Solar Probe Plus FIELDS Quarterly Management July 18, 2013.
-
Upload
owen-pierce -
Category
Documents
-
view
217 -
download
3
Transcript of Solar Probe Plus FIELDS Quarterly Management July 18, 2013.
Solar Probe Plus FIELDS
Quarterly Management
July 18, 2013
• Project Overview• Project Organization• Spacecraft Accommodation/Instrument Suite Measurements• Technical Status• Special Topics: Antenna TRL 6 Status, Frequency Plan• Project Schedule• Project Risk (Summary; Detail Description of any New, Yellow, or
Red Risks; UFE threats/liens)• Total Cumulative Project Cost• Project Labor: Prime and Major Subs• Subcontractor Summary• Issues and Concerns• Lunch
QUARTERLY MGMT AGENDA
FIELDS OverviewObservations• Measure electric and magnetic fields and waves• Measure pointing flux, absolute plasma density and electron
temperature, S/C floating potential and density fluctuations, and radio emissions
Measurements• Magnetic field vectors DC-64kHz• Electric field vectors DC-1MHz• Plasma waves 5Hz to 1MHz• Quasi-thermal Noise 10 kHz to 2.5MHz• Radio emissions 1MHz to 20 MHz
3
UCB Electric Field Antenna
LPC2E Search-Coil Magnetometer (SCM)
GSFC Fluxgate Magnetometer (MAG)
Project Status Update• System Reliability Redesign Complete• Internal ICD Drafts Complete
Funding• Definitized Contract Value: $13.65
M• Definitized Funding Value (mod 17): $ 7.56
M• Unallocated Future Expense : $ 0.61
M• End Date:
3/14/2014• Current EAC: $13.65
M
Milestones (Phase B) FIELDS Specification Dev (L2) Oct, 2012 MEP Specification Dev (L3) Jan, 2013• DCB & AEB Detailed Dsn Sep 2013• RFS Detailed Dsn Oct 2013• FPGA Reviews Oct 2013• IPDR Nov 19,
2013
FIELDS Organization
FIELDS PIStuart Bale
Advisors
SAG: A. Balogh, J.-L.Bougeret, P.J. Kellogg, F.S. Mozer
FIELDSScience Team
FIELDS PM
P. Harvey
Finances
M. Willer
Electrical
K. Goetz
SMA
J. Fischer
Scheduling
D. Meilhan
Antennas
D. Glaser
AEBJ. BonnellS. Heavner
DCB/RFS
M. PulupaD. Gordon
D. Seitz
TDS/LNPS
K. Goetz
DFB
R. Ergun
MAG
R. MacDowall
SCMV.
Krasnosselskikh
UCB
LASP
UMN
GSFC
LPC2E
VariousFIELDS DPM
L. Hayes
Preamps
D. Seitz
Mechanical
P. Turin
MEP
W. Donakowski
Thermal
M. D. Aguado
Parts
A. Le
FIELDS Overview
5
Electric Field Antennas
2.3 m Tip-to-Hinge
Preamps located at Hinge
Mag Boom
MAG (Inboard)
MAG (Outboard)
SCM
Main Electronics
Package (MEP)
Main Electronics Package (2 parts):• Data Controller Board (DCB) – UCB• Radio Frequency Spectrometer (RFS) - UCB• Time Domain Sampler (TDS) - UMinn• Digital Fields Board (DFB) - LASP• 2 Antenna Electronics Boards (AEB) – UCB• 2 MAG Electronics Boards (MAG) – GSFC• 2 Low Noise Power Supplies (LNPS) - UMinn
*: SCM at end of boom
*
V5
6
System Redesign
Time Domain Sampler(TDS)
Digital Fields Board(DFB)
Magnetom
eter Electronics
AntennaElectronics
Board(AEB1)Data Control
Board(DCB)
Low Noise Power Supply
(LNPS2)
P3x26
P3x67
P3x66
P3x13
P3x45
P3x44
P3x63
P3x11
P3x42
P3x32
P3x27
P3x64
P3x83
Radio Frequency
Spectrometer (RFS)
P3x12
Magnetom
eter Electronics
P3x73P3x71
P3x72
P3x31
P3x41
P3x22
Low Noise Power Supply
(LNPS1)
P3x04
P3x03
P3x02
P3x01
P3x23
Antenna Electronics
Board(AEB2)
P3x54
P3x53
P3x56
P3x52
P3x51
P3x57
P3x58
P3x38
P3x37
P3x36
P3x34
P3x33
P3x35
P3x43
P3x65
V1
V2
V3
V4
PA1 PA4PA3PA2
E-Field Antennas
P8w01
P8x01
P8y01
P8z01
MAGo MAGi
SCM MAGi
Inboard
MAGo
Outboard
Mag Boom SensorsV5
PA5
P0w01P0x02
P0y01
P0z01
P0x01
P3x81
P3x62
P3x61
P3x82
Side 1 Side 2
S/C C&DHSide-ASide-B
S/C Op. PowerSurv. Power
S/C sampled temps.
S/C C&DHSide-ASide-B
S/C Op. PowerSurv. Power
S/C sampled temps.
