Kelvin-Helmholtz instability in solar spicules

Q: How can I download an article?

To download an article from SID, first log in to the site, search for the article title, and click on the 'Download Article' option.

Q: How can I download an ISI article?

To download an ISI article on SID, enter the keyword or article title in the search bar, view the relevant results, click on the desired article, and select the 'Download Article' option.

Q: How can I access the SID database?

To access the SID database, visit SID.ir, create an account, and log in to access scientific resources.

Q: Is downloading articles from SID free?

Some articles on SID are available for free, while others require payment. Details are specified on the article's page.

EBADI H.

مرکز اطلاعات علمی Scientific Information Database (SID) - Trusted Source for Research and Academic Resources

Journal Paper

Paper Information

Journal: Iranian Journal of Physics Research Year:2016 | Volume:16 | Issue:3 Page(s): 41-45

Download Full-Text

Persian Verion

View:

610

Download:

139

Cites:

Information Journal Paper

Title

Kelvin-Helmholtz instability in solar spicules

Author(s)

EBADI H. | Issue Writer Certificate

Keywords

sunQ2

spiculesQ1

Astrophysical Magneto Hydrodynamics (MHD) wavesQ1

Kelvin-Helmholtz instabilityQ1

Abstract

Magneto hydrodynamic waves, propagating along spicules, may become unstable and the expected instability is of Kelvin-Helmholtz type. Such instability can trigger the onset of wave turbulence leading to an effective plasma heating and particle acceleration. In present study, two-dimensional magneto hydrodynamic simulations performed on a Cartesian grid is presented in spicules with different densities, moving at various speeds depending on their environment. Simulations being applied in this study show the onset of Kelvin-Helmholtz type instability and transition to turbulent flow in spicules. Development of Kelvin-Helmholtz instability leads to momentum and energy transport, dissipation, and mixing of fluids. When magnetic fields are involved, field amplification is also possible to take place.

Cites

No record.

References

No record.

Cite

APA: Copy

EBADI, H.. (2016). Kelvin-Helmholtz instability in solar spicules. IRANIAN JOURNAL OF PHYSICS RESEARCH, 16(3 ), 41-45. SID. https://sid.ir/paper/1672/en

Vancouver: Copy

EBADI H.. Kelvin-Helmholtz instability in solar spicules. IRANIAN JOURNAL OF PHYSICS RESEARCH[Internet]. 2016;16(3 ):41-45. Available from: https://sid.ir/paper/1672/en

IEEE: Copy

H. EBADI, “Kelvin-Helmholtz instability in solar spicules,” IRANIAN JOURNAL OF PHYSICS RESEARCH, vol. 16, no. 3 , pp. 41–45, 2016, [Online]. Available: https://sid.ir/paper/1672/en

Related Journal Papers