Add to ORKG• We use the newly calibrated MDI data (1996~2008) as input to the Wang-Sheeley-Arge (WSA) model to predict the solar wind parameters: speed and interplanetary magnetic field (IMF) polarity at 1 AU. • We propose a new polar field extrapolation scheme for the input data
The declining phases of solar cycles are known for their high speed solar wind streams that dominate...
It took the solar polar passage of Ulysses in the early 1990s to establish the global structure of t...
International audienceAccurate reconstruction of global solar-wind structure is essential for connec...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
The prediction of the background global solar wind is a necessary part of space weather forecasting....
This presentation is the first in a series which will provide independent validation of community mo...
In this paper, we propose a modified procedure to infer the interplanetary magnetic field (IMF) pola...
I develop and document a set of procedures which test the quality of predictions of solar wind speed...
[1] The photospheric and heliospheric magnetic fields have been continuously observed at the L1 poin...
International audienceAims:In a previous work, Ulysses data was analyzed to build a complete axisymm...
We have performed systematic global magnetohydrodynamic (MHD) simulation studies driven by an ideali...
Mars’ plasma environment is strongly driven by its interaction with the solar wind, however the lack...
The solar wind fills the heliosphere and is the background medium in which coronal mass ejections pr...
The origins of the solar wind and the interplanetary magnetic field sector structure in the beginnin...
The declining phases of solar cycles are known for their high speed solar wind streams that dominate...
It took the solar polar passage of Ulysses in the early 1990s to establish the global structure of t...
International audienceAccurate reconstruction of global solar-wind structure is essential for connec...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
The prediction of the background global solar wind is a necessary part of space weather forecasting....
This presentation is the first in a series which will provide independent validation of community mo...
In this paper, we propose a modified procedure to infer the interplanetary magnetic field (IMF) pola...
I develop and document a set of procedures which test the quality of predictions of solar wind speed...
[1] The photospheric and heliospheric magnetic fields have been continuously observed at the L1 poin...
International audienceAims:In a previous work, Ulysses data was analyzed to build a complete axisymm...
We have performed systematic global magnetohydrodynamic (MHD) simulation studies driven by an ideali...
Mars’ plasma environment is strongly driven by its interaction with the solar wind, however the lack...
The solar wind fills the heliosphere and is the background medium in which coronal mass ejections pr...
The origins of the solar wind and the interplanetary magnetic field sector structure in the beginnin...
The declining phases of solar cycles are known for their high speed solar wind streams that dominate...
It took the solar polar passage of Ulysses in the early 1990s to establish the global structure of t...
International audienceAccurate reconstruction of global solar-wind structure is essential for connec...