Space Weather: Solar Radio Noise and Its Effect On Wireless Communication

摘要：ATM 00- 77273提案标题：太阳射电噪声及其对无线通信的影响首席研究员：戴尔加里，NJIT研究人员将指定太阳射电通量密度水平和波动作为频率的函数和作为太阳周期相位的函数。主要的工作是分析三个数据集：（1）固定频率无线电突发测量观测获得的一个网络（RINGS）在过去的40年由美国空军。(2)数据来自瑞士苏黎世ETH操作的Phoenix-2光谱仪。(3)欧文斯谷射电天文台的太阳射电暴定位器。该分析将为现代通信系统的设计者提供重要的统计措施。分析还将确定观测到的高通量密度太阳活动的射电数据饱和现象，究竟是起着辅助作用，还是太阳物理过程所固有的。测定结果对太阳物理学有直接意义。

ABSTRACT: ATM 00-77273Proposal Title: Solar Radio Noise and Its Effect On Wireless CommunicationPrincipal Investigator: Dale Gary, NJIT The investigators will specify solar radio flux density levels and fluctuations as a function of frequency and as a function of solar cycle phase. The main effort is to analyze three datasets: (1) Fixed frequency radio burst measurements observations obtained over the past forty years from a network (RSTN) operated by the United States Air Force. (2) Data from the Phoenix-2 spectrometer operated by ETH in Zurich, Switzerland. (3) The solar radio burst locator at the Owens Valley Radio Observatory. The analysis will provide statistical measures of importance to designers of modern communications systems. The analysis will also determine whether an observed saturation of RSTN data on solar events at high flux density is instrumental in origin or is inherent to the physical process on the Sun. Result of this determination are of direct interest to solar physics.