a European Approach 22-24 October 2014 Firenze, Italy Juha-Pekka Luntama Space Weather Manager ESA SSA Programme Office
Solar Activity and Earth's Climate
Rasmus E. Benestad Solar Activity and Earth's Climate Second Edition Published in association with Springer Praxis ids Publishing Publisl PRAXI Chichester, UK Contents Preface to the second edition Preface
Digital Audio and Video Broadcasting Antenna Components and Systems
Digital Audio and Video Broadcasting Antenna Components and Systems KATHREIN, founded in 1919 in Rosenheim, Germany, is an international enterprise active in antenna and communications technology. For
RECOMMENDATION ITU-R F.1113. (Question ITU-R 157/9) b) that systems using this mode of propagation are already in service for burst data transmission,
Rec. ITU-R F.1113 1 RECOMMENDATION ITU-R F.1113 RADIO SYSTEMS EMPLOYING METEOR-BURST PROPAGATION (Question ITU-R 157/9) (1994) Rec. ITU-R F.1113 The ITU Radiocommunication Assembly, considering a) that
Space Weather Research in KASI. Yeon-Han Kim & KASI people Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI)
Space Weather Research in KASI Yeon-Han Kim & KASI people Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI) I. SSD in KASI Sun-Earth Connection (CME geoeffectiveness) Solar
INTRODUCTION TO SOLAR WEATHER & HF PROPAGATION. Lewis Thompson W5IFQ September 27, 2011
INTRODUCTION TO SOLAR WEATHER & HF PROPAGATION Lewis Thompson W5IFQ September 27, 2011 PRESENTATION Ionospheric propagation NVIS Long-Range Frequency Selection (Critical Frequency & MUF) Propagation modeling
Intended Procurements in the Space Weather (SWE) Segment. SSA Industry Day 11 June 2013, ESOC
Intended Procurements in the Space Weather (SWE) Segment SSA Industry Day 11 June 2013, ESOC Juha-Pekka Luntama SSA Space Weather Segment Manager ESA Unclassified Releasable to the Public SSA/SWE Precursor
This report describes the tool and how to use it, and summarizes three real-life examples.
FINAL REPORT February 2015 A decision tool for remote camera systems Jim Thomasson INTRODUCTION Designing a camera system for remote locations can be a challenging endeavour. As camera and communication
Earth s Magnetic Field
Earth s Magnetic Field We ve been talking about magnets for the past two lessons and finding out all about what they are and how they work. Well, I ve got a little surprise for you. Right under your feet,
The main purpose of the study was to answer the three following questions:
MEETING DATE: March 19, 2003 SUBJECT: Cellular Phones In The Subway RECOMMENDATION It is recommended that: 1. the Commission authorize staff to issue a Request for Expression of Interest (REOI) to determine
Seeing the Northern Lights Top 5 Tips to Your Success. 01793 752 532
Seeing the Northern Lights Top 5 Tips to Your Success Tip 1: To see the northern lights or aurora borealis it s best to be in the arctic. In the Northern Hemisphere, the auroral zone runs along the northern
700 and 800 MHz Band Slot Antennas
Low Group Delay, Wide Bandwidth UHF Slot Antennas Omni-directional and Directional Patterns Available Low RFR Models Available Top or Side Mount Models Horizontal, Elliptical, or Circular Polarization
OPTICAL PARTICLE SIZER MASS CALIBRATION METHOD
OPTICAL PARTICLE SIZER MASS CALIBRATION METHOD APPLICATION NOTE OPS-001 The Optical Particle Sizer (OPS) is calibrated for size with Polystyrene Latex (PSL) spheres (per ISO 12501-1/4) at TSI. This method
Cluster-II: Scientific Objectives and Data Dissemination
r bulletin 102 may 2000 Cluster-II: Scientific Objectives and Data Dissemination C. Ph. Escoubet Space Science Department, ESA Directorate of Scientific Programmes, ESTEC, Noordwijk, The Netherlands Scientific
A Plan of Action Under LTSP III
A Plan of Action Under LTSP III William Liu and Robert Rankin Department of Physics, University of Alberta David Boteler Geomagnetic Laboratory, Geological Survey of Canada Submitted to the Canadian Space
SPEED, VELOCITY, AND ACCELERATION
reflect Look at the picture of people running across a field. What words come to mind? Maybe you think about the word speed to describe how fast the people are running. You might think of the word acceleration
Wireless Optical Mouse
Wireless Optical Mouse User s Manual Model PD950P FCC STATEMENT PD950P This device complies with part 15 of FCC Rules. Operation is subject to the following two conditions: (1) this device may not cause
GENSO. A Global Educational Network for Satellite Operations
GENSO A Global Educational Network for Satellite Operations A Typical Student Space Segment Satellite in Low-Earth Orbit, often Sun Synchronous, Low-power transmitters, Standard communications protocols
Earth, Sun and Moon is a set of interactives designed to support the teaching of the QCA primary science scheme of work 5e - 'Earth, Sun and Moon'.
