These two months in NCT project Jeng-Lun Chiu (Alan) Department of Physics, NTHU / SSL, UCB 2007/03/20 NTHU HEAG meeting.

Slides:



Advertisements
Similar presentations
Digital Image Processing
Advertisements

Modelling complexity in the upper atmosphere using GPS data Chris Budd, Cathryn Mitchell, Paul Spencer Bath Institute for Complex Systems, University of.
Navigation Fundamentals
Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.
Tom Wilson, Department of Geology and Geography Environmental and Exploration Geophysics II tom.h.wilson Department of Geology.
European Repeat Station Workshop Bucharest May 2007 UK repeat station programme Tom Shanahan and Susan Macmillan.
Repeat station crustal biases and accuracy determined from regional field models M. Korte, E. Thébault* and M. Mandea, GeoForschungsZentrum Potsdam (*now.
Geomagnetism (I).
New software for the World Magnetic Model (WMM) Adam Woods (1, 2), Manoj Nair (1,2), Stefan Maus (1,2), Susan McLean (1) 1. NOAA’s National Geophysical.
Status report on Light Simulator Claudia Cecchi Francesca Marcucci Monica Pepe Software meeting Udine January
Solidified iron km ,00012,000 solid mantle Mg(Fe) silicates crust Rapidly convecting, electrically conducting, fluid iron The outer core:
1 ADN Geospatial & Temporal March Geospatial Purpose Describe geospatial coverage of resources where resources are: – Curriculum, activities,
Observations of Open and Closed Magnetic Field Lines at Mars: Implications for the Upper Atmosphere D.A. Brain, D.L. Mitchell, R. Lillis, R. Lin UC Berkeley.
Geographic Datums Y X Z The National Imagery and Mapping Agency (NIMA) and the Defense Mapping School Reviewed by:____________ Date:_________ Objective:
Where we are going today… GPS GPS GIS GIS Hey, there are exams next week. Oct. 4 th and 6 th. Powerpoints now online. Hey, there.
Solidified iron km ,00012,000 solid mantle Mg(Fe) silicates crust Rapidly convecting, electrically conducting, fluid iron The outer core:
GTECH 201 Session 08 GPS.
Des Éléments Importants des Systèmes de Référence et de la Géodésie au CERN Mark Jones EN\MEF-SU.
Conversion from Latitude/Longitude to Cartesian Coordinates
Geographic Information Systems in Water Science Unit 4: Module 1, Lecture 2 – Coordinate Systems and Common GIS data formats.
Introduction.
Geomagnetic field Inclination
Using GPS in Algebra I One activity that interests and engages students in mathematics.
Principles of the Global Positioning System Lecture 10 Prof. Thomas Herring Room A;
Geodesy, Map Projections and Coordinate Systems
Section 1: Finding Locations on EarthFinding Locations on Earth
Kick off meeting, swarm E2E study, nio #1 8-Sep-15 Development Approach Task 1: Industrial Module –to be used by industry for their system simulation –Output:
Geometric Correction It is vital for many applications using remotely sensed images to know the ground locations for points in the image. There are two.
Modern Navigation Thomas Herring MW 10:30-12:00 Room
EISCAT Radar Summer School 15th-26th August 2005 Kiruna
SU 4100 GEODETIC POSITIONING Instructor: Indra Wijayratne.
Geography 370 Locating Positions on the Earth
Faculty of Applied Engineering and Urban Planning Civil Engineering Department Geographic Information Systems Spatial Referencing Lecture 4 Week 6 1 st.
How Does GPS Work ?. Objectives To Describe: The 3 components of the Global Positioning System How position is obtaining from a radio timing signal Obtaining.
Outline  Construction of gravity and magnetic models  Principle of superposition (mentioned on week 1 )  Anomalies  Reference models  Geoid  Figure.
Secular variation in Germany from repeat station data and a recent global field model Monika Korte and Vincent Lesur Helmholtz Centre Potsdam, German Research.
