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Study of Atmospheric Gradients and Neutral forcing (SAGAN) Mission Vaibhav Kumar Tanish Himani Swapnil Pujari Mark Mote Matthew Owczarski

SAGAN Final JPL Presentation

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Page 1: SAGAN Final JPL Presentation

Study of Atmospheric Gradients and Neutral forcing (SAGAN) Mission

Vaibhav Kumar

Tanish Himani

Swapnil Pujari

Mark Mote

Matthew Owczarski

Page 2: SAGAN Final JPL Presentation

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Mission Relevance

• IMCC Request for Proposals calls for a mission designed to “understand how the ionosphere is driven by, and participates in, the global circulation of plasma and energy throughout the coupled ionosphere-magnetosphere system”

• Our Science Goal: To understand how lower atmospheric wave energy, neutral forcing and current drifts in the low altitude ionosphere affect the near-Earth plasma.

2

Page 3: SAGAN Final JPL Presentation

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Mission Relevance

3

Space Studies Board,. The 2013-2022 Decadal Survey In Solar And Space Physics. Division on Engineering & Physical Sciences: N.p., 2012. Web. 13 Sept. 2015. Solar And Space Physics: A Science For A Technological Society.

Page 4: SAGAN Final JPL Presentation

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Mission Relevance

4

Space Studies Board,. The 2013-2022 Decadal Survey In Solar And Space Physics. Division on Engineering & Physical Sciences: N.p., 2012. Web. 13 Sept. 2015. Solar And Space Physics: A Science For A Technological Society.

Page 5: SAGAN Final JPL Presentation

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Mission Relevance

• The Decadal Survey committee recommends the following: – Science Goals: Determine the dynamics and coupling of

Earth’s magnetosphere, ionosphere and atmosphere and their response to solar and terrestrial inputs.

– Guiding Principles: To make transformational scientific progress, the Sun, Earth, and heliosphere must be studied as a coupled system.

5

Page 6: SAGAN Final JPL Presentation

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Mission Relevance

6

NASA,. NASA 2014 Science Plan. NASA, 2014. Web. 13 Sept. 2015.

Page 7: SAGAN Final JPL Presentation

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Mission Relevance

7

• The NASA Science Plan highlights the following ideas for future potential missions based on the science goals highlighted in the Decadal Survey:

Page 8: SAGAN Final JPL Presentation

Motivation/

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Summary

Background– F region

• The F region of the ionosphere contains ionized gases at a height of ~150–800 km above sea level

• The F region has the highest concentration of free electrons and ions anywhere in the atmosphere.

8Image Credit: Encyclopedia Britannica,. The Day-And-Night Differences In The Layers Of Earth's Ionosphere.. 2012. Web. 13 Sept. 2015.

Page 9: SAGAN Final JPL Presentation

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Background– Spread-F Depletions

• Spread-F Depletions are the occurrence of the post sunset and nighttime plasma irregularities in the F-region ionosphere. – Broad range scale sizes over several orders of magnitude from ~10 cm

to ~100 km.

9

Image Credit: Chapagain, Narayan P. "Dynamics of equatorial spread F using ground-based optical and radar measurements." (2011).

Page 10: SAGAN Final JPL Presentation

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Science Traceability Matrix

10

Page 11: SAGAN Final JPL Presentation

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STM – Primary Science Objective

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Science Objectives

Measurement Requirements Instrument

Functional

Requirements

Mission Top

Level

RequirementObservablesPhysical

Parameters

PRIMARY SCIENCE OBJECTIVE

An enhanced vertical drift

in the F-region after

sunset is characteristic of

the low-latitude

ionosphere, whose

intensity exhibits

seasonal, longitudinal,

solar cycle, ionospheric

storm and neutral forcing

dependencies.

Presence of indicators

(ion species) that the

constellation is straddling

a nightside enhancement Ion spectrum

measurement,

ion and electron

distributions,

electric and

magnetic fields

using four point

method

Wide dynamic range in energy

coverage from spacecraft potential to

40keV/e.

Maintaining

electrostatic &

electromagnetic

cleanliness of

measurement probes by

introducing constant

satellite spin.

Separate the major mass ion species,

that is those that contribute

significantly to total mass density to

confirm night time enhancement using

Ion Spectrometry

Presence of tangential

DC electric and normal

magnetic fields

Oscillating electric-field in three axis in

the range 50–8000 Hz and amplitude

range 10 mV m-1 to 1 V m-1.

Continuous active

spacecraft potential

control to maintain

ground voltage

Time delays between signals from four

different antenna elements(Electric

field measurement) on the same

spacecraft, with a time resolution of

110 s.

Measurements required

for a minimum of one

seasonal cycle

Presence of a vertical ion

flux over baseline value

Three-dimensional velocity distribution

of electrons in the energy range from

0.59 eV to 26.4 keV

Deployment of

measurement devices

on external booms to

reduce noise.

Page 12: SAGAN Final JPL Presentation

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STM – Secondary Science Objectives• Objective 1: Spread-F depletions at lower latitudes can be

appropriately explained by the formation of a vortex in the ambient plasma at sunset due to the different velocities of plasma and neutral gasses.

• Objective 2: An enhanced vertical drift in the F-region dynamo after sunset results in large scale electric fields that lead to night time enhancements of global ionospheric storms.

12

Image Credit: Chapagain, Narayan P. "Dynamics of equatorial spread F using ground-based optical and radar measurements." (2011).

Page 13: SAGAN Final JPL Presentation

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Summary

Measurement Technique

• Spatial correlation of a control volume – Requires 4 non-coplanar points of measurement

• Simplest such configurations is a tetrahedron

• Similar non-coplanar measurement technique used previously by ESA Cluster mission and NASA MMS mission

13

Page 14: SAGAN Final JPL Presentation

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Mission Statement

The SAGAN mission will investigate the impact of atmospheric wave energy, neutral forcing, and current drifts on low & mid-latitude structuring in near-Earth

Plasma in the ionosphere. This will be achieved through simultaneous in-situ measurements of electric and

magnetic flux, electron density, and ion composition in the ionosphere using a microsatellite constellation.

