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1 UNCLASSIFIED – FOUO – Not for Public Release UNCLASSIFIED – FOUO – Not for Public Release Operational Space Environment Network Display (OpSEND) & the Scintillation Network Decision Aid Dr. Keith Groves, Prog Mgr Ionospheric Impacts to RF Systems Space Vehicles Directorate Air Force Research Laboratory
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1 UNCLASSIFIED – FOUO – Not for Public Release Operational Space Environment Network Display (OpSEND) & the Scintillation Network Decision Aid Dr. Keith.

Dec 24, 2015

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Page 1: 1 UNCLASSIFIED – FOUO – Not for Public Release Operational Space Environment Network Display (OpSEND) & the Scintillation Network Decision Aid Dr. Keith.

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UNCLASSIFIED – FOUO – Not for Public Release

UNCLASSIFIED – FOUO – Not for Public Release

Operational Space Environment Network Display (OpSEND) & the

Scintillation Network Decision Aid

Dr. Keith Groves, Prog MgrIonospheric Impacts to RF Systems

Space Vehicles DirectorateAir Force Research Laboratory

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Disturbed Ionospheric Regions andSystems Affected by Scintillation

SATCOM

AURORAL IRREGULARITIES

GPS

PLASMA BUBBLES

GPS SATCOM

MAGNETICEQUATOR

DAY NIGHT

EQUATORIAL F LAYERANOMALIES

SBR

POLAR CAPPATCHES

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Operational Space Environment Network Display (OpSEND)

• OpSEND incorporates state-of-the-art sensors, models, and display tools to generate Space Weather impact maps :

– UHF Satellite Communication (SATCOM) Scintillation Map

– HF Illumination Map

– Radar Auroral Clutter Map

– Estimated GPS Single-Frequency Error Map

• OpSEND team received Air Force Merewether Award

UHF SATCOM Scintillation Map

GPS Single-Frequency Error Map

HF Illumination Map Radar Auroral Clutter Map

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Radar Auroral Clutter

Ionosphere

GPS

UHF SATCOM

GPS 1-Freq Error

HF Illumination

COMM NETS

Ionosonde Network foF2

TEC and Scintillation

Magnetometer Network

DMSP

OpSEND System Architecture

UHF Scintillation

Operational, Real-time Assimilation Models

AFWA

Sensors Space Weather Impact Maps

Magnetic Activity

SCINDA/IMS Network

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SCINTILLATION NETWORK DECISION AID(SCINDA)

• Ground-based sensor network

– Passive UHF / L-band /GPS scintillation receivers

– Measures scintillation intensity, eastward drift velocity, and TEC

– Automated real-time data retrieval via internet

• Data drives assimilative/empirical model providing simplified visualizations of scintillation disturbances

– Output spans frequencies from 200 MHz to 2 GHz

• Graphical output tailored to specific applications (UHF SATCOM, at present)

A regional nowcasting system to support users of space-based RF

communication and navigation systems

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Scintillation Map

SCINDA User Product Example

Scintillation

Warning Areas

Watch Areas

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Present and anticipated thru 2008*

SCINDA Ground Stations

30N

0

30S

210E 240E 270E 300E 330E 0 30E 60E 90E 120E 150E

Existing Sites UN IHY Sites Other/collaboration

*Future sites shown represent approximate desired locations; actual sites TBD

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GPS Positioning Errors During Solar Max

Scintillation can cause rapid fluctuations in GPS position fix; Typical night from recent field experiments

Scintillation can cause rapid fluctuations in GPS position fix; Typical night from recent field experiments

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Summary

• Ionospheric scintillation occurs routinely at low latitudes independent of magnetic activity

• Scintillation can affect the performance of space-based communication and navigation systems operating at frequencies below about 2 GHz

• Scintillation affects 2-frequency GPS systems, but no error-estimation model currently exists

• Exploiting collaborations with international partners and the UN, AFRL plans to add 10-15 new ground stations over the next three years

• Coordination with C/NOFS equatorial satellite planned to maximize scientific contribution to understanding Spread F

• Ground-station support leveraged across AFRL, AFOSR, AFWA and NSF

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Why Africa?

• Historical ground-based data sets are sparse/non-existent

– Ground-based observations critical to understanding scintillation environment

• ROCSAT in situ (600 km) observations indicate frequent F region irregularities

– Activity present nearly year-round

• DMSP observations show similar peak in bubble occurrence (Huang et al 2004)

• Goal is to characterize irregularity development over Africa in the context of global patterns of scintillation occurrence

Adapted from S.Y. Su, 2005

Fundamental gap in knowledge of the space environment over Africa

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Space Science across Africa

• UN Basic Space Science Initiative (BSSI) focused on IHY 2007-2011

• Currently establishing contacts through academia, international partners, US State Department, etc.

• AFRL to participate in UN-sponsored Nov. workshop to identify host nation partners

• Goal is to establish robust monitoring network with scientific collaboration across Africa and Asia

AFRL hopes to develop 5-8 new sites in Africa over the next 3 years

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SCINDA Ionospheric Parameter Measurements

• VHF (~250 MHz) & GPS scintillation parameters– S4 scintillation index

– Intensity spectrum

– Fading probability density function

– Temporal decorrelation of intensity

– Data quality flags based upon parameter consistency, and reconciliation between S4 index and the fading PDF

• Ionospheric zonal drift estimates obtained from VHF spaced antenna observations

• GPS Total Electron Content (TEC) and phase scintillation data

• Raw data (10-50 Hz) can be recorded as desired

Real-time output from SCINDA sensors includes: