Jamison Hawkins Lockheed Martin Corporation Music Also Sprach Zarathustra by Richard Strauss performed by John Williams and the Boston Symphony Orchestra Philips 1983 GOESR Over 100 Remote Sensing Satellites ID: 806843
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Slide1
NOAA’s GOES-R
Spacecraft
Jamison Hawkins
Lockheed Martin Corporation
Slide2Slide3Music:
Also Sprach
Zarathustra
by Richard Strauss
performed by John Williams and the Boston Symphony Orchestra
Philips, 1983
Slide4GOES-R
Over 100 Remote Sensing Satellites
More than 500 Instruments
Successfully Built and Delivered:
50 Years of Delivering Earth Observation Advances
Slide52010
1980
Satcom 3R
Aurora 1
Satcom 4
Spacenet-1
Spacenet-2
Satcom 1R
Satcom 2R
BS-2A
GSTAR-1
ASC-1
Satcom Ku-2
GSTAR-2
BS-2B
Satcom Ku-1
Satcom C1
ASTRA-1A
GSTAR-3
PanAmSat-1
Spacenet-3R
BS-3A
GSTAR-4
ASTRA-1B
Anik-E2
Spacenet-4
Aurora-2
BS-3B
Anik-E1
NSS-K
Satcom C4
Satcom C3
Telstar
401
402R
ACTS
BS-3N
Chinastar-1
AsiaSat 2
Koreasat
EchoStar
Inmarsat-3/F
AMC
Intelsat-VIII
1
2
NSS-803
4
5
NSS-806
1
2
101
102
III
IV
1
2
3
4
5
1
2
3
AP
Telkom I
1985
1990
1995
2000
ABS-1
6
8
7
Nimiq-1
JCSAT-110
Iridium
(89 buses)
4
3
ACeS Garuda-1
10
2005
IKONOS
N-STAR c
VII
NSS-6
RCA Astro Electronics
GE Astro Space
Martin Marietta Astro Space
Lockheed Martin CSS
NSS-7
A2100 bus
Legend
EchoStar
Koreasat
1958 SCORE 1st Communications Payload
Nimiq-2
Rainbow-1
18
11
15
16
Between 1975 and 1980
BSE, Satcom 1, Satcom2, Anik-B
ASTRA IKR
ASTRA IL
JCSAT 9, 10
JCSAT 11, 12
EchoStar X
SIRIUS 4
BSAT-3a
VINASAT 1
Satisfying Global Market Needs for Over 25 Years
Our A2100-Based GOES-R Solution Provides Highest Value and Performance, A2100 spacecraft have accumulated 200 years of on-orbit operation without a failure
14
Slide6GOES-R Overview
A collaborative
development and
acquisition
Flight Project -
led by
NASA
Ground
Segment
Project - led by NOAA
Scheduled for
launch in 2015
Six advanced instruments
New and improved capabilities for
decreased
lead times for
severe weather warnings
better storm tracking capabilities
solar, space weather, and climate analysesadvanced products for aviation, transportation, commerce
Extending the continuity of NOAA’s 40-year geostationary mission, GOES-R will be the next weather sentinel for
monitoring threatening weather, and providing data for forecasting and environmental analyses
Slide7Satellite Driving Requirements
Provide
precision, stable space platforms
at two operational geostationary orbital locations (75W and 135W) carrying the baseline instrument set
Operational Mission
-
First Launch 2015
:
Provide continuity and improvements over the current system with
spacecraft bus reliability of 0.81
after 10 years of on-orbit operation preceded by 5 years ground storage & up to 5 years on-orbit storage
Spacecraft
On-Orbit Life of 15 years
with orbit East-West and North-South position maintained to within +/-0.1 degree. Support
9 station location changes
Collect and transmit up to
140Mbps (coded) Instrument Payload data
from each location continuously.
C
ontinue
Rebroadcast function
at L-Band up to 31 Mbps utilizing dual polarization
Provide
continuing and new services
(Search & Rescue, Data Collection, EMWIN)
Slide8Visible
& IR Imagery
Lighting Mapping
Space Weather Monitoring
Solar Imaging
Advanced Baseline Imager (ABI)
Geostationary Lightning Mapper (GLM)
Space Environment In-Situ Sensor Suite (SEISS)
Magnetometer
Solar Ultra-Violet Imager (SUVI)
Extreme UV/X-Ray Irradiance Sensors (EXIS)
GOES-R
is
the next generation
of
NOAA geostationary
satellites that will provide a major improvement in
quality, quantity and timeliness
of data collected.
GOES-R Mission
Slide9ABI
GLM
SUVI
Magnetometer
Star trackers
SEISS
EXIS
Slide10ABI
GLM
SUVI
Magnetometer
Star trackers
SEISS
EXIS
Greg Mandt – 1.8 m
Slide11GOES-R Spacecraft Configuration (External)
UHF ANT
S
-
BAND
DIPOLE
ABI
SGPS
MPS
-
LO
EHIS
SUVI
SIS ELECTRONICS
EARTH POINTING OMNI ANT
SOLAR ARRAY
MPS
-
HI
SUN
SENSOR
STAR TRACKERS
GPS
ANT
GLM
X
-
BAND ANT
AFT HEMI +
BICONE OMNI ANT
L
-
BAND GRB
ANT
EXIS
UHF ANT
S
-
BAND
DIPOLE
ABI
SGPS
MPS
-
LO
EHIS
SUVI
SIS ELECTRONICS
SOLAR ARRAY
MPS
-
HI
SUN
SENSOR
GPS
ANT
GLM
X
-
BAND ANT
MAGNETOMETER
L
-
BAND GRB
ANT
EXIS
SEISS
Dimensions:
5.4m from LV adapter
to top of ABI
S/A Panels are
approx. 1m x 4m
each
Slide12Notable Performance Elements
Operates through daily station-keeping and momentum adjust maneuvers
Low risk station-keeping operations
Increased instrument availability
Decreased propellant required due to high efficiency thruster
Yaw flip improves ABI radiometric response
Outage twice per year
Total time of noncompliance for instrument interface requirements <120 min per year
Vibration Isolation for optical bench
Slide13Animation shows the vibration-isolation impact
ABI
and GLM are mounted
on stiff
optical bench
Dynamics are tunable to optimize system performance
Couple instrument motion to IMU and star trackers with low thermal distortion
High-accuracy attitude determination system on the instrument optical bench
High accuracy star trackers
High-bandwidth, low-latency and low-noise IMU for effective motion compensation
ABI & GLM Decoupled from Bus
Design
Elements Support Precision
INR for Users
Augmented attitude control array damping
demonstrated with risk-reduction tests
Slide14Optical Bench Vibration Isolation Impact
Slide15GOES-R Satellite Production and Support Locations
Slide16NOAA’s GOES-R
Spacecraft