Baseflow, a component of the total streamflow, plays a key role in maintaining aquatic habitats, particularly during extreme drought events. This study investigated baseflow response to a prolonged and extreme meteorological drought event in the Baiyangdian Basin(BYD basin), a temperate water-limited basin in North China. Applying a precipitation series, piecewise regression was used to determine this extreme meteorological drought event, while the Automatic Baseflow Identification Technique(ABI... 相似文献
Precise measurements of neutron star(NS) velocities provide critical clues in regard to the supernova physics and evolution of binary systems. Based on Gaia Data Release 2(DR2), we selected a sample of 24 young( 3 Myr) pulsars with precise parallax measurements and measured the velocity of their local standard of rest(LSR) and the velocity dispersion among their respective local stellar groups. The median velocity difference between thus calculated LSRs and the Galactic rotation model is ～ 7.6 km s~(-1),small compared to the typical velocity dispersion of ～ 27.5 km s~(-1). For pulsars off the Galactic plane,such differences grow significantly to as large as ～ 40 km s~(-1). More importantly, the velocity dispersion of stars in the local group of low-velocity pulsars can be comparable to their transverse velocities, suggesting that the intrinsic velocities of NS progenitors should be taken into account when we consider their natal kicks and binary evolution. We also examined the double NS system J0737-3039 A/B, and measured its transverse velocity to be 26_(-13)~(+18) km s~(-1) assuming nearby Gaia sources are representative of their birth environment. This work demonstrated the feasibility and importance of using Gaia data to study the velocity of individual systems and velocity distribution of NSs. 相似文献
