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Calibration and validation of the Polarimetric Radio Occultation and Heavy Precipitation experiment aboard the PAZ satellite
This paper presents the calibration and validation studies for the Radio Occultation and Heavy Precipitation experiment aboard the PAZ satellite. These studies, necessary to assess and characterize the noise level and robustness of the differential phase shift (ΔΦ) observable of polarimetric radio o...
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Published in: | Atmospheric measurement techniques 2020-03, Vol.13 (3), p.1299-1313 |
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description | This paper presents the calibration and validation studies for the Radio Occultation and Heavy Precipitation experiment aboard the PAZ satellite. These studies, necessary to assess and characterize the noise level and robustness of the differential phase shift (ΔΦ) observable of polarimetric radio occultations (PROs), confirm the good performance of the experiment and the capability of this technique in sensing precipitation. It is shown how all the predicted effects that could have an impact into the PRO observables (e.g., effect of metallic structures nearby the antenna, the Faraday rotation at the ionosphere, signal impurities in the transmission, and altered cross-polarization isolation) are effectively calibrated and corrected, and they have a negligible effect on the final observable. The on-orbit calibration, performed using an extensive dataset of free-of-rain and low-ionospheric activity observations, is successfully used to correct all the collected observations, which are further validated against independent precipitation observations confirming the sensitivity of the observables to the presence of hydrometeors. The validation results also show how vertically averaged ΔΦ can be used as a proxy for precipitation. |
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Joseph ; de la Torre Juárez, Manuel ; Iijima, Byron ; Wang, Kuo Nung ; Cardellach, Estel</creator><creatorcontrib>Padullés, Ramon ; Ao, Chi O ; Turk, F. Joseph ; de la Torre Juárez, Manuel ; Iijima, Byron ; Wang, Kuo Nung ; Cardellach, Estel</creatorcontrib><description>This paper presents the calibration and validation studies for the Radio Occultation and Heavy Precipitation experiment aboard the PAZ satellite. These studies, necessary to assess and characterize the noise level and robustness of the differential phase shift (ΔΦ) observable of polarimetric radio occultations (PROs), confirm the good performance of the experiment and the capability of this technique in sensing precipitation. It is shown how all the predicted effects that could have an impact into the PRO observables (e.g., effect of metallic structures nearby the antenna, the Faraday rotation at the ionosphere, signal impurities in the transmission, and altered cross-polarization isolation) are effectively calibrated and corrected, and they have a negligible effect on the final observable. The on-orbit calibration, performed using an extensive dataset of free-of-rain and low-ionospheric activity observations, is successfully used to correct all the collected observations, which are further validated against independent precipitation observations confirming the sensitivity of the observables to the presence of hydrometeors. The validation results also show how vertically averaged ΔΦ can be used as a proxy for precipitation.</description><identifier>ISSN: 1867-8548</identifier><identifier>ISSN: 1867-1381</identifier><identifier>EISSN: 1867-8548</identifier><identifier>DOI: 10.5194/amt-13-1299-2020</identifier><language>eng</language><publisher>Katlenburg-Lindau: Copernicus GmbH</publisher><subject>Antennas ; Antennas (Electronics) ; Atmosphere ; Atmospheric precipitations ; Atmospheric water ; Calibration ; Electromagnetism ; Experiments ; Faraday effect ; Global positioning systems ; GPS ; Heavy metals ; Heavy precipitation ; Hydrometeors ; Impurities ; Ionosphere ; Isolation ; Noise levels ; Polarimetry ; Precipitation ; Proxy ; Radio ; Radio occultation ; Rainfall ; Receivers & amplifiers ; Satellites ; Upper atmosphere</subject><ispartof>Atmospheric measurement techniques, 2020-03, Vol.13 (3), p.1299-1313</ispartof><rights>COPYRIGHT 2020 Copernicus GmbH</rights><rights>2020. 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It is shown how all the predicted effects that could have an impact into the PRO observables (e.g., effect of metallic structures nearby the antenna, the Faraday rotation at the ionosphere, signal impurities in the transmission, and altered cross-polarization isolation) are effectively calibrated and corrected, and they have a negligible effect on the final observable. The on-orbit calibration, performed using an extensive dataset of free-of-rain and low-ionospheric activity observations, is successfully used to correct all the collected observations, which are further validated against independent precipitation observations confirming the sensitivity of the observables to the presence of hydrometeors. 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Joseph</au><au>de la Torre Juárez, Manuel</au><au>Iijima, Byron</au><au>Wang, Kuo Nung</au><au>Cardellach, Estel</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Calibration and validation of the Polarimetric Radio Occultation and Heavy Precipitation experiment aboard the PAZ satellite</atitle><jtitle>Atmospheric measurement techniques</jtitle><date>2020-03-19</date><risdate>2020</risdate><volume>13</volume><issue>3</issue><spage>1299</spage><epage>1313</epage><pages>1299-1313</pages><issn>1867-8548</issn><issn>1867-1381</issn><eissn>1867-8548</eissn><abstract>This paper presents the calibration and validation studies for the Radio Occultation and Heavy Precipitation experiment aboard the PAZ satellite. These studies, necessary to assess and characterize the noise level and robustness of the differential phase shift (ΔΦ) observable of polarimetric radio occultations (PROs), confirm the good performance of the experiment and the capability of this technique in sensing precipitation. It is shown how all the predicted effects that could have an impact into the PRO observables (e.g., effect of metallic structures nearby the antenna, the Faraday rotation at the ionosphere, signal impurities in the transmission, and altered cross-polarization isolation) are effectively calibrated and corrected, and they have a negligible effect on the final observable. The on-orbit calibration, performed using an extensive dataset of free-of-rain and low-ionospheric activity observations, is successfully used to correct all the collected observations, which are further validated against independent precipitation observations confirming the sensitivity of the observables to the presence of hydrometeors. The validation results also show how vertically averaged ΔΦ can be used as a proxy for precipitation.</abstract><cop>Katlenburg-Lindau</cop><pub>Copernicus GmbH</pub><doi>10.5194/amt-13-1299-2020</doi><tpages>15</tpages><orcidid>https://orcid.org/0000-0001-8908-0972</orcidid><orcidid>https://orcid.org/0000-0003-2058-3779</orcidid><orcidid>https://orcid.org/0000-0002-9599-6132</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Antennas Antennas (Electronics) Atmosphere Atmospheric precipitations Atmospheric water Calibration Electromagnetism Experiments Faraday effect Global positioning systems GPS Heavy metals Heavy precipitation Hydrometeors Impurities Ionosphere Isolation Noise levels Polarimetry Precipitation Proxy Radio Radio occultation Rainfall Receivers & amplifiers Satellites Upper atmosphere |
title | Calibration and validation of the Polarimetric Radio Occultation and Heavy Precipitation experiment aboard the PAZ satellite |
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