SWEAPInterface
P3x24
P3x21
SSL / Berkeley
U. Minnesota
LASP / Colorado
GSFC / NASA
LPC2E / CNES
0 1 2 3 4 5 6 7 8
S/C Bulkhead Conn. S/C Bulkhead Conn.
3.2m
7
System RedesignMEP Stack Up• Side 1
– LNPS1– MAGo (Outboard)– DCB/RFS– AEB1– DFB
• Side 2– AEB2– TDS– MAGi (Inboard)– LNPS2
• Every other slice is bolted to S/C Panel (June meeting AI)
8
MassFIELDs Mass Tracking Report Feb 13 2013 Jun 30 2013
FIELDS Instrument Suite # FLIGHT HARDWARE MASS FLIGHT HARDWARE MASS
Subsystem/Component
Flight Units
Unit Mass,
kg(CBE)
Total Mass,
kgCBE
Contin-gency %
Total Mass w/Contingency
Unit Mass,
kg(CBE)
Total Mass,
kgCBE
Contin-gency %
NTEMass(kg)
5.1 PWI Instrument5.1.1 Main Electronics Package (MEP)
Data Control Bd. (DCB) 1 0.495 0.495 20% 0.594 0.495 0.495 20% 0.594Radio Freq. Spec. (RFS) 1 0.100 0.100 20% 0.120 0.100 0.100 20% 0.120Time Dom. Samp. (TDS) 1 0.335 0.335 20% 0.402 0.335 0.335 20% 0.402Dig. Fields Bd. (DFB) 1 0.437 0.437 20% 0.524 0.437 0.437 20% 0.524Ant. Elec. Bd. (AEB1) 1 0.362 0.362 20% 0.434 0.362 0.362 20% 0.434Ant. Elec. Bd. (AEB2) 1 0.362 0.362 20% 0.434Chassis 1 3.054 3.054 20% 3.665 3.517 3.517 20% 4.237Low Noise P.S. (LNPS1) 1 0.475 0.475 25% 0.594 0.475 0.475 25% 0.594Low Noise P.S. (LNPS2) 1 0.475 0.475 25% 0.594HarnessesMEP B/P Harness 1 0.229 0.229 20% 0.275 0.229 0.229 20% 0.275Harness to SWEAP 1 0.065 0.065 20% 0.078 0.101 0.101 -23% 0.078
5.1.2 E-Field SensorsE-Field Preamps (V1-V4) 4 0.126 0.504 20% 0.605 0.126 0.504 20% 0.605Electric Field Antennas 4 0.440 1.760 20% 2.112 0.440 1.760 20% 2.112E-Field 3rd axis (V5) 1 0.058 0.058 20% 0.070 0.058 0.058 20% 0.070Antenna Whip brackets 4 0.059 0.236 20% 0.283 0.059 0.236 20% 0.283Antenna Mounting blocks 4 0.125 0.500 25% 0.625 0.125 0.500 25% 0.625E-Field Preamp Harness 4 0.296 1.183 20% 1.419 0.327 1.309 8% 1.419E-Field 3rd axis harness 1 0.184 0.184 20% 0.221 0.184 0.184 20% 0.221Preamp Blanket/Heater 4 0.045 0.180 20% 0.216 0.045 0.180 20% 0.216Antenna Actuator Harness 4 0.209 0.834 20% 1.001 0.209 0.836 20% 1.001
5.1.3 Search Coil MagnetometerSCM Sensor 1 0.520 0.520 15% 0.598 0.520 0.520 15% 0.598SCM Harness 1 0.377 0.377 15% 0.433 0.377 0.377 15% 0.433SCM Blanket/Heater 1 0.160 0.160 15% 0.184 0.160 0.160 15% 0.184
5.2 MAG InstrumentMAG Electronics (in MEP) 2 0.381 0.761 15% 0.875 0.381 0.761 15% 0.875MAG Sensor Head 2 0.385 0.770 15% 0.886 0.385 0.770 15% 0.886MAG Harness 2 0.256 0.511 15% 0.588 0.256 0.511 15% 0.588MAG Blankets/Heater 2 0.050 0.100 20% 0.120 0.050 0.100 20% 0.120
FIELDS TOTAL 14.19 19.3% 16.92 15.65 18.3% 18.52
MEP (excl. Harness) 6.02 7.21 7.55 9.08
MASS Tracking
System Redesign– Two AEB’s– Two LNPS’s– TDS w/ SC I/F
2/27/2013 NTE set by APL, see table to right3/5/2013 Start showing Mag boom mass
4/25/2013 Update with backshells on harnesses4/25/2013 Remove mag boom mass5/31/2013 Add redundancy elements5/31/2013 Contingency column becomes NTE5/31/2013 Remove backshells until lien is authorized5/31/2013 Updated preamp harness length, SWEAP harness
9
PowerFIELDs Power Tracking Report Jan 28 2013 Jun 30 2013
FIELDS Instrument Suite # FLIGHT HARDWARE POWER FLIGHT HARDWARE POWER
Subsystem/Component
Flight Units
Total Power,
WCBE
Contin-gency %
Total Power
w/Conting
ency
Total Power,
WCBE
Contin-gency %
NTEPower(W)
