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The helioseismic and magnetic imager (hmi) investigation for the solar dynamics observatory (sdo)
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Duvall Jr., T. L. Title, A. M. Schrijver, C. J. Bush, R. I. Scherrer, Philip Hanby Liu, Y. Schou, Jesper Bogart, R. S. Tomczyk, S. Kosovichev, A. G. Tarbell, T. D. Zhao, J. Hoeksema, J. T. |
| Copyright Year | 2011 |
| Description | The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal processes and dynamics of the corona and heliosphere, and precursors of solar disturbances for space-weather forecasts. A brief overview of the instrument, investigation objectives, and standard data products is presented. |
| File Size | 787519 |
| Page Count | 21 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20140010272 |
| Archival Resource Key | ark:/13960/t7jq5zm0g |
| Language | English |
| Publisher Date | 2011-10-18 |
| Access Restriction | Open |
| Subject Keyword | Helioseismology Magnetic Field Solar Dynamics Observatory Photosphere Solar Corona Data Management Magnetic Variations Solar Interior Sunspots Solar Magnetic Field Dynamo Theory Solar Observatories Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
