{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,11]],"date-time":"2025-10-11T01:39:14Z","timestamp":1760146754811,"version":"build-2065373602"},"reference-count":27,"publisher":"MDPI AG","issue":"23","license":[{"start":{"date-parts":[[2024,12,3]],"date-time":"2024-12-03T00:00:00Z","timestamp":1733184000000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"funder":[{"DOI":"10.13039\/501100001809","name":"National Natural Science Foundations of China","doi-asserted-by":"publisher","award":["41931073","41874187","CMA2024QN09","2021YFA0718600"],"award-info":[{"award-number":["41931073","41874187","CMA2024QN09","2021YFA0718600"]}],"id":[{"id":"10.13039\/501100001809","id-type":"DOI","asserted-by":"publisher"}]},{"DOI":"10.13039\/501100002885","name":"Meteorological Administration \u2018Ionospheric Forecast and Alerting\u2019 Youth Innovation Team","doi-asserted-by":"publisher","award":["41931073","41874187","CMA2024QN09","2021YFA0718600"],"award-info":[{"award-number":["41931073","41874187","CMA2024QN09","2021YFA0718600"]}],"id":[{"id":"10.13039\/501100002885","id-type":"DOI","asserted-by":"publisher"}]},{"DOI":"10.13039\/501100012166","name":"National Key R&amp;D Program of China","doi-asserted-by":"publisher","award":["41931073","41874187","CMA2024QN09","2021YFA0718600"],"award-info":[{"award-number":["41931073","41874187","CMA2024QN09","2021YFA0718600"]}],"id":[{"id":"10.13039\/501100012166","id-type":"DOI","asserted-by":"publisher"}]}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Remote Sensing"],"abstract":"<jats:p>Initial comparisons of the OI 135.6 nm and LBH radiances collected by the FY3E\/TriIPM and TIMED\/GUVI from 1 January 2023 to 15 May 2024 at 0500 LT and 1700 LT are performed in this study. The analysis reveals that the consistencies of the OI 135.6 nm and LBH radiances are better at 1700 LT than those at 0500 LT in the Northern and Southern Hemispheres, and that the consistencies of the LBH radiances are better than those of OI 135.6 nm in both hemispheres at 0500 LT and 1700 LT. Moreover, compared to the equinoxes, the measurements of FY3E\/TriIPM and TIMED\/GUVI agree well in summer and winter, especially at 1700 LT. Despite the observed consistencies between these two instruments, differences are also existent, especially for the OI 135.6 nm in equinoxes at 1700 LT and at latitudes between 30\u00b0S and 60\u00b0S at 0500 LT, which may be due to the altitudinal and responsivity differences between these two instruments. This study illustrates the possibility of the fusion of FUV observations from multiple sources for future modeling.<\/jats:p>","DOI":"10.3390\/rs16234528","type":"journal-article","created":{"date-parts":[[2024,12,3]],"date-time":"2024-12-03T09:18:32Z","timestamp":1733217512000},"page":"4528","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":0,"title":["Initial Cross-Validation of the OI 135.6 nm and LBH Radiances from FY3E\/TriIPM and TIMED\/GUVI"],"prefix":"10.3390","volume":"16","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-3605-6244","authenticated-orcid":false,"given":"Qian","family":"Ye","sequence":"first","affiliation":[{"name":"Key Laboratory of Space Weather, National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing 100081, China"},{"name":"Innovation Center for Feng Yun Meteorological Satellite (FYSIC), Beijing 100081, China"}]},{"given":"Qian","family":"Song","sequence":"additional","affiliation":[{"name":"Key Laboratory of Space Weather, National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing 100081, China"},{"name":"Innovation Center for Feng Yun Meteorological Satellite (FYSIC), Beijing 100081, China"}]},{"given":"Tian","family":"Mao","sequence":"additional","affiliation":[{"name":"Key Laboratory of Space Weather, National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing 100081, China"},{"name":"Innovation Center for Feng Yun Meteorological Satellite (FYSIC), Beijing 100081, China"}]},{"given":"Xiaoxin","family":"Zhang","sequence":"additional","affiliation":[{"name":"Key Laboratory of Space Weather, National Satellite Meteorological Center (National Center for Space Weather), China Meteorological Administration, Beijing 100081, China"},{"name":"Innovation Center for Feng Yun Meteorological Satellite (FYSIC), Beijing 100081, China"}]}],"member":"1968","published-online":{"date-parts":[[2024,12,3]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"813","DOI":"10.1016\/S0273-1177(02)00886-4","article-title":"The use of far ultraviolet remote sensing to monitor space weather","volume":"31","author":"Paxton","year":"2003","journal-title":"Adv. Space Res."