Page 15: SAGAN Final JPL Presentation

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Mission Objectives

1) Insert four identical microsatellites into a tetrahedron formation consisting of three distinct orbital planes about a reference orbit

2) The four satellites must maintain a close tetrahedron structure continuously throughout the orbit, for the duration of the mission based on the reference orbit

3) Science payload data must be collected and stored on-board for each microsatellite

4) The science data from each microsatellite shall be returned back to the ground station and archived.

Page 16: SAGAN Final JPL Presentation

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Mission Success Criteria

Source Mission Success Criteria Minimum Full

MO - 1 Each satellite shall achieve sucessful launch vehicle seperation and detumbling X

MO - 1 Establish communication link and perform health checks for all subsystems and payload for each satellite X

MO - 1 Perform necessary maneuver to achieve desired orbit for each satellite X

MO - 2 Relative distances during the close approach tetrahedron must be less than 150 km X

MO - 3 Each satellite shall achieve an angular rotation rate of 3 RPM to achieve electromagnetic cleanliness for the payload X

MO - 3 Coherent measurements of vertical drift in the F-region at the day/night terminator must be measured for 6 months X

MO - 4 6 months of payload data from all payload instruments on each satellite must be transmitted to the ground station X

MO - 3 Coherent measurements of vertical drift in the F-region at the day/night terminator must be measured for 24 months X X

MO - 3 One coherent measurement of spread-F depletions post-sunset must be measured X X

MO - 3One coherent measurement of vertical depletions and large scale current drifts in the F-region during an ionospheric

storm at the day-night terminator must be measuredX X

MO - 4 24 months of payload data from all instruments on each satellite must be transmitted to the ground station X X

Page 17: SAGAN Final JPL Presentation

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Summary

Concept of Operations

Page 18: SAGAN Final JPL Presentation

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Summary

Trajectory Design• Orbit plane 1 (“reference orbit”): 550 km circular orbit inclined at

30°. Contains Sat #1 and Sat #2 phased 0.85° apart.

• Orbit plane 2: Eccentric to reference orbit (~535 km by 565 km altitude) with same inclination and period. Contains Sat #3 initially phased 0.42° from Sat #1

• Orbit plane 3: Eccentric to reference orbit (~535 km by 565 km altitude) with 30.2° inclination and same period. Contains Sat #4 initially phased 0.60° from Sat #1Orbital Parameters Satellite 1 Satellite 2 Satellite 3 Satellite 4

Altitude at Perigee (km) 550 550 535 535

Altitude at Apogee (km) 550 550 565 565

Semimajor Axis (km) 6928 6928 6928 6928

Eccentricity 0 0 0.0022 0.0022

Period (seconds) 5738.82 5738.82 5738.82 5738.82

Inclination (°) 30 30 30 30.2

Longitude of Ascending

Node at Launch (°)280.31 280.31 280.31 280.31

Phase from Satellite #1 (°) 0 0.85 0.42 0.6

Page 19: SAGAN Final JPL Presentation

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Trajectory Design (cont.)

View gifs online

Page 20: SAGAN Final JPL Presentation

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Management

Summary

Trajectory Design (cont.)

Page 21: SAGAN Final JPL Presentation

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Trajectory Design (cont.)

Page 22: SAGAN Final JPL Presentation

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Summary

Trajectory Design (cont.)

Page 23: SAGAN Final JPL Presentation

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Summary

Two Weeks in the Life

Page 24: SAGAN Final JPL Presentation

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Summary

• The spacecraft structure is an “extruded hexagon” – Driven by solar array sizing and ESPA Grande size limits

– Consists of two main equipment platforms (MEP) with unobstructed field of view and one internal main equipment platform

• 4 bulkheads and 6 spars along vertices of hexagon. – Machined from Aluminum 6061 T-651 and 0.25” thick

Structure

Page 25: SAGAN Final JPL Presentation

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Summary

Structure

• Optimal mass reducing design is an isogrid design– Array of equilateral triangles to increase structural

performance

– 75% mass reduction for equivalent flat plate

– 24 #10-32 holes for bolting instruments to the structure

Page 26: SAGAN Final JPL Presentation

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Summary

Overall CAD

10 m2.5 m

10 m

0.45 m

0.9

m

0.9

9 m

Page 27: SAGAN Final JPL Presentation

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Summary

Science Instruments

Science Payload

FieldsEnergetic Particles

Potential Control

Page 28: SAGAN Final JPL Presentation

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Systems

Engineering

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Management

Summary

Science Instrument – Fields Group

Electric Fields and Waves (EFW):

• Measure electric field and density fluctuations • Four orthogonal booms carrying spherical sensors

deployed to 10 m in the spin plan

Spatio Temporal Analysis of Field Fluctuations (STAFF):

• Measures magnetic fluctuations up to 4 kHz• Four 2.5m long boom-mounted three axis search coil

magnetometers and two data-analysis packages

Digital Wave Processing (DWP): • Signal processing package responsible for coordinating

Fields operations and selecting operational modes (burst and nominal)

Page 29: SAGAN Final JPL Presentation

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Summary

Science Instrument – Energetic Particles

Plasma Electron & Current Experiment (PEACE):

• Measures the distribution function of the electrons in the energy range of 0.59 eV to 26.4 eV

Cluster Ion Spectrometer (CIS)• Ionic plasma spectrometry package containing a Hot

Ion Analyzer (HIA) and time-of-flight ion Composition and Distribution Function Analyzer (CODIF)

• CODIF measures the distributions of the major ions • HIA designed for ion-beam and solar-wind

measurements

Page 30: SAGAN Final JPL Presentation

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Summary

Science Instrument – Potential Control

Active Spacecraft Potential Control (ASPOC)

• Active charge neutralization device equipped with ion emitters of the liquid-metal ion-source type

• Mitigates effects of surface charging by active charge neutralization

Page 31: SAGAN Final JPL Presentation

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Summary

Telecommunications

• High science data acquisition rate

• Two ground station locations: Melbourne, Florida & Brisbane, Australia

IRIS Transponder V2 (NASA JPL)

