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Radio telescope in central New Mexico
The Long Wavelength Array (LWA) is a radio telescope in central New Mexico. It began preliminary tests of the hardware in 2011, and began regular operations
Long_Wavelength_Array
Radio astronomy observatory in New Mexico, US
The Karl G. Jansky Very Large Array (VLA) is a centimeter-wavelength radio astronomy observatory in the southwestern United States built in the 1970s.
Very_Large_Array
Astronomical observatory in California, USA
spiral pattern. The Owens Valley Long Wavelength Array, commissioned in 2013, is a duplicate of the Long Wavelength Array in New Mexico. It consists of 288
Owens Valley Radio Observatory
Owens_Valley_Radio_Observatory
Subfield of astronomy that studies celestial objects at radio frequencies
Earth's surface are limited to wavelengths that can pass through the atmosphere. At low frequencies or long wavelengths, transmission is limited by the
Radio_astronomy
Directional radio antenna used in radio astronomy
Jansky's antenna was an array of dipoles and reflectors designed to receive short wave radio signals at a frequency of 20.5 MHz (wavelength about 14.6 meters)
Radio_telescope
International radio telescope project
Very Long Baseline Interferometry[unreliable source?] Electronic MultiBeam Radio Astronomy ConcEpt e-MERLIN Expanded Very Large Array Long Wavelength Array
Square_Kilometre_Array
Astronomical observatory in Cheshire, England
investigate cosmic rays. The equipment was a GL II radar system working at a wavelength of 4.2 m, provided by J. S. Hey. He intended to use the equipment in Manchester
Jodrell_Bank_Observatory
Effort to find civilizations not from Earth
lifted 3 kilometres (1.9 miles) above the ground in a dirigible tuned to a wavelength between 8 and 9 km, using a "radio-camera" developed by Amherst College
Search for extraterrestrial intelligence
Search_for_extraterrestrial_intelligence
Radio telescope at Jodrell Bank Observatory, Cheshire, England
of the dish so that it could be used on centimetre wavelengths, for research at these wavelengths for the Ministry as well as "other purposes". Although
Lovell_Telescope
Array of antennas creating a steerable beam
the size of an antenna array must extend many wavelengths to achieve the high gain needed for narrow beamwidth, phased arrays are mainly practical at
Phased_array
Class of directive antennas
reflector to be placed at 1⁄4 of a wavelength behind the elements, and this can be seen in many common reflector arrays like television antennas. However
Reflective_array_antenna
Radio pulsar in the constellation Leo
Off-pulse emissions from the young pulsar were detected by the Expanded Long Wavelength Array, suggesting the presence of a pulsar wind nebula around it. PSR
PSR_B0950+08
Former radio telescope in Puerto Rico, United States
tropic climate. The platform had a rotating, bow-shaped track 93 m (305 ft) long, called the azimuth arm, carrying the receiving antennas and secondary and
Arecibo_Telescope
It is located at the Long Wavelength Array site, adjacent to the Very Large Array. LEDA principally comprises a "large-N" array correlator (512 inputs
Large Aperture Experiment to Detect the Dark Ages
Large_Aperture_Experiment_to_Detect_the_Dark_Ages
at the Longest Wavelengths (DSL) project, is a planned Chinese space mission. The basic concept of the project is to launch an array of satellites to
Hongmeng_project
Welsh physicist (1911–1991)
Latin American Millimeter Array (LLAMA, Argentina/Brazil) Long Wavelength Array (LWA, New Mexico, US) Low-Frequency Array (LOFAR, Netherlands) MeerKAT
Edward_George_Bowen
Canadian radio telescope
Intensity and Real-time Analysis eXperiment (HIRAX), a proposed radio telescope array in South Africa in the same frequency band as CHIME Canadian Hydrogen Observatory
Canadian Hydrogen Intensity Mapping Experiment
Canadian_Hydrogen_Intensity_Mapping_Experiment
Physics research center
SETI Research Center has several SETI searches operating at various wavelengths, from radio, through infrared, to visible light. These include SERENDIP
Berkeley_SETI_Research_Center
Topics referred to by the same term
