A first generation numerical geomagnetic storm prediction scheme

Details A first generation numerical geomagnetic storm prediction scheme A first generation numerical geomagnetic storm prediction scheme

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986p%26ss...34...77a&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 34, Jan. 1986, p. 77-92.

Computer Science

17

Auroras, Computerized Simulation, Magnetic Storms, Convection, Interplanetary Magnetic Fields, Magnetic Equator, Solar Flares, Solar Rotation, Solar Wind

Scientific paper

The development of a prediction scheme for geomagnetic storms, which evaluates solar wind quantities and geomagnetic disturbances is described. The codes used in the calculation of the solar wind speed, solar wind magnetic field magnitude, the polar angle of the solar wind magnetic field vector, and the auroral discharge power as a function of time are analyzed. With the auroral discharge power and IMF components data, the geometry of the auroral oval, the cross-polar cap potential, the magnetic fields of the ring current and auroral electrojets, the total energy injection rate into the polar ionosphere, the atmospheric temperature, and electron density profile in the ionosphere are computed. The cause of variations in the north-south components of the IMF, which affects the predictability of the scheme, is investigated.

Affiliated with

Also associated with

No associations

Rating

A first generation numerical geomagnetic storm prediction scheme does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A first generation numerical geomagnetic storm prediction scheme, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A first generation numerical geomagnetic storm prediction scheme will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1847523