A 22 GHz Pseudo-correlation Water Vapor Radiometer.
| dc.contributor.advisor | Reeves Díaz, Rodrigo Andrés | es |
| dc.contributor.author | Pena Contreras, Leidy | es |
| dc.date.accessioned | 2023-07-11T15:16:13Z | |
| dc.date.accessioned | 2024-05-15T19:14:27Z | |
| dc.date.accessioned | 2024-08-28T22:32:03Z | |
| dc.date.available | 2023-07-11T15:16:13Z | |
| dc.date.available | 2024-05-15T19:14:27Z | |
| dc.date.available | 2024-08-28T22:32:03Z | |
| dc.date.issued | 2023 | |
| dc.description | Tesis para para optar al grado académico de Magíster en Astronomía. | es |
| dc.description.abstract | The radiation that comes from celestial objects is affected by different atmospheric com ponents, mainly by water vapor, which is a highly variable component. This molecule can scatter, absorb and re-emit radiation and, therefore, attenuate it, affecting astronomical ob servations. Water vapor radiometry is an accurate method to measure the water vapor con tent in the atmosphere and, at altitudes < 4000 masl, the 22 GHz emission line is chosen to estimate the amount of water vapor present in the at the time of the astronomical observa tion. This instrument, which is under development at CePIA UdeC laboratory, will provide a notable improvement in the measurement of the line profile of water vapor and will allow atmospheric characterizations that can be validated with other instruments in places where this quantity is relevant. The architecture designed for this project corresponds to a self-calibrated instrument, het erodine and is based on the pseudo-correlation principle. It consists of three parts: frontend, where incoming the RF signal is at a frequency range of 20 - 26 GHz; analog backend, where the RF signal is converted to a manageable frequency range of 0 - 6 GHz, called Intermediate Frequency (IF); and finally, the digital backend where the IF signal is processed in real-time through FFT, with a high spectral resolution of 62.5 kHz; the spectrum is divided intro three bands of 2 GHz each, in different Nyquist zones. Each output of the spectrometer is directly proportional to the brightness temperature of the load or the input, that provides a stable output measurement over time. Design simulations are carried out, mathematical analyzes, data was generated to con firm the proper operation of the radiometer, commercial components are currently acquired, integration of the system is happening, simulations of the expected input signal; and, simu lations of vertical water vapor recovery development techniques are used that will later lead to a prototype of a high-sensitivity tuned 22 GHz precipitable water vapor radiometer. | en |
| dc.description.campus | Concepción | es |
| dc.description.departamento | Departamento de Astronomía | es |
| dc.description.facultad | Facultad de Ciencias Físicas y Matemáticas | es |
| dc.description.sponsorship | ANID, Proyecto FONDEF/IDEA I+D 19I10300 | |
| dc.identifier.doi | https://doi.org/10.29393/TMUdeC-59PL1PC59 | |
| dc.identifier.uri | https://repositorio.udec.cl/handle/11594/10948 | |
| dc.language.iso | en | en |
| dc.publisher | Universidad de Concepción | es |
| dc.rights | Creative Commoms CC BY NC ND 4.0 internacional (Atribución-NoComercial-SinDerivadas 4.0 Internacional) | en |
| dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/4.0/ | en |
| dc.title | A 22 GHz Pseudo-correlation Water Vapor Radiometer. | es |
| dc.type | Tesis | es |