Search references for X RAY-INTERFEROMETER. Phrases containing X RAY-INTERFEROMETER
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An X-ray interferometer is analogous to a neutron interferometer. It has been suggested that it may offer the very highest spatial resolution in astronomy
X-ray_interferometer
Imaging systems using changes in phase
interferometry or X-ray Talbot interferometry (XTI), and polychromatic far-field interferometry (PFI). Since the first X-ray grating interferometer—consisting
Phase-contrast_X-ray_imaging
Interferometer using neutron diffraction to make precise measurements
time-dilation differences along the two paths. Like X-ray interferometers, neutron interferometers are typically made from a single large crystal of silicon
Neutron_interferometer
Form of electromagnetic radiation
Nöhammer B, Solak H, Ziegler (2002). "Differential x-ray phase contrast imaging using a shearing interferometer". Applied Physics Letters. 81 (17): 3287–3289
X-ray
Measurement method using interference of waves
Solak, H H & Ziegler E (2002). "Differential x-ray phase contrast imaging using a shearing interferometer". Applied Physics Letters. 81 (17): 3287–3289
Interferometry
Material with a continuous, unbroken crystal lattice
fingerprint reader, optical disks for long-term data storage, and X-ray interferometer. Indium phosphide: these single crystals are particularly appropriate
Single_crystal
Gravitational-wave detector in Italy
interferometer is a large-scale scientific instrument near Pisa, Italy, for detecting gravitational waves. The detector is a Michelson interferometer
Virgo_interferometer
Gravitational wave observatory site
The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational
LIGO
Relativistic effect due to rotation
Sagnac effect manifests itself in a setup called a ring interferometer or Sagnac interferometer. A beam of light is split and the two beams are made to
Sagnac_effect
Telescope in the Atacama Desert, Chile
combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer also includes a set of four 1.8-metre
Very_Large_Telescope
Physics experiment
creating an interference pattern. Another version is the Mach–Zehnder interferometer, which splits the beam with a beam splitter. In the basic version of
Double-slit_experiment
Technique to characterize materials using X-ray radiation
X-ray spectroscopy is a general term for several spectroscopic techniques for characterization of materials by using x-ray radiation. When an electron
X-ray_spectroscopy
Taiwanese astrophysicist (b. 1932)
Today 17, 5, 21 (1964) "A Tunable X-ray Interferometer and the Empirical Determination of Phase Diffracted X-rays" "Supernovae, Neutrinos, and Neutron
Hong-Yee_Chiu
Former radio telescope in Green Bank, West Virginia
telescope interferometer that operated simultaneously at 2.25 and 8.3 GHz to monitor transient, galactic X-ray binaries, AGN's and Gamma-ray sources. Amongst
Green_Bank_Interferometer
Optical device with parallel mirrors
In optics, a Fabry–Pérot interferometer (FPI), or etalon, is an optical cavity made from two parallel reflecting surfaces (mirrors). Optical waves can
Fabry–Pérot_interferometer
Collapsed core of a massive star
and is associated with kilonovae and short gamma-ray bursts. In 2017, the LIGO and Virgo interferometer sites observed GW170817, the first direct detection
Neutron_star
Type of common-path interferometer
diffraction interferometer (PDI) is a type of common-path interferometer. Unlike an amplitude-splitting interferometer, such as a Michelson interferometer, which
Point diffraction interferometer
Point_diffraction_interferometer
Device that narrows or straightens a beam of particles or waves
a shearing interferometer. In X-ray optics, gamma ray optics, and neutron optics, a collimator is a device that filters a stream of rays so that only
