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  5. New low power pulse compressed ionosonde at Gibilmanna Ionospheric Observatory
 
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New low power pulse compressed ionosonde at Gibilmanna Ionospheric Observatory

Author(s)
Baskaradas, J. A.  
TRIL fellow, The Abdus Salam International Centre for Theoretical Physics (ICTP), Trieste, Italy  
Bianchi, C.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Pezzopane, M.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Romano, V.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Sciacca, U.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Scotto, C.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Tutone, G.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Zuccheretti, E.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Date Issued
2005
Issue/vol(year)
3/48 (2005)
Language
eng
Subjects
01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques  
URI
https://www.earth-prints.org/handle/2122/911
Subjects

ionosonde

automatic ionogram sc...

ionospheric data

vertical soundings

Abstract
A digital low power pulse compressed ionosonde was developed at the Istituto Nazionale di Geofisica e Vulcanologia
(INGV), Rome, Italy. The aim of this Advanced Ionospheric Sounder, AIS-INGV, is to reduce the transmitted
power and, consequently, weight, size, power consumption and hardware complexity. To compensate the
power reduction the most advanced HF radar techniques such as the pulse compression and a phase coherent integration
are used. The ionosonde is completely programmable and a PC supports the data acquisition, control, storage
and on-line processing. The first prototype was installed at Gibilmanna Ionospheric Observatory (Sicily), an
interesting location in the center of Mediterranean area. The new ionosonde will contribute to ionospheric database
and real time knowledge of South European ionospheric conditions for space weather applications. In this work the
first results (ionograms and autoscaled characteristics) are presented and briefly discussed.
Type
article
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rome library|catania library|milano library|napoli library|pisa library|palermo library
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