Interplanetary coronal mass ejection observed at STEREO-A, Mars, comet 67P/Churyumov-Gerasimenko, Saturn, and New Horizons en route to Pluto: Comparison of its Forbush decreases at 1.4, 3.1, and 9.9 AU
- Submitting institution
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The University of Leicester
- Unit of assessment
- 9 - Physics
- Output identifier
- 1983
- Type
- D - Journal article
- DOI
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10.1002/2017JA023884
- Title of journal
- Journal of Geophysical Research: Space Physics
- Article number
- -
- First page
- 7865
- Volume
- 122
- Issue
- 8
- ISSN
- 2169-9402
- Open access status
- Compliant
- Month of publication
- June
- Year of publication
- 2017
- URL
-
-
- Supplementary information
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https://doi.org/10.1002/2017JA023884
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
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50
- Research group(s)
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B - Planetary Science
- Citation count
- 46
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- Milan contributed to the interpretation of the data, particularly the New Horizons observations, which lacked a magnetometer. He interpreted a sudden drop in mass density and ram pressure as the presence of a magnetic cloud, a characteristic feature of a coronal mass ejection (CME). This strengthened the argument that the CME had been detected in the out heliosphere. He also contributed text to the discussion of the CME in the New Horizons data and to the editing of the manuscript.
- Non-English
- No
- English abstract
- -
