Switchbacks Explained: Super-Parker Fields—The Other Side of the Sub-Parker Spiral

We provide a simple geometric explanation for the source of switchbacks and associated large and one-sided transverse flows in the solar wind observed by the Parker Solar Probe (PSP). The more radial, sub-Parker spiral structure of the heliospheric magnetic field observed previously by Ulysses, ACE,...

Celý popis

Uložené v:

Podrobná bibliografia
Vydané v:	The Astrophysical journal Ročník 909; číslo 1; s. 95 - 105
Hlavní autori:	Schwadron, N. A., McComas, D. J.
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Philadelphia The American Astronomical Society 01.03.2021 IOP Publishing
Predmet:	Active solar corona Astrophysics Charged particles Critical point Field strength Heliospheric magnetic field Interplanetary magnetic fields Magnetic fields Rarefaction Solar coronal holes Solar coronal loops Solar coronal plumes Solar coronal waves Solar magnetic field Solar magnetic fields Solar probes Solar spicules Solar wind Solar wind flow Solar wind velocity Spirals Wind speed
ISSN:	0004-637X, 1538-4357
On-line prístup:	Získať plný text
Tagy:	Pridať tag Žiadne tagy, Buďte prvý, kto otaguje tento záznam!

Buďte prvý, kto okomentuje tento záznam!