},{"key":"ref_2","doi-asserted-by":"crossref","unstructured":"Qin, J. (2020). Far ultraviolet remote sensing of the nighttime ionosphere using the OI 130.4-nm emission. J. Geophys. Res. Space Phys., 125.","DOI":"10.1029\/2020JA028049"},{"key":"ref_3","doi-asserted-by":"crossref","first-page":"20180098","DOI":"10.1098\/rsta.2018.0098","article-title":"Ionospheric response to solar and interplanetary disturbances: A swarm perspective","volume":"377","author":"Balasis","year":"2019","journal-title":"Philos. Trans. R. Soc. A Math. Phys. Eng. Sci."},{"key":"ref_4","doi-asserted-by":"crossref","first-page":"e2023EA003222","DOI":"10.1029\/2023EA003222","article-title":"Inferring the ionospheric state with the far ultraviolet imager on the Fengyun-4C geostationary satellite: Retrieval algorithm and verification","volume":"10","author":"Qin","year":"2023","journal-title":"Earth Space Sci."},{"key":"ref_5","doi-asserted-by":"crossref","first-page":"A26","DOI":"10.1051\/swsc\/2013048","article-title":"Geomagnetic response to solar and interplanetary disturbances","volume":"3","author":"Saiz","year":"2013","journal-title":"J. Space Weather Space Clim."},{"key":"ref_6","doi-asserted-by":"crossref","first-page":"1","DOI":"10.1007\/BF01206000","article-title":"Ultraviolet spectroscopy and remote sensing of the upper atmosphere","volume":"Volume 58","author":"Meier","year":"1991","journal-title":"Space Science Reviews"},{"key":"ref_7","doi-asserted-by":"crossref","first-page":"12217","DOI":"10.1029\/95JA00574","article-title":"Satellite remote sensing of thermospheric O\/N2 and solar EUV: 1. Theory","volume":"100","author":"Strickland","year":"1995","journal-title":"J. Geophys. Res. Space Phys."},{"key":"ref_8","doi-asserted-by":"crossref","first-page":"e2020JA028108","DOI":"10.1029\/2020JA028108","article-title":"Observation of postsunset OI 135.6 nm radiance enhancement over South America by the GOLD mission","volume":"126","author":"Cai","year":"2021","journal-title":"J. Geophys. Res. Space Phys."},{"key":"ref_9","doi-asserted-by":"crossref","first-page":"e2020JA027810","DOI":"10.1029\/2020JA027810","article-title":"Variations of lower thermospheric FUV emissions based on GOLD observations and GLOW modeling","volume":"125","author":"Greer","year":"2020","journal-title":"J. Geophys. Res. Space Phys."},{"key":"ref_10","doi-asserted-by":"crossref","first-page":"859","DOI":"10.1029\/2012JA018112","article-title":"The effect of the 135.6 nm emission originated from the ionosphere on the TIMED\/GUVI O\/N2 ratio","volume":"118","author":"Kil","year":"2013","journal-title":"J. Geophys. Res. Space Phys."},{"key":"ref_11","doi-asserted-by":"crossref","first-page":"1577","DOI":"10.5194\/amt-15-1577-2022","article-title":"Far-ultraviolet airglow remote sensing measurements on Feng Yun 3-D meteorological satellite","volume":"15","author":"Wang","year":"2022","journal-title":"Atmos. Meas. Tech."},{"key":"ref_12","doi-asserted-by":"crossref","first-page":"4915","DOI":"10.1016\/j.eswa.2014.02.026","article-title":"Learned lessons in credit card fraud detection from a practitioner perspective","volume":"41","author":"Caelen","year":"2014","journal-title":"Expert Syst. Appl."},{"key":"ref_13","doi-asserted-by":"crossref","unstructured":"Fayyad, J., Jaradat, M.A., Gruyer, D., and Najjaran, H. (2020). Deep learning sensor fusion for autonomous vehicle perception and localization: A review. Sensors, 20.","DOI":"10.3390\/s20154220"},{"key":"ref_14","doi-asserted-by":"crossref","first-page":"4","DOI":"10.1016\/j.inffus.2013.12.002","article-title":"Medical image fusion: A survey of the state of the art","volume":"19","author":"James","year":"2014","journal-title":"Inf. Fusion"},{"key":"ref_15","doi-asserted-by":"crossref","unstructured":"Joshi, N., Baumann, M., Ehammer, A., Fensholt, R., Grogan, K., Hostert, P., Jepsen, M., Kuemmerle, T., Meyfroidt, P., and Mitchard, E. (2016). A review of the application of optical and radar remote sensing data fusion to land use mapping and monitoring. Remote Sens., 8.","DOI":"10.3390\/rs8010070"},{"key":"ref_16","doi-asserted-by":"crossref","unstructured":"Mohammadi, N., and Taylor, J.E. (December, January 27). Smart city digital twins. Proceedings of the 2017 IEEE Symposium Series on Computational Intelligence (SSCI), Honolulu, HI, USA.","DOI":"10.1109\/SSCI.2017.8285439"},{"key":"ref_17","doi-asserted-by":"crossref","unstructured":"Meier, R.R., Crowley, G., Strickland, D.J., Christensen, A.B., Paxton, L.J., Morrison, D., and Hackert, C.L. (2005). First look at the 20 November 2003 superstorm with TIMED\/GUVI: Comparisons with a thermospheric global circulation model. J. Geophys. Res. Space Phys., 110.","DOI":"10.1029\/2004JA010990"},{"key":"ref_18","doi-asserted-by":"crossref","unstructured":"Zhang, Y., Paxton, L.J., Morrison, D., Wolven, B., Kil, H., Meng, C.