Determining & Evaluating High Risk Conjunction Events
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Transcript of Determining & Evaluating High Risk Conjunction Events
Determining & Evaluating High Risk Conjunction Events
Improving Space Operations Workshop
Boulder, CO5 – 6 April 2011
Introduction
• Conjunction Assessment Process• Collision Probability• Sigma Level Analysis• Alignment of Radial Vectors• Collision Probability Sensitivity• Maximum Collision Probability• High Risk Events
Conjunction Assessment Process (1/2)
• Conjunction assessment is performed based on state and state uncertainty data generated and disseminated by the JSpOC.
• Close approach predictions are generated based on a 5-day screening span.
• Results are sent out daily, or more frequently for high risk conjunction events.
• Predictions are made using data from the JSpOC high-accuracy space object catalog.
Conjunction Assessment Process (2/2)
• The typical conjunction assessment process for a satellite program is to receive Orbital Conjunction Messages (OCMs) for secondary objects that are predicted to violate a designated screening volume around the primary satellite.
• OCMs contain sufficient data to calculate a Pc value; i.e., state vector and state uncertainty data.
• The screening volume must be large enough to capture close approaches with objects with a wide range of covariance sizes—this can result in large amounts of data and many conjunction events that are not a threat.
Collision Probability (1/2)
• Collision probability (Pc) is a measure of the overlap of the error distribution of the two objects, where the error distribution is given by the covariance matrix.
• When the covariances of the objects are combined, Pc can be thought of as the relationship of the miss vector to the combined covariance.
Primary & Secondary object with covariance ellipsoids
Combined covariance with keep-out region positioned by miss vector
Collision Probability (2/2)
• Pc is used as the primary measure of risk since it captures the miss distance, the relative geometry, and the associated uncertainty of the close approach.
• A conjunction assessment process based on miss distance alone does not account for the uncertainty inherent in the problem.
• Miss distance is used as the basis of the screening process, leading to the receipt of many OCMs for conjunction events with zero Pc values.
• This approach can lead to large amounts of data; especially for satellites in LEO.
Sigma Level Analysis (1/2)
• The miss vector and the state uncertainty of the two objects can be used for a streamlined screening process.
• The sigma level can be calculated using the Radial, Intrack, and Crosstrack (RIC) directions of the primary.
where and
• OCMs are not required for these calculations.
𝑅𝑎𝑑𝑖𝑎𝑙 𝑠𝑖𝑔𝑚𝑎𝑙𝑒𝑣𝑒𝑙=𝜌𝑅
𝜎𝑅𝑝+𝜎 𝑅𝑠
𝐼𝑛−𝑝𝑙𝑎𝑛𝑒𝑠𝑖𝑔𝑚𝑎𝑙𝑒𝑣𝑒𝑙=√𝜌 𝐼❑2+𝜌𝐶
❑2
𝜎 𝐼 𝑝+𝜎 𝐼 𝑠=
𝜌 𝐼𝐶
𝜎 𝐼𝑝+𝜎 𝐼𝑠
Sigma Level Analysis (2/2)
�̂�𝑝
𝐼𝑝�̂�𝑝
𝜌𝜌𝑅
• The two semi-major axes equal the largest possible in-plane uncertainty component, ; and the semi-minor axis equals the sum of the radial uncertainties, .
• A high sigma level from either calculation should result in a near zero Pc value, but a low sigma level does not necessarily lead to a high Pc value.
• A sigma level > 4 is recommended.
𝜌 𝐼𝐶𝜌𝐶
𝜌𝐶
Sigma Level Analysis Results
• Sample report of data required:
• Sample results with corresponding collision probability:
Predicted Miss Distances Primary Error at TCA Secondary Error at TCA
Total Radial Intrack Cross-track
Radial Intrack Cross-track
Radial Intrack Cross-track
Case Radial Sigma Level
In-plane Sigma Level
Collision Probability
1 2.29 0.35 7.78e-5
2 1.13 3.42 5.18e-9
3 -9.29 0.05 0
4 0.84 0.36 1.18e-3
5 4.17 0.09 4.74e-012
Alignment of Radial Vectors
• The Radial unit vectors of the two objects nearly align for conjunction events, therefore, the Radial direction can be decoupled from the Intrack and Crosstrack directions.
𝜑
�̂�𝑝
�̂�𝑝 𝐼𝑝𝜌 𝐼𝐶
𝑟𝑝 𝑟 𝑠
Earth center
�̂�𝑠
𝐼 𝑠
�̂� 𝑠
Since for tangible conjunction events, is small and the two Radial unit vectors can be considered collinear for the purposes of this analysis.
𝜌𝑅
𝜑
𝜌 𝐼𝐶
Collision Probability Sensitivity
• Covariance size can be scaled to determine the sensitivity of the Pc value.
• Since covariance is propagated from OD epoch to Time of Close Approach (TCA), a reduction in covariance size gives an indication of how the Pc will evolve.
• This calculation is performed with a static miss distance.
0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1-10
-9
-8
-7
-6
-5
-4
Normalized Covariance Size
log
Pc
Collision Probability Sensitivity
Maximum Collision Probability
• The Pc sensitivity curve allows evaluation of the Pc max condition.
• Pc max tends to occur when the miss vector lies on the 1-sigma uncertainty ellipsoid.
• Most conjunction events evolve to the left of the Pc max condition.
• Those that don’t tend to be of concern …
• Notice that in this example the covariance was enlarged to show Pc max.
0 0.5 1 1.5 2 2.5 3 3.5 4-10
-9
-8
-7
-6
-5
-4
-3
-2
Normalized Covariance Size
log
Pc
Pc .
0 0.5 1 1.5 2 2.5 3 3.5 40
2
4
6
8
10
12
Sig
ma
Leve
l
Collision Probability Sensitivity
Radial Sigma LevelIn-plane Sigma Level
High Risk Events
• Some conjunction events show little change in Pc as the covariance is contracted.
• This occurs when the miss vector is within the 1 or 2-sigma of the combined covariance ellipsoid.
• This condition can be a sign that the conjunction event will remain a threat as the TCA approaches.
0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1-4
-3.5
-3
-2.5
Normalized Covariance Size
log
Pc
Pc .
0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.5
1
1.5
2
2.5
Sig
ma
Leve
l
Collision Probability Sensitivity
Radial Sigma LevelIn-plane Sigma Level