La ionosfera: comunicare... naturalmente!

La ionosfera è la parte della media-alta atmosfera compresa tra i 60 e i 1000 km di quota. Essa è caratterizzata da una concentrazione di elettroni tale da modificare la propagazione delle onde radio che la attraversano

Tecniche radio per investigare la ionosfera terrestre

Nel seminario vengono presentate in modo generale le principali tecniche sperimentali di investigazione della ionosfera terrestre. Per ognuna di esse sono descritti gli elementi su cui si basa, pregi, difetti e le grandezze ionosferiche oggetto delle loro misure. Vengono presentate, poi, tre tecniche in modo approfondito, utilizzate anche nelle attività sperimentali dell'Istituto Nazionale di Geofisica e Vulcanologia: sondaggio verticale, riometro e GPS per scintillazioni

Sporadic E layer at mid-latitudes: average properties and influence of atmospheric tides

Abstract. This paper describes a study of the daily variability shown by the main characteristics of the sporadic E (Es) layer, that is the top frequency (ftEs) and the lowest virtual height (h'Es). The study is based on ionograms recorded by the Advanced Ionospheric Sounder by the Istituto Nazionale di Geofisica e Vulcanologia (AIS-INGV) ionosondes installed in the ionospheric stations at Rome (41.8° N, 12.5° E) and Gibilmanna (37.9° N, 14.0° E), Italy, during the summer (June, July, August and September) of 2013, a year falling in the ascending phase of solar cycle 24. The ftEs presents a diurnal variation characterized by two maxima, the first around noon is very well defined and the second in the evening/night is much less defined; the amplitude of both maxima decreases from June to September accompanied by a general decrease of the ftEs values which is more pronounced in the daytime than in the nighttime. h'Es also presents a diurnal variation characterized by two maxima but, unlike ftEs, these present the same amplitude which is independent from the considered month. Assuming that both ftEs and h'Es trends are influenced by the atmospheric tides, the height–time–intensity (HTI) technique was applied to deeply investigate how these waves control the Es dynamics. The HTI study, along with a fast Fourier transform analysis, show that a well-defined semidiurnal periodicity characterizes the Es layer dynamics most accurately in June and July, while in August and September the daytime semidiurnal periodicity becomes weaker and the role of the diurnal periodicity is consequently highlighted

Ionospheric vertical radio soundings

The presentation deals with one of the most popular technique to investigate the terrestrial ionosphere: the vertical radio sounding. The basic elements of the radar theory are explained starting from the envelope radar up to the most sophisticated techniques of the coded radars. Antennas design elements and problems are highlighted along with the most common solutions. Then the principles of the ionospheric measurements are reported from the ionogram to the ionospheric parameters and to the density profile. A real example of a geomagnetic storm is also presented

Rilevamento delle sorgenti doppler della ionosfera tramite radar-HF

Il presente lavoro contiene un insieme di concetti di base utili per comprendere la cosiddetta tecnica della “interferometria doppler”, usata, nell’ambito degli studi sulla ionosfera, per ricavare informazioni sulla conformazione e velocità degli strati riflettenti (operazione chiamata anche sky mapping). È utile ricordare, infatti, che il sondaggio ionosferico tradizionale consente solo la determinazione dell’altezza virtuale di ogni strato, pensato come un unico oggetto riflettente piano. Tale determinazione è giunta nel tempo ad avere una risoluzione molto spinta, dell’ordine di qualche chilometro, tuttavia una ionosonda tradizionale non possiede la capacità di individuare la struttura degli strati riflettenti

Ionospheric radars development

The presentation deals with one of the most popular technique to investigate the terrestrial ionosphere: the vertical radio sounding. The basic elements of the radar theory are explained starting from the envelope radar up to more sophisticated techniques of the coded radars. Antennas design elements and problems are highlighted along with the most common solutions. Then the principles of the ionospheric measurements are reported from the ionogram to the ionospheric parameters and to the density profile. A detailed analysis of the ionosonde system installed at Tucumán Ionospheric Observatory, Argentina, is performed

Glacio RADAR system and results

Since 1997 the Istituto Nazionale di Geofisica e Vulcanologia (INGV) in Italy has been involved in the development of the airborne RES system named Glacio RADAR, which is continuously upgraded. Radio Echo Sounding (RES) techniques are widely used in glaciological measurements. They are based on the use of radar systems, to obtain information concerning ice thickness of ice sheets and ice shelves, internal layering of glaciers, detection of inhomogeneities, exploration of subglacial lakes and identification of physical nature of subglacial interface. The Glacio RADAR is mounted on an aircraft and flies at an altitude around 300m above the ice surface during the survey. The first prototype operates in bistatic mode with separate transmit and receive one wire folded dipole installed beneath the aircraft wings. It works at 60 MHz with an envelope pulse width variable between 0.3 s and 1 s. The receiving window is 64 s which implies a maximum penetration depth (range) in the ice of about 5.3 km. The horizontal sampling rate is 10 traces/s at a mean aircraft speed of about 70 m/s. This would produce roughly 143 traces per kilometre (horizontal resolution of 1 trace every 7 m). The Navigation and geographical information is based on a on board GPS receiver giving longitude, latitude, altitude and time for the acquired radar trace. This radar was used in several Italian Antarctic Expeditions (1997, 1999, 2001 and 2003) and highlights of data results from these expeditions are presented here

Rilevamento delle sorgenti doppler della ionosfera tramite radar-HF

Il presente lavoro contiene un insieme di concetti di base utili per comprendere la cosiddetta tecnica della “interferometria doppler”, usata, nell’ambito degli studi sulla ionosfera, per ricavare informazioni sulla conformazione e velocità degli strati riflettenti (operazione chiamata anche sky mapping). È utile ricordare, infatti, che il sondaggio ionosferico tradizionale consente solo la determinazione dell’altezza virtuale di ogni strato, pensato come un unico oggetto riflettente piano. Tale determinazione è giunta nel tempo ad avere una risoluzione molto spinta, dell’ordine di qualche chilometro, tuttavia una ionosonda tradizionale non possiede la capacità di individuare la struttura degli strati riflettenti

Satellite traces, range spread-F occurrence, and gravity wave propagation at the southern anomaly crest

Range spread-F (RSF) and occurrence of “satellite” traces prior to RSF onset were studied at the southern peak of the ionospheric equatorial anomaly (EA). Ionograms recorded in September 2007 at the new ionospheric station of Tucumán, Argentina (26.9° S, 294.6° E, dip latitude 15.5° S), by the Advanced Ionospheric Sounder (AIS) developed at the Istituto Nazionale di Geofisica e Vulcanologia INGV), were considered. Satellite traces (STs) are confirmed to be a necessary precursor to the appearance of an RSF trace on the ionograms. Moreover, an analysis of isoheight contours of electron density seems to suggest a relationship between RSF occurrence and gravity wave (GW) propagation

THE NEW INGV DIGITAL IONOSONDE: DESIGN REPORT

The ionosonde is a system which exploits the radar technique: it applies electromagnetic waves with variable frequency in the HF band to measure the ionospheric layers electron density, height and other parameters. This paper is a technical report on the new digital ionosonde (AIS-INGV), which was designed both for research purposes and for the routine service of the HF radiowave propagation forecast. It has been developed almost completely within the Laboratorio di Geofisica Ambientale (LGA) at the Istituto Nazionale di Geofisica e Vulcanologia (INGV). It exploits advanced techniques for the signal analysis, recent technological devices and PC resources. The report is divided into two parts; the first is a general description of the design development, the second is a more detailed description of the blocks and circuits actually built and tested, directed to a specialist reader