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Solar radio phenomena and their physical interpretation
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Denisse, J. F. |
| Organization | The National Aeronautics and Space Administration (NASA) |
| Copyright Year | 1961 |
| Abstract | CENTIMETER BURSTS AND TYPE 4 BURSTS ARE INTERPRETED AS SYNCHROTRON RADIATION. TYPE 3 AND TYPE 2 BURSTS ARE PROBABLY DUE TO EXCITATION OF OSCILLATIONS OF THE CORONAL PLASMA BY HIGH ENERGY PARTICLES. THE PARTICLES THAT CREATE TYPE R ARE PROBABLY TRAPPED IN A MAGNETO-DYNAMIC WAVE. RADIO STORMS ARE SIMILARLY DUE TO PARTICLES EJECTED DURING AN ERUPTION AND REMAINING-TRAPPED FOR SEVERAL DAYS IN THE MAGNETIC CONFIGURATIONS NEAR THE SUN. |
| File Size | 663779 |
| File Format | |
| Alternate Webpage(s) | http://www.archive.org/details/nasa_techdoc_19980228280 |
| Archival Resource Key | ark:/13960/t74t7gq7g |
| Language | English |
| Publisher Date | 1961-09-01 |
| Publisher Institution | NASA (non Center Specific) |
| Access Restriction | Open |
| Subject Keyword | Reynolds Number Flat Plates Attitude (inclination) Air Flow Aerodynamic Coefficients Pressure Distribution Two Dimensional Models Circular Cylinders Aerodynamic Drag Minimum Drag Mach Number Lift Drag Ratio Forebodies Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
