Polarimetric radar interferometry for improved mine detection and surface clutter rejection

A recently developed technique, polarimetric radar interferometry, is applied to tackle the problem of the detection of buried objects embedded in surface clutter. An experiment with a fully polarimetric radar in an anechoic chamber has been carried out using different frequency bands and baselines. The processed results show the ability of this technique to detect buried plastic mines and to measure their depth. This technique enables the detection of plastic mines even if their backscatter response is much lower than that of the surface clutter.

Ensemble prediction for nowcasting with a convection-permitting model—I: description of the system and the impact of radar-derived surface precipitation rates

A key strategy to improve the skill of quantitative predictions of precipitation, as well as hazardous weather such as severe thunderstorms and flash floods is to exploit the use of observations of convective activity (e.g. from radar). In this paper, a convection-permitting ensemble prediction system (EPS) aimed at addressing the problems of forecasting localized weather events with relatively short predictability time scale and based on a 1.5 km grid-length version of the Met Office Unified Model is presented. Particular attention is given to the impact of using predicted observations of radar-derived precipitation intensity in the ensemble transform Kalman filter (ETKF) used within the EPS. Our initial results based on the use of a 24-member ensemble of forecasts for two summer case studies show that the convective-scale EPS produces fairly reliable forecasts of temperature, horizontal winds and relative humidity at 1 h lead time, as evident from the inspection of rank histograms. On the other hand, the rank histograms seem also to show that the EPS generates too much spread for forecasts of (i) surface pressure and (ii) surface precipitation intensity. These may indicate that for (i) the value of surface pressure observation error standard deviation used to generate surface pressure rank histograms is too large and for (ii) may be the result of non-Gaussian precipitation observation errors. However, further investigations are needed to better understand these findings. Finally, the inclusion of predicted observations of precipitation from radar in the 24-member EPS considered in this paper does not seem to improve the 1-h lead time forecast skill.

Temporal and spatial variability of auroral forms in the 10–14 MLT sector: Relationship to plasma convection and solar wind-magnetosphere coupling

Ground-based observations of dayside auroral forms and magnetic perturbations in the arctic sectors of Svalbard and Greenland, in combination with the high-resolution measurements of ionospheric ion drift and temperature by the EISCAT radar, are used to study temporal/spatial structures of cusp-type auroral forms in relation to convection. Large-scale patterns of equivalent convection in the dayside polar ionosphere are derived from the magnetic observations in Greenland and Svalbard. This information is used to estimate the ionospheric convection pattern in the vicinity of the cusp/cleft aurora. The reported observations, covering the period 0700-1130 UT, on January 11, 1993, are separated into four intervals according to the observed characteristics of the aurora and ionospheric convection. The morphology and intensity of the aurora are very different in quiet and disturbed intervals. A latitudinally narrow zone of intense and dynamical 630.0 nm emission equatorward of 75 degrees MLAT, was observed during periods of enhanced antisunward convection in the cusp region. This (type 1 cusp aurora) is considered to be the signature of plasma entry via magnetopause reconnection at low magnetopause latitudes, i.e. the low-latitude boundary layer (LLB I,). Another zone of weak 630.0 nm emission (type 2 cusp aurora) was observed to extend up to high latitudes (similar to 79 degrees MLAT) during relatively quiet magnetic conditions, when indications of reverse (sunward) convection was observed in the dayside polar cap. This is postulated to be a signature of merging between a northward directed IMF (B-z > 0) and the geomagnetic field poleward of the cusp. The coexistence of type 1 and 2 auroras was observed under intermediate circumstances. The optical observations from Svalbard and Greenland were also used to determine the temporal and spatial evolution of type 1 auroral forms, i.e. poleward-moving auroral events occurring in the vicinity of a rotational convection reversal in the early post-noon sector. Each event appeared as a local brightening at the equatorward boundary of the pre-existing type 1 cusp aurora, followed by poleward and eastward expansions of luminosity. The auroral events were associated with poleward-moving surges of enhanced ionospheric convection and F-layer ion temperature as observed by the EISCAT radar in Tromso. The EISCAT ion flow data in combination with the auroral observations show strong evidence for plasma flow across the open/closed field line boundary.

Causes of plasma flow bursts and dayside auroral transients: An evaluation of two models Invoking reconnection pulses and changes in the Y component of the magnetosheath field

Longitudinal flow bursts observed by the European Incoherent Scatter (EISCAT) radar, in association with dayside auroral transients observed from Svalbard, have been interpreted as resulting from pulses of enhanced reconnection at the dayside magnetopause. However, an alternative model has recently been proposed for a steady rate of magnetopause reconnection, in which the bursts of longitudinal flow are due to increases in the field line curvature force, associated with the By component of the magnetosheath field. We here evaluate these two models, using observations on January 20, 1990, by EISCAT and a 630-nm all-sky camera at Ny Ålesund. For both models, we predict the behavior of both the dayside flows and the 630-nm emissions on newly opened field lines. It is shown that the signatures of steady reconnection and magnetosheath By changes could possibly resemble the observed 630-nm auroral events, but only for certain locations of the observing site, relative to the ionospheric projection of the reconnection X line: however, in such cases, the flow bursts would be seen between the 630-nm transients and not within them. On the other hand, the model of reconnection rate pulses predicts that the flows will be enhanced within each 630-nm transient auroral event. The observations on January 20, 1990, are shown to be consistent with the model of enhanced reconnection rate pulses over a background level and inconsistent with the effects of periodic enhancements of the magnitude of the magnetosheath By component. We estimate that the reconnection rate within the pulses would have to be at least an order of magnitude larger than the background level between the pulses.

