AMUSE
发表于 2025-3-21 17:19:17
书目名称Sources and Scintillations影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0872096<br><br> <br><br>书目名称Sources and Scintillations读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0872096<br><br> <br><br>
忙碌
发表于 2025-3-21 21:45:57
Looking Into Pulsar Magnetospheresttering angle that may beas large as 0.1 radians, and a typical decorrelation time of 10. seconds. Refractive scattering due tolarge scale inhomogeneities is also possible, with a typical angle of 10. radians and a correlationtime of the order of 10. seconds. Some of the magneto spheric propagation effects may have alreadybeen observed.
别炫耀
发表于 2025-3-22 02:51:11
The Galactic Distribution of Electron Density Microstructure Inferred from Radio Scattering ObservatGalactic distribution of electron density andits fluctuations, as inferred from a number of observables, including angular and pulse broadening,diffractive scintillations, and dispersion measures. Propects for improving the Galactic model areoutlined.
Coordinate
发表于 2025-3-22 06:27:42
Incompressible MHD Turbulencee cascade dynamics. Slowwaves play a passive role and adopt the spectrum set by the shear Alfvén waves. Cascades composedentirely of shear Alfvén waves do not generate a significant measure of slow waves. MHD turbulenceis anisotropic with energy cascading more rapidly along .⊥. than along .∥. Anisot
碳水化合物
发表于 2025-3-22 09:34:36
http://reply.papertrans.cn/88/8721/872096/872096_5.png
minaret
发表于 2025-3-22 16:33:40
The Parkes Multibeam Pulsar Survey and Interstellar Scatteringreceiver on the Parkes 64-m radiotelescope.It is an international collaboration between groups at Jodrell Bank Observatory, MassachusettsInstitute of Technology, Bologna Astronomical Observatory and the ATNF. The survey commencedin 1997 August, and has so far succeeded in finding more than 550 previ
Regurgitation
发表于 2025-3-22 18:30:41
Frequency Structure of Radio Scintillations for Several Pulsarservations made with differentinstruments and at different radio frequencies. All objects but the pulsar B1508+55 were detected tohave more than one frequency scale. The obtained values of scattering parameters are not contrary ingeneral to the Kkolmogorov form of density fluctuation spectrum.
Heretical
发表于 2025-3-22 21:12:51
http://reply.papertrans.cn/88/8721/872096/872096_8.png
小隔间
发表于 2025-3-23 03:13:24
Scattering Of The Low Frequency Pulsar Radiationgest uniform sample of directmeasurements of pulsar scattering τ. , which make it feasible to analyze the dependence of this valueon other pulsar parameters. The measured dependence of τ. on dispersion measure τ.(.) =40(./100). is close to theoretically expected relation τ.(.) α ... A frequency depe
CAMP
发表于 2025-3-23 08:56:18
Scintillation Observations Of Strong Northern Pulsarst also affects the precision of pulse timingobservations. Using a pulsar timing system developed at the Urumqi Astronomical Observatory 25 mtelescope, we observed diffractive scintillation dynamic spectra for several strong northern pulsars.This paper introduces the observing system and discusses th