Local welfare assistance scheme, program related to Social Fund Long Wavelength Array, radio telescope in New Mexico LTE-WLAN Aggregation, a way of combining
LWA
interferometric array of 1024 6-meter (20ft) diameter radio telescopes, operating at 400-800MHz, that will be deployed at the Square Kilometer Array site in the
Hydrogen Intensity and Real-time Analysis eXperiment
Hydrogen_Intensity_and_Real-time_Analysis_eXperiment
Radio telescope network located mainly in the Netherlands
Kilometre Array Pathfinder Giant Metrewave Radio Telescope Long Wavelength Array (LWA) LORUN: LOFAR at Radboud University Nijmegen MeerKAT: Karoo Array Telescope
Low-Frequency_Array
Fiber-optic communications technology
In fiber-optic communications, wavelength-division multiplexing (WDM) is a technology which multiplexes a number of optical carrier signals onto a single
Wavelength-division multiplexing
Wavelength-division_multiplexing
Ability of any image-forming device to distinguish small details of an object
of the wavelength of the waves to the aperture width. For this reason, high-resolution imaging systems such as astronomical telescopes, long distance
Angular_resolution
Object detection system using radio waves
phase gradient across the array. For example, array elements producing a 5 degree phase shift for each wavelength across the array face will produce a beam
Radar
American mathematical physicist (1910–1994)
has been abandoned, similar research continues at the much larger Long Wavelength Array in central New Mexico. In early November 1959, President Dwight
Charles_Critchfield
Image sensor made of light-sensing pixels
P D (2005-05-01). "1024 × 1024 pixel mid-wavelength and long-wavelength infrared QWIP focal plane arrays for imaging applications". Semiconductor Science
Staring_array
Observatory in northern California, USA
the Western United States. The observatory is home to the Allen Telescope Array and one of the three CHIME FRB outriggers, as well a number of other smaller
Hat_Creek_Radio_Observatory
Chinese radio astronomy experiment
interferometric imaging radio telescope arrays have been built for this experiment. These are the cylinder array and the dish array. In the full-scale stage, the
Tianlai_experiment
66-telescope radio observatory in Chile
observe electromagnetic radiation at millimeter and submillimeter wavelengths. The array has been constructed on the 5,000 m (16,000 ft) elevation Chajnantor
Atacama Large Millimeter Array
Atacama_Large_Millimeter_Array
radio astronomy. The list includes both single dishes and interferometric arrays. The list is sorted by region, then by name; unnamed telescopes are in reverse
List_of_radio_telescopes
Observatory
Detail from below Plaque inside the building Historical control electronics Array of brushes. The brushes allowed the mirror to move continuously in the military
Stockert_Radio_Telescope
Antenna consisting of two rod-shaped conductors
intended wavelength (or frequency) of operation. The most commonly used is the center-fed half-wave dipole which is just under a half-wavelength long. The
Dipole_antenna
Infrared imaging used to reveal temperature
thermal imaging cameras use focal plane arrays (FPAs) that respond to longer wavelengths (mid- and long-wavelength infrared). The most common types are InSb
Thermography
System of ten radio telescopes
other small measurement errors. The Very Long Baseline Array usually makes radio observations at wavelengths from three millimeters to 90 centimeters
Very_Long_Baseline_Array
Antenna constructions for different applications
long wavelengths in the lower HF band the array may be made of ground-mounted monopoles instead of dipoles. Yagi–Uda coplanar parasitic dipole array,
Antenna_types
Dispersive optical device
disperser with high wavelength resolving power. In a virtually imaged phased array, the phased array is the optical analogue of a phased array antenna at radio
Virtually_imaged_phased_array
Spectrograph equipped with an integral field unit
combine spectrographic and imaging capabilities in the optical or infrared wavelength domains (0.32 μm – 24 μm) to get from a single exposure spatially resolved
Integral_field_spectrograph
