General Disclaimer. One or more of the Following Statements may affect this Document

Similar documents
The Los Alamos Laboratory: Space Weather Research and Data

Reduction of Trapped Energetic Particle Fluxes in Earth and Jupiter Radiation Belts

Quantum Dot Spectrum Converter Coverglass for Enhanced High Efficiency Photovoltaics

Space Radiation Mitigation for Fox-1

TACSAT-4 SOLAR CELL EXPERIMENT: TWO YEARS IN ORBIT

Chapter 7. Solar Cell

NPSAT1 Solar Cell Measurement System

A L A BA M A L A W R E V IE W

S5p INTENTIONALLY BLANK

PERFORMANCE MEASUREMENTS OF THE SUB MILLIMETER WAVE ASTRONOMY SATELLITE (SWAS) SOLAR ARRAY DEPLOYMENT SYSTEM

Tuesday, December 11th. To be handed in both as a hard copy (in my mailbox in LGRT 1127A) and on SPARK (as a turnitin assignment).

PRACTICE NO. PD-AP-1309 PREFERRED PAGE 1 OF 5 RELIABILITY PRACTICES ANALYSIS OF RADIATED EMI FROM ESD EVENTS CAUSED BY SPACE CHARGING

Implementation of One Diode Model Solar Cell Capacitance to Measure Temperature

Solar Cell Radiation Environment Analysis Models (SCREAM)

Radiation Effects on Electronics. Dr. Brock J. LaMeres Associate Professor Electrical & Computer Engineering Montana State University

Design, Fabrication and Performance of the Silicon Charge Detector for the ISS-CREAM

Cosmic Ray Telescope for the Effects of Radiation to Spacecraft Thermal Interface Control Document

Solar & Electric Sailing Overview

INTERPLANETARY EXPLORATION-A CHALLENGE FOR PHOTOVOLTAICS 1 INTRODUCTION

PREFERRED RELIABILITY PRACTICES. Practice:

UV LED charge control at 255 nm

PRISMATIC COVERS FOR BOOSTING THE EFFICIENCY OF HIGH-CONCENTRATION PV SYSTEMS

WISE Science Data System Single Frame Position Reconstruction Peer Review: Introduction and Overview

About the Van Allen Probes Mission

The 2007 CubeSat Developers' Workshop SwissCube Project

INJUN. The discovery of the geomagnetically trapped. A Radiation Research Satellite. G. F. Pieper

B THE SOLAR ARRAY. Theory

CHARGING ANALYSIS OF ENGINEERING TEST SATELLITE VIII (ETS-VIII) OF JAPAN

Solar Energetic Particles measured by AMS-02

NOAA Space Weather Prediction Center Data and Services. Terry Onsager and Howard Singer NOAA Space Weather Prediction Center

SIMULATION OF SPACE RADIATION FOR NANOSATELLITES IN EARTH ORBIT *

Reliability of Spacecraft. Power Systems

Van Allen Probes Mission and Applications

Megavolt Parallel Potentials Associated With Double Layer Streams In The Earth s Outer Radiation Belt

DRAFT. Robotic Lunar Exploration Program Lunar Reconnaissance Orbiter 431-ICD Date: September 15, 2005

Space environment (natural and artificial) Realtime solar activity and space environment information for spacecraft operation

Cosmic Ray Telescope for the Effects of Radiation to Spacecraft Thermal Interface Control Document

High resolution THz scanning for optimization of dielectric layer opening process on doped Si surfaces

Solar Photovoltaics under Partially Shaded Conditions. Vivek Agarwal Dept of Electrical Engineering

Instructor Resources

3.4 Plasma Data Sets Polar/CAMMICE/MICS Spacecraft Detector

Solar particle events contribution in the space radiation exposure on electronic equipment

Lunar Reconnaissance Orbiter Project. Cosmic Ray Telescope for the Effects of Radiation to Spacecraft Mechanical Interface Control Document

StellarXplorers IV Qualifying Round 2 (QR2) Quiz Answer Key

Quantum Dot Technology for Low-Cost Space Power Generation for Smallsats

Radiation Analysis of InGaP/GaAs/Ge and GaAs/Ge Solar Cell: A comparative Study

Introduction to Photovoltaics

EE 446/646 Photovoltaic Devices I. Y. Baghzouz

USING SPACE WEATHER VARIABILITY IN EVALUATING THE RADIATION ENVIRONMENT DESIGN SPECIFICATIONS FOR NASA'S CONSTELLATION PROGRAM

Solar System Exploration in Germany

Line-Focus and Point-Focus Space Photovoltaic Concentrators Using Robust Fresnel Lenses, 4-Junction Cells, & Graphene Radiators

MAE 5595: Space Environments and Spacecraft Interactions. Lesson 4: Introduction

Absolute Radiometric Calibration Using a Solar Reflector in Near-Geosynchronous Orbit

