Speaker
Norayr Galikyan
(National Research Nuclear University MEPhI)
Description
The magnetic field in the inner heliosphere, including both regular and irregular components, was modelled. The regular component is described by Parker’s model, which assumes that the magnetic field is frozen inside the solar wind plasma. To include the irregular component of the field, a Gaussian random field was generated on the field source surface, and later transported into the inner heliosphere along the regular component field lines. An agreement between the model and the observed field by spacecrafts such as ACE, Ulysses, Voyager, and Parker Solar Probe is shown for different heliolatitudes and helioradiuses.
Primary authors
Norayr Galikyan
(National Research Nuclear University MEPhI)
Mr
Vladislav Alekseev
(Yaroslavl State University. PG Demidov)
Dr
Andrey Mayorov
(National Research Nuclear University MEPhI)
Mr
Rustam Yulbarisov
(National Research Nuclear University MEPhI)