Set of multiple antennas which work together
d=\lambda /2} , with λ {\displaystyle \lambda } being the wavelength, then the magnitude of the array factor has a period, in the domain of u {\displaystyle
Antenna_array
observatories are located in space to observe astronomical objects in wavelengths of the electromagnetic spectrum that cannot penetrate the Earth's atmosphere
List of astronomical observatories
List_of_astronomical_observatories
Array used for astronomical observations
research at radio wavelengths, leading to the development of large instruments such as the Very Large Array and the Atacama Large Millimeter Array. Optical/infrared
Astronomical_interferometer
Type of phased-array radar
active electronically scanned array (AESA) is a type of phased array antenna, which is a computer-controlled antenna array in which the beam of radio waves
Active electronically scanned array
Active_electronically_scanned_array
Loudspeaker system composed of linearly-mounted, in-phase speakers
At frequencies below 100 Hz (wavelength of 11.3 feet (3.4 m)) the line array which is less than approximately 3 meter long will start to become omnidirectional
Line_array
Class of large multielement directional wire radio transmitting antennas
of short wavelength radio waves and to determine their suitability for long-distance transmissions. Franklin invented the first curtain array aerial system
Curtain_array
Type of radio antenna consisting of a loop or coil
or full-wave loops; they have a perimeter close to one or more whole wavelengths at the operating frequency, which makes them self-resonant at that frequency
Loop_antenna
New class of galactic astronomical transients - LPTs
naturally explains sources found in binaries, and is supported by multi-wavelength detections of optical counterparts that hint at white dwarf companions
Long_Period_Radio_Transients
Imaging instrument aboard the James Webb Space Telescope
both the short and long wavelengths; however, the short wavelength arm has twice the resolution. The long wavelength arm has one array per side (two overall)
NIRCam
Global radio telescope array
(EHT) is a telescope array consisting of a global network of radio telescopes. The EHT project combines data from several very-long-baseline interferometry
Event_Horizon_Telescope
Regions of an electromagnetic field
vanish a few wavelengths away from the radiating part of the antenna, and conversely ensure that at distances a small fraction of a wavelength from the antenna
Near_and_far_field
Series of cosmic microwave background experiments at the South Pole
sky at 100 and 150 GHz (3 mm and 2 mm wavelength) with an angular resolution of 1.0 and 0.7 degrees. It had an array of 98 detectors (50 at 100 GHz and 48
BICEP_and_Keck_Array
Multi-wavelength imaging method
acquire images of an area at different wavelengths, and snapshot hyperspectral imagers, which uses a staring array to generate an image in an instant. Whereas
Hyperspectral_imaging
Research project to observe air showers
The Telescope Array project is an international collaboration involving research and educational institutions in Japan, The United States, Russia, South
Telescope_Array_Project
Form of electromagnetic radiation
with wavelengths longer than that of visible light but shorter than microwaves. The infrared spectral band begins with the waves that are just longer than
Infrared
Color model based on red, green and blue
wavelengths would activate both the medium and long wavelength cones of the retina, but not equally—the long-wavelength cells will respond more. The difference
RGB_color_model
Gravitational-wave astronomy technique
applications for pulsar timing arrays, the best known is the use of an array of millisecond pulsars to detect and analyse long-wavelength (i.e., low-frequency)
Pulsar_timing_array
US Naval Station in California
com. "Long Wavelength Array". www.phys.unm.edu. Kassim, N. E.; Polisensky, E. J. (2005). "2005ASPC..345..114K Page 114". From Clark Lake to the Long Wavelength
Field_Clark's_Dry_Lake
use a similar spectrometer and data processing unit to BIRS. The Long Wavelength Array (LWA) was 'inspired by Bill Erickson's historical legacy' and BIRS
