SUMMARY
The PACS instrument of the Herschel Space Observatory exhibits a resolution of 5" at a scan speed of 20''/sec, which degrades to 10'' at 60''/sec. This degradation occurs because the bolometric detector cannot respond quickly enough to the increased scan speed, resulting in a smeared temperature-based signal that affects spatial resolution. The phenomenon is analogous to lag in analog TV cameras, where moving objects appear smeared due to insufficient time for the sensor to register the image fully. The relationship between scan speed and resolution is critical for effective data interpretation in astronomical observations.
PREREQUISITES
- Understanding of bolometric imaging systems
- Familiarity with the PACS instrument and its specifications
- Knowledge of signal processing in astronomical data
- Basic principles of angular resolution and scan speed in telescopes
NEXT STEPS
- Review the PACS observers manual for detailed specifications and operational guidelines
- Study the effects of scan speed on resolution in bolometric imaging systems
- Learn about the convolution of time sensitivity functions in signal processing
- Explore the principles of angular resolution in astronomical instruments
USEFUL FOR
Astronomers, astrophysicists, and researchers involved in observational astronomy, particularly those working with bolometric imaging and the Herschel Space Observatory.