Solar Wind Forecast by Using Interplanetary Scintillation Observations

Details Solar Wind Forecast by Using Interplanetary Scintillation Observations Solar Wind Forecast by Using Interplanetary Scintillation Observations

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..663f&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 663-666 (2010).

Computer Science

1

Solar Wind, Interplanetary Matter, Tomography, Solar Activity, Satellites, Artificial, Particle Emission, Solar Wind, Heliosphere/Interstellar Medium Interactions, Computed Tomography, Solar Activity, Artificial Earth Satellites

Scientific paper

Interplanetary scintillation (IPS) allows us to determine solar wind velocity and density structures over a relatively short time by employing computer assisted tomography. This method can be applied to forecast solar wind changes for a few days prior to its reaching Earth. We have been attempting solar wind forecasting by using IPS data observed at Solar-Terrestrial Environment Laboratory (STELab), Japan. Here we introduce the solar wind forecast using STELab-IPS and evaluated dependences of the accuracy of the STELab-IPS forecasts on a number of line-of-sight observed with IPS and a solar activity by comparing comparing them with in situ measurements.

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