Collimator
Method of detecting gravitational waves
interferometric gravitational-wave search refers to the use of extremely large interferometers built on the ground to passively detect (or "observe") gravitational
Ground-based interferometric gravitational-wave search
Ground-based_interferometric_gravitational-wave_search
XN – (celestial object) x-ray nova XRF – (celestial object) x-ray flash XRISM - X-Ray Imaging and Spectroscopy Mission, an X-ray space telescope (pronounced
List_of_astronomy_acronyms
Brightest star in the constellation Aquila
estimated breakup speed of 400 km/s. A study with the Palomar Testbed Interferometer revealed that Altair is not spherical, but is flattened at the poles
Altair
Series of NASA satellites
specific wavelength/energy regions of the electromagnetic spectrum: gamma rays, X-rays, visible and ultraviolet light, and infrared light. The Hubble Space
Great_Observatories_program
1887 investigation of the speed of light
{\textstyle vT_{3}} in the x direction. This inclined travel path follows from the transformation from the interferometer rest frame to the aether rest
Michelson–Morley_experiment
Description of physical properties at the atomic and subatomic scale
illustrating the discretization of energy for bound states. The Mach–Zehnder interferometer (MZI) illustrates the concepts of superposition and interference with
Quantum_mechanics
Phenomenon resulting from the superposition of two waves
double-slit experiment, laser speckle, anti-reflective coatings and interferometers. In addition to the classical wave model for understanding optical
Wave_interference
Physical model of propagating energy
radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, to gamma rays. All forms of EMR travel at the speed of light in a vacuum and exhibit
Electromagnetic_radiation
Astrophysical phenomenon
Supernovae". Supernovae and Gamma-Ray Bursters. Lecture Notes in Physics. Vol. 598. pp. 21–36. arXiv:astro-ph/0301107. CiteSeerX 10.1.1.256.2965. doi:10.1007/3-540-45863-8_3
Supernova
Instrument that makes distant objects appear magnified
from space. X-rays are much harder to collect and focus than electromagnetic radiation of longer wavelengths. X-ray telescopes can use X-ray optics, such
Telescope
Brightest star in the constellation Auriga
relatively close, at 42.9 light-years (13.2 parsecs). It is one of the brightest X-ray sources in the sky, thought to come primarily from the corona of Capella
Capella
NASA project
Constellation-X (Con-X) (cancelled - Merged with International X-ray Observatory (IXO)): the next-generation X-ray space observatory Laser Interferometer Space
Beyond_Einstein_program
mirror LOFT - Large Observatory For X-ray Timing Large Ultraviolet Optical Infrared Surveyor Large Interferometer For Exoplanets Nautilus Deep Space Observatory
List of proposed space telescopes
List_of_proposed_space_telescopes
Quantum states light can be in
quantities in laser interferometers, such as in Sagnac interferometers measuring rotation changes and in Michelson interferometers observing gravitational
Squeezed_states_of_light
analysis. Single-shot multi-contrast x-ray imaging gained its importance recently in contrast to Talbot–Lau interferometer because of the less optical element
Single-shot multi-contrast X-ray imaging
Single-shot_multi-contrast_X-ray_imaging
Type of stellar collision
GW170817 was observed in 2017. On 17 August 2017, the LIGO and Virgo interferometers observed GW170817, a gravitational wave associated with the merger
Neutron_star_merger
Supernova remnant in the constellation Cassiopeia
Cas X-1 is Cas A, a Type II SNR at RA 23h 18m Dec +58° 30′. The designations Cassiopeia X-1, Cas XR-1, Cas X-1 are no longer used, but the X-ray source
Cassiopeia_A
2015 detection made by LIGO interferometers