5.1 PWI Instrument5.1.1 Main Electronics Package (MEP)
Data Control Bd. (DCB) 1 1.79 20% 2.15 2.21 -1% 2.18Radio Freq. Spec. (RFS) 1 0.46 20% 0.55 0.49 14% 0.55Time Dom. Samp. (TDS) 1 1.70 20% 2.04 1.70 20% 2.04Dig. Fields Bd. (DFB) 1 1.80 20% 2.16 1.90 14% 2.16Ant. Elec. Bd. (AEB1) 1 1.42 15% 1.63 0.98 20% 1.17Ant. Elec. Bd. (AEB2) 1 0.72 20% 0.86Chassis 1Low Noise P.S. (LNPS1) 1 5.97 20% 7.16 4.00 20% 4.80Low Noise P.S. (LNPS2) 1 2.94 20% 3.53HarnessesMEP B/P Harness 1 0.00 0.00Harness to SWEAP 1 0.00 0.00
5.1.2 E-Field SensorsE-Field Preamps (V1-V4) 4 1.11 15% 1.28 1.11 15% 1.28Electric Field Antennas 4E-Field 3rd axis (V5) 1 0.12 15% 0.14 0.12 15% 0.14Antenna Whip brackets 4Antenna Mounting blocks 4E-Field Preamp Harness 4 0.00 0.00 0.00 0.00E-Field 3rd axis harness 1 0.00 0.00 0.00 0.00Preamp Blanket/Heater 4 0.00 0.00 0.15 0.00Antenna Actuator Harness 4 0.00 0.00 0.00 0.00
5.1.3 Search Coil MagnetometerSCM Sensor 1 0.29 10% 0.32 0.29 10% 0.32SCM Harness 1 0.00 0.00 0.00 0.00SCM Blanket/Heater 1 0.78 15% 0.90 0.78 15% 0.90
5.2 MAG InstrumentMAG Electronics (in MEP) 2 1.92 10% 2.11 1.92 10% 2.11MAG Sensor Head 2 0.00 10% 0.00 0.00 0.00MAG Harness 2 0.00 0.00 0.00 0.00MAG Blankets/Heater 2 1.85 15% 2.12 2.00 6% 2.12
FIELDS TOTAL 19.21 17.5% 22.56 21.30 13.4% 24.16
MEP total 15.06 17.81 16.85 19.40
Power Tracking
2/27/2013 NTE set by APL, see table to right3/4/2013 Add heater to 3rd axis, need at least .15W
3/21/2013 Remove +/-6VA from AEB, improves efficiency#3/21/2013 Change DCB, to use 4VA3/21/2013 Change MAG heater power to 0.7W, maintain 0degC5/8/2013 Change DFB from 1.8 to 1.9W5/8/2013 Make the Contingency column NTE, i.e. fix it.
5/31/2013 Add AEB2 and LNPS25/31/2013 Updated NTE, adding 1.6W to value 22.56W6/10/2013 updated DCB/RFS, see tab F1.LNPS
6/18/13 Compiled side 1 and side 2 power6/30/2013 Updated DCB, based on D. Gordon email
10
TRL6 Status
See : 130718 SPP Fields ANT TRL6 Review_w_Backup_Slides
11
Preamp / RFS Development• Preamp
– Parts selection completed– Dual input JFET will require qual and screening– SQPL JFETs are available in same package, as backup
plan (4x poorer noise performance– All other components are SQPL– Breadboard complete– Testing is under way
• RFS Analog Breadboard– Reconfigured analog chain– Breadboard design and layout completed– All components are SQPL
Preamp breadboard
RFS Analog breadboard
FPGA Daughter Board Development
• FPGA ETU Daughter board schematics and layout completed– This board houses the Actel/Microsemi reprogrammable FPGA (ProASIC3000)– Fabrication and population scheduled to accommodate integration with DCB-RFS_ADC ETU1– HDLP Connectors delivery expected in September, 2013– Used by DCB, TDS, and DFB
Daughter board de-insertion hardwareETU FPGA Daughter board layout
13
DCB/RFS_ADC ETU1 Development
• DCB_RFS-ADC Schematics Completed– Schematic Review held in June, 2013– BOM released and parts have been ordered
• DCB_RFS-ADC PCB Layout CompletedBoards can be driven by the RFS Frontend ETU1 boards (will be eventually integrated during the ETU2 stage)
FPGA Daughter Bd CPU Memory: SRAM, EEPROM & PROM
FLASH
RFS Memory (SRAM)
RFS ADCs and Data Buffers
Instrument & LNPS I/Fs
S/C I/F
We are checking the layout & expect to have boards in August, 2013.
