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...Math 252 Fall 2002 Introduction to Matrix Exponentials
Generalities. A system of autonomous linear differential equations can be written as dY = AY dt where A is an n by n matrix and Y = Y (t) is a vector listing the n dependent variables. (In most ...
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...Electronic Journal of Dierential Equations, Vol. 1998(1998), No. 32, pp. 112. ISSN: 1072-6691. URL: http:/ejde.math.swt.edu or http:/ejde.math.unt.edu ftp 147.26.103.110 or 129.120.3.113 (login: ftp)
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642:550 Math Summer 2003 MTTh 6:15 8:45 PM Hill 525 Prof. Bumby Supplement 9: Numerical Methods in Linear Algebra 1. Introduction Chapter 7 of the textbook describes computer algorithms for solving equations and nding eigenvalues and eigenvectors. Some tools used in the description are based on topics that we have not yet introduced. This supplement describes alternative approaches allowing these topics to be covered earlier, while we continue to rely on the textbook for most of the details. 2. Two kinds of numbers In order to facilitate hand computation, most exercises done so far used matrices with integer entries and relied on methods that were able to give exact answers easily with this data. These same methods can be programmed to give exact answers to problems involving integer matrices. If a system supporting arbitrary precision is used, then exact answers can be obtained even if the numbers in the problem are very large. If the numbers appearing throughout the solution are also required to be integers, division must be avoided. Some special methods that rely on matrix multiplication for most calculations were introduced. Most applications involve numbers that are obtained as measurements. The appropriate tools for computing with such numbers are oating point representations on a computer (or calculator), Such representations are essentially approximations. Arithmetic with these quantities introduces round off and truncation errors. These errors are not mistakes. They are the result of limitations in the computer representation of real numbers. The subject of Numerical Analysis deals with nding methods of computation that control error while giving ef cient procedures for computing the desired quantities. Such methods are often iterative, generating a sequence that, if calculated exactly, converges to the desired quantity. The process is stopped when it can give no improvement with the available data. A oating point number consists of a sign, an exponent, and a mantissa packed into a xed number of bits according to an established standard. Here, the mantissa is the collection of digits relative to the scale set by the exponent. Calculators use base 10, and would write something like 5.237 1021 . The internal representation in a computer is more likely to be in binary so that the exponent represents a power of 2. What is important is that numbers can be scaled over a very large range, and show a xed number of signi cant digits that is the same independent of the size of the number or whether the number is positive or negative. (The number zero has a special representation distinct from all others.) This means that the appropriate measure of accuracy of a computation is relative error obtained by dividing the difference between correct and computed values by the correct value. The exact de nition is not important one only works with bounds on the error to determine how much of the mantissa can be trusted. Relative error behaves reasonable when numbers are multiplied or divided, but addition or subtraction can be troublesome. If numbers are of much different sizes, the smaller one will be written to the scale of the larger causing initial digits to be padded with 0 by shifting and the later digits get shifted off the end and lost. The situation is worse if the sum is smaller then the numbers being combined since there are not enough digits to give much accuracy 642:550, Summer 2003, Supplement 9, p. 2 after the number is written to its proper scale. This leads to an apparent breakdown of the rules of algebra in which equivalent expressions can give very different answers. 3. Ef cient computation The small problems used as exercises allow many ways of presenting the solution with no preferred method. We have given suggestions that aim to use a structured computation in which the location in which as quantity appears indicates its signi cance. The biggest danger in hand or semi-automatic computation (where you use a calculator for parts of the calculation, but record the steps by hand) is that an incorrect value (often only the sign of one number)will get written somewhere affecting all subsequent steps. The best protection against mistakes is to check the answer with the original data. It is also useful to have some theoretical properties of the answer that can be easily veri ed. A verbal description of the computation is not as useful. You need to be able to nd mistakes and correct them. Only correct answers are to be accepted. Some of this applies also to machine computation. The computation will be done by a program that records intermediate results according to a plan. Once the program is accepted as correct, special tricks may be used to save time or space in the computation. For example, in an LU factorization program, the answer will overlay the original matrix. This is not recommended for hand computation, but machines are not confused by it. The routine for printing the answer can separate the