Researchers have demonstrated ALMA's unprecedented capability for
polarimetry in millimeter wavebands.
See also: ALMA News as of July 19, 2016 «ALMA Achieved Highest Sensitivity
Polarimetry in Millimeter Wavelength»
Not exact matches
This is GPI imaging
polarimetry of the circumstellar disk around HR 4796A, a ring of dust and planetesimals similar
in some ways to a scaled up version of the solar system's Kuiper Belt.
«This is the very first step
in the research on dust evolution with
polarimetry, and I believe the future progress will be full of excitement.»
Only 55 million lightyears away, SN 2017cbv was one of the closest supernovae discovered
in recent years, found by the DLT40 survey using the Panchromatic Robotic Optical Monitoring and
Polarimetry Telescope (PROMPT)
in Chile, which monitors galaxies nightly at distances less than 40 megaparsecs (120 million light - years).
GPI imaging
polarimetry of the circumstellar disk around HR 4796A, a ring of dust and planetesimals similar
in some ways to a scaled up version of the solar system's Kuiper Belt.
We find that the near - side gap edge revealed by
polarimetry matches the sharp crescent seen
in previous ADI imaging very well.
A dedicated instrument for the direct detection of planets, SPHERE, is composed of a polametric camera
in visible light, the Zurich IMager POLarimeter (ZIMPOL), and two near - infrared sub-systems: the Infra - Red Dual - beam Imager and Spectrograph (IRDIS), a multi-purpose camera for imaging,
polarimetry, and long - slit spectroscopy, and the integral field spectrograph (IFS), an integral field spectrograph.
Here we present new J - band imaging
polarimetry of LkC... ▽ More LkCa 15 hosts a pre-transitional disk as well as at least one accreting protoplanet orbiting
in its gap.
Polarimetry is an important method to investigate magnetic fields
in the Universe and astronomers eager to use ALMA for unveiling magnetic mysteries, such as the launching mechanism of high energy jets from supermassive black holes.
The science verification activities for
polarimetry is introduced
in an article «Polarization observations with ALMA»
in the serial column Bienvenido a ALMA!»
HBOI researchers and colleagues collected more than 1,500 video -
polarimetry measurements from live fish from distinct habitats under a variety of viewing conditions, and have revealed for the first time that fish have an «omnidirectional» solution they use to camouflage themselves, demonstrating a new form of camouflage
in nature — light polarization matching.
By combining expertise from various fields — coronagraphy and high contrast imaging from solar physics, polishing,
polarimetry and adaptive optics from astronomical communities and the experience of each institutional partner, this telescope will make significant advances
in several fields.
In Polarimetry of Stars and Planetary Systems.
«Toward Exploring the Synergy Between Cloud Radar
Polarimetry and Doppler Spectral Analysis
in Deep Cold Precipitating Systems
in the Arctic.»