is a set of interactives designed to support the teaching of the QCA primary science scheme of work 5e - ''. Learning Connections Primary Science Interactives are teaching tools which have been created
2. Orbits. FER-Zagreb, Satellite communication systems 2011/12
2. Orbits Topics Orbit types Kepler and Newton laws Coverage area Influence of Earth 1 Orbit types According to inclination angle Equatorial Polar Inclinational orbit According to shape Circular orbit
CHAPTER 6 INSTRUMENTATION AND MEASUREMENTS 6.1 MEASUREMENTS
CHAPTER 6 INSTRUMENTATION AND MEASUREMENTS 6.1 MEASUREMENTS Atmospheric electricity is a field that is very easy to get into because it does not require a large capital investment for measuring equipment.
PIXIE/Polar A Success Story! PIXIE (Polar Ionospheric X-ray Imaging Experiment)
PIXIE/Polar A Success Story! PIXIE (Polar Ionospheric X-ray Imaging Experiment) Norsk Romsenter 8 mai 2008 Polars siste runddans Professor Johan Stadsnes ved Universitet i Bergen er vemodig, men mest stolt
12.5: Generating Current Electricity pg. 518
12.5: Generating Current Electricity pg. 518 Key Concepts: 1. Electrical energy is produced by energy transformations. 2. Electrical energy is produced from renewable and non-renewable resources. 4. Electrical
Astrophysical Techniques. C R Kitchin
Astrophysical Techniques C R Kitchin University of Hertfordshire Observatory Third Edition SUB Gottingen 7 210 119 268 99 A 8843 Institute of Physics Publishing Bristol and Philadelphia Contents Preface
The Earth's Atmosphere. Layers of the Earth's Atmosphere
The Earth's Atmosphere The atmosphere surrounds Earth and protects us by blocking out dangerous rays from the sun. The atmosphere is a mixture of gases that becomes thinner until it gradually reaches space.
MIMO Antenna Systems in WinProp
MIMO Antenna Systems in WinProp AWE Communications GmbH Otto-Lilienthal-Str. 36 D-71034 Böblingen mail@awe-communications.com Issue Date Changes V1.0 Nov. 2010 First version of document V2.0 Feb. 2011
Precision on earth. Reliability in space. RUAG Space.
Precision on earth. Reliability in space. RUAG Space. Image: ESA Precision on earth. Reliability in space. RUAG Space is the leading supplier of products for the space industry in Europe. Experience, outstanding
Study the following diagrams of the States of Matter. Label the names of the Changes of State between the different states.