14
AEB Development• Antenna Electronics Board
– Parts list Complete, 1 to qualify (from RBSP)– Breadboard in test (1 channel)– Common ICD to DCB/TDS in process
AEB single channel breadboard in testing
15
UMN Activity
• Preliminary designs are moving along• Breadboarding is advanced• Parts identification is moving along
– PEM obtained and in up-screening process (starting with a DPA)
• Embraced the FPGA daughter board concept• Redundancy/Reliability trade issues resolved
– FIELDS now separated into two halves• FIELDS1/DCB and FIELDS2/TDS• No single point FIELDS failure
– UMN split single LNPS into two pieces– UMN added a S/C interface to the TDS
• Systems Engineering has moved to UMN
16
TDS FPGA Block Diagram
17
UMN ActivityTDS BB2 – being populated
FPGA daughter board outlline
ProASIC3000 flash-based FPGA (in BGA)
LNPS BB1 demonstration
SPP Fields DFB
DFB Science:• Finalized Sensor inputs; gain states, band-pass (except SCM – in process)• Defined: Coordinated Burst implementation, Digital Burst Memory (size & no of
buffers and channels), Spectra and Cross-Spectra
DFB Prototype:• Prototype design complete, layout review Tues 7/16, quick turn fab planned• All FPGA modules for prototype bring-up complete • Board will be used for most of early development and then for testing/characterization
of Sidecar ASICs after moving to ETU board
DFB ETU:• Schematic in process for Xilinx FPGA Daughter Card• FPGA development status shown in separate slides
DFB Flight:• Received Sidecar ASICs; EIDP/workmanship deviation released this week, risk added• Continued EEE parts submittal to PCB for approval, no known issues at this time
SPP Quarterly Review 7/18/13
Like
lihoo
d of
Occ
urre
nce
(pro
babi
lity)
Consequence of Occurrence (Impact)
5
4
3
2
1
1 2 3 4 5
High Medium Low (Criticality)P = PerformanceC = CostS = ScheduleM = Mass
ID TITLE P I Crit Retire At
F-DFB01 Sidecar workmanship 2 3L
Post PDR characterization testing
F-DFB01PM
SPP Quarterly Review 7/18/13
If the Sidecar experiences latent failure and/or has reliability issues, then the lack of a complete EIDP and respective workmanship could hinder the debug/troubleshooting, and have the potential to degrade performance and warrant possible redesign which could increase needed mass and power. Risk mitigation plan is to perform characterization and environmental testing on Sidecars. These parts have prior electrical burn-in testing hence characterization and environmental tests will demonstrate good rigor to retire the risk.
Risk rating: Probability 2, Impact 3; not likely to occur based on successful burn-in testing completed by vendor [GSFC/Teledyne]; consequences slightly higher based on possibility of reverting to backup plan of discrete ADCs. Proposed/heritage ADCs are not as rad-tolerant, require more board space (mass increases), more power, and/or could drive science return. Newer, more viable, ADCs identified but require radiation testing.
DFB Sidecar Risk
20
DFB Block Diagram
SPP Quarterly Review 7/18/13
DFB FPGA Architecture
SPP Quarterly Review 7/18/13
22
DFB FPGA Development Status
SPP Quarterly Review 7/18/13
7/18/13
Module Name VHDL Code Simulation Lab Testing
Top Level Module 100% 0% 0%SIDECAR ASIC Interface 100% 60% 0%Mid-Freq Filters 100% 25% 0%Low-Freq Filters 100% 25% 0%Triggers 100% 0% 0%Waveform Player 75% 0% 0%Digital Burst Memory (DBM) [Prototype] 100% 0% 0%Digital Burst memory (DBM) [Flight] 0% 0% 0%Spectra/Cross-Spectra 50% 0% 0%SDRAM controller fpr DBM 50% 0% 0%SRAM controller for Spectra/Cross-Spectra 100% 20% 0%SRAM controller for Data Processor 100% 20% 0%Command Processor 75% 20% 0%Data Processor (CCSDS packetizer, data compression) 50% 0% 0%
SCM Calibration Signal Generator 0% 0% 0%Simulation Testbench 20% 10% 0%
SPP MAG Status
• Some scheduled MAG activities have slipped; however, we are now in receipt of most information (ICDs, etc.) and materials needed, and we have a clear understanding of the path to PDR.
• The AC Heater (ACHE) PCBs have been laid out and procured. They will arrive next week and will be populated and tested ASAP.
• Macor bobbins and other procurements are nearing completion, facilitating the build up of the ETUs.
• Significant progress with thermal modeling for the MAG sensors has allowed a better understanding of constraints and mitigations of the thermal range; we are interested in results from Gail Martin on any additional power available.
• Thermal testing (-50 to +50 C) of GSE sensor (Macor base) is currently being conducted in a non-windowed thermal vacuum chamber (see photo on next slide). First goal is to determine how fast we can cycle.
• Design of a composite base for the ETU MAG sensors is completed.
• Ongoing concerns include: MAG sensor placement on boom relative to spacecraft, power, etc., available to increase low end MAG sensor temperature, alignment error budget numbers, boom harness plan, conclusion of L4 requirements & ICDs
MAG thermal vacuum chamber #1
• Chamber shown at right permits operating over a large temperature range (order of -100 to +100 C) at < 10^-5 torr. (Same aluminum cylinder is also the “insert” for the windowed TV chambers.)
• Currently instrumented (8 thermistors) and being used to determine the rate at which we can cycle the MAG “GSE” sensor temperature, which has consequences for all future thermal testing.
• Since chamber has no windows, the sensor alignment inside chamber cannot be determined, i.e., no calibration over temperature.