other interferometers of a similar size, such as the Virgo, GEO 600 and planned KAGRA and INDIGO detectors. In practice at least two interferometers would
First observation of gravitational waves
First_observation_of_gravitational_waves
Subfield of astronomy that studies celestial objects at radio frequencies
astronomy to achieve high angular resolution, as the resolving power of an interferometer is set by the distance between its components, rather than the size
Radio_astronomy
Study involving matter and electromagnetic radiation
been associated with a spectral signature in the context of the Laser Interferometer Gravitational-Wave Observatory (LIGO). Spectroscopy is a branch of science
Spectroscopy
Optical setup to obtain interference pattern by reflection
"Application Note 49: Theory of Lloyd's Mirror Interferometer" (PDF). Newport Corporation. Retrieved 16 February 2014. Li, X.; Shimizu, Y.; Ito, S.; Gao, W.; Zeng
Lloyd's_mirror
Swiss physicist (1854–1949)
Thunersee) was a Swiss physicist, one of the inventors of the Mach–Zehnder interferometer. Zehnder studied mechanical engineering in Zurich from 1873 to 1875
Ludwig_Zehnder
Spatial frequency of a wave
an essential role in optics and the physics of wave scattering, such as X-ray diffraction, neutron diffraction, electron diffraction, and elementary particle
Wavenumber
Gravitational-wave signal detected in 2017
degrees. In particular, the absence of a clear detection by the Virgo interferometer implied that the source was localized within one of its blind spots
GW170817
Belongs to a category of experiments
The Free-orbit Experiment with Laser Interferometry X-Rays (FELIX) belongs to a category of experiments exploring whether macroscopic systems can be in
Free-orbit experiment with laser interferometry X-rays
Free-orbit_experiment_with_laser_interferometry_X-rays
Ways in which length, distance or range can be measured
approaches are the rulers, followed by transit-time methods and the interferometer methods based upon the speed of light. Surveying is one ancient use
Length_measurement
Type of x-ray binary
Be–white dwarf X-ray binary systems (BeWDs) are a rare type of X-ray binary consisting of a white dwarf that accretes matter from a rapidly-rotating Be
Be–white dwarf X-ray binary system
Be–white_dwarf_X-ray_binary_system
Imaging method
analyzer crystal also for differential measurement, and x-ray interferometry uses a crystal interferometer to measure the phase directly. The advantages of these
Phase-contrast_imaging
gamma-rays. The development of space observatories after 1960 allowed access to several bands impossible to observe from the ground, including X-rays and
History_of_the_telescope
Scientific study of celestial objects
objects. A few observatories have been constructed, such as the Laser Interferometer Gravitational Observatory LIGO. LIGO made its first detection on 14
Astronomy
Extreme Magnetism - 2012 International X-ray Observatory - 2011 Terrestrial Planet Finder - 2011 Laser Interferometer Space Antenna - 2011 Space Interferometry
List_of_NASA_cancellations
Astronomical observatory in Hawaii
objects. The LWS is now retired from science observations. Keck Interferometer The Interferometer allowed the light from both Keck telescopes to be combined
W._M._Keck_Observatory
Galaxy in the constellation Serpens
Chandra X-ray Observatory, Hubble Space Telescope, Spitzer Space Telescope, the Very Large Array, and the Multi-Element Radio Linked Interferometer Network
3C_321
Small number of stars that orbit each other
of the system. Examples of binary systems are Sirius, Procyon and Cygnus X-1, the latter of which consists of a star and a black hole. Multiple-star
Star_system
Supermassive black hole at the center of the Milky Way
Horizon Telescope Collaboration. The image, which is based on radio interferometer data taken in 2017, confirms that the object contains a black hole.