Describe the strength of attractive forces between particles. Describe the amount of space between particles. Can the particles in this state be compressed? Do the particles in this state have a definite
Svalbard Science Forum. Work group Research education 30th of January 2014
Svalbard Science Forum Work group Research education 30th of January 2014 Work group, research and education Data from RiS Research in the protected areas today Research in the protected areas in the future
Space Weather Measurements. Mary Kicza Assistant Administrator NOAA Satellite & Info. Service (NESDIS) Space Weather Enterprise Forum
Continuity of Critical Space Weather Measurements Mary Kicza Assistant Administrator NOAA Satellite & Info. Service (NESDIS) Space Weather Enterprise Forum May 19, 2009 NOAA Space Weather Requirements
Status report of CDF database and TDAS plug-in for SD data developed by ERG-SC
Status report of CDF database and TDAS plug-in for SD data developed by ERG-SC T. Hori, N. Nishitani, Y. Miyashita, T. Segawa, Y. Miyoshi, K. Seki (STEL) K. Hosokawa (UEC) Y. Tanaka, A. S. Yukimatsu, N.
Space Weather: Forecasting & Impacts on Critical Infrastructure
Space Weather: Forecasting & Impacts on Critical Infrastructure Dr. Genene Fisher Senior Advisor for Space Weather National Weather Service AMS Washington Forum 12 April 2012 Outline Solar Activity Update
Propagation: The science and study of radio wave reflection, refraction, diffraction, absorption, polarization, and scattering.
Propagation: The science and study of radio wave reflection, refraction, diffraction, absorption, polarization, and scattering. Hamvention Reuben Meeks, W8GUC Electronics, R.F. Engineer, Frank J. Beafore
Studies on the ionospheric region during low solar activity in Brazil
Studies on the ionospheric region during low solar activity in Brazil Claudia M. N. Candido National Institute for Space Research - INPE Brazil 1 Plasma Bubbles-Spread-F OI 630.0-nm Peak at 250 km - F-layer
The NOAA National Climatic Data Center Data availability, WDC-A, and GCOS data sets
NEESPI Regional Science Team Meeting, Helsinki, Finland 2-6 June 2008 The NOAA National Climatic Data Center Data availability, WDC-A, and GCOS data sets Dr. Karsten A. Shein Data Quality Administrator
Photosynthesis. Grade-Level Expectations The exercises in these instructional tasks address content related to the following grade-level expectations:
GRADE 5 SCIENCE INSTRUCTIONAL TASKS Photosynthesis Grade-Level Expectations The exercises in these instructional tasks address content related to the following grade-level expectations: SI-M-A5 Use evidence
4-1-3 Space Weather Forecast Using Real-time Data
4-1-3 Space Weather Forecast Using Real-time Data In recent years, advances in telecommunications technology have made it possible to collect space-based and ground-based observation data needed for space
How To Understand The Aurora Lights
The Northern Lights From myths to modern science Pål Brekke Norwegian Space Centre 1 EISCAT (Njål Gulbrandsen) "No pencil can draw it, no colours can paint it, and no words can describe it in all its magnificence."
Digital Active Indoor Antenna SRT ANT 10 ECO
Digital Active Indoor Antenna SRT ANT 10 ECO Picture similar User Manual Table of contents 1.0 INTRODUCTION 1 2.0 PACKAGE CONTENT 1 3.0 SAFETY NOTES 2 4.0 CONNECTING THE ANTENNA 2 1.0 INTRODUCTION Thank
Chang e-3 s Progress and Achievement 2/2014
Chang e-3 s Progress and Achievement 2/2014 Main content 1. Chinese Lunar Exploration Program 2. Chang e-3 s Progress 3. Chang e-3 s Achievement Chinese Lunar Exploration Program Phase I Orbital missions
Magnets and Magnetism
1 What You Will Learn Describe the properties of magnets. Explain why some materials are magnetic and some are not. Describe four kinds of magnets. Give two examples of the effect of Earth s magnetic field.
As you learned in the previous activity, energy is either potential energy or kinetic energy. Each can take many forms.
