Add to ORKGel ke ler C.N. Arged, G.L. Siscoee, H.E. Spencee using the WSA estimates of solar wind speed at L1, which allows for 3–4 days lead times. We compare the prediction solar wind with the coupled magnetosphere–ionospher-e–atmosphere system. It is presently expected that the backbone of this coupled model will be based o
This database is the basis for the analysis described in the manuscript 'Timing of the solar wind p...
GNSS positioning errors, spacecraft operations failures and power outages potentially originate from...
© 2017, Springer Science+Business Media B.V. An exospheric kinetic solar wind model is interfaced wi...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
The Wang–Sheeley–Arge (WSA) method is used to predict the solar wind speed (and certain other parame...
The prediction of the background global solar wind is a necessary part of space weather forecasting....
The near‐Earth space environment is strongly driven by the solar wind and interplanetary magnetic fi...
of a mean flow, a solar tide, and a 4-day traveling wave, the thermospheric SS–AS winds are increasi...
We present in this paper an operational solar wind prediction system. The system is an outcome of th...
Predictions of the physical parameters of the solar wind at Earth are at the core of operational spa...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
Observations of the fast, high-latitude solar wind throughout Ulysses ’ three orbits show that solar...
Emanating from the base of the Sun’s corona, the solar wind fills the interplanetary medium with a m...
[1] It has been postulated that steady magnetospheric convection (SMC), a mode of response of the Ea...
he magnetosphere is the region of space dominated by the magnetic field of the Earth. The size of th...
This database is the basis for the analysis described in the manuscript 'Timing of the solar wind p...
GNSS positioning errors, spacecraft operations failures and power outages potentially originate from...
© 2017, Springer Science+Business Media B.V. An exospheric kinetic solar wind model is interfaced wi...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
The Wang–Sheeley–Arge (WSA) method is used to predict the solar wind speed (and certain other parame...
The prediction of the background global solar wind is a necessary part of space weather forecasting....
The near‐Earth space environment is strongly driven by the solar wind and interplanetary magnetic fi...
of a mean flow, a solar tide, and a 4-day traveling wave, the thermospheric SS–AS winds are increasi...
We present in this paper an operational solar wind prediction system. The system is an outcome of th...
Predictions of the physical parameters of the solar wind at Earth are at the core of operational spa...
The Wang-Sheeley-Arge (WSA) model is regularly used to predict the background solar wind speed and t...
Observations of the fast, high-latitude solar wind throughout Ulysses ’ three orbits show that solar...
Emanating from the base of the Sun’s corona, the solar wind fills the interplanetary medium with a m...
[1] It has been postulated that steady magnetospheric convection (SMC), a mode of response of the Ea...
he magnetosphere is the region of space dominated by the magnetic field of the Earth. The size of th...
This database is the basis for the analysis described in the manuscript 'Timing of the solar wind p...
GNSS positioning errors, spacecraft operations failures and power outages potentially originate from...
© 2017, Springer Science+Business Media B.V. An exospheric kinetic solar wind model is interfaced wi...