microscopic
发表于 2025-3-23 11:08:08
Radio Observations of the Quiet Sun,missions from chromospheric and coronal heating events. Here we review observations of the quiet Sun using radio telescopes and discuss current science problems that will be addressed with future facilities such as the Frequency Agile Solar Radiotelescope (FASR).
放弃
发表于 2025-3-23 17:34:07
http://reply.papertrans.cn/88/8715/871459/871459_12.png
labyrinth
发表于 2025-3-23 18:06:15
http://reply.papertrans.cn/88/8715/871459/871459_13.png
braggadocio
发表于 2025-3-24 00:09:53
Solar and Solar Radio Effects on Technologies,as also increased in number and in their design and operational complexity. A brief history of the influences of solar-produced effects on technologies is provided, beginning with the deployment of the initial electrical telegraph communications systems in the 19th century. An overview is provided o
结束
发表于 2025-3-24 03:46:04
http://reply.papertrans.cn/88/8715/871459/871459_15.png
生命层
发表于 2025-3-24 07:16:42
The Frequency Agile Solar Radiotelescope,on, high-fidelity, and high-dynamic-range images over a broad range of radio frequencies ~ 0.05–24 GHz). That is, FASR will perform broadband imaging spectroscopy, producing unique data and enabling a wide variety of radio-diagnostic tools to be exploited to study the Sun from the mid-chromosphere t
Dictation
发表于 2025-3-24 13:57:26
Radio Spectral Diagnostics,be used to determine parameters of the emitting particles and the ambient solar atmosphere in the emitting volume. After generation, the propagation of radiation in the solar atmosphere leads to changes in the spectrum that can be exploited to gain further information about the atmospheric parameter
噱头
发表于 2025-3-24 15:34:17
http://reply.papertrans.cn/88/8715/871459/871459_18.png
Brittle
发表于 2025-3-24 21:24:28
http://reply.papertrans.cn/88/8715/871459/871459_19.png
padding
发表于 2025-3-25 01:11:13
Coronal Magnetic Field Measurements Through Quasi-Transverse Propagation, the QT-propagation are discussed. The first part of the chapter briefly outlines the relevant geometry and mathematical relations. Then the state of the art in the coronal magnetography and some possibilities are demonstrated. We discuss use of the technique for coronal magnetography and give some