There are 4350 abstracts currently viewable.
Add New E-Print
Heating of Flare Loops With Observationally Constrained Heating Functions
Submitted: 2011-12-30 11:57
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
. Sorry for any incovenience.
Authors: Qiu J., Liu W-J, Longcope D. W.
Publication Status: ApJ, in press
Last Modified: 2012-01-04 12:16
Go to main E-Print page.
View all abstracts by submitter.
Could switchbacks originate in the lower solar atmosphere? II. Propagation of switchbacks in the solar corona
Solar large-scale magnetic field and cycle patterns in solar dynamo
Three-dimensional magnetic reconnection in astrophysical plasmas
Energy partition in a confined flare with an extreme-ultraviolet late phase
Alfvén wave heating in partially ionized thin threads of solar prominences
He I 10830Å Dimming During Solar Flares, I: The Crucial Role of Non-Thermal Collisional Ionisations
Separating aa-index into Solar and Hale Cycle Related Components Using Principal Component Analysis
Inward Propagating Plasma Parcels in the Solar Corona: Models with Aerodynamic Drag, Ablation, and Snowplow Accretion
Energetics and 3-D Structure of Elementary Events in Solar Coronal Heating
Stellar Superflares Observed Simultaneously with Kepler and XMM-Newton
Medium-term predictions of F10.7 and F30 cm solar radio flux with the adaptive Kalman filter
Resonances in a Coronal Loop Driven by Torsional Alfvén Waves Propagating from the Photosphere
Effects of external flow on resonant absorption of coronal loop kink oscillations driven by an external fast wave: Selective excitation problem
Emerging Dimming as Coronal Heating Episodes
Proxy-Based Prediction of Solar Extreme Ultraviolet Emission using Deep Learning
The source of the major solar energetic particle events from super active region 11944
Critical decay index for eruptions of ‘short’ filaments
Thermal Trigger for Solar Flares I: Fragmentation of the Preflare Current Layer
The Evolution of Plasma Composition During a Solar Flare
Large-amplitude prominence oscillations following the impact by a coronal jet
MSU Solar Physics.
Max Millennium Science Mail Archive.
Max Millennium Message of the Day Mail Archive.
Max Millennium Flare Catalog
© 2000-2020 Solar Physics Group - Montana State University