Bruny Island Radio Spectrometer
Bruny_Island_Radio_Spectrometer
Radio aerial composed of directly-connected and passive elements
create a particular radiation pattern. A two-element array with the elements spaced a quarter wavelength apart has a distinct cardioid radiation pattern when
Driven_and_parasitic_elements
Isolated radio pulsar in the constellation Puppis
(2020-08-11). "Detecting pulsar polarization below 100 MHz with the Long Wavelength Array". Monthly Notices of the Royal Astronomical Society. 496 (3): 3623–3634
PSR_B0628−28
Concept in the psychophysics of vision
inter-converted if modulation depth is known) illumination intensity; the wavelength (or wavelength range) of the illumination (this parameter and the illumination
Flicker_fusion_threshold
Device that transmits and receives radio waves
half-wavelengths in length) at about the same frequency, as is the case where the conductors are all part of the same active or passive antenna array. Because
Antenna_(radio)
Electromagnetic radiation with wavelengths from 1 m to 1 mm
electromagnetic radiation with wavelengths shorter than other radio waves but longer than infrared waves. Its wavelength ranges from about one meter to
Microwave
Russian military radar system
first radar with an active electronically scanned array (AESA) antenna operating at meter wavelengths. The radar was introduced in 2001 as a replacement
Nebo-SVU
by the University of Tasmania; the 22m dish of Mopra, part of the Long Baseline Array, operated by CSIRO; the 25m dish of Sheshan near Shanghai, operated
Joint Institute for Very Long Baseline Interferometry European Research Infrastructure Consortium
Joint_Institute_for_Very_Long_Baseline_Interferometry_European_Research_Infrastructure_Consortium
Color filter array
A Bayer filter mosaic is a color filter array (CFA) for arranging RGB color filters on a square grid of photosensors. Its particular arrangement of color
Bayer_filter
American astronomer
Astronomy Department of the University of New Mexico, working on the Long Wavelength Array project from 2005-2018. American Astronomical Society's Harlow Shapley
Hélène_R._Dickel
1990s astrophysics experiment in Utah
Shower Array (CASA) was a significant ultra high high-energy astrophysics experiment operating in the 1990s. It consisted of a very large array of scintillation
Chicago_Air_Shower_Array
Scattering from arrays of atoms
fronts scattered by lattice planes leads to a strict relation between the wavelength and scattering angle. This law was initially formulated for X-rays, but
Bragg's_law
Citizen science project
Twenty-Centimeters (FIRST) survey which was observed at the Very Large Array between 1993 and 2011. Also used was data from the Australia Telescope Large
Radio_Galaxy_Zoo
Process of hair removal by exposure to laser pulses
output wavelengths between 400 nm and 1200 nm. Filters are applied to block shorter wavelengths, thereby only using the longer, "redder" wavelengths. IPLs
Laser_hair_removal
Radio telescope array in California
The Allen Telescope Array (ATA), formerly known as the One Hectare Telescope (1hT), is a radio telescope array dedicated to astronomical observations and
Allen_Telescope_Array
state active phased array antenna Selex RAN-40L – 3D multibeam long range L-Band radar with a fully solid state active phased array antenna J/FPS-1 J/FPS-2
List_of_radars
metro and long-haul dense wavelength-division multiplexing (WDM) systems. The company had a patented a Distributed Feedback Laser (DFB)-array technology
Santur_Corporation
Perception caused by wavelengths of light
the wavelength of light, in this case, air molecules), the luster of opals, and the blue of human irises. If the microstructures are aligned in arrays, for
Color
Astronomical radio observatory
operate a radio telescope at submillimeter wavelengths, that can work in stand alone mode or join a Very Long Baseline Interferometry (VLBI) network. The
Large Latin American Millimeter Array
Large_Latin_American_Millimeter_Array
Type of radio antenna
wavelength, depending on the specific design. The directors are slightly shorter than the driven element, while the reflector(s) are slightly longer.
