Add to ORKGThe principal features that might exist in the terrestrial paleoionosphere, if the geomagnetic field were to assume a quadrupole form during a polarity reversal are discussed. Complicated phenomena would be expected to occur at magnetic equators and magnetospherically-driven plasma convection might occur at latitudes where the magnetic field is steeply inclined. The influence of magnetic field strength on ionospheric structure is considered in general terms
We study the topological structure of the magnetosphere for northward IMF. Using a magnetospheric m...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Precipitation from the inner edge of the electron plasma sheet creates a density maximum in the auro...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95169/1/jgra17275.pd
It is well known that the ionosphere plays a role in determining the global state of the magnetosph...
Three models for the magnetosphere-ionosphere coupling feedback instability are considered. The fir...
Ionospheric disturbance electric fields of magnetospheric origin play an important role in determini...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
In this report we use electric field data measured aboard the low-altitude Ogo 6 spacecraft [Heppner...
It is well known that convection electric fields have an important effect on the ionosphere at high ...
The paper presents results from the numerical study of the magnetosphere-ionosphere interactions dri...
The Ninth Symposium on Polar Science/Ordinary sessions: [OS] Space and upper-atmosphere sciences, We...
International audienceWe propose a simple illustrative axisymmetric model of the plasma flow and cur...
Using the OGO-5 fluxgate magnetometer data, the polar cap boundary is identified in the high altitud...
International audienceWe present two event studies illustrating the detailed relationships between p...
We study the topological structure of the magnetosphere for northward IMF. Using a magnetospheric m...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Precipitation from the inner edge of the electron plasma sheet creates a density maximum in the auro...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95169/1/jgra17275.pd
It is well known that the ionosphere plays a role in determining the global state of the magnetosph...
Three models for the magnetosphere-ionosphere coupling feedback instability are considered. The fir...
Ionospheric disturbance electric fields of magnetospheric origin play an important role in determini...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
In this report we use electric field data measured aboard the low-altitude Ogo 6 spacecraft [Heppner...
It is well known that convection electric fields have an important effect on the ionosphere at high ...
The paper presents results from the numerical study of the magnetosphere-ionosphere interactions dri...
The Ninth Symposium on Polar Science/Ordinary sessions: [OS] Space and upper-atmosphere sciences, We...
International audienceWe propose a simple illustrative axisymmetric model of the plasma flow and cur...
Using the OGO-5 fluxgate magnetometer data, the polar cap boundary is identified in the high altitud...
International audienceWe present two event studies illustrating the detailed relationships between p...
We study the topological structure of the magnetosphere for northward IMF. Using a magnetospheric m...
The solar-wind magnetosphere interaction primarily occurs at altitudes where the dipole component of...
Precipitation from the inner edge of the electron plasma sheet creates a density maximum in the auro...