Thermal Modeling of the CX Satellite Jacob Boettcher Thermal Team Lead 4/5/02.

Slides:



Advertisements
Similar presentations
PH 508: Spacecraft systems
Advertisements

Bare rock model Assumptions
Seasons.
Solar Orbiter EUV Spectrometer
(theta) dependence of intensity theta A’A >. Energy per square meter decreases at lower sun angles and shorter daylight periods.
1 Space thermal environment Isidoro Martínez 11 July 2008.
Solar radiation and earth energy balance 1) Paul’s Demo 2) Magnitude of Solar Radiation ( Estimate of the power of Garden lights ) 2) Earth energy balance.
Simple Model of the greenhouse effect Includes atmosphere layer. Atmosphere layer passes all solar radiation. Atmosphere layer absorbs all IR from Earth.
Solar constant The solar constant is the amount of incoming solar radiation per unit area, measured on the outer surface of Earth's atmosphere, in a plane.
Atmospheric Chemistry Global Warming. GasMole Percent N O Ar0.934 CO O3O3 1.0 x Composition of Atmosphere:
1 Aerospace Thermal Analysis Overview G. Nacouzi ME 155B.
THE RADIATION BUDGET (Exercise) Exercise: Monitor radiation budget at 2 sites (urban rural) using instruments.
Atmospheric Chemistry Global Warming. GasMole Percent N O Ar0.934 CO O3O3 1.0 x Composition of Atmosphere:
METO 621 Lesson 27. Albedo 200 – 400 nm Solar Backscatter Ultraviolet (SBUV) The previous slide shows the albedo of the earth viewed from the nadir.
Lecture 1: Introduction to the planetary energy balance Keith P Shine, Dept of Meteorology,The University of Reading
Earth-Atmosphere Energy Balance Earth's surface absorbs the 51 units of shortwave and 96 more of longwave energy units from atmospheric gases and clouds.
Pat Arnott, ATMS 749 Atmospheric Radiation Transfer Chapter 6: Blackbody Radiation: Thermal Emission "Blackbody radiation" or "cavity radiation" refers.
FASTRAC Thermal Model Analysis By Millan Diaz-Aguado.
The Greenhouse Effect Garver GEO 307. Take home points from Chapter 2  EMR carries energy through space  If an object can absorb energy, it can also.
CE 401 Climate Change Science and Engineering solar input, mean energy budget, orbital variations, radiative forcing January 2012.
Thermal Subsystem PDR Josh Stamps Nicole Demandante Robin Hegedus 12/8/2003.
LSU 06/21/2004Thermal Issues1 Payload Thermal Issues & Calculations Ballooning Unit, Lecture 3.
SATELLITE METEOROLOGY BASICS satellite orbits EM spectrum
ATMOSPHERE HEATING RATE: CLOUD FREE ATMOSPHERE. Words and Equation from Petty: Radiative Heating Rate.
Radiation and Conduction in the Atmosphere
Lecture 3 read Hartmann Ch.2 and A&K Ch.2 Brief review of blackbody radiation Earth’s energy balance TOA: top-of-atmosphere –Total flux in (solar or SW)=
Water Vapour & Cloud from Satellite and the Earth's Radiation Balance
Thermal Subsystem Peer Review Objective: To maintain all components of the space craft within their specific temperature range.
Satellite Image Basics  Visible: Senses reflected solar (lunar) radiation Visible –Cloud thickness, texture; not useful at night  Infrared (IR): Senses.
USAFA Department of Astronautics I n t e g r i t y - S e r v i c e - E x c e l l e n c e Astro 331 Thermal Control Subsystem (TCS)—Intro Lesson 37 Spring.
LionSat Thermal Subsystem Team Members: Nathan Hermanson Adam McDonald Joel Thakker.
Goals for Today 1.PREDICT the consequences of varying the factors that determine the (a) effective radiating temperature and (b) mean surface temperature.
Science 3360 Lecture 5: The Climate System
Thermal Control Subsystem
Thermal Design Matthieu GASQUET Cranfield University / Rutherford Appleton Laboratory Coseners House July 9th 2002 EUS consortium meeting.
Green House Effect and Global Warming. Do you believe that the planet is warming? 1.Yes 2.No.
Blackbody Radiation/ Planetary Energy Balance
Wes Ousley June 28, 2001 SuperNova/ Acceleration Probe (SNAP) Thermal.
LIVE INTERACTIVE YOUR DESKTOP November 7, 2011 NASA Temperature & Earth Climate Course: Modeling Hot and Cold Planets Presented by: Alissa Keil.
Global Change: Class Exercise Global Energy Balance & Planetary Temperature Mteor/Agron/Envsci/Envst 404/504.
Solar Orbiter EUS: Thermal Design Progress Bryan Shaughnessy, Rutherford Appleton Laboratory 1 Solar Orbiter EUV Spectrometer Thermal Design Progress Bryan.
Introduction to On-Orbit Thermal Environments
The Greenhouse Effect Solar Radiation, Earth's Atmosphere, and the Greenhouse Effect. Martin Visbeck DEES, Lamont-Doherty Earth Observatory
Green House Effect and Global Warming. Do you believe the Earth is warming? A.Yes B.No.
Rose Navarro HMI Lead Thermal Engineer
How the Greenhouse Effect Works/Feedback factors
explore • inspire • engage
simple analysis detailed analysis control methods
LAT Requirements Verification in TVAC
PRELIMINARY MAP - Sun On Secondary Reflector Analysis #4
Preliminary MAP - Sun On Secondary Reflector Analysis #3
12: Greenhouses and the Earth System
Complex models are needed to represent the processes occurring in and between the atmosphere, oceans and land surface. Source: Climate Change 2007: The.
Topic- Black-Body Radation Laws
Chapter 1: Earth as a System
UNIT 4: CLIMATE CHANGE.
GLOBAL ENERGY BUDGET - 2 The Greenhouse Effect.
Global Change: Class Exercise
Atmospheric Heating Notes
Global Change: Class Exercise
JOSH STAMPS ROBIN HEGEDUS
LRO CRaTER Preliminary Temperature Predictions Design A Concept  Old Concept April 12, 2005 Cynthia Simmons/ESS.
ATM OCN Fall 2000 LECTURE 8 ATMOSPHERIC ENERGETICS: RADIATION & ENERGY BUDGETS A. INTRODUCTION: What maintains life? How does Planet Earth maintain.
Greenhouse Gases.
UNIT 4: CLIMATE CHANGE.
Place these answers onto your Meteorology Chapter 17 Worksheets.
Conversations with the Earth Tom Burbine
Global Change: Class Exercise
Global Change: Class Exercise
CLIMATE CHANGE.
Presentation transcript:

Thermal Modeling of the CX Satellite Jacob Boettcher Thermal Team Lead 4/5/02

Overview Brief description of the thermal design process Discuss the reasons for an orbit revaluation Describe the procedure used to perform the orbit revaluation Present the results

Thermal Design Philosophy Thermal Control System had to be entirely passive – Places requirement that the spacecraft absorb and emit the right balance of radiation Required accurate model of the thermal environment – Must know if the spacecraft can achieve a steady thermal state

Thermal Modeling Process Create 3-D model of the spacecraft for radiation view-factor calculation – SUPVIEW Determine the Beta Angle – FINDB6 Calculate Thermal Inputs – ALBTIME2 & ALBEDO Determine overall radiation model – REFLECT Input thermal conductances and capacitances into model to get temperature profiles – TAK III

Reasons for Orbit Revaluation CX was designed to operate in a particular orbit – Altitude: 705 km; Local Time: 10am-10pm Needed to see if other orbits would satisfy: – Power requirements (solar panels) – Science requirements (instruments) – Thermal requirements (radiation budget)

Evaluated Orbits Selected based on the following criteria: Must be sun-synchronous (constant beta angle) Science must have pass time between 9am-9pm & 12am-12pm Altitude must be above 500 km (drag effects) Power required local time of 10:30am-10:30 pm or earlier Each ran with hot and cold case values for Solar flux, Earth IR Emission, and Direct Solar Albedo

Subsystem Thermal Requirements

Results

Conclusions No single orbit satisfied all thermal requirements Science subsystem only subsystem not to be satisfied by any other orbit Closer to the original orbit the better – All subsystems, except Science, satisfied with local times between 10am-10pm & 10:30am-10:30pm

Questions?