Parker spirals - A Study on the Structure of the Interplanetary Magnetic Field
2018-08
Loading...
Persistent link to this item
Statistics
View StatisticsJournal Title
Journal ISSN
Volume Title
Title
Parker spirals - A Study on the Structure of the Interplanetary Magnetic Field
Authors
Published Date
2018-08
Publisher
Type
Scholarly Text or Essay
Abstract
The Parker spiral’s accuracy is investigated through its prediction for the angle of the interplanetary magnetic field observed by satellites near 1 AU. Simulations were run using simple solar wind parameters and results were compared with measured data from STEREO A and B. Several distribution plots are made to numerically analyze the prediction quality over a six-year period. Investigation was focused on the difference between prediction quality in the ecliptic plane and in three-dimensional space.
This paper is a result of a preliminary analysis on a program written to investigate the Parker spirals. The program, a deployable Python flask application, is a major part of the URS project and is subject to further improvements as this project will continue to be carried on. The next steps will be to analyze solar energetic events using the Parker spiral in conjunction with other instruments. Additionally, this model will be compared with other existing, more complicated models for the interplanetary magnetic field to yield meaningful comparisons for the accuracy in predicting the magnetic field structure.
Description
Faculty advisor: Cynthia Cattell
Related to
Replaces
License
Series/Report Number
Funding information
This research was supported by the Undergraduate Research Opportunities Program (UROP).
Isbn identifier
Doi identifier
Previously Published Citation
Suggested citation
Vo, Tien. (2018). Parker spirals - A Study on the Structure of the Interplanetary Magnetic Field. Retrieved from the University Digital Conservancy, https://hdl.handle.net/11299/199856.
Content distributed via the University Digital Conservancy may be subject to additional license and use restrictions applied by the depositor. By using these files, users agree to the Terms of Use. Materials in the UDC may contain content that is disturbing and/or harmful. For more information, please see our statement on harmful content in digital repositories.