– X-Band (Rx/Tx)

– Scalable RF Output Power

– Radiation Tolerant

– BPSK Modulation with Convolution R=1/4, K=7 & R.S. (255,223)

ViaSat X-Band Ground Station

– 5.4m reflector

– 31.5 dB Gain

– Automated X-Y tracking

– Multiple Spacecraft Per

Antenna (MSPA) capability

AntDevCo Medium Gain X-Band Patch Antenna

– 16.5 dB Gain

– 30° full beamwidth

Page 32: SAGAN Final JPL Presentation

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Summary

Attitude Determination and Control• Attitude knowledge (0.1°) requirement• High torque (0.11 Nm) & angular momentum (24 Nms)

requirement• Required Slew Rate & Angular Acceleration for a single ground

station pass

Page 33: SAGAN Final JPL Presentation

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Summary

Attitude Determination and Control

Page 34: SAGAN Final JPL Presentation

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Summary

Propulsion

• Driven from ΔV budget and science instrument design– Can’t have artificial electric fields present near the

measurement probe

• Aerojet Rocketdyne MPS-230– Modified to use AF-M315E “Green” Monopropellant

– 22 N primary thruster with four 1 N ADCS thrusters

Page 35: SAGAN Final JPL Presentation

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Guidance, Navigation, and Control

• GNSS Satellites used for precise inertial position and velocity for each satellite– Auto/cross-correlation measurement technique

– Collision Risk

NovAtel GPS-703-GGG

• High vibration variant available

• GPS, GLONASS, Galileo, BeiDousignal reception

NovAtel OEM 615

• L1/L2 precise point positioning (PPP) < 1.5 m

• Handles ionospheric effect through linear combination of L1 and L2 carrier phase

Page 36: SAGAN Final JPL Presentation

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Summary

Electrical Power System• Science, Comms, ADCS components drive large power demands

• Solar Incidence Angle varies for spinning spacecraft– Average projected area used (0.56 m2)

• Solar Aspect Angle within ±15°

Clyde Space FLEX EPSClyde Space Batteries• 6 X 30 Whr

batteries, sync with PDM board

• Built in heaters

MMA Body Mounted Solar Panels• 1 custom sized panel per face

on hexagonal structure

• Triple Junction, 28.3% efficiency

• Dimensions: 0.43 m X 0.7 m

• 92 W Peak Sunlight Power

Page 37: SAGAN Final JPL Presentation

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Summary

C&DH and FSW• Proton 200k DSP Processor Board

– 2 flight computers in cold-string configuration

• NASA core Flight System (cFS) Application Suite

Page 38: SAGAN Final JPL Presentation

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Summary

Thermal

Low (°C) High (°C)

ASPOC -25 65

EFW -60 100

STAFF -60 100

DWP -55 150

CIS -20 40

PEACE -40 85

IRIS Transponder V2 -25 75

AntDevCo X-Band MGA -40 70

RSI 45 Reaction Wheels -20 65

BCT FleXcore with IMU -40 85

BCT Nano Star Tracker -40 70

Adcole Mini Spinning Sun Sensor -40 70

Rocketdyne MPS-230 -22 50

Propellant Tank -40 80

NovAtel OEM615 Reciever -40 85

NovAtel GPS-703-GGG Antenna -40 85

C&DH Proton 200k Lite Processor Board -20 40

Clyde Space FLEX EPS -40 85

CS 30 Whr Battery -10 50

MMA Body Mounted Solar Panels -100 150

Overall Thermal Range -10 40

EPS

Telecom

Operating Thermal RangeComponent NameSubsystem

Science Payload

Propulsion

ADCS

GNC

Aluminum paint coatingAbsorptivity = 0.4Emissivity = 0.53

Page 39: SAGAN Final JPL Presentation

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Summary

CAD – Exploded View

Page 40: SAGAN Final JPL Presentation

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Master Equipment ListSubsystem Component Name Quantity

CBE Mass

(kg)TRL Contingency

MEV

Mass (kg)

Subsystem

MEV Mass

(kg)

ASPOC 1 1.85 6 25% 2.31

EFW 1 3.16 6 25% 3.95

STAFF 1 3.03 6 25% 3.79

DWP 1 2.05 6 25% 2.56

CIS 1 10.79 6 25% 13.49

PEACE 1 5.49 6 25% 6.86

Custom Hexagonal Structure 1 48.24 7 20% 57.89

Side Body Radiation Shielding 6 0.81 7 20% 5.85

Top/Bottom Radiation Shielding 2 1.33 7 20% 3.19

IRIS Transponder V2 1 1.10 7 20% 1.32

AntDevCo X-Band MGA 1 0.30 8 10% 0.33

RSI 45 Reaction Wheels 2 7.70 7 20% 18.48

BCT Nano Star Tracker 2 0.35 8 10% 0.77

BCT FleXcore with IMUs 1 0.85 7 20% 1.02

Adcole Mini Spinning Sun Sensor 1 0.25 7 20% 0.30

NovAtel OEM615 Reciever 1 0.02 8 10% 0.03

NovAtel GPS-703-GGG Antenna 1 0.50 8 10% 0.55

Rocketdyne MPS-230 1 0.40 6 25% 0.50

Propellant Tank 1 1.00 6 25% 1.25

Thermal Bright Aluminum Paint 1 4.88 8 15% 5.61 5.61

C&DH Proton 200k DSP Processor Board 2 0.20 7 20% 0.48 0.48

Clyde Space 3G FLEX EPS 1 0.17 7 20% 0.21

CS 30 Whr Battery 6 0.26 8 10% 1.72

MMA Body Mounted Solar Panels 6 1.50 6 25% 11.25

143.7

8.39

300

152.1

97%

32.96

1.65

1.75

13.17

0.58

66.93

20.57

Science

Payload

Telecom

Propulsion

EPS

GNC

Structures

ADCS

MEV Dry Mass (kg)

Propellent Mass (kg)

MPV Mass (kg)

MEV Wet Mass (kg)

Margin (%)

MEV Wet Mass152.1 kg

Margin97%

Page 41: SAGAN Final JPL Presentation

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Summary

Subsystem Component Quantity ContingencyCBE Power

Draw (W)

