USA As Represented by Secretary of the Navy

David Mozurkewich

Sergio R Restaino

Henrique Schmitt

Arsen R Hajian

John Thomas Armstrong

J Thomas Armstrong

An interferometry system including a first telescope for simultaneously receiving a first optical/infrared signal and a first radio signal from a target; a second telescope configured to simultaneously receive a second optical/infrared signal and a second radio signal from the target; a first beam splitter communicatively connected to the first telescope, where the first beam splitter is configured to separate the first optical/infrared signal from the first radio signal; a second beam splitter communicatively connected to the second telescope, where the second beam splitter is configured to separate the second optical/infrared signal from the second radio; and a first optical/infrared interferometer configured to detect an interferometry image of the target using the first and second optical/infrared and radio signals.

Phasing an optical interferometer using the radio emission from the target being observed

A dispersing Fourier Transform interferometer (DFTS) includes a Fourier Transform Spectrometer having an input for receiving a source light and an output, and a dispersive element having an input coupled to the Fourier Transform Spectrometer output and an output for providing the resulting multiple narrowband interferogram outputs of different wavelengths representative of the source light input. A processor applies a sparse sampling algorithm for determining the best fit between a set of model interferograms and the set of data interferograms. The model interferogram is inferred as specified at a discrete set of lags, a difference is determined between the model interferogram and the data interferogram, and an optimization method determines the model interferogram best matched to the data interferogram. The DFTS interferometer improves the sensitivity of a standard FTS by including a dispersive element, increasing the SNR by a factor of (R)as compared to the FTS, where Ris the resolving power of the conventional dispersing spectrometer (i.e. R=&#x3bb;/&#x394;&#x3bb;).

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Seabrook, MD, United States of America

David Mozurkewich