Smart Multi-Sensor System for Remote Air Quality Monitoring Using Unmanned Aerial Vehicle and LoRaWAN.

Deaths caused by respiratory and cardiovascular diseases have increased by 10%. Every year, exposure to high levels of air pollution is the cause of 7 million premature deaths and the loss of healthy years of life. Air pollution is generally caused by the presence of CO, NO2, NH3, SO2, particulate matter PM10 and PM2.5, mainly emitted by economic activities in large metropolitan areas. The problem increases considerably in the absence of national regulations and the design, installation, and maintenance of an expensive air quality monitoring network. A smart multi-sensor system to monitor air quality is proposed in this work. The system uses an unmanned aerial vehicle and LoRa communication as an alternative for remote and in-situ atmospheric measurements. The instrumentation was integrated modularly as a node sensor to measure the concentration of carbon monoxide (CO), nitrogen dioxide (NO2), ammonia (NH3), sulfur dioxide (SO2), and suspended particulate mass PM10 and PM2.5. The optimal design of the multi-sensor system has been developed under the following constraints: A low weight, compact design, and low power consumption. The integration of the multi-sensor device, UAV, and LoRa communications as a single system adds aeeded flexibility to currently fixed monitoring stations.

Theory of a rotationally shearing interferometer.

We developed a general theory about the performance of a rotational shearing interferometer. We apply the aberration theory to the detection of planets outside our planet system. We considered cases when the mutual coherence functions of the on-axis and the off-axis system are 0 and 1.

Error compensation in a pointing system based on Risley prisms.

Risley prisms are widely used for beam pointing in several optical systems. The exact solution for the inverse problem does not exist, except using numerical methods. However, the errors introduced by misalignment are usually greater than the approximation errors. We present a novel method to compensate alignment errors in pointing systems based on Risley prisms. The prism model that we used is based on paraxial approximation with an additional vector to compensate typical alignment errors. Simulation and experimental results show that the improvement in pointing accuracy is achievable even in comparison with exact ray tracing methods.

Telescope array for extrasolar planet detection from the far side of the Moon.

We propose that an array of 4×4 small-diameter telescopes, possibly 1 m in radius, be placed on the far side of the Moon for continuous monitoring of nearby stars for the existence of a planetary companion, similar to the Earth, and feasible for human colonization. The advantages of this location include long intervals of darkness, availability of a rigid platform in the form of a moon body, and most importantly, the absence of the atmosphere that allows the complete transmission of radiation in the spectral range from UV to millimeter waves. The task is facilitated in that the telescopes would act as light "buckets" to collect photons during long integration periods. All other technology has already been demonstrated, as humans in person delivered optical elements to the Moon's surface during the Apollo era. The disadvantages are primarily operational, in terms of requiring the establishment of a human habitat on the Moon. Likewise, all aspects of constructing a large 75 m by 75 m mirror array on the Moon's surface will be challenging. Simultaneously, the decreased gravity requires less effort and less energy to perform the construction tasks. The absence of atmosphere permits the search to extend from less than 10 to 300 µm to find Earth-like or even much colder planets.

Effects of misalignment errors on the optical transfer functions of synthetic aperture telescopes.

A segmented or diluted aperture optical system will undergo phase errors as a result of errors in the positioning of the segments. The errors associated with a segmented primary mirror limit the image quality obtainable with synthetic aperture telescopes. Here we study the effects of segmentation errors on image quality, considering both the phase angle and the amplitude of the optical transfer function (OTF). We show that, in these kinds of telescope, phasing and alignment errors among segments reduce the amplitude and distort the phase angle of the OTF.