Yagi–Uda_antenna
Comparing widely separated telescope wavefronts
Very Long Baseline Array (VLBA), which uses ten dedicated, 25-meter telescopes spanning 5351 miles across the United States, is the largest VLBI array that
Very-long-baseline interferometry
Very-long-baseline_interferometry
Form of radar used to create images of landscapes
large-aperture (in one dimension) phased array. The SAR simulates (rather than synthesizes) that long one-dimensional phased array. Although the term in the title
Synthetic-aperture_radar
Technique to analyze the infrared spectrum of matter
50 μm (200 cm−1) became known as the far-infrared region; at very long wavelengths it merges into the microwave region. Measurements in the far infrared
Fourier-transform infrared spectroscopy
Fourier-transform_infrared_spectroscopy
Star system in the constellation Ara
confirmed source of long-period radio transients (LPTs). The object was first detected by the Australian Square Kilometre Array Pathfinder (Murchison
ASKAP_J1745-5051
Radio observatory in France
telescopes in the world. Long established are also the radio heliograph, a T-shaped array, and the decametric array operating at wavelengths between 3 m and 30 m
Nançay_Radio_Observatory
Type of radio antenna
at VHF and UHF frequencies in place of a quarter-wavelength whip antenna, which is inconveniently long and cumbersome at these frequencies. Many years
Rubber_ducky_antenna
Optical device for selecting part of a spectrum
mechanically selectable narrow band of wavelengths of light or other radiation chosen from a wider range of wavelengths available at the input. The name is
Monochromator
Radio telescope in Western Australia
Widefield Array (MWA) is a joint project between an international consortium of organisations to construct and operate a low-frequency radio array. "Widefield"
Murchison_Widefield_Array
Instrument that makes distant objects appear magnified
(electromagnetic radiation) in different frequency bands. As wavelengths become longer, it becomes easier to use antenna technology to interact with
Telescope
Telescope in the Atacama Desert, Chile
larger simultaneous wavelength coverage. A new detector focal plane array of three Hawaii 2RG detectors with a 5.3 μm cut-off wavelength replaced the existing
Very_Large_Telescope
Practical physics application
LED is a long-lived light source, but certain mechanisms can cause slow loss of efficiency of the device or sudden failure. The wavelength of the light
Light-emitting_diode_physics
Flash of gamma rays from a distant galaxy
After the initial flash of gamma rays, a longer-lived afterglow is emitted, usually in the longer wavelengths of X-ray, ultraviolet, optical, infrared
Gamma-ray_burst
Color space represented by the response of the three types of cones of the human eye
eye, named for their responsivity (sensitivity) peaks at long, medium, and short wavelengths. The numerical range is generally not specified, except that
LMS_color_space
Information method in electromagnetic radiation
modulation of the phase, frequency or both of electromagnetic radiation in the wavelength band of visible or infrared light. The light signal is compared with standard
Optical_heterodyne_detection
composed of four detectors that operated simultaneously at different wavelengths; all four were in use until 2009 May 15 when the Spitzer cryostat ran
Infrared_Array_Camera
Radio telescope array
were arranged in a 'compact array', with a maximum baseline of about 100 m. All antenna pairs were correlated, so some long baseline data were always available
Ryle_Telescope
Astronomy with terahertz (< 1 mm)-range light
astronomy project, the Atacama Large Millimeter Array (ALMA), an interferometer for submillimetre wavelength observations made of 54 12-metre and 12 7-metre
Submillimetre_astronomy
Class of radio antenna
since they are more compact. Monopoles five-eights (5/8 = 0.625) of a wavelength long are also common, because at this length a monopole radiates a maximum
Monopole_antenna
Range of spectroscopic analysis
intensity may be measured as a function of wavelength. Fixed monochromators are used with CCDs and photodiode arrays. As both of these devices consist of many
Ultraviolet–visible spectroscopy
Ultraviolet–visible_spectroscopy
Lithography using 13.5 nm UV light
function of incident angle and wavelength, with longer wavelengths reflecting more near normal incidence and shorter wavelengths reflecting more away from
Extreme ultraviolet lithography
Extreme_ultraviolet_lithography
South Pole experiment for detecting ultra high energy electron neutrinos
