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Random fluctuations in radio waves of celestial origin
In astronomy, interplanetary scintillation refers to random fluctuations in the intensity of radio waves of celestial origin, on the timescale of a few
Interplanetary_scintillation
Phased array radio telescope built in 1967
The Interplanetary Scintillation Array (also known as the IPS Array or Pulsar Array) is a radio telescope that was built in 1967 at the Mullard Radio
Interplanetary Scintillation Array
Interplanetary_Scintillation_Array
Array of antennas creating a steerable beam
Ryle after several large phased arrays were developed at the University of Cambridge Interplanetary Scintillation Array. This design is also used for radar
Phased_array
Observatory in the United Kingdom
array Surviving Yagi antennas of the Cambridge Low Frequency Synthesis Telescope Two Half-Mile Telescopes Remains of the Interplanetary Scintillation
Mullard Radio Astronomy Observatory
Mullard_Radio_Astronomy_Observatory
Northern Irish physicist (born 1943)
she worked with Antony Hewish and others to construct the Interplanetary Scintillation Array just outside Cambridge to study quasars, which had recently
Jocelyn_Bell_Burnell
Pulsar in the constellation Vulpecula
Vulpecula. In 1967, a radio signal was detected using the Interplanetary Scintillation Array of the Mullard Radio Astronomy Observatory in Cambridge, UK
PSR_B1919+21
Radio telescope network located mainly in the Netherlands
Telescope) or two-dimensional arrays of omnidirectional antennas (e.g. Antony Hewish's Interplanetary Scintillation Array). LOFAR combines aspects of many
Low-Frequency_Array
British radio astronomer (1924–2021)
primarily for studying interplanetary scintillation. In 1965 he secured funding to construct his design, the Interplanetary Scintillation Array, at the Mullard
Antony_Hewish
Array used for astronomical observations
Air Shower Array (CASA) Infrared Optical Telescope Array (IOTA) Interplanetary Scintillation Array (IPS array) also called the Pulsar Array LOFAR (LOw
Astronomical_interferometer
Telescope operating group at Mullard Radio Astronomy Observatory
Telescope The One-Mile Telescope The Interplanetary Scintillation Array which discovered the first pulsar The 4C Array which made the 4C catalogue The Cambridge
Cavendish_Astrophysics_Group
Pulsar in the constellation Vulpecula
Jocelyn Bell and her PhD supervisor Antony Hewish using the Interplanetary Scintillation Array. Shortly after the discovery of pulsars, Franco Pacini and
PSR_B1937+21
Pulsar–white dwarf binary system in Taurus constellation
by Jocelyn Bell and her adviser, Antony Hewish using the Interplanetary Scintillation Array. Franco Pacini and Thomas Gold quickly put forth the idea
PSR_J0348+0432
Astrophysics observatory in southern India
universe. The telescope is currently being used mainly to observe interplanetary scintillation, which may provide valuable information about the solar wind
Ooty_Radio_Telescope
Type of neutron star with beams of radiation
cause scattering of the radio waves from the pulsar. The resulting scintillation of the radio waves—the same effect as the twinkling of a star in visible
Pulsar
NASA satellite of the Explorer program
double scintillation counter that measured 55- to 500-MeV protons in six energy intervals and protons above 600 MeV, (2) a single scintillator that measured
Explorer_12
Pulsar–white dwarf binary system in Scorpius constellation
1967 by Jocelyn Bell and her adviser Antony Hewish using the Interplanetary Scintillation Array. Franco Pacini and Thomas Gold quickly put forth the idea
PSR_J1614−2230
NASA satellite of the Explorer program
double scintillation counter telescope that measured 55- to 500-MeV protons in six energy intervals and protons above 600 MeV, (2) a single scintillator that
Explorer_14
Mexican physicist
of the radio telescope, called the Interplanetary Scintillation Observatory and known in English as the Mexican Array Radio Telescope or MEXART, was completed
Silvia_Bravo
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
Artyukh, Vadim S. (January 2002). Investigations of AGNS by the Interplanetary Scintillation Method. p. 185. ISBN 978-1-4020-0048-5. Kuzmin, Arkady (January
Pushchino Radio Astronomy Observatory
Pushchino_Radio_Astronomy_Observatory
Blazar in the constellation of Ophiuchus
Vijayanarasimha, U.; Ananthakrishnan, S.; Swarup, G. (February 1985). "Interplanetary scintillation observations of 57 flat-spectrum sourcesat 327 MHz". Monthly
PKS_1741−03
High-energy particle, mainly originating outside the Solar System
several arrays use water/ice-Cherenkov detectors as alternative or in addition to scintillators. By the combination of several detectors, some EAS arrays have
Cosmic_ray
solar axions from the early 2000s onwards Multi-spectral solar telescope array (MSSTA), a rocket launched payload of UV telescopes in the 1990s Leoncito
List_of_solar_telescopes
Indian radio astronomer
fields of solar radio emission, radio galaxies, quasars, pulsars, interplanetary scintillation, dark matter and cosmology. Govind Swarup was born in the town
Govind_Swarup
US Moon-orbiting ice-finding satellite
science instrument was a scintillation neutron detector composed of elpasolite (Cs2YLiCl6:Ce or CLYC). This material is a scintillator, which measurably glows