1 Geospatial Purpose Describe geospatial coverage of resources where resources are: – Web-based activities, modules etc. – Datasets – Model output – Visuals.
Geomagnetism: Lecture 1 This lecture is based largely on:
Environmental and Exploration Geophysics I tom.h.wilson Department of Geology and Geography West Virginia University Morgantown, WV.
© NERC All rights reserved UK Repeat Station Report T J G Shanahan and S Macmillan June 2009 MagNetE Workshop Helsinki, Finland.
© NERC All rights reserved Chris Turbitt Observatories Manager Geomagnetism Team British Geological Survey BGS Observatory Network.
Tom Wilson, Department of Geology and Geography Environmental and Exploration Geophysics II tom.h.wilson Department of Geology.
Introducing POMME Potsdam Magnetic Model of the Earth Star camera calibration Ring current field Static and annually varying external fields Internal field.
GP33A-06 / Fall AGU Meeting, San Francisco, December 2004 Magnetic signals generated by the ocean circulation and their variability. Manoj,
Models of the Earth Chapter 3. Ch03\80017.html.
Geomagnetism: Lecture 1 This lecture is based largely on:
Geology 5660/6660 Applied Geophysics 28 Mar 2014 © A.R. Lowry 2014 For Mon 31 Mar: Burger (§7.4–7.6) Last Time: Earth’s Main Magnetic Field Earth’s.
Geography 70  Basic Geodesy  Map Projections  Coordinate Systems  Scale Locating Positions on the Earth.
1) Magnetic total field (T) obtained from airborne survey (see R.J.Blakely, 1995) (ΔT) Total field anomaly (IGRF removal), which satisfy potential theory,
Models of the Earth Section 1 Preview Key Ideas Latitude Longitude Comparing Latitude and Longitude Great Circles Finding Direction Section 1: Finding.
ST236 Site Calibrations with Trimble GNSS
Study on the Impact of Combined Magnetic and Electric Field Analysis and of Ocean Circulation Effects on Swarm Mission Performance by S. Vennerstrom, E.
Study of an Improved Comprehensive Magnetic Field Inversion Analysis for Swarm MTR, E2Eplus Study Work performed by Nils Olsen, Terence J. Sabaka, Luis.
Future China Geomagnetism Satellite Mission (CGS) Aimin Du Institute of Geology and Geophysics, CAS 2012/11/18 Taibei.
Earth’s Dynamic Magnetic Field: The State of the Art Comprehensive Model Terence J. Sabaka Geodynamics Branch NASA/GSFC with special thanks to Nils Olsen.
What is a geomagnetic storm? A very efficient exchange of energy from the solar wind into the space environment surrounding Earth; These storms result.
The Earth’s Magnetic Field
Geomagnetism Part II: The Earth’s Magnetic Field
1 NGA Mission - Data – Collaboration 2009 Workshop on Monitoring North American Geoid Change 21 Oct 2009 NGA Mission - Data – Collaboration 2009 Workshop.
Tom Wilson, Department of Geology and Geography Environmental and Exploration Geophysics I tom.h.wilson Department of Geology and.
Geology 5660/6660 Applied Geophysics 1 Apr 2016 © A.R. Lowry 2016 For Mon 4 Apr: Burger (§ ) Last Time: Magnetics (Measurement, Anomalies)
The Global Positioning System Rebecca C. Smyth April 17 - May 2, 2001.
Geodesy, Map Projections and Coordinate Systems Geodesy - the shape of the earth and definition of earth datums Map Projection - the transformation of.
Unit: 5 Mapping Earth Why Mapping?. Mapping Earth Whether you think about it or not. Your life (especially this day in age) is effected directly by having.
Geology 5660/6660 Applied Geophysics 30 Mar 2016
Chapter 3 Objectives Distinguish between latitude and longitude.
Lecture 4 Geographic Coordinate System
Tidal Corrections to Direction Observations
Outline Construction of gravity and magnetic models Reference models
Session 5: Higher level products (Internal)
Presentation transcript:

These two months in NCT project Jeng-Lun Chiu (Alan) Department of Physics, NTHU / SSL, UCB 2007/03/20 NTHU HEAG meeting

Outline Magnetic declination survey Magnetic declination survey Ground Support Equipment (GSE) Ground Support Equipment (GSE) PIXON algorithm PIXON algorithm Future work Future work

Magnetic declination survey Magnetic declination angle = Magnetic declination angle = the horizontal angle between true north and the field vector (measured positive eastwards) Pointing & Aspect – magnetometer Pointing & Aspect – magnetometer Position feedback Position feedback Field vector (magnetic north pole) + magnetic declination angle [model]  true north pole (position feedback for motor) Field vector (magnetic north pole) + magnetic declination angle [model]  true north pole (position feedback for motor)

Alice Springs 23˚ 37’12” S 133˚ 55’12” E Fort Sumner ˚ N, ˚ W

Quadratic approach -- Method Adopted in the previous flight Adopted in the previous flight Altitude & Latitude: linear fit Altitude & Latitude: linear fit Longitude: Quadratic fit Longitude: Quadratic fit D = a + bL + cL 2 D = a + bL + cL 2  [D] = k[L]  k = [D][L] -1  [D] = k[L]  k = [D][L] -1 2 elevations x 2 latitudes x 3 longitudes  12 points 2 elevations x 2 latitudes x 3 longitudes  12 points Interpolation Interpolation

Quadratic approach -- Result Previous Fort Sumner, NM, USA Previous Fort Sumner, NM, USA ( ˚ N, ˚ W) ( ˚ N, ˚ W) May 1, 2004 (assumed in calculation) May 1, 2004 (assumed in calculation) 2x2x3 points within 0~50 km & 32~36˚ N & 96~112˚ W 2x2x3 points within 0~50 km & 32~36˚ N & 96~112˚ W  Error in Dec.: ΔD = +0.02˚ ~ -0.01˚ (OK!!) Next Alice Springs, Aus. Next Alice Springs, Aus. (23˚ 37 ’ 12 ” S, 133˚ 55 ’ 12 ” E) (23˚ 37 ’ 12 ” S, 133˚ 55 ’ 12 ” E) Dec. 1, 2008 Dec. 1, x2x3 points within 0~50 km & 21~25˚ S & 113~153˚ E (with 5,10,20˚ steps in longitude) 2x2x3 points within 0~50 km & 21~25˚ S & 113~153˚ E (with 5,10,20˚ steps in longitude)  Error in Dec.: ΔD ~ 20”, 1’, 7’ Note: accuracy for D in model is claimed to be within 30 ”

Alice Springs 23˚ 37’12” S 133˚ 55’12” E Fort Sumner ˚ N, ˚ W

Earth’s magnetic field The main field generated in Earth ’ s conducting, fluid outer core (Bm) The main field generated in Earth ’ s conducting, fluid outer core (Bm) The crustal field from Earth ’ s crust/upper mantle (Bc) The crustal field from Earth ’ s crust/upper mantle (Bc) The combined disturbance field from electrical currents flowing in the upper atmosphere and magnetosphere, which also induce electrical currents in the sea and the ground (Bd) The combined disturbance field from electrical currents flowing in the upper atmosphere and magnetosphere, which also induce electrical currents in the sea and the ground (Bd)

Earth's main magnetic field dominates, accounting for over 95% of the field strength at the Earth ’ s surface. Earth's main magnetic field dominates, accounting for over 95% of the field strength at the Earth ’ s surface. The WMM represents only the main geomagnetic field. The WMM represents only the main geomagnetic field. Secular variation is the slow change in time of the main magnetic field. Secular variation is the slow change in time of the main magnetic field. Observed magnetic field is a sum of contributions: Observed magnetic field is a sum of contributions: B(r, t) = Bm(r, t) + Bc(r) + Bd(r, t)

World Magnetic Model (WMM) Producer -- The U.S. National Geophysical Data Center (NGDC) and the British Geological Survey (BGS) produced the WMM with funding provided by National Geospatial-Intelligence Agency (NGA) in the USA and by the Defence Geographic Imagery and Intelligence Agency (DGIA) in the UK. Producer -- The U.S. National Geophysical Data Center (NGDC) and the British Geological Survey (BGS) produced the WMM with funding provided by National Geospatial-Intelligence Agency (NGA) in the USA and by the Defence Geographic Imagery and Intelligence Agency (DGIA) in the UK.NGDCBGSNGDCBGS Data -- (Danish Oersted and German CHAMP ) satellite (good global coverage & low noise level ) and (ground) observatory (hourly mean data) data provide an exceptional quality data set for modeling the behavior of the main magnetic field in space and time. Data -- (Danish Oersted and German CHAMP ) satellite (good global coverage & low noise level ) and (ground) observatory (hourly mean data) data provide an exceptional quality data set for modeling the behavior of the main magnetic field in space and time.OerstedCHAMPOerstedCHAMP Model -- The WMM consists of a degree and order 12 spherical-harmonic main (i.e., core-generated) field model. Model -- The WMM consists of a degree and order 12 spherical-harmonic main (i.e., core-generated) field model. ( comprised of 168 spherical-harmonic Gauss coefficients and degree and order 12 spherical-harmonic Secular-Variation (SV) (core-generated, slow temporal variation) field model (determined to degree and order 8) ) ( comprised of 168 spherical-harmonic Gauss coefficients and degree and order 12 spherical-harmonic Secular-Variation (SV) (core-generated, slow temporal variation) field model (determined to degree and order 8) )

Input parameters & valid entries: Input parameters & valid entries: Latitude to degrees Longitude to degrees Altitude Sea level to 1,000,000 meters (referenced to the WGS 84 ellipsoid) Date Base epoch of the current model to epoch + 5 yearsLatitude to degrees Longitude to degrees Altitude Sea level to 1,000,000 meters (referenced to the WGS 84 ellipsoid) Date Base epoch of the current model to epoch + 5 years Output -- seven magnetic components: Output -- seven magnetic components: F - Total Intensity of the geomagnetic field H - Horizontal Intensity of the geomagnetic field X - North Component of the geomagnetic field Y - East Component of the geomagnetic field Z - Vertical Component of the geomagnetic field I (DIP) - Geomagnetic Inclination D (DEC) - Geomagnetic Declination (Magnetic Variation)F - Total Intensity of the geomagnetic field H - Horizontal Intensity of the geomagnetic field X - North Component of the geomagnetic field Y - East Component of the geomagnetic field Z - Vertical Component of the geomagnetic field I (DIP) - Geomagnetic Inclination D (DEC) - Geomagnetic Declination (Magnetic Variation) At given (h, φ, λ, t) (h: geodetic altitude; φ and λ: geodetic latitude and longitude; t: time in decimal year) 1. the ellipsoidal geodetic coordinates (h, φ, λ)  spherical geocentric coordinates (r, φ´, λ) 1. the ellipsoidal geodetic coordinates (h, φ, λ)  spherical geocentric coordinates (r, φ´, λ) 2. Determine the Gauss coefficients of degree n and order m for the desired time 2. Determine the Gauss coefficients of degree n and order m for the desired time 3. Compute the field vector components X´, Y´ and Z´ in geocentric coordinates 3. Compute the field vector components X´, Y´ and Z´ in geocentric coordinates 4. the geocentric vector components X´, Y´ and Z´ are transformed back into the geodetic reference frame, 4. the geocentric vector components X´, Y´ and Z´ are transformed back into the geodetic reference frame, 5. the magnetic elements H, F, D, I, and the grid variation, GV, are computed from the vector components 5. the magnetic elements H, F, D, I, and the grid variation, GV, are computed from the vector components

Certain local, regional, and temporal magnetic declination anomalies can exceed 10˚ (not common but do exist). Certain local, regional, and temporal magnetic declination anomalies can exceed 10˚ (not common but do exist). Declination anomalies of the order of 3˚ or 4˚ are not uncommon but are of small spatial extent and are relatively isolated. Declination anomalies of the order of 3˚ or 4˚ are not uncommon but are of small spatial extent and are relatively isolated. From a global main field perspective, the declination error of WMM2005 is estimated to be less than 1.0˚ at the Earth ’ s surface over the entire 5-year life span of the model. From a global main field perspective, the declination error of WMM2005 is estimated to be less than 1.0˚ at the Earth ’ s surface over the entire 5-year life span of the model. (< 30 ” ) (< 30 ” )