factors. The fast Fourier transform gives an example where ef cient use of space is an essential part of the computation. The matrices shown in formula (16) on page 191 of the text cannot appear as explicit arrays. The n 2 elements of such an array could not be written by a program that is supposed to run in only n log n steps. (the type of steps are that counted may lead to a higher power of log n, but certainly not n 2 ). The calculation will have a vector of n numbers as input and produce another such vector as output. The linear transformations represented by those matrices must be applied to vectors, but the program doing it will not use the matrix. Since the matrices only have two nonzero elements in each row, a sparse matrix data structure could be use that only records the nonzero entries and their location, but the special forms of the linear transformations appearing in this computation may lead to programs that don t appear to use matrices at all. The use of Householder matrices to compute the Q R factorization is mentioned in section 7.3 of the text (pages 374-5). It concludes with the observation that Q can be stored as a product of Householder matrices instead of being computed as a single orthogonal matrix. This is ef cient because a single Householder matrix can be represented by a unit vector in the direction being re ected. Thus, n such matrices need only n 2 locations no more than the whole product. Also, Q need not be seen to be used. A typical application involves multiplying a single vector by Q T . Using the factored form takes no longer that using a computed product. Either way, there are only n 2 products of numbers to be found. 4. Vector and matrix norms There are several ways to measure the size of a vector v Rn . The most familiar is the Euclidean length (v T v)1/2 . This is used in the text. In order to have a suitable foundation to work with this de nition, much of chapter 6 is a prerequisite. We will work through chapter 6, but it is convenient to look at some features of numerical methods earlier. We shall use a norm that is easier to work with: the maximum of the absolute values of the entries of v. This is mentioned brie y in exercise 7.2.10, where it is given the name maximum norm, and it plays a role in Gershgorin s Theorem mentioned before exercise 7.4.4. It 642:550, Summer 2003, Supplement 9, p. 3 was also implicit in our treatment of the Perron-Frobenius Theorem. There are many other vector norms: all that a function N (v) needs to earn that designation is that (1) N (v) 0 for all v with N (v) = 0 if and only if v = 0; (2) N ( v) = | | N (v); (3) N (v0 + v1 ) N (v0 ) + N (v1 ). Here, (1) is a positivity condition; (2) says that the norm is homogeneous of degree 1; and (3) is the triangle inequality. Both candidates for vector norms have these properties. If you have a vector norm N (v), there is an associated matrix norm on n by n matrices M de ned by N (M) = sup { N (Mv) : N (v) = 1 }. Because of positivity and homogeneity, this is equivalent to the least upper bound of N (Mv)/N (v) for all nonzero vectors v. Proposition. The matrix norm corresponding to the maximum norm is N (M) = max i j mi j . Proof. N (v) 1 says that all v j 1. In this case, m i j vj j j m i j vj j mi j vj , so N (M) is no larger than our proposed value. To see that it is at least this large, nd the row i where the sum attains its maximum and choose v j = 1 so that m i j = m i j v j . Then our proposed value is N (Mv)/N (v) for this v. 5. Perron-Frobenius revisited The rst bound that we obtained on the dominant eigenvalue of a positive matrix was actually the maximum norm of the matrix. More generally, we have. Proposition. If N (M) is any matrix norm induced from a vector norm N (v), then the absolute values of all eigenvalues of M are at most N (M). Proof. If Mv = v, then N (Mv) = N ( v) = | | N (v), but N (Mv) N (M)N (v). A change of basis can change the norm of a vector or a matrix. However, while N (S 1 M S) is not the same as N (M), it is always a matrix norm of M. Indeed, if the original norm is induced by the vector norm N (v), this is induced by N (Sv), which is easily seen to be a vector norm. 642:550, Summer 2003, Supplement 9, p. 4 For application to the Perron-Frobenius theorem, let S be a diagonal matrix the divides the j th coordinate of a vector by the j th coordinate of a given positive vector v0 . To say that Mv0 v0 , component by component, is to say that N (S 1 M S) . This shows that the dominant eigenvalue is bounded above by any such . This complements our earlier result that said that Mv0 v0 implies that is a lower bound on the dominant eigenvalue. 6. Power methods Positive matrices give good examples of the use of the power method for nding eigenvalues, since we know that the dominant eigenvalue belongs to a positive eigenvector. After some steps of the form vk+1 = Mvk from any positive starting vector v0 , the bounds on the ratios of corresponding components of vk+1 and vk give bounds on the dominant eigenvalue. Although the power method seems impressive when rst met, it soon begins to feel painfully slow. The shifted inverse power method does a good job of improving the rate of convergence while retaining the same ease of analysis. For positive matrices, this change can be done in a way that also involves nding the dominant eigenvalue of a positive matrix. 7. Exercises Let M= 4 7 5 32 15 22 1. Find the maximum norm of M. 2. Start from v0 = [1, 1, 1]T and use the power method vk+1 = Mvk to compute v1 , v2 and v3 . Use this to get upper and lower bounds on the dominant eigenvalue of M.