Lunar_Polar_Hydrogen_Mapper
Radio astronomy research institute in Pune, India
Astronomy and Astrophysics, which includes studies of the Sun, Interplanetary scintillations, pulsars, the Interstellar medium, Active galaxies and cosmology
National Centre for Radio Astrophysics
National_Centre_for_Radio_Astrophysics
NASA satellite of the Explorer program
with thin and thick Caesium iodide (CsI) scintillators (one each) and an anticoincidence plastic scintillation counter. The telescope axis was normal to
Explorer_21
NASA/DLR solar probes launched in 1974–76
distribution of cosmic rays. The three detectors (semiconductor detector, scintillation counter, and Cherenkov detector) were encapsulated in an anti-coincidence
Helios_(spacecraft)
NASA satellite of the Explorer program
with thin and thick Caesium iodide (CsI) scintillators (one each) and an anticoincidence plastic scintillation counter. The telescope axis was normal to
Explorer_18
NASA satellite of the Explorer program
study the magnetosphere. It was the eighth and last in a series of the Interplanetary Monitoring Platform. Explorer 50 was a drum-shaped spacecraft, 135.6 cm
Explorer_50
NASA satellite of the Explorer program
satellite of the Interplanetary Monitoring Platform. Explorer 43 continued the study, begun by earlier IMPs, of the interplanetary and outer magnetospheric
Explorer_43
Chemical element with atomic number 55 (Cs)
bromide (CsBr) and fluoride (CsF) crystals are employed for scintillators in scintillation counters widely used in mineral exploration and particle physics
Caesium
NASA satellite of the Explorer program
with thin and thick Caesium iodide (CsI) scintillators (one each) and an anticoincidence plastic scintillation counter. The telescope axis was parallel
Explorer_34
Association, and also B-M-I Array, microwave telescope it operated BIS – (organization) British Interplanetary Society BITP – (organization) – Bogolyubov
List_of_astronomy_acronyms
NASA satellite of the Explorer program
Explorer 28, also called IMP-C, IMP-3 and Interplanetary Monitoring Platform-3, was a NASA satellite launched on 29 May 1965 to study space physics, and
Explorer_28
NASA satellite of the Explorer program
a Thor-Delta 1604. Explorer 47 was the ninth overall launch of the Interplanetary Monitoring Platform series, but received the launch designation "IMP-7"
Explorer_47
Italian-American experimental physicist (1905–1993)
Williams. At this time, the extremely fast response of the newly developed scintillation counters offered a new way to study the structure of air showers. To
Bruno_Rossi
NASA satellite of the Explorer program
versus E telescope with thin and thick CsI scintillators (one each) and an anticoincidence plastic scintillation counter. The telescope axis was parallel
Explorer_41
American military satellite
array, the infrared array was also designed for a specific laser program: the Low Power Chemical Laser (LPCL) at White Sands, New Mexico. The array's
LACE_(satellite)
Quasar located in the constellation Hercules
having a size less than 7 x 4 arcseconds and has no signs of interplanetary scintillations. A total intensity image shows the source is asymmetric with
3C_336
Quasar in the constellation Sagittarius
Parkes Observatory in Australia. In 1984, it was found to display interplanetary scintillation, suggesting structure on angular scales of less than an arc second
PKS_1830−211
Vehicle or machine designed to fly in space
Salyut 1 in 1971. Space telescopes avoid the filtering and distortion (scintillation) of electromagnetic radiation which they observe, and avoid light pollution
Spacecraft
International Reference Ionosphere Interplanetary magnetic field Interplanetary medium Interplanetary scintillation Interstellar medium Interstellar nebula
List of plasma physics articles
List_of_plasma_physics_articles
Non-periodic comet
tail on 5 January 1974 also served as an opportunity to study interplanetary scintillation. A hundred years from now, how will our great, great grandchildren
C/1973_E1_(Kohoutek)
University explained the erratic fluctuations as being the result of scintillation caused by vibrations in the Earth's atmosphere, which no longer occurs
History of gamma-ray burst research
History_of_gamma-ray_burst_research
NASA satellite of the Explorer program
spin-stabilized spacecraft and based on the design of the prior IMP (Interplanetary Monitoring Platform) series of spacecraft. ISEE-1 and ISEE-2 were launched
ISEE-1
research on the identification of pre-solar molecular cloud material in interplanetary dust particles (see below). JPL · 7861 7862 Keikonakamura 1981 EE28
Meanings of minor-planet names: 7001–8000
Meanings_of_minor-planet_names:_7001–8000
Cosmic ray observatory at the University of Notre Dame
placed in a northern Indiana soybean field, but a leading expert in scintillation detector technology from Krakow, Poland then visiting the Notre Dame
Project_GRAND
INTERPLANETARY SCINTILLATION-ARRAY
INTERPLANETARY SCINTILLATION-ARRAY
Girl/Female
Tamil
Meghamala | மேகமாலா
Array of clouds
Meghamala | மேகமாலா
Girl/Female
Tamil
Kadambini | காதமà¯à®ªà®¿à®¨à¯€
An array of clouds
Kadambini | காதமà¯à®ªà®¿à®¨à¯€
Biblical
prepared; arrayed
Girl/Female
Assamese, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Oriya, Sanskrit, Sindhi, Tamil, Telugu
An Array of Clouds
Girl/Female
Biblical
Prepared, arrayed.