• We can calibrate zero levels, etc., before and after thermal cycling. If they do not change, then we can conclude that calibration as a function of temperature will be possible – adequate for PDR. TVC #1 working in GSFC Mag Lab.
FIELDS ScheduleSummary of FIELDS Activities Worked ICD’s between MEP boards Built Breadboards Reviewed Parts lists with PMPCB Coordinated Reviews of Project documents
Tested Antenna Thermal Test Model (France) Completed Optical properties tests Conducted Distortion tests
MAG TVAC Chamber Completed Breadboard Tests in Progress MEP ETU Frame designs Accommodating AEB and RFS
Planned Peer Reviews with Team(SPF_MGMT_011F_ReviewMatrix.xls)
Keys to Next Quarter (to Nov 2013) Level 4 Instrument Requirements Peer Reviews Complete Layouts Nearing Completion Pre-IPDR Documents Complete Antenna at TRL 6 FIELDS Phase CDE Proposal
FIELDS ScheduleReviews
pPD
R
iPD
R
PD
R
pCD
R
iCD
R
CD
R
iPE
R
iPS
R
MO
R
SIR
PE
R
PS
R
OR
R
FR
R
LRR
Current Date
Var
ious
11/1
3/20
13
1/14
/201
4
Var
ious
1/20
/201
5
3/2/
2015
5/3/
2016
10/4
/201
6
10/1
3/20
15
TB
D
10/6
/201
7
2/21
/201
8
3/20
/201
8
TB
D
7/30
/201
8
pPDR pCDR pPER pPSRFIELDS Mission Lvl X X X X X X X X XFIELDS Inst. Lvl X X X X
MEPDCB-RFS Board X X 10/16/2013 12/22/2014DCB FPGA X X 10/16/2013 11/25/2014DCB FSW X X 10/17/2013 11/24/2014AEB Board X X 10/15/2013 10/31/2014Preamps X X 10/15/2013 10/31/2014DFB Board X X 10/29/2013 12/3/2014DFB FPGA X X 10/29/2013 12/3/2014DFB ASIC X X 10/30/2013 12/3/2014TDS Board X X 10/16/2013 10/23/2014TDS FPGA X X 10/16/2013 10/23/2014TDS FSW X X 10/17/2013 11/20/2014LNPS Board X X 10/15/2013 9/4/2014SCM Sensors X X 9/6/2013 < 4/7/2014Chassis X X 7/17/2013HarnessThermal
Antenna System X X 5/21/2013 12/23/2014MechanismHarnessThermal
V5 System X X 7/17/2013 12/23/2014MechanismHarnessThermal
MAG System X X X X 10/22/2013 1/14/2015 8/27/2014 3/31/2016Electronic BoardMAG FPGA X X 8/26/2013 3/24/2014SensorHarnessThermal
FIELDS SOC X X
Peer Review Preliminary DatesPeer Review Schedules
FIELDS iPDR Readiness Schedule
FIELDS Schedule
ID Critical UniqueID
Task Name Duration Start
51 No 6430 MEP iPDR READY 38 d 9/18/1352 No 6431 DCB iPDR READY 0 d 9/18/1353 No 6435 AEB iPDR READY 0 d 11/11/1354 No 6432 RFS iPDR READY 0 d 11/11/1355 No 6520 MEP Chassis iPDR READY 0 d 10/24/1356 No 6433 TDS iPDR READY 0 d 11/6/1357 No 6436 LNPS iPDR READY 0 d 11/5/1358 No 6434 DFB iPDR READY 0 d 10/24/1359 No 6439 ANT iPDR READY 0 d 11/11/1360 No 6478 PA iPDR READY 0 d 8/5/1361 No 6440 MAG iPDR READY 0 d 10/21/1362 No 6482 SCM iPDR READY 0 d 10/8/1363 No 6615 iPDR Package Preparation 1 d 11/12/13
11/11
9/18
11/11
11/11
10/24
11/6
11/5
10/24
11/11
8/5
10/21
10/8
11/12
6/9 9/29 1/19 5/11 8/31 12/21 4/12 8/2May 21 January 11 September 1 April 21
CRITICAL PATH
ETU I&T
FLT I&T
ETU DFBFLT ANTs
iCDR
Like
lihoo
d of
Occ
urre
nce
(pro
babi
lity)
Consequence of Occurrence (Impact)
5
4
3
2
1
1 2 3 4 5
High Medium Low (Criticality)P = PerformanceC = CostS = ScheduleM = Mass
PF1
Evaluation Date: 07/12/13
PF2
PF5
PF6
PF7PSF9
FIELDS Instrument Risks Status
ID TITLE P I Crit Retire AtF9 Magnetic Sensor Qualification 3 4 M MAG Thm Test by I-CDR (~1/15)
F12 Magnetic Cleanliness 4 3M
Mission I&T (~8/16)
F7 ElectroStatic Contamination 3 3M
Mission I&T (~8/16)
F16 MEP Thermal Environment 3 3M
Parts confirmed at I-PDR (11/13)
F5 Survival Thermal Environment 3 4M
SCM & MAG Env. Qual (~11/14)
F10 Antenna Qualification 2 3L
Ant. Qual (11/13)
F6 Magnetic Sensor Interference 4 3L
ETU I&T (~8/14)
F11 SCM dependence on Solar Orbiter 2 2L
SO FLT SCM Complete
F1S/C Conducted and Radiated Noise
Contamination 1 3L
Mission I&T (~8/16)
F2 Plasma Wake Effects 1 3L
Mission CDR (~3/15)
CSF10CSF11
PF12
Mitigation Plans in Place for All FIELDS Risks
SF14
PF16
FIELDS Funding
Spending : -15%Runout : Sept. 2013
FIELDS UCB Labor
Labor cumulative over budget by 6%
FIELDS Subcontracts
Invoiced
Date ofRecentInvoice Period
BalanceAvailable
(when Mods are finalized) Mod
End-Date(expected)
$53,152.47 6/7/2013 Feb-May-13 $36,928.53 13 11/14/2013
$27,966.38 2/2/2012 Sep11-Jan12
$51,113.62 11 9/14/2013
$665,804.44 6/6/2013 May-13 $74,219.56 11 12/31/2012
$587,544.85 5/22/2013 Apr-13 $759,673.15 14 9/30/2013
Status SPONumber
SponsorAward
Number
Sub-contractNumber
Sub-contractor
Name Begin End Anticipated Amount
Obligated Amount
FundedThru
Active 030174-002 975268 7549 Universityof New
Hampshire
1-Oct-10 14-Mar-14 $90,081 $90,081 FY13
Active 030174-002 975268 7550 University of Maryland
1-Oct-10 14-Mar-14 $79,080 $79,080 FY13
Active 030174-002 975268 7447 University of
Minnesota
1-Oct-10 14-Mar-14 $740,024 $740,024 Q1FY1312/31/12
Active 030174-002 975268 7448 University of Colorado
1-Oct-10 14-Mar-14 $1,911,209 $1,347,218 9/30/2013
