supported by the National Key Research and Development Program of China(2021YFA0715101);partly supported by a National LLR station project;the National Natural Science Foundation of China(NSFC,Grant Nos.11973064 and 42101413);Jilin Province Mid-youth science and technology innovation and entrepreneurship outstanding talent project(20220508147RC);the Changchun City and Chinese Academy of Sciences Science and Technology Cooperation High-tech Industrialization Special Fund Project(21SH05)。
Lunar optical polarization is a fascinating phenomenon that occurs when sunlight reflects off the surface of the Moon and becomes polarized.This study employs a novel split-focus plane polarimetric camera to conduct t...
supported by the Science and Technology Development Fund of Macao(0020/2021/A1,0079/2018/A2);National Key Research and Development(2019YFE0123300);the National Natural Science Foundation of China(12173004,41941002)。
Physical properties(e.g.,ejecta size and distribution)of impact craters are crucial and essential to understanding the ejecta excavation and deposition process,estimating rock breakdown rate,and revealing their evolut...
The Chang’E-6 mission will first land on the far side of the moon and bring lunar samples back.As a hyperspectral imager aboard the Chang’E-6 lander,the Lunar Mineralogical Spectrometer(LMS),will achieve the goal of...
supported by the Specialized Research Fund for State Key Laboratories under Grant 202217;the Key Laboratory of Solar Activity and Space Weather(NSSC)under Grant E26600021S。
Ground-based radio observations below 30 MHz are susceptible to the ionosphere of the Earth and the radio frequency interference.Compared with other space mission concepts,making low frequency observations using an in...
the Indian Space Research Organization,Bangalore,for funding under the Ch-1 AO Research Project(ISRO/SSPO/CH-1/2016–2019)to carry out this research work。
The Mare Moscoviense is an astonishing rare flatland multi-ring basin and one of the recognizable mare regions on the Moon's farside.The mineralogical,chronological,topographical and morphological studies of the maria...
funded by the National Natural Science Foundation of China(NSFC,Grant No.12073048);supported by the Key Research Program,Chinese Academy of Sciences,Grant No.ZDBS-SSW-JS007。
The permittivity of lunar regolith is crucial for further processing and interpretation of radar data.The conventional hyperbolic fitting method ignores the antenna height and spacing and has a significant error at a ...
partially supported by Research Grant (0120U101334);the National Academy of Sciences of Ukraine for this support。
We report about observations of solar U+Ⅲ bursts on 2020 June 5 by means of a new active antenna designed to receive radiation in 4–70 MHz.This instrument can serve as a prototype of the ultralong-wavelength radio t...
funding from the Australian Government;the Government of Western Australiasupported by the B-type Strategic Priority Program of the Chinese Academy of Sciences(Grant Nos.XDB41000000 and NSFC 41972321);NSFC 41674098;CNSA D020205;the B-type Strategic Priority Program of the Chinese Academy of Sciences,Grant No.XDB18010104。
Accurate estimation of cratering asymmetry on the Moon is crucial for understanding Moon evolution history.Early studies of cratering asymmetry have omitted the contributions of high lunar obliquity and inclination.He...
the National Natural Science Foundation of China(U1831132 and 41804025);grant of Hubei Province Natural Science(2018CFA087);supported by the grant from Key Laboratory of Lunar and Deep Space Exploration,CAS;LIESMARS Special Research Funding;funded through a DAR grant in planetology from the French Space Agency(CNES)。
Observations of the sky irradiation intensity in the visible wavelengths during a solar eclipse permit to model the Sun diameter,a key number to constrain the internal structure of our star.In this paper,we present an...
The work was performed as part of the government contract of the SAO RAS approved by the Ministry of Science and Higher Education of the Russian Federation.The reported study was funded by RFBR(project No.20--32-70120);This research has made use of the SIMBAD database,operated at CDS,Strasbourg,France.
Observations by the method of lunar occultations at the 6-m telescope of the SAO RAS reach a resolution limit better than 1mas.We have devised a new method of observation,which allows obtaining the curves of lunar occ...