Near‐relativistic Electron \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $c/ v$ \end{document} Onset Plots-Reference-Cited by-同舟云学术

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Published:2006-07-20 Issue:1 Volume:646 Page:634-641
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Kahler S.,Ragot B. R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference53 articles.

1. Interplanetary pitch angle scattering and coronal transport of solar energetic particles: New information from Helios

2. Focusing anisotropy of solar cosmic rays

3. Near‐Relativistic Solar Electrons and Type III Radio Bursts

4. Delay in solar energetic particle onsets at high heliographic latitudes

5. Observations related to the acceleration, injection, and interplanetary propagation of energetic protons during the solar cosmic ray event on February 16, 1984

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