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http://hdl.handle.net/2122/3051| Authors: | Pezzopane, M.* Zuccheretti, E.* Bianchi, C.* Scotto, C.* Zolesi, B.* Cabrera, M. A.* Ezquer, R. G.* |
Title: | The new ionospheric station of San Miguel de Tucumán | Journal: | INAG-68 Web Bulletin 2007 | Series/Report no.: | / 68 (2007) | Publisher: | INAG - Ionosonde Network Advisory Group | Issue Date: | 22-Oct-2007 | URL: | http://www.ips.gov.au/IPSHosted/INAG/web-inag/2007/tucuman.pdf | Keywords: | ionosonde ionogram Tucumán Autoscala equatorial anomaly |
Subject Classification: | 01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneous 01. Atmosphere::01.02. Ionosphere::01.02.05. Wave propagation 01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques |
Abstract: | At the end of August 2007 an Advanced Ionospheric Sounder (AIS), built at the Istituto Nazionale di Geofisica e Vulcanologia (INGV), Rome, Italy, was installed at San Miguel de Tucumán, Argentina (geographical coordinates: 26.9 S, 294.6 E; magnetic coordinates: 15.5 S, 3.8 E), particularly interesting for its location, near the southern peak of the equatorial anomaly. AIS-INGV is a digital low-power pulse-compressed ionosonde. In order to reduce the transmitted power, weight, size, power consumption, and to have an excellent reliability, advanced HF-radar techniques were employed. The ionosonde is also equipped with Autoscala, a software able to perform an automatic scaling of the ionogram. |
| Appears in Collections: | Article published / in press |
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| File | Description | Size | Format | |
|---|---|---|---|---|
| tucuman.pdf | full article | 255.74 kB | Adobe PDF | View/Open |
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