Duty

Cycle

CBE Power

Draw (W)

Duty

Cycle

CBE Power

Draw (W)

Duty

Cycle

CBE Power

Draw (A)

Duty

Cycle

ASPOC 1 15% 2.7 0 2.7 0 2.7 0 2.7 1

EFW 1 15% 3.7 0 3.7 0 3.7 0 3.7 1

STAFF 1 15% 2.96 0 2.96 0 2.96 0 2.96 1

DWP 1 15% 1.41 0 1.41 0 1.41 0 1.41 1

CIS 1 15% 10.64 0 10.64 0 10.64 0 10.64 1

PEACE 1 15% 8.457 0 8.457 0 8.457 0 8.457 1

IRIS Transponder V2 1 15% 17 0.2 17 1 17 1 17 0.01

AntDevCo X-Band MGA 1 15% 10 0.2 10 1 10 1 10 0.01

RSI 45 Reaction Wheels 2 15% 7 0.5 7 0 9 1 7 0

BCT Nano Star Tracker 2 10% 1.2 1 1.2 1 1.2 1 1.2 1

BCT FleXcore with IMU 1 10% 1.05 1 1.05 1 1.05 1 1.05 1

Adcole Mini Spinning Sun Sensor 1 10% 0.5 1 0.5 1 0.5 1 0.5 1

NovAtel OEM615 Reciever 1 10% 1.2 0.5 1.2 1 1.2 1 1.2 1

NovAtel GPS-703-GGG Antenna 1 10% 0.648 0.5 0.648 1 0.648 1 0.648 1

Propulsion Rocketdyne MPS-230 1 20% 28 0 28 1 28 0 28 0

C&DH Proton 200k DSP Processor Board 1 10% 2.3 1 2.3 1 2.3 1 2.3 1

CS 3G FLEX EPS 1 10% 0.5 1 0.5 1 0.5 1 0.5 1

CS 30 Whr Battery 6 10% 0.05 1 0.05 1 0.05 1 0.05 1

10%10%

128% -30% 18%

57.7 57.7 57.7

25.3 81.9 48.9

57.7

67.7

-15%

10% 10%

Science Mode

Science

Payload

Communication

Mode

61.523.0 74.4 44.4

Telecom

EPS

Safe Mode Maneuver Mode

GNC

ADCS

Margin

System Level Contingency

MEV Power Consumption (W)

Orbit Average Power Production (W)

Total MEV Power Consumption

Power Budget

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Battery Analysis – Science ModeBattery Specs (Clyde Space 30Whr):• Quantity: 6• Capacity: 22.5 Ahr• Rated DoD: 30% = 5.25 Ahr

(tested for 5000 cycles, 35000 expected)

Results:

• 13% Battery Margin above DoD (0.65 Ahr)

• 33% Power Production Margin

• 11,000 cycles expected for 2 years

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Summary

Battery Analysis – Comms. Mode

Battery Specs (Clyde Space 30Whr):• Quantity: 6• Capacity: 22.5 Ahr• Rated DoD: 30% = 5.25 Ahr

Results:

• 16% Battery Margin above DoD (1.05 Ahr)

• Maneuver mode only during sunlight

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Summary

Thermal Energy Balance

• 1 Node Model

• Thermal Range between -10°C to 40°C

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Summary

Link BudgetItem Symbol Units Downlink Uplink

Frequency f GHz 8.45 8.45

Frequency f Hz 8.45E+09 8.45E+09

Transmitter Power (RF Output

Transmit Power)P Watts 4 20

Transmitter Power (RF Output

Transmit Power)P dBW 6 13

Transmitter Line Loss Ll dB -2 -2

Transmitter Antenna Gain Gt dBi 13.5 31.0

Equivalent Isotropic Radiated Power EIRP dBW 17.5 42.0

Propagation Path Length S m 1709926 1518364

Speed of Light c m/s 299792458 299792458

Free Space Path Loss Ls dB -175.6 -174.6

Propagation and Polarization Loss La dB -2 -2

Receive Antenna Pointing Loss Lpr dB -2 -2

Receive Antenna Gain Gr dBi 31.0 13.5

System Noise Temperature Ts K 300.0 80.0

System Noise Temperature Ts dBK 24.8 19.0

R bps 8346862 2000000

R kbps 8347 2000

R Mbps 8.35 2

Symbols per Byte - - 2 2

Eb/No Eb/No dB 6.5 26.5

Carrier-to-Noise Density Ratio C/No dB-Hz 72.7 86.5

Required Eb/No Req Eb/No dB 1.5 1.5

Implementation Loss - dB -1 -1

Margin - dB 4 24

Data Rate

Downlink8.35 Mbps

4 dB Margin

Uplink2 Mbps

24 dB Margin

Page 46: SAGAN Final JPL Presentation

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Management

Summary

Data Return Strategy• Strategy depended on high science data volume

• Average Downlink analysis performed via STK for 2 years for one satellite

• Overall Mission Operations Data Volume Analysis

Item Nominal Mode Burst Mode

Data Acquisition Time (min/orbit) 63.6 32.0

Data Volume (Mb/orbit) 46.64 190.2

Total Data Volume (Mb/orbit)

Science Data Volume Analysis

236.85

Avg # Passes per Day 14

Avg Pass Duration (minutes) 11.4

Average Gap Between Overpass (minutes) 91.6

Average Blackout period per day (hrs) 10

Downlink Data Volume Capability (Gb/orbit) 5.3

Downlink Data Volume Analysis

Number of Orbits Per Day 15

Mission Science Mode Percentage 93.5%

Science Mode Time Per 2 Weeks (days) 13

Mission Communication Mode Percentage 6.5%

Communication Mode Time Per 2 Weeks 1

Transmission Data Volume (Gb/2 weeks) 73

Science Data Volume (Gb/2 weeks) 46.7

Margin 56%

Mission Operations Data Volume Analysis

Page 47: SAGAN Final JPL Presentation

47

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Delta-V Budget

Maneuver Type Description ΔV (m/s) Margin Total ΔV (m/s)

