Search results
Results From The WOW.Com Content Network
A staring array, also known as staring-plane array or focal-plane array (FPA), is an image sensor consisting of an array (typically rectangular) of light-sensing pixels at the focal plane of a lens. FPAs are used most commonly for imaging purposes (e.g. taking pictures or video imagery), but can also be used for non-imaging purposes such as ...
Focal-plane arrays (FPAs) are widely used in radio astronomy. FPAs are arrays of receivers placed at the focus of the optical system in a radio-telescope. The optical system may be a reflector or a lens. Traditional radio-telescopes have only one receiver at the focus of the telescope, but radio-telescopes are now starting to be equipped with ...
The design was physically large, being two focal lengths in length and one focal length in diameter. There are two menisci at the front and a single strong meniscus element at the rear. The rear element is close to the film plane for low distortion and better contrast but interferes with the mirror on a single-lens reflex camera.
The two telescope receivers would have been large format focal plane arrays of either 100 or 200 bolometric detectors. [2] The aim of the experiment was to measure the B-mode polarization of the Cosmic Microwave Background between multipoles of 20 and 1000 down to a sensitivity limited by the foreground contamination due to lensing.
The LSST camera sensor Life-size model of the LSST focal plane array. The array's diameter is 64 cm, and will provide 3.2 gigapixels per image. The image of the Moon (30 arcminutes) is present to show the scale of the field of view. The model is held by Suzanne Jacoby, the Rubin Observatory communications director.
Some of the sub-arrays of the SKA will also have a very large field-of-view (FOV), making it possible to survey very large areas of sky at once. [26] One innovative development is the use of focal-plane arrays using phased-array technology to provide multiple FOVs. [27]
The angular resolution R of an interferometer array can usually be approximated by = where λ is the wavelength of the observed radiation, and B is the length of the maximum physical separation of the telescopes in the array, called the baseline. The resulting R is in radians. Sources larger than the angular resolution are called extended ...
The Karl G. Jansky Very Large Array (VLA) is a centimeter-wavelength radio astronomy observatory in the southwestern United States built in the 1970s. It lies in central New Mexico on the Plains of San Agustin , between the towns of Magdalena and Datil , approximately 50 miles (80 km) west of Socorro .