-I., Mende, S.B., and Immel, T.J. (2004). O\/N2 changes during 1\u20134 October 2002 storms: IMAGE SI-13 and TIMED\/GUVI observations. J. Geophys. Res. Space Phys., 109.","DOI":"10.1029\/2004JA010441"},{"key":"ref_19","doi-asserted-by":"crossref","first-page":"105258","DOI":"10.1016\/j.jastp.2020.105258","article-title":"Estimation of solar EUV flux from TIMED\/GUVI data","volume":"202","author":"Zhang","year":"2020","journal-title":"J. Atmos. Sol. Terr. Phys."},{"key":"ref_20","doi-asserted-by":"crossref","first-page":"e2021JA029333","DOI":"10.1029\/2021JA029333","article-title":"Ionospheric and Thermospheric Contributions in TIMED\/GUVI O 135.6 nm Radiances","volume":"126","author":"Zhang","year":"2021","journal-title":"J. Geophys. Res. Space Phys."},{"key":"ref_21","doi-asserted-by":"crossref","first-page":"4379","DOI":"10.1016\/j.asr.2023.09.036","article-title":"Impact of the February 3\u20134, 2022 geomagnetic storm on ionospheric S4 amplitude scintillation index: Observations and implications","volume":"72","author":"Duann","year":"2023","journal-title":"Adv. Space Res."},{"key":"ref_22","doi-asserted-by":"crossref","unstructured":"Gan, Q., Eastes, R.W., Burns, A.G., Wang, W., Qian, L., Solomon, S.C., Codrescu, M.V., McInerney, J., and McClintock, W.E. (2020). First synoptic observations of geomagnetic storm effects on the global-scale OI 135.6-nm dayglow in the thermosphere by the GOLD mission. Geophys. Res. Lett., 47.","DOI":"10.1029\/2019GL085400"},{"key":"ref_23","doi-asserted-by":"crossref","first-page":"e2019JA027767","DOI":"10.1029\/2019JA027767","article-title":"Comparison of GOLD night measurements with total electron content: Preliminary results","volume":"125","author":"Cai","year":"2020","journal-title":"J. Geophys. Res. Space Phys."},{"key":"ref_24","doi-asserted-by":"crossref","first-page":"1","DOI":"10.1007\/s00376-021-1304-7","article-title":"FY-3E: The first operational meteorological satellite mission in an early morning orbit","volume":"39","author":"Zhang","year":"2022","journal-title":"Adv. Atmos. Sci."},{"key":"ref_25","doi-asserted-by":"crossref","first-page":"2151","DOI":"10.1016\/j.asr.2020.07.027","article-title":"Observation of thermosphere and ionosphere using the ionosphere PhotoMeter (IPM) on the Chinese meteorological satellite FY-3D","volume":"66","author":"Jiang","year":"2020","journal-title":"Adv. Space Res."},{"key":"ref_26","doi-asserted-by":"crossref","first-page":"2781","DOI":"10.1016\/j.asr.2022.11.025","article-title":"Nightside 135.6 nm emission enhancements of mid\/low latitudes during geomagnetic storms as observed by the ionosphere PhotoMeter (IPM) on the Chinese meteorological satellite FY-3D","volume":"71","author":"Jiang","year":"2023","journal-title":"Adv. Space Res."},{"key":"ref_27","doi-asserted-by":"crossref","unstructured":"Christensen, A.B., Paxton, L.J., Avery, S., Craven, J., Crowley, G., Humm, D.C., Kil, H., Meier, R.R., Meng, C.-I., and Morrison, D. (2003). Initial observations with the global ultraviolet imager (GUVI) in the NASA TIMED satellite mission. J. Geophys. Res. Space Phys., 108.","DOI":"10.1029\/2003JA009918"}],"container-title":["Remote Sensing"],"original-title":[],"language":"en","link":[{"URL":"https:\/\/www.mdpi.com\/2072-4292\/16\/23\/4528\/pdf","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2025,10,10]],"date-time":"2025-10-10T16:45:45Z","timestamp":1760114745000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.mdpi.com\/2072-4292\/16\/23\/4528"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2024,12,3]]},"references-count":27,"journal-issue":{"issue":"23","published-online":{"date-parts":[[2024,12]]}},"alternative-id":["rs16234528"],"URL":"https:\/\/doi.org\/10.3390\/rs16234528","relation":{},"ISSN":["2072-4292"],"issn-type":[{"type":"electronic","value":"2072-4292"}],"subject":[],"published":{"date-parts":[[2024,12,3]]}}}