Modelling the high-latitude ionosphere for time-varying plasma convection

The paper discusses how variations in the pattern of convective plasma flows should beincluded in self-consistent time-dependent models of the coupled ionosphere-thermosphere system. The author shows how these variations depend upon the mechanism by which the solar wind flow excites the convection. The modelling of these effects is not just of relevance to the polar ionosphere. This is because the influence of convection is not confined to high latitudes: the resultant heating and composition changes in the thermosphere are communicated to lower latitudes by the winds which are also greatly modified by the plasma convection. These thermospheric changes alter the global distribution of plasma by modulatingthe rates of the chemical reactions which areresponsible for the loss of plasma. Hence the modelling of these high-latitude processes is of relevanceto the design and operation of HF communication, radar and navigation systems worldwide.

EISCAT observations of bursts of rapid flow in the high latitude dayside ionosphere

Observations are presented of short-lived, highly structured bursts of rapid plasma flow observed with the EISCAT radar in the high latitude dayside ionosphere. It is shown that the properties of the bursts are consistent with ionospheric perturbations caused by impulsive, localized reconnection at the Earth's magnetopause, i.e. by flux transfer events.

The DYMECS project: a statistical approach for the evaluation of convective storms in high-resolution NWP models

A new frontier in weather forecasting is emerging by operational forecast models now being run at convection-permitting resolutions at many national weather services. However, this is not a panacea; significant systematic errors remain in the character of convective storms and rainfall distributions. The DYMECS project (Dynamical and Microphysical Evolution of Convective Storms) is taking a fundamentally new approach to evaluate and improve such models: rather than relying on a limited number of cases, which may not be representative, we have gathered a large database of 3D storm structures on 40 convective days using the Chilbolton radar in southern England. We have related these structures to storm life-cycles derived by tracking features in the rainfall from the UK radar network, and compared them statistically to storm structures in the Met Office model, which we ran at horizontal grid length between 1.5 km and 100 m, including simulations with different subgrid mixing length. We also evaluated the scale and intensity of convective updrafts using a new radar technique. We find that the horizontal size of simulated convective storms and the updrafts within them is much too large at 1.5-km resolution, such that the convective mass flux of individual updrafts can be too large by an order of magnitude. The scale of precipitation cores and updrafts decreases steadily with decreasing grid lengths, as does the typical storm lifetime. The 200-m grid-length simulation with standard mixing length performs best over all diagnostics, although a greater mixing length improves the representation of deep convective storms.

An intelligent system to real time rainfall prediction using radar data

This work presents a new approach for rainfall measurements making use of weather radar data for real time application to the radar systems operated by institute of Meteorological Research (IPMET) - UNESP - Bauru - SP-Brazil. Several real time adjustment techniques has been presented being most of them based on surface rain-gauge network. However, some of these methods do not regard the effect of the integration area, time integration and distance rainfall-radar. In this paper, artificial neural networks have been applied for generate a radar reflectivity-rain relationships which regard all effects described above. To evaluate prediction procedure, cross validation was performed using data from IPMET weather Doppler radar and rain-gauge network under the radar umbrella. The preliminary results were acceptable for rainfalls prediction. The small errors observed result from the spatial density and the time resolution of the rain-gauges networks used to calibrate the radar.

Geoestatística aplicada à acumulação da precipitação pluviométrica com radar meteorológico

Pós-graduação em Agronomia (Energia na Agricultura) - FCA

Analisi di dati telerilevati ottici e radar per la gestione dei disastri: le alluvioni nel Bangladesh.