Technical Parts Approvals are all “Provisional” stuck awaiting “radiation evaluation.” MEP 65C requirement remains a power and parts concern MAG Level 3 (PAY-37) needs “5 nT accuracy” term defined better (recommend “1 degree”)
Cost Adding Redundancy may add cost, complexity and schedule
Schedule ICON selection caused temporary loss of manpower: only 1 spot remains to be filled
Retired (Listed last quarter) AEB circuitry having trouble fitting on a 6”x9” board. SCM funding was approved in France GSFC backup SCM must begin soon to be ready for iPDR FIELDS Frequency plan is a real struggle, may have power/tm impacts
FIELDS Issues & Concerns
Backup
P = PerformanceC = CostS = ScheduleM = Mass
ID Risk Mitigation PlanF1-P: S/C Conducted and Radiated Noise Contamination
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A EMI/EMC Plan Draft prior to I-PDR 06/13 1 3 3
B EMI/EMC Plan Final prior to I-CDR 01/15 1 3 3
C EMC verification at Mission I&T 08/16 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F1-P: S/C Conducted and Radiated Noise ContaminationCurrent
Assessment LOW
Likelihood Consequence Risk Grade
Risk Statement
If S/C design does not include EMI shielding and EMC mitigations 1 3 3
Then FIELDS will not be able to measure small signals as required Last Updated 08/10/11
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
F1-P: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
B CA
ID Risk Mitigation PlanF2-P: Plasma Wake Effects
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Accept risk at Mission CDR when design freezes with adequate boom length. 03/15 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F2-P: Plasma Wake EffectsCurrent
Assessment LOW
Likelihood Consequence Risk Grade
Risk Statement
If S/C plasma wake effects are as large as predicted, 1 3 3
Then near-S/C electric field sensors will be compromised. Last Updated 08/10/11
F2-P: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
AP = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF3-CS: Foreign Funding Issues
Event Date
Assessment**Likeli-hood
Conse-quence
Risk Grade
A Fund backup options for TNR and SCM 09/11 4 4 16
B Decision to proceed with foreign sources for SCMRemove TNR/HFR from CNES and select alternate option for TNR/HFR 06/12 3 4 12
CCNES proposal for next phase (SCM)Implement replacement plan for TNR/HFR include budget/schedule & open new technical risk capturing the technical development of the new option
09/12 1 4 4
D KDP-C 11/13 1 4 4
E CNES Phase C Commitment 12/13 (TBR) Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
20
15
10
5
Risk F3-CS: Foreign Funding IssuesCurrent
Assessment HIGH
Likelihood Consequence Risk Grade
Risk Statement
If foreign funding sources fail 4 4 16
Then we may lose the search coil sensors or electronics Last Updated 12/12/12
F3-CS: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
A
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
BC
D ERisk retired on 12/12/12- Replaced with risk F15
ID Risk Mitigation PlanF5-P: Survival Thermal Environment
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Preliminary thermal analysis/test to confirm if the thermal design is adequate 06/12 2 4 8B GSFC MAG Ops & Survival Thermal Test 06/12 1 4 4C APL test high-efficiency blankets on MAG Boom mock-up (prior to ETU Env. Test). 08/14 (TBR) 1 4 4D SCM & MAG Environmental Qualification 11/14 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F5-P: Survival Thermal EnvironmentCurrent
Assessment Medium
Likelihood Consequence Risk Grade
Risk Statement
If the survival thermal environment for the SCM and MAG does not meet the sensors’ minimum temperature requirements, 3 4 16
Then additional heater power will be required to avoid instrument failure. Last Updated 04/12/13
D
F5-P: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
CAB
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF6-P: Magnetic Sensor Interference
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
AMAG Boom design accommodates >1m separation by I-PDRIncreased risk liklihood dues to APL ownership of MAG boom. Will ‘buy down’ when commitment to sufficient sensor separation is made
06/13 1 3 3
B ETU I&T complete 08/14 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F6-P: Magnetic Sensor InterferenceCurrent
Assessment LOW
Likelihood Consequence Risk Grade
Risk Statement
If the MAG and SCM sensors are too close, 4 3 6
Then their interference will compromise the magnetic measurements. Last Updated 06/14/13
AB
F6-P: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF7-P: Electro Static Contamination
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A ESC plan draft complete, prior to I-PDR 06/13 2 3 6
B ESC plan final, prior to I-CDR 01/15 1 3 3
C ESC verified at Mission I&T 8/16 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F7-P: Electro Static ContaminationCurrent
Assessment MEDIUM
Likelihood Consequence Risk Grade
Risk Statement
If the S/C has areas that charge up, 3 3 9
