funded by Special Foundation of Basic Science and Technology Resources Survey of Ministry of Science and Technology of China[No.2017FY101201]。
Climate change has been referred to as one of the greatest threats to human health,with reports citing likely increases in extreme meteorological events.In this study,we estimated the relationships between temperature...
supported by the National Natural Science Foundation of China (Grant No. 41230421);the "973" project (Grant Nos. 2015CB452802 and 2013CB430101) of the Ministry of Science and Technology of China
Forecasts of the intensity and quantitative precipitation of tropical cyclones(TCs) are generally inaccurate, because the strength and structure of a TC show a complicated spatiotemporal pattern and are affected by ...
Project supported by the National Natural Science Foundation of China(Grant Nos.11275024,61274024,and 61474123);the Youth Innovation Promotion Association,China(Grant No.2013105);the Ministry of Science and Technology of China(Grant Nos.2013YQ030595-3 and 2011AA120101)
We characterized the dependence of the timing jitter of an InGaAs/InP single-photon avalanche diode on the excess bias voltage(V(ex)) when operated in 1-GHz sinusoidally gated mode.The single-photon avalanche diod...
supported by the National Basic Research Program of China (973 program, 2014CB845700);the National Natural Science Foundation of China (Grant Nos. 11322327, 11390374 and 61561053);the Natural Science Foundation of Yunnan Province (Grant Nos. 2013FB083 and 2013HB097)
HD 49798(a hydrogen depleted subdwarf O6 star) with its massive white dwarf(WD) companion has been suggested to be a progenitor candidate of a type Ia supernova(SN Ia). However, it is still uncertain whether the...
supported by the National Natural Science Foundation of China (Grant No. 10821061);the National Basic Research Program of China (Grant No. 2007CB815406);the Chinese Academy of Sciences (Grant No. KJCX2-YW-T24)
HD 49798 is a hydrogen depleted subdwarf 06 star and has an X-ray pulsating companion (RX J0648.0-4418). The X-ray pulsating companion is a massive white dwarf. Employing Eggleton's stellar evolution code with the ...