Local time dependence of polarization of geomagnetic sudden commencements (SC\u27s) at geostationary orbit was statistically analyzed, using magnetic data from GOES 2 and 3 satellites for the interval from August 1978 to August 1980. The polarization in the plane perpendicular to the geomagnetic field is counterclockwise in the morning side and clockwise in the afternoon side, when viewed along the field direction. The demarcation line across which the polarization is reversed seems to be located between 11h and 14h LT. This time span may be due to different angles at which shock fronts or discontinuities propagating in interplanetary space collide against the magnetosphere. The latitudinal reversal of polarization of SC observed in high la...
International audienceWe analyse the geomagnetic polarity time scale (GPTS) since the Upper Jurassic...
The unique network of geomagnetic observatories along 145◦E geomagnetic longitude extending from the...
7-14The defining observational characteristics of AM Her polars are their intense polarization. One...
In order to clarify local time dependence of polarization of geomagnetic sudden commencements (SC\u2...
In order to clarify characteristics of geomagnetic sudden commencements (SC\u27s) at geomagnetically...
Characteristics of geomagnetic sudden commencement (SC) observed in middle and low latitudes are dis...
A geomagnetic sudden commencement (SC) was observed by the low altitude geomagnetic satellite, MAGSA...
Local time (LT) variations of the averaged H-component amplitude of geomagnetic sudden commencements...
We have studied 41 Sudden Commencements (SC) using simultaneous magnetic field data from the CHAMP ...
A preliminary analysis shows that magnetic variations of periods 16 to 60 minutes at South Georgia a...
A statistical analysis of the polarization pattern of low-frequency geomagnetic field fluctuations ...
The relationship between the rise time, dT, and amplitude, d H, of geomagnetic sudden commencements ...
We have examined several cases of magnetosphere compression by solar wind pressure pulses using a s...
This paper tests the Araki [1994] computational model of the Earth-ionosphere system during geomagne...
Transient magnetic field variations in the dayside magnetosphere, whose magnetic signatures resemble...
International audienceWe analyse the geomagnetic polarity time scale (GPTS) since the Upper Jurassic...
The unique network of geomagnetic observatories along 145◦E geomagnetic longitude extending from the...
7-14The defining observational characteristics of AM Her polars are their intense polarization. One...
In order to clarify local time dependence of polarization of geomagnetic sudden commencements (SC\u2...
In order to clarify characteristics of geomagnetic sudden commencements (SC\u27s) at geomagnetically...
Characteristics of geomagnetic sudden commencement (SC) observed in middle and low latitudes are dis...
A geomagnetic sudden commencement (SC) was observed by the low altitude geomagnetic satellite, MAGSA...
Local time (LT) variations of the averaged H-component amplitude of geomagnetic sudden commencements...
We have studied 41 Sudden Commencements (SC) using simultaneous magnetic field data from the CHAMP ...
A preliminary analysis shows that magnetic variations of periods 16 to 60 minutes at South Georgia a...
A statistical analysis of the polarization pattern of low-frequency geomagnetic field fluctuations ...
The relationship between the rise time, dT, and amplitude, d H, of geomagnetic sudden commencements ...
We have examined several cases of magnetosphere compression by solar wind pressure pulses using a s...
This paper tests the Araki [1994] computational model of the Earth-ionosphere system during geomagne...
Transient magnetic field variations in the dayside magnetosphere, whose magnetic signatures resemble...
International audienceWe analyse the geomagnetic polarity time scale (GPTS) since the Upper Jurassic...
The unique network of geomagnetic observatories along 145◦E geomagnetic longitude extending from the...
7-14The defining observational characteristics of AM Her polars are their intense polarization. One...