Differential GPS Minimize dependence on magnetic effects Minimize dependence on magnetic effects Earth ’ s magnetic field variationsEarth ’ s magnetic field variations Gondola currentsGondola currents (~ Steve Mcbride 2005 NCT workshop) (~ Steve Mcbride 2005 NCT workshop)

Ground Support Equipment (GSE) Linux with X window for display Main Window Main Window Detector Rates Detector Rates Other Rates Other Rates (Shield rates, ) (Shield rates, Date rate history, Detector Livetimes) Card Cage Housekeeping Data Card Cage Housekeeping Data GCU Housekeeping Data GCU Housekeeping Data Command Window Command Window Pointing Display Pointing Display Spectrum Display Spectrum Display Pixel Display Pixel Display Imaging Display Imaging Display ~ S. McBride 2005 NCT workshop

GSE -- Telemetry format For NCT frame 1 frame = 80 words = 160 bytes = 1280 bits Starting with ‘ EB90h ’ in each frame from GCU to UHF Starting with ‘ EB90h ’ in each frame from GCU to UHF Starting with ‘ E0AEh ’ in each frame for events Starting with ‘ E0AEh ’ in each frame for events 1 board contains 8x2 units with 4 channels each (8x2x5) for 37x2 output 1 board contains 8x2 units with 4 channels each (8x2x5) for 37x2 output Transmission rate for telemetry = 64,000 bits/sec Transmission rate for telemetry = 64,000 bits/sec = 50 frames/sec = 50 frames/sec ~ S. McBride 2005 NCT workshop

GSE – my status Understanding the programs and data format Understanding the programs and data format Going to know about the either net, flight computer, and card cages to make a newer version GSE code for next flight Going to know about the either net, flight computer, and card cages to make a newer version GSE code for next flight

PIXON

Bayes’ Theorem: p(A,B) = p(A|B)p(B) = p(B|A)p(A) (PP93) ( p(X,Y): the joint probability distribution. ) (Puetter 1996) ( p(X|Y): the probability of X given that the value of Y is known. ) PIXON: (1). A picture element (2). A fundamental unit of information in the image. The smallest groupings of signal warranted by the quality of the data, and they are fundamental and indivisible units of picture information. An image’s pixon represent the minimum set of degrees of freedom necessary to describe the image. (PP93)

PIXON

PIXON – my status Drawing the back-projection histogram by ROOT Drawing the back-projection histogram by ROOT Trying to complete the back projection part in Andrea ’ s practice program for imaging Trying to complete the back projection part in Andrea ’ s practice program for imaging

Pointing & Aspect (III): Alan, (Boggs) Pointing & Aspect (III): Alan, (Boggs) pointing calculations (GSU & GSE) pointing calculations (GSU & GSE) pointing program pointing program magentometer/inclinometer aspect magentometer/inclinometer aspect dGPS aspect dGPS aspect solar aspect solar aspect elevation, azimuth drive testing elevation, azimuth drive testing pointing tests pointing tests flight aspect database flight aspect database Data Archiving (II): Andreas, Alan Data Archiving (II): Andreas, Alan cataloguing cataloguing data summaries data summaries storage storage GSE (III): Mark, Alan, (McBride) GSE (III): Mark, Alan, (McBride) flight GSE upgrades flight GSE upgrades card cage GSE card cage GSE commanding commanding LOS telemetry LOS telemetry

Reference Presentations in NCT NTHU in 2005/11. Presentations in NCT NTHU in 2005/11. R. C. Puetter & A. Yahil, in Astronomical Data Analysis Software and Systems VIII, D. M. Mehringer, R. L. Plante & D. A. Roberts, eds., ASP Conference Series, 172, pp , (1999). R. C. Puetter & A. Yahil, in Astronomical Data Analysis Software and Systems VIII, D. M. Mehringer, R. L. Plante & D. A. Roberts, eds., ASP Conference Series, 172, pp , (1999). (The Pixon PAGE in UCSD) (The Pixon PAGE in UCSD) (The PIXON (The PIXON

Thank You