The University of Southampton
University of Southampton Institutional Repository

A recalibration model based on the statistical regression analysis method to align the microwave data of Chang’E-1 and Chang’E-2

A recalibration model based on the statistical regression analysis method to align the microwave data of Chang’E-1 and Chang’E-2
A recalibration model based on the statistical regression analysis method to align the microwave data of Chang’E-1 and Chang’E-2

The two microwave radiometers (MRMs) onboard the Chinese Lunar explorers Chang'E-1 (CE-1) and Chang'E-2 (CE-2) are considered to be identical instruments, yet the results differ, with lunar brightness temperatures obtained by CE-2 generally lower than those of CE-1 in all four frequency channels. The differences can reach over 10 K in the same local time. We propose a recalibration model that takes into account the brightness temperature constant shift of the MRM equipment and the possibility that the Chang'E calibration antennas may have inadvertently picked up some thermal radiation from the lunar surface due to its field of view cutting into the lunar surface. These effects may have negatively influenced the accuracy of the simple two-point calibration procedure and led to the difference between the available MRM level 2C data from CE-1 and CE-2. Our recalibration model determines the correction parameters through a statistical analysis that minimizes the mismatch between the two datasets. Recalibration of the level 2C data based on our recalibration model successfully realigns the microwave brightness temperatures measured by CE-1 and CE-2.

Chang'E (CE), Microwave brightness temperature (T ), Moon, Recalibration model
0196-2892
1-11
Yang, Fan
6db7f8d2-9649-4bcb-ad3d-5d7af936fb9a
Hu, Guo-ping
28d475cc-5ca7-4c47-90b2-6bd9c6ab16a2
Chan, Kwing Lam
57e6b143-b7aa-4233-930e-22ac010f2486
Tsang, Ken-tao
4de08895-93f0-49e2-ac24-d6b5fe780479
Zheng, Yong-chun
368cf0ae-b76b-4ba4-b520-48398fd63e93
Xu, Yi
2981c7dc-5bfd-43ea-9a73-4d44d79d3951
Yu, Lu Heng Sunny
ef5bc4e3-409d-455e-a808-f5da5f3d1416
Yang, Fan
6db7f8d2-9649-4bcb-ad3d-5d7af936fb9a
Hu, Guo-ping
28d475cc-5ca7-4c47-90b2-6bd9c6ab16a2
Chan, Kwing Lam
57e6b143-b7aa-4233-930e-22ac010f2486
Tsang, Ken-tao
4de08895-93f0-49e2-ac24-d6b5fe780479
Zheng, Yong-chun
368cf0ae-b76b-4ba4-b520-48398fd63e93
Xu, Yi
2981c7dc-5bfd-43ea-9a73-4d44d79d3951
Yu, Lu Heng Sunny
ef5bc4e3-409d-455e-a808-f5da5f3d1416

Yang, Fan, Hu, Guo-ping, Chan, Kwing Lam, Tsang, Ken-tao, Zheng, Yong-chun, Xu, Yi and Yu, Lu Heng Sunny (2021) A recalibration model based on the statistical regression analysis method to align the microwave data of Chang’E-1 and Chang’E-2. IEEE Transactions on Geoscience and Remote Sensing, 60, 1-11. (doi:10.1109/TGRS.2021.3126349).

Record type: Article

Abstract

The two microwave radiometers (MRMs) onboard the Chinese Lunar explorers Chang'E-1 (CE-1) and Chang'E-2 (CE-2) are considered to be identical instruments, yet the results differ, with lunar brightness temperatures obtained by CE-2 generally lower than those of CE-1 in all four frequency channels. The differences can reach over 10 K in the same local time. We propose a recalibration model that takes into account the brightness temperature constant shift of the MRM equipment and the possibility that the Chang'E calibration antennas may have inadvertently picked up some thermal radiation from the lunar surface due to its field of view cutting into the lunar surface. These effects may have negatively influenced the accuracy of the simple two-point calibration procedure and led to the difference between the available MRM level 2C data from CE-1 and CE-2. Our recalibration model determines the correction parameters through a statistical analysis that minimizes the mismatch between the two datasets. Recalibration of the level 2C data based on our recalibration model successfully realigns the microwave brightness temperatures measured by CE-1 and CE-2.

This record has no associated files available for download.

More information

Accepted/In Press date: 25 October 2021
e-pub ahead of print date: 8 November 2021
Published date: 13 November 2021
Keywords: Chang'E (CE), Microwave brightness temperature (T ), Moon, Recalibration model

Identifiers

Local EPrints ID: 456610
URI: http://eprints.soton.ac.uk/id/eprint/456610
ISSN: 0196-2892
PURE UUID: be225ed7-ed71-4d6e-b67c-d5a196d386b7
ORCID for Lu Heng Sunny Yu: ORCID iD orcid.org/0000-0003-2207-4214

Catalogue record

Date deposited: 05 May 2022 16:52
Last modified: 17 Mar 2024 04:09

Export record

Altmetrics

Contributors

Author: Fan Yang
Author: Guo-ping Hu
Author: Kwing Lam Chan
Author: Ken-tao Tsang
Author: Yong-chun Zheng
Author: Yi Xu

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×