radio coherence. Experimentally, the goal was to detect and measure long-wavelength (radiofrequency) pulses resulting from this interaction. The experiment
Neutrino Array Radio Calibration
Neutrino_Array_Radio_Calibration
Microwave antenna
This simulates the properties of a dielectric at microwave wavelengths by a 3 dimensional array of small metal conductors, such as spheres, strips, discs
Lens_antenna
Range 3-30 GHz of the electromagnetic spectrum
frequencies is also known as the centimetre band or centimetre wave as the wavelengths range from one to ten centimetres. These frequencies fall within the
Super_high_frequency
Early warning radar
television broadcast band), that is a wavelength of 71–67 cm, with circular polarization. It is an active array (AESA); each of the 1,792 transmitting
PAVE_PAWS
Fleet of truck-mounted weather radars
quickly deployable truck-mounted weather radars managed by FARM (Flexible Array of Radars and Mesonets), an American research company affiliated with the
Doppler_on_Wheels
LONG WAVELENGTH-ARRAY
LONG WAVELENGTH-ARRAY
Surname or Lastname
English and French
English and French : nickname for a tall person, from Old English lang, long, Old French long ‘long’, ‘tall’ (equivalent to Latin longus).Irish (Ulster (Armagh) and Munster) : reduced Anglicized form of Gaelic Ó Longáin (see Langan).Chinese : from the name of an official treasurer called Long, who lived during the reign of the model emperor Shun (2257–2205 bc). his descendants adopted this name as their surname. Additionally, a branch of the Liu clan (see Lau 1), descendants of Liu Lei, who supposedly had the ability to handle dragons, was granted the name Yu-Long (meaning roughly ‘resistor of dragons’) by the Xia emperor Kong Jia (1879–1849 bc). Some descendants later simplified Yu-Long to Long and adopted it as their surname.Chinese : there are two sources for this name. One was a place in the state of Lu in Shandong province during the Spring and Autumn period (722–481 bc). The other source is the Xiongnu nationality, a non-Han Chinese people.Chinese : variant of Lang.Cambodian : unexplained.
Boy/Male
Anglo, Australian, British, Chinese, Dutch, English, German, Norse, Scandinavian
Long; Wave; Tall Man
Female/Male/Unisex
Korean
 Korean unisex name YONG means "courage." Compare with another form of Yong.
Surname or Lastname
English
English : unexplained.Chinese : from an ancient area named Cong Yang, whose residents adopted the surname.Vietnamese : unexplained.
Boy/Male
Gaelic
Fierce.
Boy/Male
French, German, Polish
Long
Girl/Female
Hindu
Beauty, Pretty
Male
English
 English short form of Spanish Alonso, LON means "noble and ready." Compare with another form of Lon.
Boy/Male
Anglo, Australian
Long
Boy/Male
Korean
East.
Boy/Male
American, Australian, Chinese, Malaysian
Dragon; Grand
Surname or Lastname
English
English : variant of Long 1.German and French (Alsace–Lorraine) : from Middle High German lunge ‘lung’, presumably applied as a nickname.Chinese : variant of Long 3.Chinese : variant of Long 4.
Boy/Male
Chinese
Intelligent.
Surname or Lastname
Norwegian
Norwegian : habitational name from any of several farmsteads in southwestern Norway, named with Old Norse lón ‘calm, deep pool (in a river)’.English : variant of Lane.Muslim : unexplained.
Surname or Lastname
English
English : nickname for the taller of two men with the same name, from Old English leng(ra) ‘longer’, ‘taller’, comparative of lang (see Lang).German : variant of Lang.Chinese : from an ancient official title, Lingguan, denoting a court official in charge of music. The character for Ling is written similarly to that for Leng (), and the surname evolved to the latter form.Cambodian : unexplained.
Girl/Female
Greek American Hawaiian English
Surname or Lastname
English (mainly East Anglia)
English (mainly East Anglia) : habitational name from Lyng in Norfolk, so named from Old English hlinc ‘hillside’, or from either of two places in Norfolk and Lincolnshire named Ling, from Old Norse lyng ‘ling’, ‘heather’. There is also a Lyng in Somerset, so named from Old English lengen ‘long place’.German : variant of Link.Chinese : from a word meaning ‘ice’. In ancient times, the imperial palace was able to enjoy ice in the summer by storing winter ice in a cellar, entrusting its care to an official called the iceman. This post was once filled during the Zhou dynasty (1122–221 bc) by a descendant of Kang Shu, the eighth son of Wen Wang, who had been granted the state of Wei soon after the establishment of the Zhou dynasty. Descendants of this particular iceman adopted the word for ice, ling, as their surname.
Girl/Female
English American
Solitary.
