Academic literature on the topic 'Arecibo Ionospheric Observatory'

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Journal articles on the topic "Arecibo Ionospheric Observatory"

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Mathews, J. D. "A short history of geophysical radar at Arecibo Observatory." History of Geo- and Space Sciences 4, no. 1 (2013): 19–33. http://dx.doi.org/10.5194/hgss-4-19-2013.

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Abstract. As Arecibo Observatory (AO) approaches its 50th anniversary, it is appropriate to review the many radars and ionospheric heaters that have been deployed on or near the 305 m dish and to summarize some of the innovative radar-based geophysical research that has resulted. The reasons William E. (Bill) Gordon developed the 305 m Arecibo dish are well known but are briefly reviewed. The early and then more recent radar/feed designs are reviewed as geophysical uses of Arecibo have evolved and as the full potential of the dish and nearby facilities was and is being realized from HF through
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Werthimer, Dan, Stuart Bowyer, David Ng, et al. "The Berkeley Seti Program: Serendip IV Instrumentation." International Astronomical Union Colloquium 161 (January 1997): 683–88. http://dx.doi.org/10.1017/s0252921100015244.

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AbstractThe SERENDIP program is an ongoing search for narrow band radio signals from extraterrestrial civilizations. Each generation SERENDIP instrument has on average been about 35 times more powerful than its predecessor. In this paper we discuss the hardware design of the latest generation instrument, SERENDIP IV, which will be deployed in early 1997 for a 21 cm sky survey at the National Astronomy and Ionospheric Center’s 305 meter radio telescope in Arecibo, Puerto Rico. SERENDIP IV is a 167 million channel spectrum analyzer, covering a 100 Mhz bandwidth, with 0.6 Hz resolution and a 1.7
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Bakhmetieva, Nataliya V., and Gennadiy I. Grigoriev. "Study of the Mesosphere and Lower Thermosphere by the Method of Creating Artificial Periodic Irregularities of the Ionospheric Plasma." Atmosphere 13, no. 9 (2022): 1346. http://dx.doi.org/10.3390/atmos13091346.

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This article presented a brief review of studies of the Earth’s ionosphere at the heights of the mesosphere and lower thermosphere by a method based on the creation of artificial periodic inhomogeneities (APIs) of the ionospheric plasma by high-frequency radiation from powerful thermal installations. APIs are created by a standing wave due to the interference between upward-propagating radio waves and those reflected from the ionosphere. API studies of the ionosphere were based on Bragg scattering of probing impulse signals from an artificial periodic structure. The method makes it possible to
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Mendillo, Michael, Jeffrey Baumgardner, Daniel Nottingham, et al. "Investigations of thermospheric-ionospheric dynamics with 6300-Å images from the Arecibo Observatory." Journal of Geophysical Research: Space Physics 102, A4 (1997): 7331–43. http://dx.doi.org/10.1029/96ja02786.

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Eccles, Vince, Hien Vo, Jonathan Thompson, Sixto Gonzalez, and Jan J. Sojka. "Database of electron density profiles from Arecibo Radar Observatory for the assessment of ionospheric models." Space Weather 9, no. 1 (2011): n/a. http://dx.doi.org/10.1029/2010sw000591.

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Hysell, David L., Miguel Larsen, and Michael Sulzer. "Observational evidence for new instabilities in the midlatitude <i>E</i> and <i>F</i> region." Annales Geophysicae 34, no. 11 (2016): 927–41. http://dx.doi.org/10.5194/angeo-34-927-2016.

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Abstract. Radar observations of the E- and F-region ionosphere from the Arecibo Observatory made during moderately disturbed conditions are presented. The observations indicate the presence of patchy sporadic E (Es) layers, medium-scale traveling ionospheric disturbances (MSTIDs), and depletion plumes associated with spread F conditions. New analysis techniques are applied to the dataset to infer the vector plasma drifts in the F region as well as vector neutral wind and temperature profiles in the E region. Instability mechanisms in both regions are evaluated. The mesosphere–lower-thermospher
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Burgin, M. S., and M. V. Popov. "Probing the ionosphere with pulses from the pulsar B2016+28 at a frequency of 324 MHz." Astronomičeskij žurnal 101, no. 3 (2024): 233–43. http://dx.doi.org/10.31857/s0004629924030044.

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Using ground-space VLBI data from the RadioAstron project archive, the phase distortions of the cross-spectrum caused by the ionosphere have been calculated and their influence on the results of determination of the visibility function has been studied. The Arecibo Observatory’s 300-meter antenna served as the ground station for the interferometer. The separation of ionospheric phase distortions from the influence of the interstellar and interplanetary medium and instrumental errors is based on different frequency dependencies of these effects. The amplitude of ionospheric phase variation caus
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Djuth, F. T., M. P. Sulzer, J. H. Elder, and V. B. Wickwar. "High-resolution studies of atmosphere-ionosphere coupling at Arecibo Observatory, Puerto Rico." Radio Science 32, no. 6 (1997): 2321–44. http://dx.doi.org/10.1029/97rs02797.

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9

Isham, Brett, Terence Bullett, Björn Gustavsson, et al. "Science goals for a high-frequency radar and radio imaging array." Frontiers in Astronomy and Space Sciences 10 (August 1, 2023). http://dx.doi.org/10.3389/fspas.2023.1064368.