Sagittarius_A*
Aspect of relativity in physics
Telescope, is under development. A space-based observatory, the Laser Interferometer Space Antenna (LISA), is also being developed by the European Space
Gravitational_wave
Concept in quantum optics
averaged over t. In optical interferometers such as the Michelson interferometer, Mach–Zehnder interferometer, or Sagnac interferometer, one splits an electric
Higher_order_coherence
Light all pointing in the same direction
X-rays are collimated to reduce the volume of the patient's tissue that is irradiated, and to remove stray photons that reduce the quality of the x-ray
Collimated_beam
laser Astrophysical maser Atmospheric-pressure laser ionization Atom interferometer Atom laser Atom probe Atomic clock Atomic coherence Atomic fountain
List_of_laser_articles
Fundamental principle of physics
x 1 + x 2 ) = F ( x 1 ) + F ( x 2 ) {\displaystyle F(x_{1}+x_{2})=F(x_{1})+F(x_{2})} and homogeneity F ( a x ) = a F ( x ) {\displaystyle F(ax)=aF(x)}
Superposition_principle
Compact astronomical body
it is indeed a black hole. X-ray binaries are binary systems that emit significant amounts of X-ray radiation. These X-ray emissions result when a compact
Black_hole
Nearest star to the Solar System
throughout the stellar body, and the resulting flare activity generates a total X-ray emission similar to that produced by the Sun. The internal mixing of its
Proxima_Centauri
Effort to find civilizations not from Earth
is designed to allow multiple observers simultaneous access to the interferometer output at the same time. Typically, the ATA snapshot imager (used for
Search for extraterrestrial intelligence
Search_for_extraterrestrial_intelligence
French physicist
his name to the Sagnac effect, a phenomenon which is at the basis of interferometers and ring laser gyroscopes developed since the 1970s. Sagnac was born
Georges_Sagnac
Locus of points at equal phase in a wave
sensor Common-path interferometer Foucault knife-edge test Multilateral shearing interferometer Ronchi tester Shearing interferometer Although an amplitude
Wavefront
Quantum physics thought experiment
packets associated with the field propagate along both paths of the interferometer, but only one packet contains a particle. The field aspect of the neutron
Wheeler's delayed-choice experiment
Wheeler's_delayed-choice_experiment
Cancelled NASA-ESA-JAXA space telescope project
program Chandra X-ray Observatory Constellation-X Observatory Great Observatories program Laser Interferometer Space Antenna Lynx X-ray Observatory XEUS
International X-ray Observatory
International_X-ray_Observatory
American astronomer
Ann Hornschemeier is an American astronomer specializing in X-ray emission from X-ray binary populations. She is the Chief Scientist for the Physics of
Ann_Hornschemeier
Hypothetical black hole formed soon after the Big Bang
the latter perspective having been strengthened by both LIGO/Virgo interferometer gravitational wave and JWST observations. Early constraints on PBHs
Primordial_black_hole
Observatory
The Multi-Element Radio Linked Interferometer Network (MERLIN) is an interferometer array of radio telescopes spread across England. The array is run from
MERLIN
System distributing location information about gamma-ray bursts
Super-Kamiokande, gravitational wave events from the LIGO, Virgo and KAGRA interferometers, and gamma-ray bursts observed by Fermi, Swift or INTEGRAL. One of the main
General_Coordinates_Network
German physicist
conventional, polychromatic X-ray sources and a grating interferometer. This enlarged the potential of X-ray phase imaging for clinical use as before the technique
Franz_Pfeiffer_(physicist)
Range of physical processes in physics
Near the end of the 19th century, the scattering of cathode rays (electron beams) and X-rays was observed and discussed. With the discovery of subatomic
Scattering
Red supergiant star in the constellation Orion
1920, Albert A. Michelson and Francis G. Pease mounted a six-meter interferometer on the front of the 2.5-meter telescope at Mount Wilson Observatory