History of Spaceflight

Unit 3: The Atom Part 1. DUE: Friday October 13, 2017

[T.EhDhhh F/6 10/2. PERFORMANCE OF 7 AD-Albl 983 NAVAL RESEARCH LAB DC ABOARD THE NTS-2 SATE-ETC(U) JUL G1 0 H WALKER UNCLASSIFIED NRR4580N

PHOTOVOLTAICS Fundamentals

NASA Future Magnetospheric Missions. J. Slavin & T. Moore Laboratory for Solar & Space Physics NASA GSFC

NPP ATMS Instrument On-orbit Performance

University of Pittsburgh

NASA s STEREO Mission

A New JPL Interplanetary Solar HighEnergy Particle Environment Model

REPORT DOCUMENTATION PAGE

Electrons are shared in covalent bonds between atoms of Si. A bound electron has the lowest energy state.

Reflectivity in Remote Sensing

Turbulence in the Solar Wind

BUILDING LOW-COST NANO-SATELLITES: THE IMPORTANCE OF A PROPER ENVIRONMENTAL TESTS CAMPAIGN. Jose Sergio Almeida INPE (Brazil)

EE 5611 Introduction to Microelectronic Technologies Fall Tuesday, September 23, 2014 Lecture 07

DRAFT. Robotic Lunar Exploration Program Lunar Reconnaissance Orbiter (LRO)

GLAST Large Area Telescope

IMESA-R Integrated Miniaturized Electrostatic Analyzer Reflight

Use precise language and domain-specific vocabulary to inform about or explain the topic. CCSS.ELA-LITERACY.WHST D

Variation of proton radiation belt deduced from solar cell degradation of Akebono satellite

Lecture 5 Junction characterisation

CM1000DUC-34SA. Mega Power Dual IGBT 1000 Amperes/1700 Volts

Study the Effect of Proton Irradiation for Photovoltaic Cells Characteristics in LEO Orbit

Extended Missions. Dr. Art Poland Heliophysics Senior Review Chair George Mason University

Nanosat Science Instruments for Modular Gravitational Reference Sensor (MGRS)

Nonionizing Energy Loss (NIEL) for Protons

The temperature dependence of the spectral and e ciency behavior of Si solar cell under low concentrated solar radiation

Spacecraft Bus / Platform

3-1. Heat Dissipation Design Method. Power Dissipation Loss Calculation Usage of The Cooler with Water Jacket 3-7 Flange Adapter Kit 3-10

Displacement Damage Characterization of Electron Radiation in. Triple-Junction GaAs Solar Cells

Mark O Neill, LLC P.O. Box 2262 Keller, TX USA

James Paul Mason CU Boulder LASP

CRaTER Pre-Environmental Review (I-PER) Science Requirements Update

Development of Microwave Engine

Look over Chapter 26 sections 1-7 Examples 3, 7. Look over Chapter 18 sections 1-5, 8 over examples 1, 2, 5, 8, 9,

Mission to Understand Electron Pitch Angle Diffusion and Characterize Precipitation Bands and Spikes. J. F. Fennell 1 and P. T.

Balloon Array for RBSP Relativistic Electron Losses

Characterization of deep defects in CdSyCdTe thin film solar cells using deep level transient spectroscopy

IRS-TR 05001: Detector Substrate Voltage and Focal Plane Temperature of the LH module

5.1 Use of the Consensus Reference Concept for Testing Radiosondes. Joe Facundo and Jim Fitzgibbon, Office of Operational Systems,

Supporting Information

Appendix D Nomenclature. Abstract

STRETCHED LENS ARRAY (SLA): A PROVEN AND AFFORDABLE SOLUTION TO SPACECRAFT CHARGING IN GEO

ECE-342 Test 2 Solutions, Nov 4, :00-8:00pm, Closed Book (one page of notes allowed)

February 1, 2011 The University of Toledo, Department of Physics and Astronomy SSARE, PVIC

LUNAR MICRO ROVER SOLAR SHROUD. Daniel Hong Department of Mechanical Engineering University of Hawai`i at Mānoa Honolulu, HI ABSTRACT

Electron Polar Cap and the Boundary oœ Open Geomagnetic Field Lines

Transcription:

General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI)

X 711-76-29 PREPRINT, RESULTS FROM THE IMP-J VIOLET SOLAR CELL EXPERIMENT AND VIOLET CELL BALLOON FLIGHTS VI(' L :XF ERI4FNT PAI Lc f y^5 ^ ti.. ^A^ 11 p -1- i,mp-j VICLL `F,L $3. S0 C`JCL 10A G. 3/t. 4 N77-30b57 Uncias 50022 EDWARD M. GADDY FEBRUARY 1976 ^. A SEP 1976 RECEIVED,ASA sn FA tul l f PUT BRANCH I& GODDARD SPACE FLIGHT CENTER GREENBELT, MARYLAND

