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 National Natural Science Foundation of China under grant Nos.12393854,12022502 and 12263007;by the High-level Talent Support program of Yunnan Province。
With great advance of ground-based extensive air shower arrays,such as LHAASO and HAWC,many very high energy(VHE)gamma-ray sources have been discovered and are being monitored regardless of the day and the night.Hence...
supported by the National Natural Science Foundation of China (12233005, 12073078 and 12173088);the science research grants from the China Manned Space Project with NO. CMS-CSST-2021-A02, CMS-CSST-2021-A04 and CMS-CSST-2021-A07;grants from the Cyrus Chun Ying Tang Foundations。
Aiming at improving the survey efficiency of the Wide Field Survey Telescope, we have developed a basic scheduling strategy that takes into account the telescope characteristics, observing conditions, and weather cond...
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...
This work was funded by the Youth Innovation Promotion Association of Chinese Academy of Sciences(CAS)(Grant No.2015334)' the National Natural Science Foundation of China(Grant No.11941002)。
The Low-Frequency Radio Spectrometer(LFRS)is a scientific payload onboard the Chang’e-4 lunar lander launched in December 2018.The LFRS provides in-situ measurements of the low-frequency radio phenomena on the far-si...
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...
supported by LIESMARS Special Research Funding;the National Natural Science Foundation of China(U1831132,41590851,11373060,10973030 and 10778635);the State Key Project for Science and Technology(2015CB857101);National Astronomical Observatories,Chinese Academy of Sciences,a grant from the Hubei Province Natural Science(2018CFA087);Open Project of Lunar and Planetary Science Laboratory,Macao University of Science and Technology(FDCT 119/2017/A3);Open Funding of Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing(KF201813)
One of the most efficient ways to probe the lunar inner structure at present is through the study of its rotation.Range and range rate(Doppler) data between the Chang’E-3 lander and station on the Earth were collecte...
supported by the National Natural Science Foundation of China (Grant Nos. 41490633 and 41590851);the open fund of the State Key Laboratory of Lunar and Planetary Sciences (Macao University of Science and Technology) (Macao FDCT Grant No. 119/2017/A3);the open fund of the Key Laboratory of Lunar and Deep Space Exploration, Chinese Academy of Sciences;supported by the National Natural Science Foundation of China (U1931211, 41972322 and 11941001);the Natural Science Foundation of Shandong Province (ZR2019MD008);Qilu (Tang) Young Scholars Program of Shandong University, Weihai (2015WHWLJH14);supported by the Program for JLU Science and Technology Innovative Research Team (JLUSTIRT, 2017TD-26);the Focus on Research and Development Plan in Shandong Province (2018GGX101028);the Shandong Provincial Natural Science Foundation (ZR2019MD015)
Chang’E-4(CE-4)successfully landed on the floor of the Von Kármán crater within the South Pole-Aitken basin(SPA).One of its scientific objectives is to determine the subsurface structure and the thickness of lunar ...
funded by the National Key Research and Development Program of China (2017YFC0305905);the Natural Science Foundation of Zhejiang Province (LR16E090001);NSFC-Zhejiang Joint Fund for the Integration of Industrialization and Informatization (U1709204)
We build a conceptual coupled model of the climate and tidal evolution of the Earth-Moon system to find the influence of the former on the latter. An energy balance model is applied to calculate steady-state temperatu...
supported in part by the Key Research Program of the Chinese Academy of Sciences under Grant (XDPB11);in part by opening fund of State Key Laboratory of Lunar and Planetary Sciences (Macao University of Science and Technology) (Macao FDCT Grant No. 119/2017/A3);in part by the National Natural Science Foundation of China (Grant Nos. 41490633, 41371332 and 41802246);in part by the Science and Technology Development Fund of Macao (Grant 0012/2018/A1)
The volume FeO and TiO_2 abundances(FTAs) of lunar regolith can be more important for understanding the geological evolution of the Moon compared to the optical and gamma-ray results. In this paper, the volume FTAs ar...