Results 101 to 110 of about 1,965,723 (227)
BALDONE OBSERVATORY IN THE CIRCLES OF TIME
1957 – The first laboratory building, known as the White House, was built near Baldone on the Riekstu hill, in the territory of the next Observatory. 01.01.1958 – The Astronomy Sector was separated from the Institute of Physics and commenced independent ...
I. Eglitis
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Siberian Radioheliograph: first results
Regular observations of active processes in the solar atmosphere have been started using the first stage of the multiwave Siberian Radioheliograph (SRH), a T-shaped 48-antenna array with a 4–8 GHz operating frequency range and a 10 MHz instantaneous ...
Lesovoi S.V. +11 more
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Fast Deep Learning–based Imaging for Synthetic Aperture Array: Application to DART
DAocheng Radio Telescope (DART) is a radio synthetic aperture array consisting of 313 antennas, dedicated to monitoring solar activities and observing cosmic radio sources.
Rui Li +7 more
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Purpose: With relation to radio astronomy, ionospheric scintillation of discrete cosmic radio sources is an undesirable effect. At the same time, ionospheric scintillations carry information on the ionospheric turbulence and are a separate object of ...
S. K. Panishko, O. A. Lytvynenko
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Feeds for the 150-foot radio telescope at the Algonquin Radio Observatory
The purpose of this report is to list the various feeds and feed attachments which have been built for use on the 150-foot radio telescope at the Algonquin Radio Observatory. The following text contains a brief description of each item. Following this, a
Lavrench, W., Hazell, J., Woods, L. W.
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Solar polarization observations at 3 and 13 mm
The first solar radio polarization observations at 3 mm (86 GHz) and 13 mm (22 GHz) were made at Aalto University Metsähovi Radio Observatory in Finland in spring 2019.
Petri Kirves +13 more
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A decametric wavelength radio telescope for interplanetary scintillation observations [PDF]
A phased array, electrically steerable radio telescope (with a total collecting area of 18 acres), constructed for the purpose of remotely sensing electron density irregularity structure in the solar wind, is presented.
Cronyn, W. M., Shawhan, S. D.
core
Investigating an Erupting Metric-decimetric Radio Depression and Its Physical Origin
We present direct metric-decimetric radio imaging observations of a fascinating quiescent filament eruption on 2024 March 17 using data from the DAocheng Radio Telescope, with a combination of the Solar Dynamics Observatory and the Chinese H α Solar ...
B. T. Wang +10 more
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Type III radio bursts associated with jets in two solar flares
Context. A challenging issue is the significant velocity discrepancy between jets and energetic electrons accelerated by magnetic reconnection in solar flares. Aims.
Tang Xiaoyu +10 more
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Solar system radio emissions studies with the largest low-frequency radio telescopes
We describe the trends and tasks in the field of lowfrequency studies of radio emission from the Solar system's objects. The world's largest decameter radio telescopes UTR-2 and URAN have a unique combination of sensitivity and time/frequency resolution parameters, providing the capability of the most detailed studies of various types of solar and ...
Zakharenko, V. +15 more
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