X-711-76-29 Preprint RESULTS FROM THE IMP-J VIOLET SOLAR CELL EXPERIMENT AND VIOLET CELL BALLOON FLIGHTS F;dward M. Gaddy February 1976 GODDARD SPACE FLIGHT CENTER Greenbelt, Maryland

RESULTS FROM THE IMP-J VIOLET SOLAR CELL EXPERIMENT AND VIOLET CELL BALLOON FLIUHTS Edward M. Gaddy ABSTRACT The IMP-J violet solar cell experiment was flown in an orbit with mild thermal cycling and low hard particle radiation. The results of the experiment show that violet cells degrade at about the same rate as conventional cells in such an orbit. Balloon flight measurements show that violet solar cells produce approximately 20% more power than conventional cells. iii

CONTENTS Page ABSTRACT... Iii INTRODUCTION...... 1 THE VIOLET CELL PANEL. ON IMP-J..................... 1 SPACE FLIGHT RESULTS... 4... 1 BALLOON FLIGHT RESULTS,, o,,,,,,,,,,,,,,,,,,, 4 DISCUSSION... 4 CONCLUSION... 4 REFERENCES... 7 ILLUSTRATIONS Figure Page 1 'rhe IMP-J Spacecraft........ 2 2 Voltage vs. Current for the IMP-J Violet Cell Panel 6 and the IMP-J Reference Cell Panel.... TABLES Table Page I Degradation of Violet Cell Current vs. Commercial Cell Current... 3 II II Results of Balloon Flight Measurements.......... 5 v

INTRODUCTION RESULTS FROM THE IM1 3 -J VIOLET SOLAR CELL EXPERIMENT AND VIOLET CELL BALLOON FLIGHTS Lindmayer and Allison publicly introduced the COMSAT violet solar cell in 1972!1) This cell represented a considerable improvement in solar cell technology, pr(xtucing at least twenty percent more power than conventional or state of the art cells available at that time l2) The violet ce!1 achieved this performance through the use of a very shal:ow junction, an improved anti-reflection coating and a superior contact geometry. This report compares the flight performance of violet cells to typical conventional cells available for space flight use in 1972.. The conventional cells used for this purpose were those specified for the solar array fo-- the Explorer 50 Spacecraft, otherwise known as Interplanetary Monitoring Platform-J (IMP-J). These cells had an efficiency of 11.0% after final assembly onto the array producing 31.7 milliampere/cm 2 at 0.470 volt at 25 C. THE VIOLET CELL PANEL ON 11%11'-J The violet cell panel is one of forty-eight solar panels m,:king up the solar array for the IMP-J spacecraft, Figure 1. It is a technology experiment flown as part of the satellite's power system. As a result, it was made as similar as practicable to the other forty-seven solar panels on the satellite. The violet cell panel used 204-2cm x 2cm x.028cm COMSAT violet cells with three in parallel by sixty-eight in series. Each cell is covered %\ ith.15mm thick ceria doped coverglasses. The other panels each have sixty-eight 2cm x 6cm x.036cm conventional solar cells in series with each cell covered by.15mm thick Doer Corning 7940 coverglasses with AR coating and 410 µm cutoff filters. All panel!. use Sylgard 186 as a celi adhesive and Sylgard 182 as a coverglass adhesive. The cells are mounted on substrates of aluminum honeycomb with aluminum face sheets. SPACE FLIGHT RESULTS During spaceflight operation, the panels are biased at 28V t 0.5V. There is a.9v drop across the panel's harness and diodes. Therefore, each cell string operates at 28.9V t.5v. Since there are sixty-eight series cells, each cell operates at.425v -E.007V. The current produced by the violet cell panel and the current of an adjacent conventional cell panel, chosen as being typical, are monitored by special circuitry. The results of these measurements, corrected for variation 1

I 4b _ Y' RFM ANTENNA (4) ACS (2) DIRECTION OF SPIN IS COUNTERCLOCKWISE 55.00" ;x' \ i I 16 2 ^ 15 3 I 14 4 13 I MAGNETOMETER 5 12 I i 11. ---=106.0U 6 I I+---- = 108.00" ---- --+ 10 ^ 8 9 \ RF ANTENNA (8) -24.00" LENGTH x ^ 55.00' -Y' kq^ _tit ^}}} f i to «T ' :,.SOLAR PAN'.. riill +--i ^I r it : ^ ^ + -..S#li7 :^.t III tft I'" ^'. Figure 1. The IMP-J Spacecraft 2