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Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Summer 2006 MTTh 6:008:30 PM Hill 705 Prof. Bumby Supplement 1, Prerequisites 1. Introduction A motivation for the subject of Linear Algebra is to organize the techniques for solving systems of linear equations. Since you should have h...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Summer 2008 MTTh 6:008:30 PM Hill 425 Prof. Bumby Supplement 7, The Perron-Frobenius Theorem. Introduction Square matrices whose entries are all nonnegative have special properties. This was mentioned briey in Section 5.3 with a sketch...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Fall 2006 MW 5:006:20 PM Hill 423 Prof. Bumby Supplement 2, The sign of a permutation 1. Introduction Proofs will not play a large role in this course. However, any calculation (and, even more so, any program that will perform a calcul...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Summer 2006 MTTh 6:008:30 PM Hill 705 Prof. Bumby Supplement 7, The Perron-Frobenius Theorem. Introduction Square matrices whose entries are all nonnegative have special properties. This was mentioned briey in Section 5.3 with a sketch...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Fall 2006 MW 5:006:20 PM Hill 423 Prof. Bumby Supplement 1, Linear Systems 1. Introduction A motivation for the subject of Linear Algebra is to organize the techniques for solving systems of linear equations. Although this course inclu...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Summer 2003 MTTh 6:158:45 PM Hill 525 Prof. Bumby Supplement 6:The Perron-Frobenius Theorem. 1. Introduction Square matrices whose entries are all nonnegative have special properties. This was mentioned briey in Section 5.3 with a sket...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 550A MATLAB Assignment #2 1 Revised 10/11/05 LAB 2: Orthogonal Projections, the Four Fundamental Subspaces, QR Factorization, and Inconsistent Linear Systems In this lab you will use Matlab to study the following topics: Geometric aspects of...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 550 Linear Algebra and Applications 1 Revised 8/04/02 Notes on MATLAB Assignments These notes are written to introduce the MATLAB part of this course. For additional MATLAB tutorial materials, go to the course web site math.rutgers.edu/courses...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Summer 2006 MTTh 6:008:30 PM Hill 705 Prof. Bumby Supplement 3, The Cauchy-Binet formula 1. Introduction The theorem that the determinant of a product of square matrices is the product of the determinants of the factors is so memorable...
Rutgers >> 642 >> 550 (Fall, 2008)
Math 642:550 Summer 2006 MTTh 6:008:30 PM Hill 705 Prof. Bumby Supplement 5, Matrix Exponentials Introduction It is now common for textbooks for a rst course in Differential Equations to describe the solution of the rst-order, linear, constant-coef...
Rutgers >> 642 >> 550 (Fall, 2008)
642:550, Summer 2004, Supplement 1 Prerequisites Summer 2004 1. Introduction A motivation for the subject of Linear Algebra is to organize the techniques for solving systems of linear equations. Since you should have had a course in which this was ...
Rutgers >> 650 >> 485 (Spring, 2008)
Dec 10th, 2003 CENTRALIZED DEPARTMENTAL PRINTING Malik S. Khan UNISYS Scholar 2003/04 Rutgers University Mechanical Engineering Outline Motivation for Project Present System Analysis Proposed System / Solution Steps to Solution - Selecting software...
Rutgers >> 670 >> 451 (Fall, 2008)
Lecture Notes Orbits and Navigation Prepared by Prof. J. Francis Spring 2005 Material from KVH Chapters 2 and 4. Figure numbers below from KVH. Motivation - Why study orbits? 1.Denes spatial and temporal resolution 2.Understand trade-offs between s...