Abstract L’utilizzo dei dati satellitari per la gestione dei disastri naturali è fondamentale nei paesi in via di sviluppo, dove raramente esiste un censimento ed è difficile per i governi aggiornare le proprie banche dati con le tecniche di rilevamento e metodi di mappatura tradizionali che sono entrambe lunghe e onerose. A supporto dell’importanza dell’impiego del telerilevamento e per favorirne l’uso nel caso di catastrofi, vi è l’operato di diverse organizzazioni internazionali promosse da enti di ricerca, da agenzie governative o da organismi sopranazionali, le quali svolgono un lavoro di cruciale valore, fornendo sostegno tecnico a chi si occupa di far giungere alle popolazioni colpite gli aiuti umanitari e i soccorsi nel più breve tempo possibile. L’attività di tesi è nata proprio dalla collaborazione con una di esse, ITHACA (Information Technology for Humanitarian Assistance, Cooperation and Action), organizzazione no-profit, fondata dal Politecnico di Torino e SiTI (Istituto Superiore sui Sistemi Territoriali per l’Innovazione), la quale a sua volta collabora con il WFP (World Food Programme) delle Nazioni Unite, realizzando cartografie speditive necessarie per la valutazione delle conseguenze di un evento catastrofico, attraverso l’impiego di dati acquisiti da satellite. Su questo tema si è inserito il presente lavoro che ha come obiettivo quello di dimostrare la valenza dei dati telerilevati, siano essi di tipo ottico o Radar, nel caso di alcuni dei disastri naturali più catastrofici, le alluvioni. In particolare è stata studiata la vulnerabilità del Bangladesh, il quale annualmente si trova ad affrontare eventi alluvionali, spesso di grave intensità. Preliminarmente allo studio, è stata condotta una ricerca bibliografica al fine di avere una buona conoscenza dell’area sia in termini geografici e fisici che di sviluppo e tipologia di urbanizzazione. E’stata indagata in particolare l’alluvione che ha colpito il paese nel Luglio del 2004, attraverso delle immagini satellitari multispettrali, in particolare Landsat 7, per un inquadramento pre-evento, ed ASTER per studiare la situazione a distanza di tre mesi dall’accaduto (immagine rilevata il 20 Ottobre 2004). Su tali immagini sono state condotte delle classificazioni supervisionate con il metodo della massima verosimiglianza che hanno portato la suddivisione del territorio in quattro classi di destinazione d’uso del suolo: urbano (Build-up), campi e vegetazione (Crops&Vegetation), sabbia e scavi (Sand&Excavation), idrografia e zone alluvionate (Water). Dalla sperimentazione è emerso come tali immagini multispettrali si prestino molto bene per l’analisi delle differenti caratteristiche del territorio, difatti la validazione condotta sulla mappa tematica derivata dall’immagine Landsat 7 ha portato ad un’accuratezza del 93% circa, mentre la validazione dell’immagine ASTER è stata solo di tipo qualitativo, in quanto, considerata l’entità della situazione rilevata, non è stato possibile avere un confronto con dei punti da assumere come verità a terra. Un’interpretazione della mappa tematica derivante dalla classificazione dell’immagine ASTER è stata elaborata incrociandola in ambiente GIS con dati forniti dal CEGIS (Center for Environmental and Geographic Information Services) riguardanti il landuse della zona in esame; da ciò è emerso che le zone destinate alla coltivazione del riso sono più vulnerabili alle inondazioni ed in particolare nell’Ottobre 2004 il 95% delle aree esondate ha interessato tali colture. Le immagini ottiche presentano un grosso limite nel caso delle alluvioni: la rilevante copertura nuvolosa che spesso accompagna siffatti eventi impedisce ai sensori satellitari operanti nel campo dell’ottico di rilevare il territorio, e per questo di frequente essi non si prestano ad essere impiegati per un’indagine nella fase di prima emergenza. In questa circostanza, un valido aiuto giunge dall’impiego di immagini Radar, le quali permettono osservazioni ad ogni ora del giorno e della notte, anche in presenza di nuvole, rendendole di fondamentale importanza nelle situazioni descritte. Per dimostrare la validità di questi sensori si sono analizzati due subset derivanti da un mosaico di immagini della nuova costellazione italiana ad alta risoluzione CosmoSkymed: il primo va dalla città di Dhaka al Golfo del Bengala ed il secondo copre la zona più a Nord nel distretto di Sylhet. Dalla sperimentazione condotta su tali immagini radar, che ha comportato come ovvio problematiche del tutto differenti rispetto alle elaborazioni tradizionalmente condotte su immagini nel campo dell’ottico, si è potuto verificare come l’estrazione dei corpi d’acqua e più in generale dell’idrografia risulti valida e di veloce computazione. Sono emersi tuttavia dei problemi, per esempio per quanto riguarda la classificazione dell’acqua in presenza di rilievi montuosi; tali complicazioni sono dovute alla presenza di zone d’ombra che risultano erroneamente assegnate alla classe water, ma è stato possibile correggere tali errori di attribuzione mascherando i rilievi con l’ausilio di una mappa delle pendenze ricavata da modelli di elevazione SRTM (Shuttle Radar Topographic Mission). La validazione dei risultati della classificazione, condotta con un grande numero di check points, ha fornito risultati molto incoraggianti (ca. 90%). Nonostante le problematiche riscontrate, il Radar, in sé o in accoppiamento con altri dati di diversa origine, si presta dunque a fornire in breve tempo informazioni sull’estensione dell’esondazione, sul grado di devastazione, sulle caratteristiche delle aree esondate, sulle vie di fuga più adatte, diventando un’importante risorsa per chi si occupa di gestire l’emergenza in caso di eventi calamitosi. L’integrazione con i dati di tipo ottico è inoltre essenziale per pervenire ad una migliore caratterizzazione del fenomeno, sia in termini di change detection che di monitoraggio post-evento.