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A medium and high-frequency antenna array for radar and radio imaging of the ionosphere is planned for installation in Aguadilla, Puerto Rico. Science goals include the study of space weather, radio propagation, meteors, lightning, and plasma physics. Radio imaging is ideal for the study of stimulated ionospheric radio emissions, such as those induced by the Arecibo Observatory high-power HF radio transmitter, which is likely to be restored to operation in the near future. The array will be complemented by a wide variety of instruments fielded by collaborators, and will be a rich source of stu
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da Silva, Caitano L., Sophia D. Salazar, Christiano G. M. Brum, and Pedrina Terra. "Survey of electron density changes in the daytime ionosphere over the Arecibo Observatory due to lightning and solar flares." Scientific Reports 11, no. 1 (2021). http://dx.doi.org/10.1038/s41598-021-89662-x.

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AbstractOptical observations of transient luminous events and remote-sensing of the lower ionosphere with low-frequency radio waves have demonstrated that thunderstorms and lightning can have substantial impacts in the nighttime ionospheric D region. However, it remains a challenge to quantify such effects in the daytime lower ionosphere. The wealth of electron density data acquired over the years by the Arecibo Observatory incoherent scatter radar (ISR) with high vertical spatial resolution (300-m in the present study), combined with its tropical location in a region of high lightning activit
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Dissertations / Theses on the topic "Arecibo Ionospheric Observatory"

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Santana, Julio III. "Investigating Ionospheric Parameters Using the Plasma Line Measurements From Incoherent Scatter Radar." Miami University / OhioLINK, 2012. http://rave.ohiolink.edu/etdc/view?acc_num=miami1344024880.

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Books on the topic "Arecibo Ionospheric Observatory"

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United States. National Aeronautics and Space Administration., ed. Radar investigations of barium releases over Arecibo Observatory, Puerto Rico. Geospace Research, Inc., 1995.

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Snežana, Stanimirović, National Radio Astronomy Observatory (U.S.), and National Astronomy and Ionosphere Center (U.S.), eds. Single-dish radio astronomy: Techniques and applications : proceedings of the NAIC-NRAO summer school held at National Astronomy and Ionosphere Center, Arecibo Observatory, Arecibo, Puerto Rico, USA, 10-15 June 2001. Astronomical Society of the Pacific, 2002.

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Radar investigations of barium releases over Arecibo Observatory, Puerto Rico. Geospace Research, Inc., 1995.

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4

National Radio Astronomy Observatory (Contributor), National Astronomy and Ionosphere Center (Contributor), and Sneezana Stanimirovic (Editor), eds. Single-Dish Radio Astronomy: Techniques and Applications : Proceedings of the Naic-Nrao Summer School Held at National Astronomy and Ionosphere Center, Arecibo Observatory, arecib. Astronomical Society of the Pacific, 2002.

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Conference papers on the topic "Arecibo Ionospheric Observatory"

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Dighe, Kalpak A., Craig A. Tepley, Raul Garcia, and Jonathan Friedman. "The Arecibo Observatory Daytime Lidar : Preliminary Results." In Optical Remote Sensing of the Atmosphere. Optica Publishing Group, 1993. http://dx.doi.org/10.1364/orsa.1993.tud.15.

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The vertical propagation of atmospheric tides and acoustic gravity waves and their corresponding travelling ionospheric disturbances play a crucial role in the transportation and balance of momentum and energy in the earth's atmosphere. The unique availability of both radar and lidar instrumentation at Arecibo can provide simultaneous access to the neutral density, temperature and wind perturbations induced by such wave activity at mesospheric and stratospheric altitudes.
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Rankin, Joanna M., C. Bassa, Z. Wang, A. Cumming, and V. M. Kaspi. "Remembering the Early Days of Pulsars at the Arecibo Ionospheric Observatory." In 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP, 2008. http://dx.doi.org/10.1063/1.2900137.

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da Silva, Caitano L., Sophia D. Salazar, Christiano G. M. Brum, and Pedrina Terra. "Lightning Effects in the Ionosphere Over The Arecibo Observatory." In 2020 XXXIIIrd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS). IEEE, 2020. http://dx.doi.org/10.23919/ursigass49373.2020.9232366.

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Tepley, Craig A. "Observations of Winds of the Stratosphere and Mesosphere at Arecibo, Puerto Rico Using a Doppler Rayleigh Lidar." In Optical Remote Sensing of the Atmosphere. Optica Publishing Group, 1993. http://dx.doi.org/10.1364/orsa.1993.wa.2.

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At the Arecibo Observatory we use a variety of radar and optical instruments to measure the properties of the Earth's atmosphere and ionosphere. With the incoherent scatter radar we are sensitive to the ionized portion of the upper atmosphere from about half an Earth radius (RE) down to nearly 60 km during daylight, and 100-150 km during the night when the molecular ionization of this lower part recombines. During both day and night, the winds and turbulent layer structures of the troposphere and stratosphere are accessible up to 25 km with the coherent scatter radar systems. We also use a var
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Altschuler, Daniel R. "The National Astronomy and Ionosphere Center’s (NAIC) Arecibo Observatory in Puerto Rico." In First tropical workshop on particle physics and cosmology and the second Latin American symposium on high energy physics. AIP, 1998. http://dx.doi.org/10.1063/1.56603.

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