E-Print Archive

There are 3928 abstracts currently viewable.


Search:

Advanced Search
Options
Main Page Add New E-Print Submitter
Information
Feedback
News Help/FAQ About Preferences
Manage Key Phrase
Notification
Anatomy of a solar flare: Part I. The solar quake measurements of the December 14, 2006 X-class flare with GONG, Hinode and RHE View all abstracts by submitter

Sarah Matthews   Submitted: 2010-05-28 01:23

Some of the most challenging observations to explain in the context of existing flare models are those related to the lower atmosphere and below the solar surface. Such observations, including changes in the photospheric magnetic field and seismic emission, indicate the poorly understood connections between energy release in the corona and its impact in the photosphere and the solar interior. Using data from Hinode, TRACE, RHESSI and GONG we study the temporal and spatial evolution of the 14 December 2006 X-class flare in the chromosphere, photosphere and the solar interior. We report for the first time the detection of a solar quake using time-distance methods applied to GONG data. We then investigate the connections between the emission at various atmospheric depths, with an emphasis on determining the origin of the acoustic responses observed with the GONG data. We report the horizontal displacements observed in the photosphere linked to the timing and locations of the solar quakes associated with this flare, their vertical and horizontal displacement velocities at different atmospheric depths and their implications for models developed for the interpretation of these observations reported in Part II.

Authors: Sarah Matthews, Sergei Zharkov, Valentina Zharkova
Projects: Hinode/SOT

Publication Status: ApJ (submitted)
Last Modified: 2010-05-28 03:01
Go to main E-Print page  Simulating the ''sliding doors'' effect through magnetic flux emergence  First observations of a dome-shaped large-scale coronal EUV wave  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

Key
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
Diagnostic Analysis of the Solar Proton Flares of September 2017 by Their Radio Bursts
Densities Probed by Coronal Type III Radio Burst Imaging
The Minimum Energy Principle Applied to Parker's Coronal Braiding and Nanoflaring Scenario
Eruptions from quiet Sun coronal bright points. I. Observations
Evolution of the transverse density structure of oscillating coronal loops inferred by forward modelling of EUV intensity
Non-stationary quasi-periodic pulsations in solar and stellar flares
Lost and found sunquake in the 6 September 2011 flare caused by beam electrons
Nonkinematic solar dynamo models with double-cell meridional circulation
Solar Kinetic Energy and Cross Helicity Spectra
Collective Study of Polar Crown Filaments in the Past Four Solar Cycles
Highly Ionized Calcium and Argon X-ray Spectra from a Large Solar Flare
Detecting the solar new magnetic flux regions on the base of vector magnetograms
A Truly Global EUV Wave From the SOL2017-09-10 X8.2 Solar Flare-CME Eruption
ALTERNATIVE ZEBRA-STRUCTURE MODELS IN SOLAR RADIO EMISSION
Photospheric Shear Flows in Solar Active Regions and Their Relation to Flare Occurrence
Linear Polarization Features in the Quiet-Sun Photosphere: Structure and Dynamics
Solar Microflares Observed by SphinX and RHESSI
Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST
Resistively-limited current sheet implosions in planar anti-parallel (1D) and null-point containing (2D) magnetic field geometries
Is It Small-scale Weak Magnetic Activity That Effectively Heats the Upper Solar Atmosphere?

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