Rutgers >> 712 >> 545 (Fall, 2008)
Lecture Notes Orbits and Navigation Prepared by Prof. J. Francis Spring 2005 Material from KVH Chapters 2 and 4. Figure numbers below from KVH. Motivation - Why study orbits? 1.Denes spatial and temporal resolution 2.Understand trade-offs between s...
Rutgers >> 712 >> 552 (Spring, 2008)
Lecture Notes Orbits and Navigation Prepared by Prof. J. Francis Spring 2005 Material from KVH Chapters 2 and 4. Figure numbers below from KVH. Motivation - Why study orbits? 1.Denes spatial and temporal resolution 2.Understand trade-offs between s...
Rutgers >> 670 >> 451 (Fall, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Orbits and Measurement Geometry (2) Eccentricity: Inclination: Perigee Height: Apogee Height: Right Ascension of Ascending Node...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Orbits and Measurement Geometry (2) Eccentricity: Inclination: Perigee Height: Apogee Height: Right Ascension of Ascending Node...
Rutgers >> 712 >> 552 (Spring, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Orbits and Measurement Geometry (2) Eccentricity: Inclination: Perigee Height: Apogee Height: Right Ascension of Ascending Node...
Rutgers >> 670 >> 451 (Fall, 2008)
Remote Sensing Homework Always answer in complete, coherent sentences and show all work! Orbits and Instruments: Due Monday, 2/2/05 Spring 2005 1. How high above the Earths surface would a satellites orbit need to be to achieve a geostationary orbi...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing Homework Always answer in complete, coherent sentences and show all work! Orbits and Instruments: Due Monday, 2/2/05 Spring 2005 1. How high above the Earths surface would a satellites orbit need to be to achieve a geostationary orbi...
Rutgers >> 712 >> 552 (Spring, 2008)
Remote Sensing Homework Always answer in complete, coherent sentences and show all work! Orbits and Instruments: Due Monday, 2/2/05 Spring 2005 1. How high above the Earths surface would a satellites orbit need to be to achieve a geostationary orbi...
Rutgers >> 670 >> 451 (Fall, 2008)
Solar Radiation Sources: K. N. Liou (2002) An Introduction to Atmospheric Radiation, Chapter 1, 2 S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology: An Introduction, Chapter 3 G. Carbone (2001) Exercises for Weather and Climate, 4th Editi...
Rutgers >> 712 >> 545 (Fall, 2008)
Solar Radiation Sources: K. N. Liou (2002) An Introduction to Atmospheric Radiation, Chapter 1, 2 S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology: An Introduction, Chapter 3 G. Carbone (2001) Exercises for Weather and Climate, 4th Editi...
Rutgers >> 712 >> 552 (Spring, 2008)
Solar Radiation Sources: K. N. Liou (2002) An Introduction to Atmospheric Radiation, Chapter 1, 2 S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology: An Introduction, Chapter 3 G. Carbone (2001) Exercises for Weather and Climate, 4th Editi...
Rutgers >> 712 >> 545 (Fall, 2008)
Lecture 7. 8 Feb 2006 Surface temperature (1) References: Martin, S., 2004, An Introduction to Ocean Remote Sensing, Cambridge University Press, 454 pp. Chapter 7. Robinson, I. S., 2004, Measuring the Oceans from Space: The principles and methods o...
Rutgers >> 670 >> 451 (Fall, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Orbits and Measurement Geometry (1) Johannes Kepler (1571 1630) German mathematician, astronomer and astrologer 1. Planets mo...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Orbits and Measurement Geometry (1) Johannes Kepler (1571 1630) German mathematician, astronomer and astrologer 1. Planets mo...
Rutgers >> 712 >> 552 (Spring, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Orbits and Measurement Geometry (1) Johannes Kepler (1571 1630) German mathematician, astronomer and astrologer 1. Planets mo...
Rutgers >> 670 >> 451 (Fall, 2008)
Lecture Notes Prepared by Prof. J. Francis Spring 2003, updated 07 Remote Sensing of Precipitation Primary reference: Chapter 9 of KVH I. Motivation - why do we need to measure precipitation with remote sensing instruments? => QPF (Quantitative pre...
