Optimization of PEDOT: PSS thin film for organic solar cell application

As a clean and renewable energy source, the development of the organics solar cells is very promising due to the inorganic solar cell inconvenient production process and material shortness. In this work, P3HT: PCBM bulk-heterojunction devices were produced by spin coating organic layers onto ITO coated glass in air, and deposited it with an Au layer as top metal electrode. Inverted devices were fabricated with and without PEDOT:PSS. Then, several attempts have been conducted to improve power conversion efficiency by optimizing different thicknesses of the interlayer between active layer and metal. Power conversion efficiency, short circuit current, open circuit voltage and fill factor were measured on all produced devices. In contrast, the devices with 50 nm thickness of PEDOT: PSS layer showed as better solar cell with 0.0394% efficiency compared to the devices without PEDOT:PSS. As a result, introduction of PEDOT:PSS layer on active layer improves hole collection at the metal / active layer interface

Investigation of planetary ionospheres

Feasibility of using radio sounding techniques to investigate ionospheric properties of planet

Ionospheric gravity wave measurements with the USU dynasonde

A method for the measurement of ionospheric Gravity Wave (GW) using the USU Dynasonde is outlined. This method consists of a series of individual procedures, which includes functions for data acquisition, adaptive scaling, polarization discrimination, interpolation and extrapolation, digital filtering, windowing, spectrum analysis, GW detection, and graphics display. Concepts of system theory are applied to treat the ionosphere as a system. An adaptive ionogram scaling method was developed for automatically extracting ionogram echo traces from noisy raw sounding data. The method uses the well known Least Mean Square (LMS) algorithm to form a stochastic optimal estimate of the echo trace which is then used to control a moving window. The window tracks the echo trace, simultaneously eliminating the noise and interference. Experimental results show that the proposed method functions as designed. Case studies which extract GW from ionosonde measurements were carried out using the techniques described. Geophysically significant events were detected and the resultant processed results are illustrated graphically. This method was also developed for real time implementation in mind

The electronic Space Weather upper atmosphere (eSWua) project at INGV: advancements and state of the art

The eSWua project is based on measurements performed by all the instruments installed by the upper atmosphere physics group of the Istituto Nazionale di Geofisica e Vulcanologia, Italy and on all the related studies. The aim is the realization of a hardware-software system to standardize historical and real-time observations for different instruments. <br><br> An interactive Web site, supported by a well organized database, can be a powerful tool for the scientific and technological community in the field of telecommunications and space weather. The most common and useful database type for our purposes is the relational one, in which data are organized in tables for petabytes data archiving and the complete flexibility in data retrieving. <br><br> The project started in June 2005 and will last till August 2007. In the first phase the major effort has been focused on the design of hardware and database architecture. The first two databases related to the DPS4 digisonde and GISTM measurements are complete concerning populating, tests and output procedures. Details on the structure and Web tools concerning these two databases are presented, as well as the general description of the project and technical features

Rocket and laboratory studies in aeronomy and astronomy

Data extracted from semi-annual status reports presented include: a list of all sounding rocket launches performed under NASA sponsorship; a list of Ph.D. and M.A. degrees awarded to students who worked in these programs; a summary bibliography of all publications through 1983; the most recent list of the publications from the IUE program; a summary of instrument development supported by the Johns Hopkins sounding rocket program; and a list of faculty and post-doctoral research associates whose work was supported by this grant

Design of a flexible and low-power ionospheric sounder

Thesis (M.S.) University of Alaska Fairbanks, 2014Characterizing the structure of the ionosphere has practical applications for telecommunications and scientific applications for studies of the near-earth space environment. Among several methods for measuring parameters of the ionosphere is ionospheric sounding, a radar technique that determines the electron content of the ionosphere as a function of height. Various research, military, and commercial institutions operate hundreds of ground-based ionosondes throughout the globe, and new ionosondes continue to be deployed in increasingly remote and distant locations. This thesis presents the design of an ionospheric sounder that reduces the power, size, and cost compared to existing systems. Key improvements include the use of an open-source software-defined radio platform and channel-aware dynamic sounding scheduling.Chapter 1. Introduction -- 1.1. A brief historical background -- 1.2. The ionosphere -- 1.3. Instruments for studying the ionosphere -- 1.4. Thesis organization -- Chapter 2. Radio waves and the ionosphere -- 2.1. Dispersion relation of electromagnetic waves in the ionosphere -- 2.2. Power reflected from the ionosphere -- 2.3 Noise in the HF spectrum -- 2.4. Ionograms -- Chapter 3. Radar principles -- 3.1. Target detection -- 3.2. Range and doppler elocity -- 3.3. Range-doppler ambiguity -- 3.4. Resolution and precision --3.5. Multi-pulse integration -- 3.6. Pulse compression -- 3.7. Practical limits of performance -- Chapter 4. Survey of current systems -- 4.1. Coherent transmission/reception and digital systems -- 4.2. Phase-coded pulses -- 4.3. Coherent integration of multiple pulses -- 4.4. Phased antenna arrays -- 4.5. O- and X-mode discrimination -- Chapter 5. System description -- 5.1. Design approach -- 5.2. Overview of the Ettus Research USRP -- 5.3. Using the USRP as a radar -- 5.4. Waveform Generation -- 5.5. Processing the received signal -- 5.6. Scheduling -- 5.7. Completing the system -- Chapter 6. Sounding results -- 6.1. Single frequency soundings -- 6.2. Swept frequency soundings -- Chapter 7. Conclusion -- 7.1. Evaluation of performance -- 7.2. Costs -- 7.3. Future improvements -- 7.4. Deploying a terrestrial ionosonde -- 7.5. Deploying a space-borne ionosonde -- References

Soundings of the ionospheric HF radio link between Antarctica and Spain

Aquest treball ha estat realitzat sota el context del projecte Antàrtic del Grup d’Investigació en Electromagnetisme i Comunicacions de La Salle (Universitat Ramon Llull). L’objectiu d’aquest projecte és l’estudi del canal ionosfèric com a canal de comunicacions digitals i el disseny de modulacions avançades adaptades. Aquest treball de tesi es centra en el sondeig del canal HF al llarg de tres campanyes consecutives des de 2009 fins 2012 entre la Base Antártica Española (BAE) i l’Observatorio de l’Ebre (OE). En primer lloc, a partir del sondeig en banda estreta s’han obtingut la disponibilitat i la freqüència de màxima disponibilitat (FLA) entre la BAE i OE en el període 2009-2012. En segon lloc, el sondeig en banda ampla ens ha permès estimar la relació senyal-soroll en banda ampla, la dispersió temporal (composite multipath spread), la dispersió freqüencial (composite Doppler spread and Doppler frequency shift) i el temps de propagació. En tercer lloc, s’ha investigat la variació intra-diària i inter-diària d’alguns paràmetres (Densitat total d’electrons, freqüències crítiques i la MUF3000) que han estat mesurades en sondeig vertical en quatre estacions situades al llarg del camí entre la BAE i OE. Finalment, s’ha estudiat la correlació entre la FLA de l’enllaç oblic i la MUF300 de les estacions intermèdies properes als punts de reflexió.Este trabajo ha sido realizado en el contexto del proyecto Antártico del Grupo de Investigación en Electromagnetismo y Comunicaciones de La Salle (Universidad Ramon Llull). El objetivo de este proyecto es el estudio del canal ionosférico como canal de comunicaciones digitales además del diseño de modulaciones avanzadas adaptadas. Este trabajo se centra en el sondeo del canal HF a lo largo de tres campañas consecutivas desde 2009 hasta 2012 entre la Base Antártica Española (BAE) y el Observatorio del Ebro (OE). Primero, a partir del sondeo en banda estrecha se han obtenido la disponibilidad y la frecuencia de máxima disponibilidad (FLA) entre la BAE y OE en el periodo 2009-2012. En segundo lugar, el sondeo en banda ancha nos ha permitido estimar la relación señal-ruido en banda ancha, la dispersión temporal (composite multipath spread), la dispersión frecuencial (composite Doppler spread and Doppler frequency shift) y el tiempo de propagación. En tercer lugar, se ha investigado la variación intra-diaria y la inter-diaria de varios parámetros (Densidad total de electrones, frecuencias críticas y la MUF3000) que han sido medidas en sondeo vertical en cuatro estaciones situadas a lo largo del camino entre la BAE y OE.Finalmente, se ha estudiado la correlación entre la FLA del enlace oblicuo y la MUF300 de las estaciones intermedias cercanas a los puntos de reflexión.This work has been done in the context of the Antarctic Project of the Research Group in Electromagnetism and Communications of La Salle (Ramon Llull University). The aim of this project is to study the ionospheric channel as a digital communications channel as well as to design specific advanced modulations specially adapted to it. This work is devoted to the HF channel sounding throughout three consecutive surveys from 2009 to 2012 between the Spanish Antarctic Station (SAS) and the Ebro Observatory (OE). First, the availability and the Frequency of Largest Availability (FLA) of the SAS-OE link have been obtained from the narrowband sounding technique from 2009 to 2012. Second, wideband sounding of the SAS-OE link has been done to estimate the wideband Signal to Noise Ratio (SNR), the time dispersion (composite multipath spread), frequency dispersion (composite Doppler spread and Doppler frequency shift), and the propagation time. Third, there has been an investigation about the day-to-day and inter-day variations of various parameters (e.g., Total Electron Density, critical frequencies, and Maximum Usable Frequency for ground distance MUF(3000)) that have been measured at four Vertical Incidence Sounding (VIS) stations located over the SAS-OE link path throughout three consecutive surveys (from 2009 to 2012). Finally, the correlation between the FLA of the SAS-OE ionospheric link and the MUF(3000) obtained from VIS stations located close to the reflection points of the same link has been studied

The NASA Suborbital Program: A status review

The status of the NASA suborbital program is reviewed and its importance to astrophysical and geophysical programs is assessed. A survey of past scientific and developmental accomplishments, an examination of the trends in program costs, and an analysis of current and future program roles are included. The technical disciplines examined are primarily those of astronomy/astrophysics/solar physics and magnetospheric/ionospheric/ atmospheric physics

Phoenix-XNS - A Miniature Real-Time Navigation System for LEO Satellites

The paper describes the development of a miniature GPS receiver with integrated real-time navigation system for orbit determination of satellites in low Earth orbit (LEO). The Phoenix-XNS receiver is based on a commercial-off-the-shelf (COTS) single-frequency GPS receiver board that has been qualified for use in a moderate space environment. Its firmware is specifically designed for space applications and accounts for the high signal dynamics in the acquisition and tracking process. The supplementary eXtended Navigation System (XNS) employs an elaborate force model and a 24-state Kalman filter to provide a smooth and continuous reduced-dynamics navigation solution even in case of restricted GPS availability. Through the use of the GRAPHIC code-carrier combination, ionospheric path delays can be fully eliminated in the filter, which overcomes the main limitation of conventional single-frequency receivers. Tests conducted in a signal simulator test bed have demonstrated a filtered navigation solution accuracy of better than 1 m (3D rms)

Design of a receiver for measurement of real-time ionospheric reflection height

Thesis (M.S.) University of Alaska Fairbanks, 2005The HF (high frequency) radar at Kodiak Island, Alaska, is part of the SuperDARN (Super Dual Auroral Radar Network) network of radars designed to detect echoes from ionospheric field-aligned density irregularities. Normal azimuth scans of the radar begin on whole minute boundaries leading to 12 s downtime between each scan. The radar makes use of this down time, by stepping through eight different frequencies for each beam direction using 1 or 2 s integration periods. A new receiver system has been developed at Poker Flat Research Range (PFRR), to utilize the ground scatter returns from radar's sounding mode of operation and calculate the ionospheric virtual reflection height. This would result in considerable improvement in the accuracy of critical frequency and Angle Of Arrival (AOA) estimations made by the Kodiak SuperDARN.Introduction -- Background -- Structure of the ionosphere -- Photoionization -- Recombination -- Layers -- Ionospheric refraction -- Ionospheric propagation -- Reflection at vertical incidence -- Virtual height concept -- Oblique incidence -- Motivation -- Problem statement and proposed solution -- Equipment overview -- Basic radar definitions -- Overview of the HF radar at Kodiak -- Frequency operation -- Sounding mode -- Antennas -- Power -- Receiver antenna -- Reflector analysis -- GPS clock card -- Clock card specifications -- Overview of PCI card countrol/status registers -- The synchronized generator : GPS mode outline -- Software time capture -- Event time capture -- Receiver card -- specifications -- The system design and implementation -- Specifications -- The pulse sequence -- The QNX operating system -- Configuring the clock card -- Configuring the GC214 -- Sampling -- Mixing -- Decimation -- Filtering -- Resampling -- GC214 latency -- Gain -- Data header format -- Direct memory access (DMA) -- DMA buffer creation -- RAM--disk -- External trigger synchronization -- Signal processing code -- Link budget -- Results and future work -- Final code -- Results -- Errors -- Applications -- Future work -- Bibliography