in the earth sun distance are presented in Table 1. All measurements were taker_ with the sunline normal to each panel at a temperature of 12 C f 3 C. I Several comments should be made about the results in Table I. The degradation shown results primarily from solar flare protons and perhaps from ultraviolet light. Practically all other sources of degradation are absent by virtue of the IMP-J's orbit. Since the orbit does not traverse the Van Allen belts. there is no damage due to trapped protons or electrons. Additionally, the thermal cycling of the panels is very light and this source of degradation is also virtually eliminated. Table I Degradation of Violet Cell Current vs. Conventional Cell Current All measurements at 12 C Reference (Conventional) Panel Violet Cell Panel Days After Current in Percent Current in Percent Launch* Amperes Degradation Amperes Degradation. Pre-Launch Ground 0.392 +1.6% 0.459 +4.1% Measurement 4. 4** 0.386 0.0% 0.441 0.0% 0 128 0.373-3.4 %Q 0.428-2.9% 280 0.371-3.9c/o 0.426-3.4% 392 0.370-4.1% 0.424-3. 9% * Launch took place on October 25, 1973. ** Fourth day measurement taken as zero. Another comment about the data in Table I concerns the ground predictions of the flight results. In the case of both panels an error was made in calibrating the telemetry to the current through the panel. Unfortunately, the exact magnitude of the error cannot be determined. It Follows that the magnitude of the current produced by the panels is not known. Oaly the percent degradation figures are accurate. However, results from the balloon flight measurements, described below, show that the ground measurements actually underestimated rather than overestimated the cur rent producing capability of the panels. 3 M

BALLOON FLIGHT RESULTS In addition to the spacecraft flight results described above, three violet cells anc' two commercial cells were flown by J. P. L. on a balloon flight. The violet cells flown on the balloon were randomly selected from the same batch of cells used for the IMP-J panel. The conventional cells flown on the balloon were selected from cells typical of those used on the IMP-J commercial panels. The balloon flight results are shown in table II. As can be seen there is good correlation beta,-en the ground measurements and the flight readings. However, in all cases the flight measurement is approximately 1.5% higher than the ground measurements. DISCUSSION The ground measurements and subsequent predictions for the balloon cells and the spacecraft panels were made using the same: solar simulator. Since the balloon flight measurements were 1.5% higher than the ground predictions, we conclude that both panels should produce about 1.51, more short circuit current thin predicted from ground measurements. Using this conclusion and observing the current-voltage curves obtained under the simulator for both the violet cell panel and conventional cell panels, Figure 2, we make the extrapolation that violet cells produce approximately 20%, more peak power than conventional cells at 25 C. The percentage is obtained from Figure 2 merely by noting that 14.4W is 201, greater than 12.OW. The estimate that both panels have flight short circuit currents some 1. 11% higher than that shown by Figure 2 does not, of course, affect the comparison. CONCLUSION The IMP-J flight results demonstrate that violet cells degrade at just about the same rate as conventional cells in the space enviroment. Violet cells generate approximately 20% more power than conventional cells available in 1972. 4

F. bu I C ao N x.^ u5 N N n y N ri0 ^ tt7 cd a o ago.^+ U^.~Qr7 G Q/ CC Gj ^to 4.. Q C "" W U to CD M v U n '1 ^'s0 s C+ Z ^ ^ cd cn H c^u r w c m b /] v ^ ^ cam C7 to n 7 M O O cd ^-+ 00 r r- C'3 ao co cc C ^' O S c3 Z y a '" U m w ro o u O y y Qi.0 Fa ^^ N ao ^O ^ U ^ Chi+" U rn > U f]. OC-1 ^", Uf v O tu, O C's O ;^ y Ct u u a^ pi W U o 0 ` U U W u V o ^ u bd 3 t+ u.q.-r N M rr ^, o a o O o u rm- ca u N 5

0. wo VIOLET CELL PANEL PEAK POWER 144.'V!, 325V 450 400 REFERENCE PANEL PEAK POWER 12.0 W C' 31-5V 350 N W w 300 a Q J J z 250 z W x D 200 U 157 100 50 0 0 10 20 30 40 50 VO'.TAGE IN VOLTS Figure 2. Voltage vs. Current for the IMP-J Violet Cull Panel and the IMP-J Reference Cell Panels, Temperature: 25*C 6

REFERENCES 1. Lindmayer, J. and J. Allison, "An Improvrd Silicon Solar Cell - The Violet Cell," Conference Record of the Ninth IEEE Photovoltaic Specialists Conferenca, IEEE 1972, pp. 83-1,44. 2. Gaddy, Edward M., "Flight Qualification Test Results for Violet Cells," Conference Record of the 'Tenth IEEE Photovoltaic Specialists Conference, IEEE 1974, pp. 153-162. Yasui, R. K. and R. F. Greenwood, "Results of the 1973 NASA/JPL Balloon Flight Solar Cell Calibration Program," NASA TR 32-1600, November 1975. 7