Rutgers >> 712 >> 545 (Fall, 2008)
Lecture Notes Prepared by Prof. J. Francis Spring 2003, updated 07 Remote Sensing of Precipitation Primary reference: Chapter 9 of KVH I. Motivation - why do we need to measure precipitation with remote sensing instruments? => QPF (Quantitative pre...
Rutgers >> 712 >> 552 (Spring, 2008)
Lecture Notes Prepared by Prof. J. Francis Spring 2003, updated 07 Remote Sensing of Precipitation Primary reference: Chapter 9 of KVH I. Motivation - why do we need to measure precipitation with remote sensing instruments? => QPF (Quantitative pre...
Rutgers >> 670 >> 451 (Fall, 2008)
Land and Ocean Color Measuring Vegetation (NDVI, EVI, and Ocean Color) Though we often take the plants and trees around us for granted, almost every aspect of our lives depends upon them. By carefully measuring the wavelengths and intensity of visib...
Rutgers >> 712 >> 545 (Fall, 2008)
Land and Ocean Color Measuring Vegetation (NDVI, EVI, and Ocean Color) Though we often take the plants and trees around us for granted, almost every aspect of our lives depends upon them. By carefully measuring the wavelengths and intensity of visib...
Rutgers >> 712 >> 552 (Spring, 2008)
Land and Ocean Color Measuring Vegetation (NDVI, EVI, and Ocean Color) Though we often take the plants and trees around us for granted, almost every aspect of our lives depends upon them. By carefully measuring the wavelengths and intensity of visib...
Rutgers >> 670 >> 451 (Fall, 2008)
Clouds and Solar Radiation Remote Sensing of the Ocean and Atmosphere Most of these notes are taken from S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology: An Introduction 1 The temperature near the surface of the Earth is in thermodyn...
Rutgers >> 712 >> 545 (Fall, 2008)
Clouds and Solar Radiation Remote Sensing of the Ocean and Atmosphere Most of these notes are taken from S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology: An Introduction 1 The temperature near the surface of the Earth is in thermodyn...
Rutgers >> 712 >> 552 (Spring, 2008)
Clouds and Solar Radiation Remote Sensing of the Ocean and Atmosphere Most of these notes are taken from S. Q. Kidder & T. H. Vander Haar (1995) Satellite Meteorology: An Introduction 1 The temperature near the surface of the Earth is in thermodyn...
Rutgers >> 670 >> 451 (Fall, 2008)
11:670:451 / 16:712:552 Remote Sensing of the Ocean and Atmosphere Homework 1 Due Monday February 11, 2008 1. In class it was shown that balancing centripetal force and gravitational force leads to an equation describing the proportionality of orbi...
Rutgers >> 712 >> 545 (Fall, 2008)
11:670:451 / 16:712:552 Remote Sensing of the Ocean and Atmosphere Homework 1 Due Monday February 11, 2008 1. In class it was shown that balancing centripetal force and gravitational force leads to an equation describing the proportionality of orbi...
Rutgers >> 712 >> 552 (Spring, 2008)
11:670:451 / 16:712:552 Remote Sensing of the Ocean and Atmosphere Homework 1 Due Monday February 11, 2008 1. In class it was shown that balancing centripetal force and gravitational force leads to an equation describing the proportionality of orbi...
Rutgers >> 670 >> 451 (Fall, 2008)
Wavelength The Electromagnetic Spectrum = c -1 c = 3x108 ms-1 microwave 1 km 1m 1cm 10 m 0.1m 0.01 m Wavelength Energy emitted by sun in various wavelenths. Difference between Black-body curve and actual emitted energy caused by absorbtio...
Rutgers >> 712 >> 545 (Fall, 2008)
Wavelength The Electromagnetic Spectrum = c -1 c = 3x108 ms-1 microwave 1 km 1m 1cm 10 m 0.1m 0.01 m Wavelength Energy emitted by sun in various wavelenths. Difference between Black-body curve and actual emitted energy caused by absorbtio...
