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4 results for “solar wind dynamic pressure”
Nighttime geomagnetic response to jumps of solar wind dynamic pressure: A possible cause of Québec blackout in March 1989
<p>This contains the original simulation data used by the paper 'Nighttime geomagnetic response to jumps of solar wind dynamic pressure: A possible cause of Québec blackout in March 1989', which will appear in Space Weather. The data were obtained by the global MHD simulation (REPPU).</p> <p>Each sav file (IDL saveset format) contains the physical variables in the ionosphere at each grid point (mlt*mlat: 321*221, starting at 0 MLT and -90 MLAT) for Run 02n, 30n, 30s, 33n, and 33s, including</p> <ul> <li>MHD time series ('time' in minutes),</li> <li>field-aligned current ('fac1' in A/m2),</li> <li>electric potential ('pot' in V),</li> <li>ionospheric conductivities ('ss11', 'ss12', and 'ss22' in S).</li> </ul> <p>The sav file can be opened by IDL. By typing, for example,<br> IDL> restore,'run02n.sav'<br> you can load the file to the memory of IDL. Type 'help' to confirm the variables that are loaded.</p>
Fitacf data for "Ionospheric Flow Vortex Induced by the Sudden Decrease in the Solar Wind Dynamic Pressure"
<p>This is the SuperDARN dataset in fitacf format (2.5) from the Hankasalmi radar. The data is used in the publication: Jin, Y., Moen, J. I., Spicher, A., Liu, J., Clausen, L. B. N., & Miloch, W. J. (2023). Ionospheric flow vortex induced by the sudden decrease in the solar wind dynamic pressure. Journal of Geophysical Research: Space Physics, 128, e2023JA031690. https://doi.org/10.1029/2023JA031690</p>
SuperDARN convection data used in the study of "Relation between Magnetopause Position and Reconnection Rate under Quasi-Steady Solar Wind Dynamic Pressure"
<p>Convection velocity data is available in the netCDF file format.</p>
The Dayside Ionosphere of Mars as controlled by the Game Between Solar Wind Dynamic Pressure and Crustal Magnetic Field Strength
<p>Including all 276 profiles like those shown in Figure 2.</p>
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