Results 101 to 110 of about 2,286 (221)
Modeling Time-variable Elemental Abundances in Coronal Loop Simulations
Numerous recent X-ray observations of coronal loops in both active regions and solar flares have shown clearly that elemental abundances vary with time.
Jeffrey W. Reep +3 more
doaj +1 more source
Lawnmower Poetry and the Poetry of Lawnmowers
Critical Quarterly, Volume 68, Issue 1, Page 4-42, April 2026.
Francesca Gardner
wiley +1 more source
On the topology of global coronal magnetic fields
This thesis considers the magnetic topology of the global solar corona. To understand the magnetic topology we use the magnetic skeleton which provides us with a robust description of the magnetic field.
Edwards, Sarah J.
core
SWIFF : space weather integrated forecasting framework [PDF]
This research has received funding from the European Commission’s FP7 Program with the grant agreement SWIFF (Project No. 2633430, swiff.eu). The KU Leuven simulations were conducted on the computational resources provided by the PRACE Tier-0 Project No.
Viviane Pierrard +84 more
core +1 more source
Development and application of a global magnetic field evolution model for the solar corona
Magnetic fields are fundamental to the structure and dynamics of the Sun’s corona. Observations show them to be locally complex, with highly sheared and twisted fields visible in solar filaments/prominences.
Yeates, Anthony Robinson
core
Observation and modeling of solar coronal loops
La corona solar está constituida por un plasma tenue altamente magnetizado en el que los mecanismos de transporte actúan fundamentalmente a lo largo de sus líneas de campo.
Mac Cormack, Cecilia
core
Magnetic Waves In Solar Coronal Loops
Final presentations of the Center for Astrophysics HEA/SSP Solar Summer Intern Program.
openaire +1 more source
The propagation and damping of slow magnetoacoustic waves in the solar atmosphere
The propagation and damping of slow magnetoacoustic waves in the solar atmosphere is investigated, with particular emphasis placed on waves with periodicities of five minutes. The basic model of a uniform temperature loop is extended by the addition of
Owen, Nicholas Robert
core
On the Existence of Long-period Decayless Oscillations in Short Active Region Loops
Decayless kink oscillations, characterized by their lack of decay in amplitude, have been detected in coronal loops of varying scales in active regions, the quiet Sun, and coronal holes. Short-period (
Arpit Kumar Shrivastav +7 more
doaj +1 more source