Girl/Female
Gujarati, Hindu, Indian, Kannada, Marathi, Sanskrit, Sindhi, Telugu
Array of Clouds
Boy/Male
Hindu, Indian, Punjabi, Sikh, Traditional
An Array of Clouds; Garland of Clouds
Girl/Female
Hindu
Array of clouds
Girl/Female
Tamil
Array of clouds
INTERPLANETARY SCINTILLATION-ARRAY
INTERPLANETARY SCINTILLATION-ARRAY
Girl/Female
Bengali, Indian, Tamil, Telugu
Favour
Boy/Male
Indian, Punjabi, Sikh
True Devotee of God
Surname or Lastname
English
English : variant spelling of Kimberley.
Girl/Female
Afghan, Arabic, Hebrew, Muslim
Chosen; Happy; Name of First Lady Ruler of Medieval Period
Boy/Male
Hindu, Indian, Marathi
The Sun
Boy/Male
Hindu, Indian
A Form of Janessa
Girl/Female
American, British, English
Based on the Initials J C; An Abbreviation of Jacinda
Girl/Female
Tamil
Arnavi | à®…à®°à¯à®¨à®¾à®µà¯€Â
Bird
Boy/Male
Gujarati, Hindu, Indian, Kannada, Tamil
Tree of Knowledge; This is the Tree Where Buddha did Meditate and Gained Lot of Knowledge
Male
English
Variant form of Norman French Gy, a derivative of Latin Wido, GUY means "wide." This name was popular until 1605 when Guy Fawkes tried to blow up Parliament after which it acquired the negative connotation "grotesque man." In Arthurian legend, this is the name of a son of Bevis of Hamptoun. In use by the English.
INTERPLANETARY SCINTILLATION-ARRAY
INTERPLANETARY SCINTILLATION-ARRAY
INTERPLANETARY SCINTILLATION-ARRAY
INTERPLANETARY SCINTILLATION-ARRAY
INTERPLANETARY SCINTILLATION-ARRAY
p. pr. & vb. n.
of Scintillate
n.
A chanting; recitation or reading with musical modulations.
n.
A shining with intermitted light; a scintillation; a sparkling; as, the twinkling of the stars.
p. pr. & vb. n.
of Array
n.
A reflecting telescope, part of which is made to rotate eccentrically, so as to produce a ringlike image of a star, instead of a point; -- used in studying the scintillation of the stars.
imp. & p. p.
of Array
a.
Emitting sparks of fire when struck with steel; scintillating; as, ignescent stones.
n.
The act of scintillating.
n.
Order; a regular and imposing arrangement; disposition in regular lines; hence, order of battle; as, drawn up in battle array.
n.
Weapons, collectively; as, an array of weaponry.
n.
One who arrays. In some early English statutes, applied to an officer who had care of the soldiers' armor, and who saw them duly accoutered.
a.
Not arrayed in the dress of a morris dancer.
a.
Between planets; as, interplanetary spaces.
n.
A flying off in small particles, as heated iron or fermenting liquors; a sparkling; scintillation.
n.
A spark or flash emitted in scintillating.
v. t.
To invest with a robe or robes; to dress; to array; as, fields robed with green.
n.
A little spark; a scintillation.
v. i.
To sparkle or shine; especially, to shine with a mild, subdued, and fitful luster; to emit a soft, scintillating light; to gleam; as, the glistening stars.
n.
Any outer covering; array; garb.