Betelgeuse
Process to photograph fluid flow
laminar to turbulent flow. Laser schlieren deflectometry Mach–Zehnder interferometer Moire deflectometry Schlieren Schlieren imaging Shadowgraph Harvard
Schlieren_photography
British astronomer and astrophysicist (1947–2026)
February 2026) was a British astronomer and astrophysicist. Initially an X-ray astronomer, he also worked on instrumentation for space missions at other
Mike_Cruise
Astronomical object appearing as a bright blob, discovered by Hanny van Arkel
European VLBI Network (EVN) and the UK's Multi-Element Radio Linked Interferometer Network (MERLIN), proposed another related explanation. They hypothesized
Hanny's_Voorwerp
Active galactic nucleus (AGN) containing a supermassive black hole
visible object. Using small telescopes and the Lovell Telescope as an interferometer, they were shown to have a very small angular size. By 1960, hundreds
Quasar
Interference pattern
effect. The phase moiré effect is the basis for a type of broadband interferometer in x-ray and particle wave applications. It also provides a way to reveal
Moiré_pattern
System of two stars orbiting each other
hole. Probably the best known example of an X-ray binary is the high-mass X-ray binary Cygnus X-1. In Cygnus X-1, the mass of the unseen companion is estimated
Binary_star
Overview of the scientific field of astronomy
Ultraviolet astronomy – 10–320 nm X-ray astronomy – 0.01–10 nm Gamma-ray astronomy – Below 0.01 nm Cosmic ray astronomy – Cosmic rays, including plasma Neutrino
Outline_of_astronomy
evolution Stellar flare Stellar flux Stellar fog Stellar halo Stellar interferometer Stellar isochrone Stellar kinematics Stellar limb-darkening Stellar
List_of_stellar_properties
Brightest quasar from Earth located in the constellation Virgo
calculated from z. Using parallax methods with the Very Large Telescope interferometer yields an angular distance estimate of DA=1.80+0.32 −0.28 Gly (552+97
3C_273
Largest type of black hole
by astronomers Bruce Balick and Robert Brown using the Green Bank Interferometer of the National Radio Astronomy Observatory. They discovered a radio
Supermassive_black_hole
Research center at Stanford University
atomic and solid-state physics, chemistry, biology, and medicine using X-rays from synchrotron radiation and a free-electron laser as well as experimental
SLAC National Accelerator Laboratory
SLAC_National_Accelerator_Laboratory
Wave that remains in a constant position
^{2}X}{\partial x^{2}}}=(ik_{x})^{2}.} Solving for X(x), X ( x ) = A k x e i k x x + B k x e − i k x x . {\displaystyle X(x)=A_{k_{x}}e^{ik_{x}x}+B_{k_{x}}e^{-ik_{x}x}
Standing_wave
Foundational principle in quantum physics
x ) x ⋅ ( − i ℏ d d x ) ψ ( x ) d x − ∫ − ∞ ∞ ψ ∗ ( x ) ( − i ℏ d d x ) ⋅ x ψ ( x ) d x = i ℏ ⋅ ∫ − ∞ ∞ ψ ∗ ( x ) [ ( − x ⋅ d ψ ( x ) d x ) + d ( x ψ
Uncertainty_principle
Branch of astronomy using gravitational waves
are several ground-based laser interferometers which span several miles/kilometers, including: the two Laser Interferometer Gravitational-Wave Observatory
Gravitational-wave_astronomy
Quasar in the constellation Ursa Major
straight and steep. When imaged by MERLIN (Multi-Element Radio-linked Interferometer Network) at 1539 MHz, the western lobe is made up of two hotspots, a
3C_254
Property in optics
X-ray Physics. Wiley-VCH. p. 25. ISBN 978-0-470-97395-0. Gullikson, Eric. "X-Ray interactions with matter". Optical constants. The Center for X-Ray Optics
Refractive_index
This is a list of lists of telescopes. List of astronomical interferometers at visible and infrared wavelengths List of astronomical observatories List
Lists_of_telescopes
Arrangement of mirrors
light. They are also used in optical parametric oscillators and some interferometers. Light confined in the cavity reflects multiple times, producing modes
Optical_cavity
the Pacific founded 1890 – Albert A. Michelson proposes the stellar interferometer 1892 – George Ellery Hale finishes a spectroheliograph, which allows
Timeline of telescopes, observatories, and observing technology
