The Relation between Type III Radio Storms and CIR Energetic Particles-Reference-Cited by-同舟云学术

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The Relation between Type III Radio Storms and CIR Energetic Particles

Published:2022-05-29 Issue: Volume: Page:
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Container-title:2022 3rd URSI Atlantic and Asia Pacific Radio Science Meeting (AT-AP-RASC)
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Author:

Gopalswamy Nat¹,Makela Pertti²,Yashiro Seiji²,Akiyama Sachiko²,Xie Hong²

Affiliation:

1. NASA Goddard Space Flight Center,Greenbelt,MD,USA,20771

2. The Catholic University of America,Washington,DC,USA,20064

Publisher

IEEE

Link

http://xplorestaging.ieee.org/ielx7/9813726/9814163/09814336.pdf?arnumber=9814336

Reference15 articles.

1. Solar Terrestrial Relations Observatory (STEREO) Observations of Stream Interaction Regions in 2007 – 2016: Relationship with Heliospheric Current Sheets, Solar Cycle Variations, and Dual Observations

2. The Radial Variation of Corotating Energetic Particle Streams in the Inner and Outer Solar System

3. A Self-consistent Simulation of Proton Acceleration and Transport Near a High-speed Solar Wind Stream

4. Energetic Particle Increases Associated with Stream Interaction Regions;cohen;Astrophys J Supp Ser,2021

5. The active region source of a type III radio storm observed by Parker Solar Probe during encounter 2

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Can Type III Radio Storms be a Source of Seed Particles to Shock Acceleration?;2022 3rd URSI Atlantic and Asia Pacific Radio Science Meeting (AT-AP-RASC);2022-05-29

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