infrared astronomy

Optical radiation, visible, UV, and infrared

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TRAIL: Webel SysML Parsing Analysis example: Optical telescopes from Wikipedia: Structure and port-based light flow model

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Near Infrared: 2.0 to 2.4: Wavelength (micrometres): K band: Most major optical telescopes and most dedicated infrared telescopes

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Many optical telescopes, such as those at Keck Observatory, operate effectively in the near infrared as well as at visible wavelengths.

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For this reason, the near infrared region of the spectrum is commonly incorporated as part of the "optical" spectrum, along with the near ultraviolet.

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Infrared radiation with wavelengths just longer than visible light, known as near-infrared, behaves in a very similar way to visible light, and can be detected using similar solid state devices ...

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Far infrared (FIR) is a region in the infrared spectrum of electromagnetic radiation. Far infrared is often defined as any radiation with a wavelength of 15 micrometers (μm) to 1 mm

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Many new types of telescopes were invented including radio telescopes and infrared telescopes

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Tutorial

TRAIL: Webel SysML Parsing Analysis example: Optical telescopes from Wikipedia: Structure and port-based light flow model

Section

Slide kind

SysML Block Definition Diagram (BDD)

The wavelength of infrared light ranges from 0.75 to 300 micrometers. Infrared falls in between visible radiation, which ranges from 380 to 750 nanometers, and submillimeter waves.

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Infrared astronomy is the branch of astronomy and astrophysics that studies astronomical objects visible in infrared (IR) radiation.

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Infrared and optical astronomy are often practiced using the same telescopes, as the same mirrors or lenses are usually effective over a wavelength range that includes both visible and infrared light.

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Giant Magellan Telescope Integral-Field Spectrograph (GMTIFS) zone

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A Systems Modeling Language v1 (SysML^®) port-based light flow model of the Giant Magellan Telescope (GMT) and Giant Magellan Telescope Integral-Field Spectrograph (GMTIFS) instrument was created as part of work for the Advanced Instrumentation and Technology Centre (AITC) within the Research School of Astronomy and Astrophysics of the Australian National University (ANU) in late 2018.

A collated PDF slide set of exported SysML diagrams of this model may b

Optical telescopes

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Giant Magellan Telescope (GMT) zone

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A Systems Modeling Language v1 (SysML^®) port-based light flow model of the Giant Magellan Telescope (GMT) was created as part of work for the Advanced Instrumentation and Technology Centre (AITC) within the Research School of Astronomy and Astrophysics of the Australian National University (ANU) in late 2018.

A collated PDF slide set of exported SysML diagrams of this model may be made available to prospective consultancy or training clients

ANU Advanced Instrumentation and Technology Centre (AITC)

Webel IT Australia has held Systems Modeling Language v1 (SysML^®) training and consultancy for the Advanced Instrumentation and Technology Centre (AITC) of the Australian National University (ANU) at Mt Stromlo, Canberra, Australia.

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