Rutgers >> 712 >> 552 (Spring, 2008)
Wavelength The Electromagnetic Spectrum = c -1 c = 3x108 ms-1 microwave 1 km 1m 1cm 10 m 0.1m 0.01 m Wavelength Energy emitted by sun in various wavelenths. Difference between Black-body curve and actual emitted energy caused by absorbtio...
Rutgers >> 670 >> 451 (Fall, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Sea Surface Temperature (2) Often the relative atmospheric transmission is plotted vs. increasing wavelength 3.5-4.1 m 10-12...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Sea Surface Temperature (2) Often the relative atmospheric transmission is plotted vs. increasing wavelength 3.5-4.1 m 10-12...
Rutgers >> 712 >> 552 (Spring, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Sea Surface Temperature (2) Often the relative atmospheric transmission is plotted vs. increasing wavelength 3.5-4.1 m 10-12...
Rutgers >> 670 >> 451 (Fall, 2008)
Lecture Notes Prof. J. Francis Spring 2003 Satellite Image Interpretation Material from An Introduction to Satellite Image Interpretation by E.D. Conway, The MD Space Grant Consortium, 1997. Chapters 3,6,7,9-12 and from KVH Ch. 5. Figure numbers be...
Rutgers >> 712 >> 545 (Fall, 2008)
Lecture Notes Prof. J. Francis Spring 2003 Satellite Image Interpretation Material from An Introduction to Satellite Image Interpretation by E.D. Conway, The MD Space Grant Consortium, 1997. Chapters 3,6,7,9-12 and from KVH Ch. 5. Figure numbers be...
Rutgers >> 712 >> 552 (Spring, 2008)
Lecture Notes Prof. J. Francis Spring 2003 Satellite Image Interpretation Material from An Introduction to Satellite Image Interpretation by E.D. Conway, The MD Space Grant Consortium, 1997. Chapters 3,6,7,9-12 and from KVH Ch. 5. Figure numbers be...
Rutgers >> 670 >> 451 (Fall, 2008)
The A-Train 1 Presentation Schedule 11/25 (Tuesday): Clouds and Climate Nick Mangieri- Noctilucent clouds using CloudSat (15-minutes) Allison Marquardt-The Earth Radiation Budget Experiment (15-minutes) Ross Alter - MODIS / Atmosphere (15-minutes) ...
Rutgers >> 712 >> 545 (Fall, 2008)
The A-Train 1 Presentation Schedule 11/25 (Tuesday): Clouds and Climate Nick Mangieri- Noctilucent clouds using CloudSat (15-minutes) Allison Marquardt-The Earth Radiation Budget Experiment (15-minutes) Ross Alter - MODIS / Atmosphere (15-minutes) ...
Rutgers >> 712 >> 552 (Spring, 2008)
The A-Train 1 Presentation Schedule 11/25 (Tuesday): Clouds and Climate Nick Mangieri- Noctilucent clouds using CloudSat (15-minutes) Allison Marquardt-The Earth Radiation Budget Experiment (15-minutes) Ross Alter - MODIS / Atmosphere (15-minutes) ...
Rutgers >> 670 >> 451 (Fall, 2008)
Remote Sensing: jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 From Geophysical Monograph 92, 1995: Mauna Loa Revealed: Structure, Composition, History and Hazards; Chapter on \"Remote Sensing of Mauna Loa\" by Kahle et al., Multispe...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing: jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 From Geophysical Monograph 92, 1995: Mauna Loa Revealed: Structure, Composition, History and Hazards; Chapter on \"Remote Sensing of Mauna Loa\" by Kahle et al., Multispe...
Rutgers >> 712 >> 552 (Spring, 2008)
Remote Sensing: jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 From Geophysical Monograph 92, 1995: Mauna Loa Revealed: Structure, Composition, History and Hazards; Chapter on \"Remote Sensing of Mauna Loa\" by Kahle et al., Multispe...
Rutgers >> 670 >> 451 (Fall, 2008)
Ground-based Remote Sensing an overview of sensors and applications Types: Passive Visible (cameras, solar radiometers, spectrometers) Infrared (total emission, spectrometers) Microwave emission Active Lidar (Light [vis] Detection and Rangi...
