Of the intense magnetic fields (greater than 13 gamma) observed at 1 AU during solar cycle 20 (1973-1975), 92% were associated with shocks, stream interfaces, or cold magnetic enhancements (CMEs). Most (52%) of the magnetic field intensity enhancements occurred at stream interfaces; 27% occurred behind shocks without interfaces; and 11% occurred in CMEs. The most intense fields (25 gamma to 37 gamma) followed shocks. Magnetic field intensities at interfaces did not exceed 25 gamma, suggesting a mechanism such as a magnetoacoustic wave limits the intensity ahead of streams. Intense magnetic fields persist longest behind shocks
Magnetic field fluctuations in magnetosheath of Explorer 34 spectral data on sunward earth hemispher
The role of high-speed solar wind streams in driving relativistic electron acceleration within the E...
We report on features of solar wind-magnetosphere coupling elicited by shocks propagating through co...
Magnetic clouds are defined as regions with a radial dimension approximately 0.25 AU (at 1 AU) in wh...
The recurrent flow and field patterns observed by HELIOS 1, and the relation between these patterns ...
The sources of magnetic fields in recurrent streams were examined. Most fields and plasmas at 1 AU w...
Two interplanetary magnetic clouds, characterized by anomalous magnetic field directions and unusual...
Recent results in interplanetary physics are examined. These include observations of shock waves and...
The large-scale radial and temporal variations of the interplanetary magnetic field strength B obser...
In situ magnetic field and plasma observations within 1 AU which describe MDH stream flows and Alfve...
Solar surface and interplanetary magnetic fields, interplanetary plasmas, and geomagnetic field sola...
International audienceWe analyzed observations of the solar activities and the solar wind parameters...
Large-scale properties of the interplanetary magnetic field as determined by the solar wind velocity...
International audienceMagnetic disturbances in the Earth's magnetosphere can be very different depen...
International audienceWe investigated geomagnetic activity which was induced by interplanetary magne...
Magnetic field fluctuations in magnetosheath of Explorer 34 spectral data on sunward earth hemispher
The role of high-speed solar wind streams in driving relativistic electron acceleration within the E...
We report on features of solar wind-magnetosphere coupling elicited by shocks propagating through co...
Magnetic clouds are defined as regions with a radial dimension approximately 0.25 AU (at 1 AU) in wh...
The recurrent flow and field patterns observed by HELIOS 1, and the relation between these patterns ...
The sources of magnetic fields in recurrent streams were examined. Most fields and plasmas at 1 AU w...
Two interplanetary magnetic clouds, characterized by anomalous magnetic field directions and unusual...
Recent results in interplanetary physics are examined. These include observations of shock waves and...
The large-scale radial and temporal variations of the interplanetary magnetic field strength B obser...
In situ magnetic field and plasma observations within 1 AU which describe MDH stream flows and Alfve...
Solar surface and interplanetary magnetic fields, interplanetary plasmas, and geomagnetic field sola...
International audienceWe analyzed observations of the solar activities and the solar wind parameters...
Large-scale properties of the interplanetary magnetic field as determined by the solar wind velocity...
International audienceMagnetic disturbances in the Earth's magnetosphere can be very different depen...
International audienceWe investigated geomagnetic activity which was induced by interplanetary magne...
Magnetic field fluctuations in magnetosheath of Explorer 34 spectral data on sunward earth hemispher
The role of high-speed solar wind streams in driving relativistic electron acceleration within the E...
We report on features of solar wind-magnetosphere coupling elicited by shocks propagating through co...