Results 11 to 20 of about 8,180,974 (123)

The Observations of Magnetic Reconnection during the Interaction Process of Two Active Region Filaments

open access: yesThe Astrophysical Journal
We investigate the interaction between two filaments (F1 and F2) and their subsequent magnetic reconnection in active region (AR) NOAA 13296 and AR NOAA 13293 on 2023 May 9, utilizing high spatial and temporal resolution and multiwavelength observational
Zongyin Wu   +13 more
doaj   +2 more sources

Solar wind dependence of ion parameters in the earth's magnetospheric region calculated from CLUSTER observations [PDF]

open access: yes, 2008
Moments calculated from the ion distributions (~0–40 keV) measured by the Cluster Ion Spectrometry (CIS) instrument are combined with data from the Cluster Flux Gate Magnetometer (FGM) instrument and used to characterise the bulk properties of the plasma
Denton, M. H., Taylor, M. G. G. T.
core   +4 more sources

Hybrid imaging and neural networks techniques for processing solar images [PDF]

open access: yes, 2006
YesSolar imaging is currently an active area of research. A fast hybrid system for the automated detection of filaments in solar images is presented in this paper. The system includes three major stages.
Qahwaji, Rami S.R., Colak, Tufan
core   +8 more sources

Filament Eruptions Outside of Active Regions as Sources of Large Solar Energetic Particle Events [PDF]

open access: yesProceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015), 2016
Gradual solar energetic (E > 10 MeV) particle (SEP) events are produced in shocks driven by fast CMEs, which are nearly always spatially associated with ARs. Several cases of SEP events associated with CMEs originating in large filament eruptions (FEs) from outside ARs have previously been known, but four more such cases from solar cycles 23 and 24 ...
Stephen W. Kahler   +6 more
openaire   +1 more source

Development and application of a global magnetic field evolution model for the solar corona [PDF]

open access: yes, 2009
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   +2 more sources

Formation and large-scale patterns of filament channels and filaments [PDF]

open access: yes, 2014
2015ASSL..415..355MThe properties and large-scale patterns of filament channels and filaments are considered. Initially, the global formation locations of filament channels and filaments are discussed, along with their hemispheric pattern.
Duncan H. Mackay   +2 more
core   +1 more source

Prediction of Space Weather Events using Solar Filaments and Sound waves as Precursors

open access: yes, 2023
This dissertation is an effort in adding to existing methods of predictive capability for space weather events such as coronal mass ejections (CMEs) and solar flares and to predict if these events will cause a geo-magnetic storm well in advance.
Venkataramanasastry, Aparna
core   +1 more source

On the topology of global coronal magnetic fields [PDF]

open access: yes, 2014
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   +2 more sources

Thermal shielding of an emerging active region [PDF]

open access: yes, 2012
Context. The interaction between emerging active regions and the pre-existing coronal magnetic field is important for better understanding the mechanisms of storage and release of magnetic energy from the convection zone to the high corona. Aims.
Regnier, Stephane, S. Régnier
core   +1 more source

Automatic detection of limb prominences in 304 A EUV images [PDF]

open access: yes, 2010
A new algorithm for automatic detection of prominences on the solar limb in 304 A EUV images is presented, and results of its application to SOHO/EIT data discussed.
Labrosse, N., Dalla, S., Marshall, S.
core   +1 more source

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