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The white light corona and photospheric magnetic fields
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | McCabe, Marie K. |
| Copyright Year | 1986 |
| Description | Some results are presented from a continuing investigation of the coronal structure vs. the photospheric magnetic field relationship. Two approaches to the problem are considered. First, the individual coronal features recorded at each limb were located on a chart of the magnetic field measured with low spatial resolution, depicting the large scale or global field configuration. Second, the characteristics of neutral line segments, defined by the presence of H alpha line filament, with no associated coronal structure were investigated. Preliminary results are discussed. |
| File Size | 301931 |
| Page Count | 5 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19870011479 |
| Archival Resource Key | ark:/13960/t1fj7bq0t |
| Language | English |
| Publisher Date | 1986-12-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Photosphere Solar Corona White Light Holography Solar Limb H Alpha Line Solar Prominences Magnetic Field Configurations Brightness Distribution Solar Magnetic Field Synoptic Measurement Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