Timeline_of_telescopes,_observatories,_and_observing_technology
Star in the constellation Boötes
measured using interferometric observations by the Navy Precision Optical Interferometer. The angular diameter, together with the star's distance, yield a radius
Beta_Boötis
Geoscientific research organization
Absolute Gravity Lab. Airborne magnetic and electromagnetic surveys. Laser Interferometer Seismological Observatory (LISO), for precision seismological observations
National Geophysical Research Institute
National_Geophysical_Research_Institute
Experiment measuring the speed of light in moving water
the relative speeds of light in moving water. Fizeau used a special interferometer arrangement to measure the effect of movement of a medium upon the speed
Fizeau_experiment
Brightest star in Earth's night sky
Richard Q. Twiss in 1959 at Jodrell Bank using their stellar intensity interferometer. In 2005, using the Hubble Space Telescope, astronomers determined that
Sirius
Quantum correlations related to wave-particle duality
Robert Hanbury Brown and Richard Q. Twiss introduced the intensity interferometer concept to radio astronomy for measuring the tiny angular size of stars
Hanbury Brown and Twiss effect
Hanbury_Brown_and_Twiss_effect
Measurement of electromagnetic radiation for astronomy
spectrum of electromagnetic radiation, including visible light, ultraviolet, X-ray, infrared and radio waves that radiate from stars and other celestial objects
Astronomical_spectroscopy
Character from Alice's Adventures in Wonderland
of its physical properties. To test this idea, researchers used an interferometer where neutron beams passed through silicon crystal. The crystal physically
Cheshire_Cat
Review of astronomy literature produced every ten years
Other priorities include Laser Interferometer Space Antenna (LISA) for measuring gravitational waves and International X-ray Observatory for investigating
Astronomy and Astrophysics Decadal Survey
Astronomy_and_Astrophysics_Decadal_Survey
Optical microscopy technique
of the object. Live cell imaging Phase-contrast imaging Phase-contrast X-ray imaging "The phase contrast microscope". Nobel Media AB. Zernike, F. (1955)
Phase-contrast_microscopy
X RAY-INTERFEROMETER
X RAY-INTERFEROMETER
Male
Scandinavian
 Variant spelling of Scandinavian Kai, CAY means "lord." Compare with another form of Cay.
Surname or Lastname
English (of Norman origin)
English (of Norman origin) : nickname denoting someone who behaved in a regal fashion or who had earned the title in some contest of skill or by presiding over festivities, from Old French rey, roy ‘king’. Occasionally this was used as a personal name.English : nickname for a timid person, from Middle English ray ‘female roe deer’ or northern Middle English ray ‘roebuck’.English : variant of Rye (1 and 2).English : habitational name, a variant spelling of Wray.Scottish : reduced and altered form of McRae.French : from a noun derivative of Old French raier ‘to gush, stream, or pour’, hence a topographic name for someone who lived near a spring or rushing stream, or a habitational name from a place called Ray.Indian : variant of Rai.
Boy/Male
Indian, Telugu
Lord Ram
Surname or Lastname
English
English : variant spelling of Ray 1–4.
Male
Hebrew
 Variant spelling of Hebrew Rav, RAB means "great" or "teacher." Compare with another form of Rab.
Male
English
Short form of English Raymond, RAY means "wise protector."
Female
Hebrew
(רֵעַ) Hebrew name RAYA means "friend." Compare with another form of Raya.
Male
English
Variant spelling of English Ray, RAE means "wise protector."Â
Boy/Male
American, Australian, British, Christian, English, German
Gray-haired
Boy/Male
English Teutonic Biblical Sanskrit
Ram.
Boy/Male
Scottish American Latin French German English
Grace.
Female
English
English name derived from the vocabulary word, GAY means "happy." Compare with masculine Gay.
Boy/Male
Hindu
Beam of light
Girl/Female
Australian, Christian
Sunshine; Bright; Day
Boy/Male
Shakespearean
Henry VI, Part 2' Lord Say.
Girl/Female
Scandinavian American
Doe.
