Statistical Relationships Between Solar Wind Parameters: Implications for Space Weather Forecasts

Heather
Elliott
Southwest Research Institute
C. Nickolos Arge, NASA Goddard Space Flight Center, Greenbelt, MD
Carl. J. Henney; Air Force Research Laboratory, AFB, NM
Maher A. Dayeh; Southwest Research Institute, San Antonio, TX
Joerg-Micha Jahn; Southwest Research Institute, San Antonio, TX
Craig E. DeForest; Southwest Research Institute, Boulder, CO
Poster
The solar wind density, temperature, and the interplanetary magnetic field strength all correlate well with the solar wind speed. By combining these relationships Wang-Sheeley-Arge (WSA) corrected speed forecasts, we can produce multiday forecasts of the solar wind density, temperature, and interplanetary field strength, and the Kp geophysical index. First, we quantify how well these relationships can work using solar wind speed observations from near Earth in the OMNI data. This establishes a baseline for developing a skill score since the measured upstream Earth are the most accurate estimate of the solar wind speed that encounters Earth. Then, we determine how well the relationships perform at forecasting density, temperature, field strength and Kp index when using multiday WSA speed forecast relative to when using the measured speeds.

Poster category:

Poster category
Solar and Interplanetary Research and Applications
Poster session day
Poster location
31