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SECCHI Instrument SuiteSystem Description
Dan MosesSECCHI Program Scientist
Naval Research Laboratory/Praxis, Inc.
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SECCHI Instrument Requirements
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• The SECCHI Instrument Requirements Are Obtained From:
1) The STEREO Science Requirements (STEREO Mission Requirements Document 460-RQMT-0001)
2) The SECCHI Science Goals (SECCHI Science Requirements & Instrument Performance Specification Document 7906-SPC-9-0-003)
• The Flow Down of STEREO Requirements and the Derivation of the SECCHI Requirements Are Detailed in the SECCHI Science Requirements & Instrument Performance Specification Document
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STEREO Science ObjectivesSECCHI Instrument Requirements Flow Down
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• Understand the Causes and Mechanisms of CME Initiation
• Characterize the Propagation of CMEs Through the Heliosphere
• Discover the Mechanisms and Sites of Energetic Particle Acceleration
• Develop a Three-Dimensional, Time-Dependent Model of the Magnetic Topology, Density, and Velocity Structure of the Ambient Solar Wind
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Mission Science Measurement Requirements SECCHI Instrument Requirements Flow Down
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1A Determine the CME Initiation Time to an Accuracy of Order 10 Minutes
1B Determine the Location of the CME Initiation to Within ±5 Degrees of Solar Latitude and Longitude
2C Determine the Evolution of the CME Mass Distribution and the Longitudinal Extent to an Accuracy of ±5 Degrees As It Propagates in the Low Corona, the Upper Corona and the Interplanetary Medium
2D Determine the CME and MHD Shock Speeds Accurate to ±10% As It Propagates in the Low Corona, the Upper Corona and the Interplanetary Medium
2E Determine the Direction of the CME and MHD Shock Propagation to Within ±5 Degrees of Latitude and Longitude As the CME Evolves in the Low Corona, the Upper Corona and the Interplanetary Medium
4J Obtain a Time Series of the Solar Wind Speed Accurate to ±10% at Two Points Separated in Solar Longitude
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SECCHI Science Measurement Goals
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1A Determine the CME Initiation Time to an Accuracy of Order 1 Minute1B Determine the Evolution of the CMEs, the Transition Region Structures, the
Coronal Structures, EUV Waves, Coronal Dimming and Global Interactions at the Highest Cadence Rate and Matching Positional Accuracy
2A Determine the Three-Dimensional Evolution of CMEs and Associated Disturbances in Ambient Structures in the Lower Corona, the Upper Corona, and in the Interplanetary Medium at the Highest Cadence Rate and Matching Positional Accuracy
2B Determine the Evolution of the Tracers of CME Interaction With the Corona and Interplanetary Medium, the CME Shock Formation, and the Ambient Material Sweep-up at the Highest Cadence Rate and Matching Positional Accuracy
3A Determine the Candidate Sites of Energetic Particle Acceleration With a Timing Accuracy of ≤ 1 Minute
3B Determine the Evolution of the CME Front at the Highest Cadence Rate and Matching Positional Accuracy
4A Determine the Three-Dimensional Shape of Coronal Loops, Coronal Streamers, and Large-Scale Coronal Structures and Solar Wind Tracers With a Positional Accuracy of ≤1250 km in the Lower Corona From the Solar Disk to 1.5 Rsun, ≤4500 km in the Lower Corona From 1.5 Rsun to 3.0 Rsun, and ≤ 11,500 km in the Upper Corona
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Coronal and CME Detection With SECCHI Coronagraphs and Heliospheric Imager
The STEREO Science Requirements Emphasis on Earth-Directed CMEs Is Addressed With HI FOVs Covering a Cone of 45 Degrees From the Ecliptic Planea Using a Combination
of Existing CoronagraphicTechniques With Stepwise Extensions of Those Techniques, CMEs Will Be Observed by SECCHI, Without Gaps, From the Inner Corona to the Orbit of the Earth
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Image Cadence Requirements to Capture CME and Solar Wind Evolution Over Individual Coverage Regions
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SECCHI Instrument PerformanceSpecification Matrix
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SCIP Assembly Configuration
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GTCOR1
COR2
EUVI
SCIP Structure
Mechanism Electronics Box
(MEB)
Camera Electronics Box
(CEB)
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SCIP Assembly With Thermal Tent(1 of 2)
Forward SCIP Closeout
Upper SCIP Closeout
Single-Layer Perforated Blanket on SCIP Bench Edges
Instrument Overlap Rings
Aft SCIPCloseout
• Top View
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SCIP Assembly With Thermal Tent(2 of 2)
• Bottom View– MEB Partially Blanketed– CEB Not Blanketed
- Blanket Between Bench and CEB– Cutouts for SCIP Mounts
SCIP Bottom Blanket
MEB Radiator Window
CEB Not Blanketed
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SCIP Assembly Subsystem Breakdown
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HI Assembly Configuration
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HI Assembly Configuration
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Diffractive Front Baffle Assembly
Inner Baffle Assembly
Side Baffle Assembly
Radiator for CCD Cooling
Rear Baffle Assembly
HI-1 Telescope
HI-2 Telescope
HI Door (One Shot)
Leg (Flexure)
Door Latch Mechanism
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HI Assembly
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Bottom View
Camera Electronics Box (CEB)
HI-2 Access Cover
Top View
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HI Assembly Subsystem Breakdown
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SECCHI Electronics Box (SEB)
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Instrument Accommodations Metrics Relationship to the Instrument Performance Metrics
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SECCHI InstrumentAccommodations Matrix
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SECCHI-B Spacecraft Accommodation
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SCIP Assembly
PLASTIC
SWAVES Antenna
HIIMPACT Boom
High GainAntenna
SWAVES Antenna
Omni Antenna
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SECCHI-B Spacecraft Accommodation
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Guide Telescope COR1 EUVI COR2SCIP Optical Bench
HI HI-1 Telescope
HI-2 Telescope
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SECCHI Accommodationin Launch Configuration
SCIP-B Not VisibleFrom the Outside of theSpacecraft Stack
HI-AHI-B
SCIP-A
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SECCHI Instrument Suite Accommodationson STEREO Observatory (+X Deck View)
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SECCHI Instrument Suite Accommodationson STEREO Observatory (-Z Deck View)
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SECCHI Physical Block Diagram
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SECCHI Electrical Block Diagram
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SECCHI Instrument SuiteOrganizational Responsibilities
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Backup
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Image Positional Accuracy Requirements Based on Velocity Accuracyand Number of Images for CME / Solar Wind Evolution Analysis
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SECCHI Observation Requirement Set Metric Relationship to theDerived Quantities in the STEREO Measurement Requirements
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SECCHI Observation Requirement Subset for EUV Emission and Visible Light Images
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SECCHI Observation Requirement Subset for 3D Images
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Image Cadence Goals to Capture CME Evolution Over Individual Coverage Regions
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