Plane Change (0.2°) 26.477 25% 33.097

Max Phasing Burn (0.85°) 11.636 25% 14.545

Radial Impulse Burn 15.886 25% 19.858

Altitude Maintainence 550 km - 2 years 22.532 25% 28.165

Attitude ControlDesaturation of Reaction

Wheels - 2 years10.649 25% 13.311

De-Orbit Drag Deorbit 0.000 0% 0.000

108.975

10%

119.872Total ΔV (m/s):

Maneuvers to Achieve

Initial Orbit

Sum of ΔV (m/s):

Overall Margin:

• Plane Change: ΔV perpendicular to orbit plane

• Phasing Burn: Elliptical transfer into same orbit

• Radial Impulse Burn: Flight path angle adjustment

• Altitude Maintenance: Ballistic coefficient and orbital parameters give ΔV needed per orbit

Page 48: SAGAN Final JPL Presentation

48

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Management Outline

Page 49: SAGAN Final JPL Presentation

49

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Program Schedule

Key Milestones

Phase A: Mission &

Systems Definition

Phase B:

Preliminary Design

Phase C: Final

Design &

Fabrication

Phase D: System

Integration, Testing,

and Verification

Phase E: Operations

Phase F: Closeout

2023

Q1 Q2 Q3 Q4

2022

Q1 Q2 Q3 Q4

2021

Q1 Q2 Q3 Q4

Project

Phase2015 2016

Q4

2017 2018 2019

Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3

2020

Q1 Q2 Q3 Q4

SRR MDR PDR ARR MRRORRTRR PLAR CERR DR

SDR – System Requirements ReviewMDR – Mission Design ReviewPDR – Preliminary Design ReviewARR – Assembly Readiness ReviewTRR – Test Readiness Review

ORR – Operational Readiness ReviewMRR – Mission Readiness ReviewPLAR – Post Launch Assessment ReviewCERR – Critical Event Readiness ReviewDR – Decommissioning Review

Page 50: SAGAN Final JPL Presentation

50

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Risk Analysis

Consequence Qualitative Definition

1 Minimal or no impact to mission

2 Small reduction in mission return

3 Cannot meet full mission success

4 Cannot meet minimum mission requirements

5 Mission catastrophe

Likelihood Qualitative Definition Probablility Range

1 Very Low < 1%

2 Low 1-5%

3 Moderate 5-15%

4 High 15-30%

5 Very High > 30%

Page 51: SAGAN Final JPL Presentation

51

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Risk Analysis (cont.)

1 2 3 4 5

5

4D

3 D' C' C

2 B A

1 B' A'

Lik

elih

oo

d

Consequence

RiskUnmitigated

Likelihood

Unmitigated

ImpactHandling Method

ACollision of two or more

satellites while crossing orbits2 5

Higher fidelity GPS and development of

collision detection algorithm

BFailure to complete design by

launch date2 4

Increased time margins to schedule and

earlier testing of lower TRL components

C Failure of ADCS actuators 3 4 Additional propellant for ADCS thruster

Reliability and environment qualifications

testing early on in Phase C

Redundancy of internal mechanisms

4 4DFailure of boom deployment

mechanism

Page 52: SAGAN Final JPL Presentation

52

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Cost Estimation Approach

• Parametric Cost Estimation– Small Satellite Spacecraft Model (SSCM)

• Accounts for both recurring and non-recurring costs

• Bottom-Up Method– Exact cost values for hardware used

– More specific to our mission

• 4 flight unit + 1 engineering unit

– Can better account for development costs for science instruments

Page 53: SAGAN Final JPL Presentation

53

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Cost Analysis – Bottom Up WBS Element Quantity Years Cost ($k)

Component

Margin (%)Final Cost ($k)

Total Hardware Cost 1 - 1,052.10$ Included 1,052.10$

IA&T N/A - 100.00$ 25% 125.00$

Total Hardware Cost 4 - 7,963.06$ Included 7,963.06$

IA&T N/A - 600.00$ 25% 600.00$

ASPOC 4 - 2,845.80$ Included 2,845.80$ EFW

STAFF

DWP 4 - 500.00$ Included 500.00$ CIS 4 - 865.00$ Included 865.00$

PEACE 4 - 875.00$ Included 875.00$ Development and IA&T 4 - 8,000.00$ 25% 10,000.00$

Principal Investigator 1 8.5 4,250.00$ 10% 4,675.00$

Mission Design Engineer 16 5 16,000.00$ 10% 17,600.00$

Mission Ops. Engineer 8 2 2,880.00$ 10% 3,168.00$

Ground Support Engineer 3 2.5 1,500.00$ 10% 1,650.00$

Science Personnel 5 8.5 6,375.00$ 10% 7,012.50$

Management 2 8 2,400.00$ 10% 2,640.00$

Launch Opportunity 1 - 6,250.00$ 10% 6,875.00$

Ground Support Equipment 2 - 2,000.00$ 25% 2,500.00$

72,997.35$

25%

91,246.69$

91,246,692.23$

-

Program Level

Flight Support

Cost ($K)

System Margin

Ground Equipment

Total Cost ($K)

Total Cost ($)

2,025.00$ Included 2,025.00$ 4

Spacecraft - Engineering Unit

Science Payload

Spacecraft - Flight Unit

Total Cost

$91,246,692.23

Page 54: SAGAN Final JPL Presentation

54

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Descope Options

• Option #1: Replace EFW and STAFF- Lower spatial and temporal resolution

- Hinder observing extrema of range of physical phenomenon

+ Development cost savings of roughly $2.5 million

+ Improves margin for science instrument development

• Option #2: Move from X-band to S-band transmission- Lower downlink rate implies longer downlink time

- Decreased time spent in science mode

+ Cost savings in purchase and maintenance of ground station

+ Relaxes ADCS slew requirements due to greater beam width

Page 55: SAGAN Final JPL Presentation

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

55

Conclusion

• SAGAN mission will help answer fundamental science questions deemed relevant by the RFP

• Highest spatial/temporal resolution of near Earth plasma ever attempted

• Suite of instruments and subsystem design fully closes the mission design outlined by the requirements

• Within cost cap of typical NASA Small Satellite Mission– ~$92 million cost (36% less)

55

Page 56: SAGAN Final JPL Presentation

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

56

Acknowledgements• Dr. Glenn Lightsey – Professor of Aerospace Engineering

• Terry Stevenson – Graduate Teaching Assistant

• Jason Swenson – Graduate Teaching Assistant

• Dr. Carol Paty – Professor of Earth and Atmospheric Sciences

• Dr. Sara Spangelo – Systems Engineer, JPL

• Dr. Morris Cohen – Professor of Electrical and Computer Engineering

56

Page 57: SAGAN Final JPL Presentation

“Somewhere, something incredible is waiting to be known.”

-Carl Sagan

Page 58: SAGAN Final JPL Presentation

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Background – Atmospheric Waves

• Atmospheric waves are global-scale waves – Excited by regular solar differential heating (solar thermal tides)

– The gravitational tidal force of the moon (gravitational tides)

– Neutral forcing.

58

Altitude-Latitude structure of electron density (in MHz) due to TW3 type tidal waves

Page 59: SAGAN Final JPL Presentation

Motivation/

Background

Mission

Overview

Flight System

Systems

Engineering

Program

Management

Summary

Background – Ionospheric Storms• Ionospheric Storms: Disturbances due to solar activity, when

affecting the ionosphere, are ionospheric storms– Tend to generate large disturbances in ionospheric density distribution,

total electron content, and the ionospheric current system

59Image Credit: Chapagain, Narayan P. "Dynamics of equatorial spread F using ground-based optical and radar measurements." (2011).

Measurement of the ionosphere's total electron content (TEC) using GPS Mapping

Page 60: SAGAN Final JPL Presentation

MMS Mission

• Studying magnetic field turbulence measurements at the bow shock

• Studying magnetic reconnection

• Highly elliptical orbit at ~10 earth radii away

• 4 satellites are a measurement technique for spatial and temporal autocorrelation

12/4/2015 60

Page 61: SAGAN Final JPL Presentation

Level 1 RequirementsMDR Mission Design Requirements Source Verification

MDR - 1 The mission duration shall last at least 6 months with a goal of 24 months in the initial orbit MO - 3 Inspection

MDR - 2Satellites #1 and #2 must be placed in the reference orbit (circular, 550 km altitude, 30° inclination,),

phased 0.85° degrees apartMO - 1 Analysis

MDR - 3Satellite #3 must be eccentric to the reference orbit such that it maintains the same period as Satellite #1

with altitude at perigee of 535 km, altitude at apogee of 565 km, and phased 0.42° from Satellite #1MO - 1 Analysis

MDR - 4

Satellite #4 must be positively inclined to the reference constellation orbit by 0.2 degrees and eccentric to

the reference orbit such that it maintains the same period as Satellite #1 with altitude at perigee of 535 km,

altitude at apogee of 565 km, and phased 0.60° from Satellite #1

MO - 1 Analysis

MDR - 5Once in tetrahedron formation, each satellite shall maintain the orbital parameters of period, eccentricity,

inclination, and phase from Satellite #1 for the duration of the missionMO - 3 Analysis

MDR - 6 End of life drag deorbit plan must be initiated in order to meet the 25 year deorbit plan set forth by NASA MO - 2 Analysis

FSR Flight System Requirements Source Verification

FSR - 1 Each satellite must be able to withstand the launch vehicle environment MO - 1 Analysis

FSR - 2 Each satellite must be able to survive during operations in space for mission duration MO - 3 Testing

FSR - 3Each satellite must maintain spacecraft attitude relative to other satellites and maintain correct orbital

parameters for the tetrahedron formationMO - 2 Analysis

FSR - 4 Each satellite must have the ability to store and relay payload and state data back to ground station MO - 3 Testing

Page 62: SAGAN Final JPL Presentation

Level 1 Requirements (cont.)SPR Science Payload Requirements Source Verification

SPR - 1The science payload must cover a wide range of energies, from spacecraft potential to 40 keV/e for ion

spectroscopy measurementsMO - 3 Testing

SPR - 2The science payload shall measure a wide dynamic range in energy coverage from spacecraft potential to

40 keV/e.MO - 3 Testing

SPR - 3The science payload must measure electric-field in the frequency range of 50–8000 Hz and amplitude range

10 mV m-1

to 1 V m-1

.MO - 3 Testing

SPR - 4 The science payload shall measure with a time resolution of 1.10E-5 s. MO - 3 Testing

SPR - 5The science payload must measure three-dimensional velocity distribution of electrons in the energy range

from 0.59 eV to 26.4 keVMO - 3 Testing

SPR - 6 The science payload must measure three-axis magnetic fluctuations up to 4 kHz MO - 3 Testing

SPR - 7 The science payload must maintain electromagnetic cleanliness for the duration of the mission MO - 3 Testing

SPR - 8 The science payload must actively maintain ground potential for optimum measurments MO - 3 Testing

GSR Ground System Requirements Source Verification

GSR - 1 The ground system shall downlink science data and telemetry from all satellites with a margin of atleast 2 dB MO - 3 Testing

GSR - 2 The ground system must uplink commands to all satellites with a margin of atleast 15 dB MO - 3 Testing

GSR - 3 The ground system shall comprehensively archive all data received MO - 3 Testing

GSR - 4The mission personnel must perform all necessary mission operations for the lifetime of the mission and

transfer all science data to science personnelMO - 3 Testing

Page 63: SAGAN Final JPL Presentation

Level 2 RequirementsADCS ADCS Requirements Source Verification

ADCS - 1ADCS maintain spin stabilization in inertial space during all modes of

operation FSR - 2 Analysis

ADCS - 2ADCS shall be able to reorient the spacecraft within a full range of

motion for orbit insertion and maintenanceFSR - 3 Analysis

ADCS - 3ADCS shall maintain a solar aspect angle of 90 ± 15° during science

(nominal) mode for power acquisitionFSR - 2 Analysis

ADCS - 4

ADCS shall maintain a slew rate of at least 0.74°/s with

a ±15° transverse pointing accuracy for periods of at least 773 s in

order to relay data to the ground stations

FSR - 4 Analysis

ADCS - 5ADCS shall maintain a pointing knowledge of 0.1° for attitude

determination during science modeFSR - 3 Testing

ADCS - 6ADCS shall provide each satellite with a rotation rate of 3 rpm in

order to maintain electromagnetic cleanlinessSPR - 7 Analysis

ADCS - 7ADCS thrusters shall be capable of dumping additional momentum

(relative to the nominal spin rate) over the period of the missionFSR - 4 Analysis