Rutgers >> 712 >> 545 (Fall, 2008)
Ground-based Remote Sensing an overview of sensors and applications Types: Passive Visible (cameras, solar radiometers, spectrometers) Infrared (total emission, spectrometers) Microwave emission Active Lidar (Light [vis] Detection and Rangi...
Rutgers >> 712 >> 552 (Spring, 2008)
Ground-based Remote Sensing an overview of sensors and applications Types: Passive Visible (cameras, solar radiometers, spectrometers) Infrared (total emission, spectrometers) Microwave emission Active Lidar (Light [vis] Detection and Rangi...
Rutgers >> 670 >> 451 (Fall, 2008)
Remote Sensing of the Atmosphere and Ocean John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Active microwave systems (2) Satellite Altimetry * range data processing * applications Altimeters (nadir pointing radar) sea...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing of the Atmosphere and Ocean John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Active microwave systems (2) Satellite Altimetry * range data processing * applications Altimeters (nadir pointing radar) sea...
Rutgers >> 712 >> 552 (Spring, 2008)
Remote Sensing of the Atmosphere and Ocean John Wilkin jwilkin@rutgers.edu IMCS Building Room 214C 732-932-6555 ext 251 Active microwave systems (2) Satellite Altimetry * range data processing * applications Altimeters (nadir pointing radar) sea...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing of the Ocean and Atmosphere: John Wilkin jwilkin@rutgers.edu IMCS Building Room 211C 732-932-6555 ext 251 Orbits and Measurement Geometry Stewart, R. H., 1985, Methods of Satellite Oceanography, University of California Press, 360 pp...
Rutgers >> 670 >> 451 (Fall, 2008)
Remote Sensing: John Wilkin wilkin@marine.rutgers.edu IMCS Building Room 211C 732-932-6555 ext 251 Active microwave systems (2) Satellite Altimetry * the movie * applications Altimeters (nadir pointing radar) sea surface height (long wavelengths ...
Rutgers >> 712 >> 545 (Fall, 2008)
Remote Sensing: John Wilkin wilkin@marine.rutgers.edu IMCS Building Room 211C 732-932-6555 ext 251 Active microwave systems (2) Satellite Altimetry * the movie * applications Altimeters (nadir pointing radar) sea surface height (long wavelengths ...
Rutgers >> 712 >> 552 (Spring, 2008)
Remote Sensing: John Wilkin wilkin@marine.rutgers.edu IMCS Building Room 211C 732-932-6555 ext 251 Active microwave systems (2) Satellite Altimetry * the movie * applications Altimeters (nadir pointing radar) sea surface height (long wavelengths ...
Rutgers >> 712 >> 545 (Fall, 2008)
John Wilkin jwilkin@rutgers.edu 732-932-6555 ext 251 Remote Sensing of the Atmosphere and Ocean http:/marine.rutgers.edu/~wilkin Room 211C IMCS Building Lecture 1. Satellite orbits References: Kidder and Vonder Harr chapter 2, Stewart chapter 15. P...
Rutgers >> 690 >> 372 (Spring, 2008)
PHYSICAL REVIEW D 71, 103515 (2005) Cosmological parameter analysis including SDSS Ly forest and galaxy bias: Constraints on the primordial spectrum of uctuations, neutrino mass, and dark energy Uros Seljak,1,2 Alexey Makarov,1 Patrick McDonald,1 S...
Rutgers >> 690 >> 372 (Spring, 2008)
The Astrophysical Journal, 659:98Y121, 2007 April 10 # 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A. A NEW HUBBLE SPACE TELESCOPE DISCOVERIES OF TYPE Ia SUPERNOVAE AT z ! 1: NARROWING CONSTRAINTS ON THE EARLY BEHAV...
Rutgers >> 690 >> 372 (Spring, 2008)
A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey Peacock et al. 2001 Nature Vol. 410 Review Large scale structure formed from the Hubbles Law ( v = H 0r gravitational collapse of small uctuations i...
Rutgers >> 690 >> 372 (Spring, 2008)
THE ASTROPHYSICAL JOURNAL, 542 : 281307, 2000 October 10 ( 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE MACHO PROJECT : MICROLENSING RESULTS FROM 5.7 YEARS OF LARGE MAGELLANIC CLOUD OBSERVATIONS C. ALCOCK,1,2 R...
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