Chowdhary, J., B. Cairns, M.I. Mishchenko, and L.D. Travis, 2005: Using multi-angle multispectral photo -
polarimetry of the NASA Glory mission to constrain optical properties of aerosols and clouds: results from four field experiments.
In
Polarimetry of Stars and Planetary Systems.
AMiBA, a millimeter interferometer like ALMA, was constructed by ASIAA (Academia Sinica Institute of Astronomy and Astrophysics) and National Taiwan University for
polarimetry of microwave background radiation and detection of distant clusters of galaxies using the Sunyaev Zeldovich effect.
Here we present new J - band imaging
polarimetry of LkCa 15 with SPHERE IRDIS, yielding the most accurate and detailed scattered - light images of the disk to date down to the planet - hosting inner regions.
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.
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 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.
Not exact matches
The enhanced X-Ray Timing and
Polarimetry (eXTP) mission would be China's most ambitious space science satellite yet — and its most expensive, with an estimated price tag
of $ 473 million.
One source
of excitement is a $ 440 - million X-ray telescope led by the CNSA, called Enhanced X-ray Timing and
Polarimetry (eXTP).
«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).
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.
«This observation has certainly verified the high capability
of the
polarimetry observation with ALMA,» said Hiroshi Nagai at the National Astronomical Observatory
of Japan and the leader
of the verification team.
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.
See also: ALMA News as
of July 19, 2016 «ALMA Achieved Highest Sensitivity
Polarimetry in Millimeter Wavelength»
Using novel instrumentation SON has a network
of telescopes that, while
of modest aperture, now have unique capabilities to do 1e - 5 broadband
polarimetry.
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.
Rapid development
of anisotropic ice.crystal - alignment fabrics inferred from englacial radar
polarimetry, central West Antarctica.
By using a low - scattered light telescope with the contrast enhancement techniques
of coronagraphy and
polarimetry, regions around extremely bright sources can be seen.
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.
They used a single 360 degree camera around the horizontal plane
of the targets and used both light microscopy and full - body video -
polarimetry.
The main techniques will be high - dynamic range imaging, imaging
polarimetry, aperture
polarimetry, spectropolarimetry, coronagraphy, and adaptive optics assistance for many
of these techniques.
He is also the founder and president
of the SearchLight Observatory Network (SON), which leads a worldwide campaign for doing ultra-sensitive
polarimetry.
Braak, C.J., J.F. de Haan, J.W. Hovenier, and L.D. Travis, 2002: Spatial and temporal variations
of Venus haze properties obtained from Pioneer Venus Orbiter
polarimetry.