5-10 October 2015
Milan Hotel 4*
Europe/Moscow timezone

Electron velocity distribution function in the heliosphere from thermal to highest energy.

8 Oct 2015, 15:00
15m
Bellini (Milan Hotel 4*)

Bellini

Milan Hotel 4*

Milan Hotel 4*, Shipilovskaya Street, 28A, Moscow, Russia, 115563

Speaker

Ksenia Kaportseva (MSU)

Description

Review presented of recent publications about experimental data, theoretical models and interpretations. The sources of electrons in the heliosphere are numerous and mainly related to the Sun, Interpalanetary and interstellar medium, planets and other astrophysical objects. The energy spectra of electrons from thermal to highest energies are composed from different components due to transport processes in the phase space from mentioned sources. They are of fundamental physical interest per se and of technical applications as well. We summarize the gained knowledge in the visual simple shape as tables, plots and formulae for the aim to turn attention on unsolved questions and possible perspectives of obtaining new information.
Presentation type Section talk (10+5 min)

Primary authors

Igor Veselovsky (НИИЯФ МГУ, ИКИ РАН) Ksenia Kaportseva (MSU)

Presentation Materials

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