Skip to content Skip to navigation
University of Warwick
  • Study
  • |
  • Research
  • |
  • Business
  • |
  • Alumni
  • |
  • News
  • |
  • About

University of Warwick
Publications service & WRAP

Highlight your research

  • WRAP
    • Home
    • Search WRAP
    • Browse by Warwick Author
    • Browse WRAP by Year
    • Browse WRAP by Subject
    • Browse WRAP by Department
    • Browse WRAP by Funder
    • Browse Theses by Department
  • Publications Service
    • Home
    • Search Publications Service
    • Browse by Warwick Author
    • Browse Publications service by Year
    • Browse Publications service by Subject
    • Browse Publications service by Department
    • Browse Publications service by Funder
  • Help & Advice
University of Warwick

The Library

  • Login
  • Admin

Reproducible aspects of the climate of space weather over the last five solar cycles

Tools
- Tools
+ Tools

Chapman, Sandra C., Watkins, Nicholas W. and Tindale, Elizabeth (2018) Reproducible aspects of the climate of space weather over the last five solar cycles. Space Weather, 16 (8). pp. 1128-1142. doi:10.1029/2018SW001884 ISSN 1542-7390.

[img]
Preview
PDF
WRAP-reproducible-aspects-climate-space-weather-Chapman-2018.pdf - Published Version - Requires a PDF viewer.
Available under License Creative Commons: Attribution 3.0 Intergovernmental Organisation (IGO).

Download (2155Kb) | Preview
[img] PDF
WRAP-reproducible-aspects-climate-space-weather-Chapman-2018.pdf - Accepted Version
Embargoed item. Restricted access to Repository staff only - Requires a PDF viewer.

Download (4Mb)
Official URL: http://dx.doi.org/10.1029/2018SW001884

Request Changes to record.

Abstract

Each solar maximum interval has a different duration and peak activity level, which is reflected in the behavior of key physical variables that characterize solar and solar wind driving and magnetospheric response. The variation in the statistical distributions of the F10.7 index of solar coronal radio emissions, the dynamic pressure PDyn and effective convection electric field Ey in the solar wind observed in situ upstream of Earth, the ring current index DST, and the high‐latitude auroral activity index AE are tracked across the last five solar maxima. For each physical variable we find that the distribution tail (the exceedences above a threshold) can be rescaled onto a single master distribution using the mean and variance specific to each solar maximum interval. We provide generalized Pareto distribution fits to the different master distributions for each of the variables. If the mean and variance of the large‐to‐extreme observations can be predicted for a given solar maximum, then their full distribution is known.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
Library of Congress Subject Headings (LCSH): Space environment, Solar cycle, Magnetosphere, Solar wind
Journal or Publication Title: Space Weather
Publisher: Wiley-Blackwell Publishing, Inc.
ISSN: 1542-7390
Official Date: 24 August 2018
Dates:
DateEvent
24 August 2018Published
27 July 2018Available
16 July 2018Accepted
Volume: 16
Number: 8
Page Range: pp. 1128-1142
DOI: 10.1029/2018SW001884
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Open Access (Creative Commons)
Date of first compliant deposit: 31 July 2018
Date of first compliant Open Access: 12 March 2021
RIOXX Funder/Project Grant:
Project/Grant IDRIOXX Funder NameFunder ID
FA9550-17-1-0054Air Force Office of Scientific Researchhttp://dx.doi.org/10.13039/100000181
ST/N504506/1[STFC] Science and Technology Facilities Councilhttp://dx.doi.org/10.13039/501100000271
UNSPECIFIEDUS-UK Fulbright Commissionhttp://dx.doi.org/10.13039/501100000592

Request changes or add full text files to a record

Repository staff actions (login required)

View Item View Item

Downloads

Downloads per month over past year

View more statistics

twitter

Email us: wrap@warwick.ac.uk
Contact Details
About Us