论文部分内容阅读
Summary ·Background and Motivation ·3-D Forbush Decrease Numerical Model · Simulation Results ·Conclusion
A 3-D SDE Numerical Model for the Simulation of Electron Forbush Decreases
【摘 要】
：
Summary ·Background and Motivation ·3-D Forbush Decrease Numerical Model · Simulation Results ·Conclusion
【机 构】
：
NationalSpaceScienceCenter,ChineseAcademyofScienceNorth-WestUniversity,SouthAfricaFloridaInstituteof
【出 处】
：
第8届高海拔宇宙线探测国际研讨会(The 8th International Workshop on Air Showe
【发表日期】
：
2017年12期
其他文献
The Outline:Introduction to pulsar and VLBI observations Introduction to pulsar and VLBI observations The challenge of pulsar VLBI observations The history and
会议
Outline Doppler Imaging(non-Zeeman):Rationale,performance and limitations DI--What do we learn?Conclusions
会议
Using the timing method to search circumbinary planets--A possible giant planet orbiting the catacly
The DWARF Project Eclipsing Binaries:Precise Clocks to Detect Extrasolar Planets(i) systems with K or/and M dwarf components(ii) systems with hot subdwarf(sd) a
会议
OUTLINE Background NG-DRAPS Future Plan New technology→Data Rate VLBI High stability frequency standard High accuracy time synchronization High speed recording
会议
Outline Background of LSI+61 303 VLBA Observations Results Future Plan Background of LSI+61 303Binary:Be star(B0)+compact object Microquasar or Pulsar wind D～2 k
会议
Outline Broadband Cryogenic Receiver(1.2-6.9 GHz）Feed & LNA Research Broadband Receivers Review
会议
Outline VLBI system of FAST Introduction Test of Roach2 & Mark IV Plan of test observation Drift mode Tracking mode
会议
分析了UT1实验及初步结果，介绍了DiFX+AIPS数据检查、比较了几何时延模型、进行了时频稳定性评估实验。初步走通UT1流程，具备天体测量和成图观测能力。
介绍了CEI测量系统结构、分析了测量结果以及CEI技术在GEO卫星轨道监测中的应用。增加实时标校后，改善了观测的数据质量；尤其对于白天的数据；气温变化引起电缆温度变化对观测相
LHAASO could provide useful data on solar diurnal anisotropy～100 GeV LHAASO may reconstruct shower events for cosmic rays down to about～100 GeV.
会议