Capabilities of and Results From the SPEAR Ionospheric Heating Facility

Details Capabilities of and Results From the SPEAR Ionospheric Heating Facility Capabilities of and Results From the SPEAR Ionospheric Heating Facility

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsa53c..05y&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #SA53C-05

Physics

6944 Nonlinear Phenomena (4400, 7839), 7803 Active Perturbation Experiments, 7836 Mhd Waves And Instabilities (2149, 2752, 6050), 7867 Wave/Particle Interactions (2483, 6984), 7894 Instruments And Techniques

Scientific paper

The SPEAR (Space Plasma Exploration by Active Radar) high power radio frequency system at 78 degrees north on Svalbard started operations in 2004. Several campaigns coordinated with the EISCAT Svalbard Radar (ESR) have been run since that time. The capabilities of the SPEAR system have been extended during each campaign, and the current capabilities of the system will be described, along with the plans for the development of the system over the next few years. The results of high power ionospheric modification experiments performed with SPEAR in coordination with both the ESR, the CUTLASS HF coherent radars and HF Doppler experiments during the first years of operations will be summarised, and future experimental plans outlined.

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