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Spectral stability - PowerPoint PPT Presentation


The Expanded Very Large Array

The Expanded Very Large Array

The Expanded Very Large Array. Michael P. Rupen NRAO/Socorro. Why Expand the VLA? Unique Radio Capabilities. Magnetic Fields. Low Obscuration. No dust no bias see inner cores, where the action is. Polarization Faraday rotation Zeeman splitting. Sgr A *. The Evolving Universe.

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478 views • 33 slides



NPP CrIS Long Wave FOV1 Spectral Noise Anomaly

NPP CrIS Long Wave FOV1 Spectral Noise Anomaly

NPP CrIS Long Wave FOV1 Spectral Noise Anomaly. Xin Jin NOAA/STAR ICVS & CrIS Cal/Val Team. LW calibration targets show spectral instability in the past three months (July ~ Sept. 2013). Only LW FOV1 has such an anomaly; all other bands/FOVs are good.

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340 views • 18 slides


Contents

Contents

Contents. Optical Fibers ; Optical Fiber Sensors; Microstructured Optical Fibers ; Suspended Core Fibers : Tapering; Setup; Spectral Response; Strain and Temperature Characterization; Conclusions. n 1. n 2. n 1. Optical Fiber.

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401 views • 13 slides


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