Boy/Male
American, British, Christian, Danish, English, Finnish, French, German, Gujarati, Hindu, Indian, Kannada, Latin, Malayalam, Marathi, Scottish, Swedish, Tamil, Telugu
Regal; Counsellor; Abbreviation of Raymond; Advice; Beam of Light; Grace; Well Advised Protector; Wise Protector; Dear Brook; Abbreviation of R
Girl/Female
American, German, Hebrew, Latin, Scandinavian
Female Sheep; Ewe; Nickname of Rachel
Female
English
English name, possibly derived from the vocabulary word ray, RAE means "sunbeam."
Female
English
 English name derived from the vocabulary word, DAY means "day." Feminine form of Middle English Daye, meaning "day."
X RAY-INTERFEROMETER
X RAY-INTERFEROMETER
Boy/Male
Afghan, African, American, Arabic, Celebrity, Chinese, Danish, Finnish, French, German, Greek, Hebrew, Hindu, Indian, Iranian, Kannada, Lebanese, Malaysian, Muslim, Parsi, Pashtun, Sindhi, Swahili, Swedish, Tamil
God; Excellent; Noble; Sublime; Light; Lofty; To Ascend; Exalted One; Also Mohammad's Son-in-law; Elevated
Boy/Male
Hindu, Indian, Punjabi, Sikh
All Pervading Light; Lamp that Gives Light to All
Male
English
English unisex name derived from the month name, which was originally the seventh month of the Roman year, SEPTEMBER means "seventh."
Girl/Female
American, Australian, Dutch, French, German, Greek, Jamaican, Latin, Swedish
Rose Bush; Horse; Fame; Rose; A Flower Name; Form of Rose; Small Rose
Girl/Female
Muslim/Islamic
Of the Night
Boy/Male
Hindu, Indian
Name of Lord Shiva
Girl/Female
Tamil
Covered with gold
Boy/Male
American, Australian, British, Chinese, Danish, English, French, German, Italian, Latin
Eighth Child; This Name was Given to the Eighth Child in a Large Family
Boy/Male
American, Australian, Chinese, Christian, Dutch, Hebrew
Father of a Multitude; Breath; He who is High is Father; Diminutive of Abraham
Girl/Female
Muslim/Islamic
Clean tidy
X RAY-INTERFEROMETER
X RAY-INTERFEROMETER
X RAY-INTERFEROMETER
X RAY-INTERFEROMETER
X RAY-INTERFEROMETER
n.
The merrymaking of May Day.
n.
One of the component elements of the total radiation from a body; any definite or limited portion of the spectrum; as, the red ray; the violet ray. See Illust. under Light.
n.
Right of way. See below.
n.
Faith; as, by my fay.
n.
A symbol representing ten units, as 10, x, or X.
n.
One of a number of lines or parts diverging from a common point or center, like the radii of a circle; as, a star of six rays.
n.
Length of space; distance; interval; as, a great way; a long way.
n.
In a restricted sense, any of the broad, flat, narrow-tailed species, as the skates and sting rays. See Skate.
v. i.
To lay snares for rabbits.
superl.
Not distilled; as, raw water
superl.
Not tanned; as, raw hides
superl.
Gray-haired; gray-headed; of a gray color; hoary.
v. i.
To shine, as with rays.
n.
To send forth or shoot out; to cause to shine out; as, to ray smiles.
v. i.
To take a position; to come or go; as, to lay forward; to lay aloft.
n.
A species of armadillo of the genus Xenurus (X. unicinctus and X. hispidus); the tatouay.
n.
One of a system of diverging lines passing through a point, and regarded as extending indefinitely in both directions. See Half-ray.
adv.
Crosswise; in the form of an X.
n.
A line of light or heat proceeding from a radiant or reflecting point; a single element of light or heat propagated continuously; as, a solar ray; a polarized ray.
a.
Of or pertaining to the laity, as distinct from the clergy; as, a lay person; a lay preacher; a lay brother.