ADCS - 8ADCS shall reorient spacecraft during the end of life operations to

deorbit within 25 yearsMDR - 6 Analysis

TCS Thermal Control System Requirements Source Verification

TCS - 2TCS must maintain a temperature range between -10° C and 40° C

at all times bfore and after deployment from launch vehicleFSR - 2 Analysis

Page 64: SAGAN Final JPL Presentation

Level 2 Requirements (cont.)

CDH Command & Data Handling Requirements Source Verification

CDH - 1C&DH shall be able to process spacecraft telemetry at a minimum

rate of 5 HzFSR - 4 Testing

CDH - 2 C&DH shall handle subsystem control at a minimum rate of 10 Hz FSR - 2 Testing

CDH - 3C&DH shall store at least 240 Mb of data per orbit and at least 215

orbits worth of dataFSR - 4 Testing

CDH - 5 C&DH shall provide data interfaces for each subsystem FSR - 4 Testing

EPS Electrical Power System Requirements Source Verification

EPS - 1EPS shall provide 25.3 Watts to the spacecraft bus and 0 Watts to

the payload during safe modeFSR - 2 Testing

EPS - 2EPS shall provide 14.63 Watts to the spacecraft bus and 34.6

Watts to the payload during science modeFSR - 2 Testing

EPS - 3EPS shall provide 67.7 Watts to the spacecraft bus and 0 Watts to

the payload during communications modeFSR - 2 Testing

EPS - 4EPS shall provide 81.9 Watts to the spacecraft bus and 0 Watts to

the payload during thrust modeFSR - 2 Testing

EPS - 6EPS shall store 22.5 Amp-Hrs of electrical power during mission

lifetimeFSR - 2 Testing/Analysis

Page 65: SAGAN Final JPL Presentation

Level 2 Requirements (cont.)PROP Propulsion System Requirements Source Verification

PROP - 1Propulsion must provide 34 m/s of ΔV in order to achieve a 0.2°

plane changeMDR - 2 Testing

PROP - 2Propulsion must provide 20 m/s of ΔV in order to create the desired

eccentric orbit of 535 km by 565 km altitudeMDR - 2 Testing

PROP - 3Propulsion must provide 29 m/s of total ΔV over 24 months to

perform station keepingMDR - 2 Testing

PROP - 4Propulsion must provide 15 m/s of total ΔV per satellite in order to

perform phasing maneuversMDR - 2 Testing

PROP - 5Propulsion must provide 14 m/s of total ΔV per satellite in order to

desaturate the reaction wheelsMDR - 2 Testing

COMMS Communication Systems Requirements Source Verification

COMMS - 1Comms shall uplink at a minimum rate of 2 Mbps per orbit with a 24

dB margin to ground stationGSR - 2 Testing

COMMS - 2Comms shall downlink all data captured in 197 within 14 ground

station passes with a 4 dB marginGSR - 1 Testing

COMMS - 3Comms shall allow uplink and downlink occur only to the assigned

ground stationsFSR - 4 Analysis

Page 66: SAGAN Final JPL Presentation

Level 2 Requirements (cont.)STRUCT Structures Requirements Source Verification

STRUCT - 1 The volume of each satellite must be under 1 m3 FSR - 1 Inspection

STRUCT - 2 The mass of each satellite must be under 300 kg FSR - 1 Inspection

STRUCT - 3Structure must survive a dynamic load equivalent to 4.55 g's during

launchFSR - 1 Analysis

STRUCT - 4Structure must be stiff enough to survive a 20-45Hz oscillation along

all axis with a safety factor of 11 during launchFSR - 1 Analysis

STRUCT-5 Structure must facilitate body mounted solar arrays FSR-2 Analysis

STRUCT - 6Structure must be able to maintain internal temperature and radiation

levels up to 1 kRad at all time.FSR - 2 Analysis

STRUCT - 7The shape of the structure must be optimized to maximize projected

area for solar energy and internal volume within the volume FSR - 2 Analysis

GNC Guidance, Navigation, and Control Requirements Source Verification

GNC - 1GNC shall acquire intertial position vectors within a 1.2 m precision

for formation flyingFSR - 3 Analysis

GNC - 2GNC shall acquire intertial velocity vectors within a 10 m/s precision

for formation flyingFSR - 3 Analysis

GNC - 3GNC shall maintain the commanded orbit track of each satellite with

an absolute position error of no more than 1 km MDR - 3 Analysis

Page 67: SAGAN Final JPL Presentation

ADCS – Slew Phasing

12/4/2015 67

Page 68: SAGAN Final JPL Presentation

Work Breakdown Structure

Page 69: SAGAN Final JPL Presentation

Cost Estimation (MEL)

Subsystem Component Name Quantity TRL Cost FY'15 ($)Contingency

(%)

Component Cost

($)

Subsystem Cost

($)