Topic 6: Forms of Potential Energy As you learned in the previous activity, energy is either potential energy or kinetic energy. Each can take many forms. Forms of potential energy include Stored Mechanical
BSA Technical Information
BSA Technical Information Electrical Isolation of Co-Located Horizontally and Vertically Stacked Antennas Introduction: Service providers are facing rapidly increasing pressure from zoning boards to co-locate
Germanium Diode AM Radio
Germanium Diode AM Radio LAB 3 3.1 Introduction In this laboratory exercise you will build a germanium diode based AM (Medium Wave) radio. Earliest radios used simple diode detector circuits. The diodes
Solar System Overview
Solar System Overview Planets: Four inner planets, Terrestrial planets Four outer planets, Jovian planets Asteroids: Minor planets (planetesimals) Meteroids: Chucks of rocks (smaller than asteroids) (Mercury,
Solar Wind Control of Density and Temperature in the Near-Earth Plasma Sheet: WIND-GEOTAIL Collaboration. Abstract
1 Geophys. Res. Letters, 24, 935-938, 1997. Solar Wind Control of Density and Temperature in the Near-Earth Plasma Sheet: WIND-GEOTAIL Collaboration T. Terasawa 1, M. Fujimoto 2, T. Mukai 3, I. Shinohara
Friday 20 January 2012 Morning
THIS IS A NEW SPECIFICATION H Friday 20 January 2012 Morning GCSE TWENTY FIRST CENTURY SCIENCE PHYSICS A A181/02 Modules P1 P2 P3 (Higher Tier) *A131500112* Candidates answer on the Question Paper. A calculator
Annual Report of RWC Korea 2013-2014
Annual Report of RWC Korea 2013-2014 Korean Space Weather Center of National Radio Research Agency The Korean Space Weather Center (KSWC) of the National Radio Research Agency (RRA) is a government agency
THE EFFECT OF COLOUR FILTERS ON SOLAR PANELS. Katie Fitzgerald Expo Project Grade 7
THE EFFECT OF COLOUR FILTERS ON SOLAR PANELS Katie Fitzgerald Expo Project Grade 7 OBSERVATION By using a solar light instead of electricity, one can assist in lightening the load on our environment. By
8.2 Cells and Energy. What is photosynthesis? Photosynthesis takes place in the chloroplasts. CHAPTER 8. Solar cells and chloroplasts
CHAPTER 8 CELL PROCESSES 8.2 Cells and Energy To stay alive, you need a constant supply of energy. You need energy to move, think, grow, and even sleep. Where does that energy come from? It all starts
HD-TV100 MP Digital TV and media player
HD-TV100 MP Digital TV and media player User s manual 1. Functions overview: FULL HD TV HD Digital TV with MPEG-4(H.264)&MPEG-2, HD&SD standard DVB-T. HDMI HD format output 1080I, also compatible with
Regional Emergency Communications. John Walters W8CX Alpena RACES
Regional Emergency Communications John Walters W8CX Alpena RACES Regional Communications Needs 400 mile radius No skip zone; no dead spots No interference with or from broadcasters Reliable day/night coverage
Magnetism. Magnetism. Magnetic Fields and Magnetic Domains. Magnetic Fields and Magnetic Domains. Creating and Destroying a Magnet
Magnetism Magnetism Opposite poles attract and likes repel Opposite poles attract and likes repel Like electric force, but magnetic poles always come in pairs (North, South) Like electric force, but magnetic
Time allowed: 1 hour 45 minutes
GCSE PHYSICS Foundation Tier Paper 1F F Specimen 2018 Time allowed: 1 hour 45 minutes Materials For this paper you must have: a ruler a calculator the Physics Equation Sheet (enclosed). Instructions Answer
How Do You Make a Weather Satellite?
NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION U.S. DEPARTMENT OF COMMERCE How Do You Make a Weather Satellite? This booklet was adapted from the original work by Ed Koenig I'm a weather forecaster. I
DAB Digital Radio Broadcasting. Dr. Campanella Michele
DAB Digital Radio Broadcasting Dr. Campanella Michele Intel Telecomponents Via degli Ulivi n. 3 Zona Ind. 74020 Montemesola (TA) Italy Phone +39 0995664328 Fax +39 0995932061 Email:info@telecomponents.com
Meeting the Grand Challenge of Protecting an Astronaut s Health: Electrostatic Active Space Radiation Shielding for Deep Space Missions
Meeting the Grand Challenge of Protecting an Astronaut s Health: Electrostatic Active Space Radiation Shielding for Deep Space Missions Ram Tripathi NASA Langley Research Center NIAC 2012 Spring Symposium,
Current Staff Course Unit/ Length. Basic Outline/ Structure. Unit Objectives/ Big Ideas. Properties of Waves A simple wave has a PH: Sound and Light
Current Staff Course Unit/ Length August August September September October Unit Objectives/ Big Ideas Basic Outline/ Structure PS4- Types of Waves Because light can travel through space, it cannot be
NORWEGIAN NATIONAL REPORT ARCTIC ACCESS TO SPACE
NORWEGIAN NATIONAL REPORT ARCTIC ACCESS TO SPACE Pål Brekke (1) (1) Norwegian Space Centre, Norway, paal.brekke@spacecentre.no ABSTRACT Norway has long traditions as a space nation, much due to our northern
The new giant radio telescope LOFAR and its Scandinavian outrigger LOIS
The new giant radio telescope LOFAR and its Scandinavian outrigger A transnational, cross-disciplinary initiative to build the world s largest and first fully digital radio observatory for astrophysics,
Solar Wind: Theory. Parker s solar wind theory
Solar Wind: Theory The supersonic outflow of electrically charged particles, mainly electrons and protons from the solar CORONA, is called the SOLAR WIND. The solar wind was described theoretically by
High Resolution Planetary Imaging
High Resolution Planetary Imaging Fighting the Atmosphere Getting out of the Atmosphere Adaptive Optics Lucky Imaging Lucky Imaging is the process of capturing planets using a CCD video camera. A software
Small Satellite Attitude Determination With RF Carrier Phase Measurement
Politecnico di Torino Electronics Department IAC-09.C1.6.9 Small Satellite Attitude Determination With RF Carrier Phase Measurement Danilo Roascio, Leonardo M. Reyneri, Claudio Sansoé, Maurizio Bruno International
Cloud tracking with optical flow for short-term solar forecasting
Cloud tracking with optical flow for short-term solar forecasting Philip Wood-Bradley, José Zapata, John Pye Solar Thermal Group, Australian National University, Canberra, Australia Corresponding author:
Climate Discovery Teacher s Guide
Climate Discovery eacher s Guide Sunspots and Climate Unit:Little Ice Age Lesson: 7 Materials & Preparation ime: Preparation: 10 min eaching: 60 min Materials for the eacher: Overhead projector ransparencies
Arktis en kilde til fornybar energi?
Arktis en kilde til fornybar energi? Ånund Killingtveit 1 1 Norwegian University of Science and Technology Centre for environmental design of renewable energy - CEDREN SRREN was prepared for WG III In
INSTRUCTION MANUAL PLEASE READ ALL THE INSTRUCTIONS COMPLETELY BEFORE USE AND SAVE THIS MANUAL FOR FUTURE REFERENCE
INSTRUCTION MANUAL PLEASE READ ALL THE INSTRUCTIONS COMPLETELY BEFORE USE AND SAVE THIS MANUAL FOR FUTURE REFERENCE m Before Use Please read IMPORTANT SAFETY INSTRUCTIONS on page 10 before use. It is important
A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study
Ann. Geophysicae 17, 674±681 (1999) Ó EGS ± Springer-Verlag 1999 A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study O. Saka 1; 2, O. Watanabe 2, K. Okada
Automatic and Objective Measurement of Residual Stress and Cord in Glass
Automatic and Objective Measurement of Residual Stress and Cord in Glass GlassTrend - ICG TC15/21 Seminar SENSORS AND PROCESS CONTROL 13-14 October 2015, Eindhoven Henning Katte, ilis gmbh copyright ilis