E-Print Archive

There are 3715 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
First Simultaneous Observation of H α Moreton Wave, EUV Wave, and Filament/Prominence Oscillations View all abstracts by submitter

Ayumi Asai   Submitted: 2011-12-27 00:40

This abstract was corrupted following database problems and is being recovered. It will be restored as quickly as possible. Any questions, please send them to Alisdair. Sorry for any incovenience.


Authors: Asai, A., Ishii, T.T., Kitai R., Ichimoto, K., UeNo, S., Nagata, S., Morita, S., Nishida, K., Shiota, D., Oi, A., Akioka, M., Shibata, K.
Projects: SDO-AIA,STEREO

Publication Status: accepted by ApJL
Last Modified: 2011-12-28 12:07
Go to main E-Print page  On the physical meaning of n-distributions in solar flares  Fermi Detection of  gamma-ray emission from the M2 Soft X-ray Flare on 2010 June 12  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
Microflare Heating of a Solar Active Region Observed with NuSTAR, Hinode/XRT, and SDO/AIA
Successive Two-sided loop Jets Caused by Magnetic Reconnection between Two adjacent Filamentary Threads
Solar plasma radio emission in the presence of imbalanced turbulence of kinetic-scale Alfvén waves
Spatial Offsets in Flare-CME Current Sheets
Magnetic Flux Rope Shredding by a Hyperbolic Flux Tube: The Detrimental Effects of Magnetic Topology on Solar Eruptions
Observational Study on the Fine Structure and Dynamics of a Solar Jet. I. Energy Build-Up Process around a Satellite Spot.
Coronal Holes and Open Magnetic Flux over Cycles 23 and 24
Gradual Solar Coronal Dimming and Evolution of Coronal Mass Ejection in the Early Phase
Elongation of Flare Ribbons
The eruption of a small-scale emerging flux rope as the driver of an M-class flare and a coronal mass ejection
Magnetic Flux Cancelation as the Origin of Solar Quiet Region Pre-Jet Minifilaments
Three-dimensional oscillatory magnetic reconnection
Quasi-Periodic Radio Bursts Associated with Fast-mode Waves near a Magnetic Null Point
Onset of a Large Ejective Solar Eruption from a Typical Coronal-Jet-Base Field Configuration
Heating of an erupting prominence associated with a solar coronal mass ejection on 2012 January 27
New Evidence that Magnetoconvection Drives Solar-Stellar Coronal Heating
Beam electrons as a source of Hα flare ribbons
A hybrid supervised/unsupervised machine learning approach to solar flare prediction
Magnetohydrodynamic Simulations for Studying Solar Flare Trigger Mechanism
Sunspot Light Walls Suppressed by Nearby Brightenings

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