Surname or Lastname
Chinese
Chinese : variant of Tang 2.Chinese : variant of Tang 3.Chinese : from a modification of the character Zhong (). In the Xia dynasty (2205–1766 bc), there existed a senior adviser whose name was Zhonggu. Much later, in the Ming dynasty (1368–1644 ad), some descendants settled along a river that became known as the Tong Family river. As the Manchus moved southwards, some took up residence by this river and they too adopted Tong as their surname.Chinese : from Lao Tong, the ‘style name’ given to a son of Zhuan Xu, legendary emperor of the 26th century bc. Two of his sons became important advisers to the next emperor, Ku. Some descendants of Lao Tong adopted a character from his style name as their surname.Chinese : see also Dong.English : metonymic occupational name for a maker or user of tongs (Old English tang(e)), or a habitational name from one of the places named with this word (there are examples in Lancashire, Shropshire, and West Yorkshire), from their situation by a fork in a road or river, considered as resembling a pair of tongs.English : topographic name for someone who lived on a tongue of land, or a habitational name from a place named with this word (Old English tunge, Old Norse tunga), for example Tonge in Leicestershire.Dutch : from a short form of the personal name Antonius (see Anthony). It could also be from Dutch tong ‘tongue’ and hence a nickname for a chatterbox or scold, or possibly a shortening of Van Tongeren, a habitational name for someone from Tongeren in the province of Gelderland.
Surname or Lastname
English (Merseyside)
English (Merseyside) : unexplained.
LONG WAVELENGTH-ARRAY
LONG WAVELENGTH-ARRAY
Boy/Male
Arabic
Secrecy; Privacy
Girl/Female
Hindu, Indian
Love; Beauty; Speak Less; Brilliant
Boy/Male
Tamil
Mairava
Boy/Male
Hindu, Indian, Telugu
Cloud
Boy/Male
Hebrew American Scottish
God is my judge.
Boy/Male
Muslim
One who prostrates to the merciful (Allah)
Surname or Lastname
English
English : variant of Foulks.Possibly also an Anglicized form of French Fouquet.
Girl/Female
Gujarati, Indian, Russian
Vigilant
Boy/Male
Hebrew American English
Promise.
Girl/Female
Hindu, Indian, Tamil
Loving Actions
LONG WAVELENGTH-ARRAY
LONG WAVELENGTH-ARRAY
LONG WAVELENGTH-ARRAY
LONG WAVELENGTH-ARRAY
LONG WAVELENGTH-ARRAY
a.
Long-breathed; hence, tediously long in speaking; consuming much time; as, a long-winded talker.
superl.
Extended to any specified measure; of a specified length; as, a span long; a yard long; a mile long, that is, extended to the measure of a mile, etc.
a.
Having the power of retaining the breath for a long time; long-winded.
n.
A long sound, syllable, or vowel.
adv.
To a great extent in apace; as, a long drawn out line.
a. & adv.
Long.
a.
Having a long tongue.
adv.
At a point of duration far distant, either prior or posterior; as, not long before; not long after; long before the foundation of Rome; long after the Conquest.
superl.
Drawn out in a line, or in the direction of length; protracted; extended; as, a long line; -- opposed to short, and distinguished from broad or wide.
n.
Long patience of offense.
superl.
Drawn out or extended in time; continued through a considerable tine, or to a great length; as, a long series of events; a long debate; a long drama; a long history; a long book.
a.
Having a long horn or horns; as, a long-horned goat, or cow; having long antennae, as certain beetles (Longicornia).
adv.
Through an extent of time, more or less; -- only in question; as, how long will you be gone?
a.
Having long arms; as, the long-armed ape or gibbon.
adv.
To a great extent in time; during a long time.
n.
The longest dimension; the greatest extent; -- in the phrase, the long and the short of it, that is, the sum and substance of it.
a.
Having a long waist; long from the armpits to the armpits to the bottom of the waist; -- said of persons.
n.
Long-sightedness.
a.
Having a long life; having constitutional peculiarities which make long life probable; lasting long; as, a long-lived tree; they are a longlived family; long-lived prejudices.
superl.
Slow in passing; causing weariness by length or duration; lingering; as, long hours of watching.