ASPOC 1 6 569,160.00$ 25% 711,450.00$

EFW 1 6

STAFF 1 6

DWP 1 6 100,000.00$ 25% 125,000.00$

CIS 1 6 173,000.00$ 25% 216,250.00$

PEACE 1 6 175,000.00$ 25% 218,750.00$

Custom Hexagonal Structure 1 7 7,650.00$ 20% 9,180.00$

Side Body Radiation Shielding 6 7 3,750.00$ 20% 4,500.00$

Top/Bottom Radiation Shielding 2 7 1,250.00$ 20% 1,500.00$

IRIS Transponder V2 1 7 250,000.00$ 20% 300,000.00$

AntDevCo X-Band MGA 1 8 36,000.00$ 10% 39,600.00$

RSI 45 Reaction Wheels 2 7 168,000.00$ 20% 201,600.00$

BCT Nano Star Tracker 2 8 136,000.00$ 10% 149,600.00$

BCT FleXcore 1 7 110,000.00$ 20% 132,000.00$

Adcole Mini Spinning Sun Sensor 1 7 15,000.00$ 20% 18,000.00$

NovAtel OEM617 Reciever 1 8 2,775.62$ 10% 3,053.18$

NovAtel GPS-703-GGG Antenna 1 8 1,595.00$ 10% 1,754.50$

Rocketdyne MPS-230 1 6

Propellant Tank 1 6

Propellant (AF-M315E) 1 6 3,500.00$ 25% 4,375.00$

C&DH Proton 200k Lite Processor Board 1 7 75,000.00$ 20% 90,000.00$ 90,000.00$

Clyde Space 3G FLEX EPS 1 7 13,500.00$ 20% 16,200.00$

CS 30 Whr Battery 3 8 5,400.00$ 10% 5,940.00$

MMA Body Mounted Solar 6 6 436,677.96$ 25% 545,847.45$

Thermal Bright Aluminum Paint 4 8 94,148.00$ 10% 103,562.80$ 103,562.80$

Total Cost: 3,846,137.93$

Structures

ADCS

15,180.00$

501,200.00$

EPS

Propulsion353,380.00$

Telecom

GNC

Science

Payload

405,000.00$

567,987.45$

25%

25%

506,250.00$

441,725.00$

1,777,700.00$

339,600.00$

4,807.68$

446,100.00$

Page 70: SAGAN Final JPL Presentation

Cost Estimation (Parametric - SSCM)WBS Element Driver - Subsystem Mass (kg) Cost ($k)

Structures 66.93 5,837.06$

Telecom 1.65 595.12$

ADCS & GNC 21.15 6,994.21$

Propulsion 1.75 95.08$

C&DH 0.48 685.84$

EPS 13.17 4,709.98$

Thermal 5.61 514.39$

WBS Element Driver - S/C Bus Cost ($K) Cost ($k)

Science Instruments 77,726.69$ 31,090.68$

Integration, Assembly & Test 19,431.67$ 2,701.00$

Program Level 19,431.67$ 4,449.85$

Launch & Orbital Operations 19,431.67$ 1,185.33$

Ground Support Equipment 19,431.67$ 1,282.49$

Total Cost - 1 Satellite ($K) 36,823.02$

Total Cost - 1 Satellite ($) 36,823,021.58$

Total Cost - 4 Satellites($K) 118,436.05$

Total Cost - 4 Satellites ($) 118,436,050.95$

Spacecraft

Payload

Ground Equipment

Flight Support

Program Level

Spacecraft Integration, Assembly, and Test

Page 71: SAGAN Final JPL Presentation

Cost Phasing

12/4/2015 71

Page 72: SAGAN Final JPL Presentation

Propulsion Trade Study

12/4/2015 72

Specifications Weight AR MR-111C AR MPS-230 Airbus S10 AR R-6D

Propellant Type - Mono Mono Bi Bi

Dry Mass of Thruster 1 S - - -

Propellant Toxicity 2 S + S S

Isp 3 S + + +

Nominal Thrust 3 S + + +

Propellant Mass Required for ΔV 3 S + + +

Power Requirement 2 S - - S

Attitude Control Thrusters 3 S + - -

TRL Level 2 S - S S

Total + 14 9 9

Total - 5 6 4

Total S 0 4 6

Page 73: SAGAN Final JPL Presentation

Drag Calculations

Page 74: SAGAN Final JPL Presentation

Data Return Strategy – STK Ground Pass

12/4/2015 74

Page 75: SAGAN Final JPL Presentation

Data Return Strategy – STK Ground Pass

Access # Access Start (UTCG) Access End (UTCG) Duration (sec) Asset Full Name Data Volume (Gb)

428 2/1/21 7:10 2/1/21 7:21 666 Brisbane 5.56

429 2/1/21 8:50 2/1/21 9:03 772 Brisbane 6.44

430 2/1/21 9:32 2/1/21 9:38 339 Melbourne 2.83

431 2/1/21 10:31 2/1/21 10:44 780 Brisbane 6.51

432 2/1/21 11:10 2/1/21 11:22 704 Melbourne 5.88

433 2/1/21 12:13 2/1/21 12:26 779 Brisbane 6.50

434 2/1/21 12:51 2/1/21 13:04 777 Melbourne 6.49

435 2/1/21 13:55 2/1/21 14:07 775 Brisbane 6.47

436 2/1/21 14:32 2/1/21 14:45 780 Melbourne 6.51

437 2/1/21 15:36 2/1/21 15:48 684 Brisbane 5.71

438 2/1/21 16:14 2/1/21 16:27 781 Melbourne 6.52

439 2/1/21 17:21 2/1/21 17:25 185 Brisbane 1.55

440 2/1/21 17:55 2/1/21 18:08 761 Melbourne 6.35

441 2/1/21 19:37 2/1/21 19:48 612 Melbourne 5.11

78.4Total Data Volume (Gb):

12/4/2015 75

Page 76: SAGAN Final JPL Presentation

Solar Panel Sizing

Pe (W) 46

Pd (W) 91.9

Max Eclipse % 31.3%

Max Sunlight % 68.7%

Te (s) 2170.75

Td (s) 4757.35

Xe 0.6

Xd 0.8

Psa (W) 160.35

Mean Solar Flux (W/m2) 1370

Solar Cell Efficiency (%) 28.30%

Po (W/m2) 387.71

Id 0.77

θ 15

PBOL (W/m2) 288.36

PEOL (W/m2) 285.49

Area - Sollar Array (m2) 0.5617

Solar Area Sizing

Base Edge (m) 0.43

Height (m) 0.7

Best Case Projected Area (m2) 0.602

Worst Case Projected Area (m2) 0.5213

Avg Projected Area (m2) 0.5617

Minimum Solar Panel Face Sizing

12/4/2015 76