Then their potential will compromise the electric field measurements. Last Updated 08/10/11
F7-P: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
AB
C
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF8-PSM: Magnetic Sensor / SCM Dynamic Range
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
AMAG/FGM Trade Closure SCM Dynamic range portion is retired, the SCM/MAG compatibility is still an issue 6/25/12: decision made to cover gap in dynamic range by sampling the MAG faster
6/12 Retired Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F8-PSM: Magnetic Sensor / SCM Dynamic RangeCurrent
Assessment Retired
Likelihood Consequence Risk Grade
Risk Statement
If the combined MAG & SCM concept does not cover the required dynamic range and bandwidth, 3 3 9
Then there may be a loss of data in certain frequency bands. Last Updated 06/25/2012
A
F8-PSM: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
Risk Retired
ID Risk Mitigation PlanF9-PS: Magnetic Sensor Qualification
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Plan thermal testing of a representative MAG sensor (by I-PDR) 11/13 2 4 8
B MAG Thermal Test by FIELDS Instrument CDR 12/14 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F9-PS: Magnetic Sensor QualificationCurrent
Assessment MEDIUM
Likelihood Consequence Risk Grade
Risk Statement
If the MAG sensor is not qualified for the number of operational thermal cycles, 3 4 12
Then the sensor may fail in orbit. Last Updated 08/10/11
AB
F9-FS: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF10-PS: Antenna Qualification
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Obtain Nb materials for testing - complete 01/12 2 3 6
B Nb material testing, Glenn Research Ctr (high temp testing complete), Southern Research, MSFC, APL, Surface Optics
2/12 – 8/12 1 3 3
C APL measuring material properties of the coupons that underwent high-temp testing at Glenn Research and tube straightness being evaluated. 04/13 1 3 3
D Antenna ETU thermal testing; Antenna Qualification (I-PDR) ~11/13 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F10-PS: Antenna QualificationCurrent
Assessment Low
Likelihood Consequence Risk Grade
Risk Statement
If the antenna cannot be qualified to meet thermal requirements, 1 3 3
Then the antenna will need to be re-designed. Last Updated 05/17/2013
A
C
F10-PS: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
BD
ID Risk Mitigation PlanF11-S: SCM Dependence on Solar Orbiter
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Solar Orbiter ETU complete TBD 1 2 2
B Re-plan SCM ETU testing as needed TBD 1 2 2
C Re-plan SCM FLT integration as needed TBD 1 2 2
D SO Flight SCM Complete TBD Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F11-S: SCM Dependence on Solar OrbiterCurrent
Assessment LOW
Likelihood Consequence Risk Grade
Risk Statement
If Solar Orbiter is delayed, 1 2 4
Then the SCM for FIELDS delivery will be delayed. Last Updated 12/12/12
AB C D
F11-S: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF12-P: Magnetic Cleanliness
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Magnetics plan draft (prior to I-PDR) 06/13 3 3 9
B Magnetics plan final (prior to I-CDR) 01/15 2 3 6
C Design freeze at M-CDR confirms long-enough MAG Boom 03/15 1 3 3
D Magnetics verified at Mission I&T 08/16 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F12-P: Magnetic CleanlinessCurrent
Assessment MEDIUM
Likelihood Consequence Risk Grade
Risk Statement
If the S/C exhibits high residual magnetic fields (AC or DC), 4 3 12
Then the magnetic measurements will be contaminated. Last Updated 08/10/11
AB
CD
F12-P: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF12-P: Magnetic Cleanliness
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Study the possibility of making a simple surface voltage measurement on the MAG boom as a baseline for the sunward electric field complete 08/2012 Drop likelihood to 1
B Add third axis electric field to the complement of measurements (draft ICD in May) 05/2013 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F13-P: Third Axis Electric Field MeasurementCurrent
Assessment LOW
Likelihood Consequence Risk Grade
Risk Statement
If S/C electrostatic center is near the TPS and highly variable, 1 3 12
Then FIELDS will fail to measure the sunward electric fields. Last Updated 2/15/2012
A
F13-P: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F14-S: Phase B ContractCurrent
Assessment MEDIUM
Likelihood Consequence Risk Grade
Risk Statement
If the UCB Phase B contract or UCB Phase B subcontracts lapse (due to insufficient lead time to get subcontracts to teammates), 4 2 8
Then then the early Phase B deliverables and testing schedule will be delayed. Last Updated 04/19/2012
A
F14-S: Phase B Contract
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016 P = Performance
C = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
ID Risk Mitigation PlanF11-S: SCM Dependence on Solar Orbiter
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Phase B contracts (to UCB and teammates) in place TBD 4 1 4
B Replan of early Phase B deliverables & testing complete TBD Retire Risk
B
Retired
ID Risk Mitigation PlanF6-P: Magnetic Sensor Interference
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A New CNES management to evaluate and sign the SCM LOA 03/13 1 3 3
B if no agreement from CNES in place by 4/13, fund backup option at GoddardFunding commitment made – retire risk 06/13 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F15-CS: SCM Funding IssuesCurrent
Assessment MED
Likelihood Consequence Risk Grade
Risk Statement
If foreign funding sources fail 3 3 12
Then we may lose the French search coil sensor and would switch to the backup Last Updated 06/14/13
A
B
F15-CS: Risk Burn Down
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
Retired
ID Risk Mitigation PlanF6-P: Magnetic Sensor Interference
Event Date
Assessment**
Likeli-hood
Conse-quence
Risk Grade
A Determine if the MAVEN thermal design is adequate for FIELDS 01/13 1 3 3
B Confirm all parts meet the MEP high temp AFT bu I-PDR 11/13 Retire Risk
* Grade = Likelihood x Consequence ** Assessment is the remaining risk assessed after successful event completion
Ris
k G
rade
25
20
15
10
5
Risk F16-P: MEP Thermal EnvironmentCurrent
Assessment MED
Likelihood Consequence Risk Grade
Risk Statement
If the MEP high temperature AFT remains over 55 deg C 3 3 12
Then FIELDS heritage electronics may need to be re-designed to accommodate the higher flight temperature. Last Updated 5/17/13
A
B
F16-P: MEP Thermal Environment
Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q4 Q1 Q2 Q3 Q42011 2012 2013 2014 2015 2016
P = PerformanceC = CostS = ScheduleM = Mass
PlanActual
Level Risk Grade*High 15-25
Medium 6-12Low 1-6
Risk Notes: April 2013
F5 – Survival Thermal Environment (chart 7)- new data elevates risk over concern regarding the MAG thermal model
(probability increase to 3). May need more heater power then what is allocated- believe an updated thermal model is needed to proceed in lowering this risk
F15 – SCM Funding (chart 17)- FIELDS had a discussion with the Backup SCM lead at GSFC; it was determined that the heritage SCM is larger and heavier than the French device.- Thus, substantial redesign work will be required to accommodate the GSFC unit.- On the plus side, though, GSFC is available to support SPP on this effort, with a baseline schedule beginning in June 2013 (if needed)- believe an updated thermal model is needed to proceed in lowering this risk
Risk Notes: February 2013
1) F10 – Antenna Qualification (chart 12): Risk burn-down updated to reflect the current state of Antenna Qualification testing:
• APL is completing materials testing on the coupons that underwent high-temp testing at Glenn Research to determine if the material properties were affected by the high temperatures.
• The antenna qualification thermal testing (currently scheduled for March 2013) may be moved to September 2014. This would still permit testing to be completed prior to FIELDS I-PDR.
2) F13 – Third Axis Electric Field (chart 15): Lowered likelihood to “1” based on the completion of determining that it’s possible to do the measurement. Added the final step of confirming the addition of this to the complement of measurements in the draft ICD in May 2013.
Risk Notes: January 2013
1) F15 – SCM Funding Issues (chart 17): Decrease the likelihood from 4 to 3 per discussions at NASA headquarters, in international affairs, are proceeding with CNES. Detailed discussions have commenced.
Risk Notes: December 2012
1) F3 - Foreign Funding (commitment) (chart 7): - Risk retired and replaced with a more relevant, SCM-specific risk; New risk F15 – SCM Funding Issues
2) F15 – SCM Funding Issues (chart 17): If foreign funding sources failthen we may lose the French search coil sensor and would switch to the backup - created to capture the SCM-specific funding issues - expect CNES to re-evaluate SCM funding by Jan or Feb ‘13 - if CNES does not sign the LOA explore:
- alternate HW source (3D Plus) for LPCE; or- funding the backup option at Goddard
3) F16 – MEP Thermal Environment (chart 18): If the MEP high temperature AFT remains over 55 deg C; Then FIELDS heritage electronics may need to be re-designed to accommodate the higher flight temperature. - MEP panel temperature is expected to be 55 deg C so, the allowable flight temperature may be 65 deg C which may lead to some parts issues. Change approach to mitigation if it's determined that parts need to be changed. - Determine if the MAVEN thermal design is adequate for FIELDS (end of 1/13)- Confirm all parts meet the MEP high temp AFT (by iPDR)