Analytical Solutions for Heat Distribution in KB Mirror Systems

Slides:



Advertisements
Similar presentations
Finite Element Method (FEM) Different from the finite difference method (FDM) described earlier, the FEM introduces approximated solutions of the variables.
Advertisements

Model 5:Telescope mirrors Reflecting telescopes use large mirrors to focus light. A standard Newtonian telescope design is depicted in figure 1: Light.
An Introduction to Heat Flow
Heat Transfer Rates Conduction: Fourier’s Law
Multidimensional Heat Transfer This equation governs the Cartesian, temperature distribution for a three-dimensional unsteady, heat transfer problem involving.
Numerical Methods Part: False-Position Method of Solving a Nonlinear Equation
MA428 Class Project The Heat Equation Temperature Distribution in a Bar with Radiating Ends.
Numerical Methods Part: False-Position Method of Solving a Nonlinear Equation
ERT 216 HEAT & MASS TRANSFER Sem 2/ Dr Akmal Hadi Ma’ Radzi School of Bioprocess Engineering University Malaysia Perlis.
1.7: Adding Like Terms TERM: A number, a variable, or the product of the two.Ex: a, 3x, 2x, 5, CONSTANT: a term with no variable (number) Ex: 4, -1, 6,
The Electromagnetic Spectrum High Harmonic Generation
Mathematical Derivation of Probability
Q1.1 Find the wavelength of light used in this 2- slits interference.
Jonathan Donkers1, Lin Zhang1+
Measuring the Thickness of Cryosheet Jets
Madhu Karra1, Jason Koglin1,2
Image Processing For Soft X-Ray Self-Seeding
Solving systems of equations
One-Dimensional Steady-State Conduction
Structure and Function: Ubiquitination of NEMO and Optineurin
Characterizing Optics with White-Light Interferometry
Matter in Extreme Conditions at LCLS:
INTRODUCTION : Convection: Heat transfer between a solid surface and a moving fluid is governed by the Newton’s cooling law: q = hA(Ts-Tɷ), where Ts is.
Kevin Shimbo1, Matt Hayes+
X-Ray Shielding Introduction Application Research Conclusions
Crystallography images
Hutch 4 (XCS) Laser System
Anomaly Detection LCLS data: Introduction Research Conclusion
MAKING WAY FOR LCLS II HERRIOTT CELL IGNIS THE NEED FOR LCLS-II
A remote EPICS monitoring tool
EASE: Alert Management
Designing and Prototyping Optics Table and Shelves
Managing Diffraction Beam
Integration of Blu-Ice into
Effects of Wrapping Vacuum
Scintillation Material Encapsulation Fixture
LCLS CXI Sample Chambers and Engineering Solutions
Values to Normalize Data
Designing a molecular probe for detection
ECE 2202 Circuit Analysis II
LAMP Vacuum System Documentation
G6PD Complex Structural Study Crystallization Setup
Your Name, Elias Catalano, Robert Sublett, Robin Curtis
Determining a Detector’s Saturation Threshold
HXRSD Helium Enclosure
Crystallography Labeling Using Machine Learning
IT Inventory and Optimization
Structural study of soluble ammonia monooxygenase
Creation and development of a PRP database
IT Inventory and Optimization
Electro Optic Sampling of Ultrashort Mid-IR/THz Pulses
Margaret Koulikova1, William Colocho+
Repeatability Test of Attocube Piezo Stages
Solving Equations Containing Fractions
Analytical Solutions for Temperature
Barron Montgomery1,2, Christopher O’Grady2, Chuck Yoon2, Mark Hunter2+
Elizabeth Van Campen, Barrack Obama2, Stephen Curry1,2, Steve Kerr2+
Advanced Methods of Klystron Phasing
Ryan Dudschus, Alex Wallace, Zachary Lentz
Jennifer Hoover1, William Colocho2
X-Ray Spectrometry Using Cauchois Geometry For Temperature Diagnostics
Redesigning of The SED Calendars
Transient Heat Conduction
Automatic compression control for the LCLS injector laser
Russell Edmonds1, Matt Hayes2+ 1LCLS Summer Research Intern
Prototype and Design of High-Speed X-Ray Chopper
Title of Your Poster Introduction Research Conclusions Acknowledgments
Reconstruction algorithms Challenges & Future work
EQUILIBRIA AND SYNCHROTRON STABILITY IN TWO ENERGY STORAGE RINGs*
DYNAMIC APERTURE OF JLEIC ELECTRON COLLIDER
Presentation transcript:

Analytical Solutions for Heat Distribution in KB Mirror Systems Jiya Janowitz1,2, Lin Zhang2+ 1Physics Department, Material Science and Engineering Department, Stanford University, 450 Serra Mall, Stanford, CA 94305, USA 2Linac Coherent Light Source, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025, USA +zhanglin@slac.stanford.edu Introduction Background* Results Cont. The high power X-ray laser produced by LCLS II will be focused using a pair of focusing optics (KB mirrors), which must be cooled to prevent deformation and damage. There are several feasible cooling configurations; performance varies with choice. The goal of this project is to analytically solve for the heat distribution across a mirror for each cooling configuration. The analytical solutions will allow the most effective cooling system to be chosen. Keywords: LCLS II, KB mirrors, cooling, heat distribution The starting point in solving these heat distributions analytically is the General Fourier Heat Conduction Equation, assuming constant thermal conductivity (k): For steady state problems, this can be simplified to: Top-Up-Side Cooling Solution Details: Figure 3*: Plot of the two eigenvalues present in the top-up-side cooling solution. It can be seen that as Depending upon the requested precision of the answer, after n > n’ Let n’ be defined as the n such that , where a is the requested precision Numerically solve for all n<n’, then use the approximation to analytically solve for all n≥n’ Given L, h, k, and the requested precision, one can use MATLAB to determine the value of n’ Example: L = 50mm, h = .005mm, and k = .138 W/m*K Precision = .1 Calculated: n’ = 3 Solution: Numerically solve for G1 through G3 and D1 through D3, then use the approximation to analytically solve for Gn and Dn, n=3,4,5,… Figure 2: 3D Steady State Full Side Cooling. This image shows one quarter of the full volume of the mirror being analyzed. The beam here has a length, Lbm, and a width, Wbm. To simplify this problem to the 2D version, simply set Lbm equal to the length of the mirror. Figure 1*: 2D Steady State Top-Up-Side Cooling. This configuration shows one quarter of the full surface of the mirror being analyzed. The beam width is a, and the mirror is cooled across d, and k is the mirror’s thermal conductivity. Results 2D Steady State Solution for Top-Up-Side Cooling: Conclusions After solving the 2D steady state versions of bottom cooling and full side cooling, I was able to derive an analytical solution for 2D steady state top-up-side cooling. Then after solving the 3D steady state solution to bottom cooling, I successfully derived a 3D steady state solution for full side cooling. The next steps in this project are to find the 3D transient state solutions for bottom and full side cooling. Then, to find the 3D transient state solution for top-up-side cooling. Finally, it is essential to use MATLAB to model all the solutions that were obtained, and check them against numerical solutions to verify their legitimacy. 3D Steady State Solution for Full Side Cooling: Acknowledgments Use of the Linac Coherent Light Source (LCLS), SLAC National Accelerator Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-76SF00515. *Lin Zhang, SLAC Engineering Seminar, 2015 Date: 08/11/2016