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Title: Where is the cosmic-ray modulation boundary of the heliosphere?

Authors:
 [1];  [2];  [3]
  1. Department of Physics and Space Sciences, Florida Institute of Technology, Melbourne, Florida 32901, USA
  2. Center for Space Research, North-West University, Potchefstroom 2520, South Africa, State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190, China
  3. Center for Space Plasma and Aeronomic Research and Department of Space Science, University of Alabama in Huntsville, Huntsville, Alabama 35899, USA
Publication Date:
Sponsoring Org.:
USDOE
OSTI Identifier:
1229627
Grant/Contract Number:  
SC0008334; SC0008721
Resource Type:
Publisher's Accepted Manuscript
Journal Name:
Physics of Plasmas
Additional Journal Information:
Journal Name: Physics of Plasmas Journal Volume: 22 Journal Issue: 9; Journal ID: ISSN 1070-664X
Publisher:
American Institute of Physics
Country of Publication:
United States
Language:
English

Citation Formats

Zhang, Ming, Luo, Xi, and Pogorelov, Nikolai. Where is the cosmic-ray modulation boundary of the heliosphere?. United States: N. p., 2015. Web. doi:10.1063/1.4928945.
Zhang, Ming, Luo, Xi, & Pogorelov, Nikolai. Where is the cosmic-ray modulation boundary of the heliosphere?. United States. https://doi.org/10.1063/1.4928945
Zhang, Ming, Luo, Xi, and Pogorelov, Nikolai. Thu . "Where is the cosmic-ray modulation boundary of the heliosphere?". United States. https://doi.org/10.1063/1.4928945.
@article{osti_1229627,
title = {Where is the cosmic-ray modulation boundary of the heliosphere?},
author = {Zhang, Ming and Luo, Xi and Pogorelov, Nikolai},
abstractNote = {},
doi = {10.1063/1.4928945},
journal = {Physics of Plasmas},
number = 9,
volume = 22,
place = {United States},
year = {Thu Aug 20 00:00:00 EDT 2015},
month = {Thu Aug 20 00:00:00 EDT 2015}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1063/1.4928945

Citation Metrics:
Cited by: 24 works
Citation information provided by
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