E-Print Archive

There are 4053 abstracts currently viewable.


Advanced Search
Main Page Add New E-Print Submitter
News Help/FAQ About Preferences
Manage Key Phrase
Transient induced MHD oscillations : A tool to probe the solar active regions View all abstracts by submitter

Dr. A.K. Srivastava   Submitted: 2011-10-07 01:37

Solar transients and eruptive phenomena which are ubiquitous in the solaratmosphere, can shed new light to the understanding of the outstanding problemslike coronal heating and the solar wind acceleration. Observations in theentire electromagnetic spectrum of such dynamical processes of large andsmall-scale transient/eruptive events, with highly dynamic magnetic fieldconfiguration, and energetic particles, provide crucial information about theplasma processes at mega-Kelvin temperature embedded in a complex magneticfield, and also energy build-up/energy-release processes, taking place in suchevents. One of the most important phenomenological aspects of solar eruptivephenomena is the induced magnetohydrodynamic (MHD) waves generated during theseenergetic processes, which carry a potential signature to probing the solaractive regions. In this paper, we briefly review the recent trends of thetransient (e.g., flares) induced quasi-periodic oscillations in the solaratmosphere and discuss their implications in diagnosing the solar activeregions, providing the clue to understanding local plasma dynamics and heating.

Authors: Srivastava, Abhishek K.; Nakariakov, V. M.; Dwivedi, B. N.; Kumar, Pankaj
Projects: None

Publication Status: 6 pages, 2 figures, to be appear in the Proc. of the 1st Asian-Pacific Solar Phys. Meeting
Last Modified: 2011-10-08 12:25
Go to main E-Print page  Benchmarking atomic data for astrophysics: Fe XVII lines  Atomic data for the X-ray lines of Fe VIII & Fe IX  Edit Entry  Download Preprint  Delete Entry 

Go to main E-Print pageGo to main E-Print page.
Previous AbstractPrevious Abstract.
Next AbstractNext Abstract.
Download PreprintDownload Preprint.
Submitter's HomepageSubmitters Homepage.
Edit EntryEdit Entry.
View All Abstracts By SubmitterView all abstracts by submitter.
Delete AbstractDelete abstract.

Latest Entries
Linear waves in a non-equilibrium ionisation partially ionised plasma
How Many Twists Do Solar Coronal Jets Release?
Different Signatures of Chromospheric Evaporation in Two Solar Flares Observed with IRIS
The Physical Nature of Spiral Wave Patterns in Sunspots
Predicting Solar Flares Using a Long Short-Term Memory Network
Coronal loop transverse oscillations excited by different driver frequencies
Solar Center-Limb Variation of the Strengths of Spectral Lines: Classification and Interpretation of Observed Trends
The plasmoid instability in a confined solar flare
High-frequency dynamics of active region moss as observed by IRIS
Extreme-ultraviolet Late Phase Caused by Magnetic Reconnection over Quadrupolar Magnetic Configuration in a Solar Flare
Two-step evolution of a rising flux rope resulting in a confined solar flare
Why torus-unstable solar filaments experience failed eruption?
The Magnetic Properties of Heating Events on High-Temperature Active Region Loops
Pulse-beam heating of deep atmospheric layers, their oscillations and shocks modulating the flare reconnection
A potential magnetic field calculator for solar physics applications using staggered grids
E and B polarizations from inhomogeneous and solar surface turbulence
Oscillations Accompanying a He I 10830 Å Negative Fare in a Solar Facula II. Response of the Transition Region and Corona
Flare reconnection-driven magnetic field and Lorentz force variations at the Sun's surface
Why Does the Solar Corona Abnormally Rotate Faster Than the Photosphere?
Impacts On Proton Fluxes Observed During Different Interplanetary Conditions

Related Pages
MSU Solar Physics.
Max Millennium Science Mail Archive.
Max Millennium Message of the Day Mail Archive.
Max Millennium Flare Catalog

Archive Maintainer
Alisdair Davey

© 2003 Solar Physics Group - Montana State University