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Examining the properties of jets in coronal holes (Document No: 20130003205)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Gaulle, Owen Tennant, A. F. Adams, Mitzi L. |
| Copyright Year | 2012 |
| Description | We examined both X-ray and Magnetic field data in order to determine if there is a correlation between emerging magnetic flux and the production of Coronal jets. It was proposed that emerging flux can be a trigger to a coronal jet. The jet is thought to be caused when local bipoles reconnect or when a region of magnetic polarity emerges through a uniform field. In total we studied 15 different jets that occurred over a two day period starting 2011-02-27 00:00:00 UTC and ending 2011-02-28 23:59:55 UTC. All of the jets were contained within a coronal hole that was centered on the disk. Of the 15 that we studied 6 were shown to have an increase of magnetic flux within one hour prior to the creation of the jet and 10 were within 3 hours before the event. |
| File Size | 827923 |
| Page Count | 1 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20130003205 |
| Archival Resource Key | ark:/13960/t38103846 |
| Language | English |
| Publisher Date | 2012-12-03 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Magnetic Flux Actuators Polarity Coronas Magnetic Fields Coronal Holes Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Presentation |
