Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Chaitanya Sishtla"'
Publikováno v:
The Astrophysical Journal Letters, Vol 963, Iss 1, p L25 (2024)
High-speed solar wind streams (HSSs) interact with the preceding ambient solar wind to form stream interaction regions (SIRs), which are a primary source of recurrent geomagnetic storms. However, HSSs may also encounter and subsequently interact with
Externí odkaz:
https://doaj.org/article/b4d2961e97f546d9a089c5c3cdf3bb0a
Alfvénic fluctuations of various scales are ubiquitous in the solar wind, with their non-linear interactions and eventual cascade resulting in an important heating mechanism to accelerate the solar wind via turbulent heating. Such fluctuations are a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::71655402cc35686fa1b23c7cd25c75d5
https://doi.org/10.5194/egusphere-egu23-6807
https://doi.org/10.5194/egusphere-egu23-6807