Results 21 to 30 of about 235 (149)
The Solar Origin of an In Situ Type III Radio Burst Event
Solar type III radio bursts are generated by beams of energetic electrons that travel along open magnetic field lines through the corona and into interplanetary space.
Meiqi Wang +6 more
doaj +1 more source
In the frame of two coordinated observational and research efforts, two full solar rotations were investigated in the times of two distinct solar minima. These two campaigns were dubbed Whole Sun Month (WSM; 10 August – 8 September 1996) and Whole Heliosphere Interval (WHI; 20 March – 16 April 2008).
Cremades Fernandez, Maria Hebe +2 more
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Damped large amplitude transverse oscillations in an EUV solar prominence, triggered by large-scale transient coronal waves [PDF]
Aims. We investigate two successive trains of large amplitude transverse oscillations in an arched EUV prominence, observed with SoHO/EIT on the north-east solar limb on 30 July 2005. The oscillatory trains are triggered by two large scale coronal waves, associated with an X-class and a C-class flare occurring in the same remote active region.
Hershaw, J. +3 more
openaire +3 more sources
We reconstruct the morphology and kinematics of a series of small transients that erupted from the Sun on 2021 April 24 using observations primarily from Parker Solar Probe (PSP). These sequential small coronal mass ejections (CMEs) may be the product of
Brian E. Wood +3 more
doaj +1 more source
The FIELDS Instrument Suite for Solar Probe Plus [PDF]
NASA's Solar Probe Plus (SPP) mission will make the first in situ measurements of the solar corona and the birthplace of the solar wind. The FIELDS instrument suite on SPP will make direct measurements of electric and magnetic fields, the properties of in situ plasma waves, electron density and temperature profiles, and interplanetary radio emissions ...
Bale, S. D. +83 more
openaire +4 more sources
Coronal and Chromospheric Dynamics of a Coronal Hole Bright Point
Data from the Atmospheric Imaging Assembly (AIA) and the Helioseismic Magnetic Imager on board the Solar Dynamics Observatory and from the Interface Region Imaging Spectograph, are used to study the evolution at different atmospheric layers of a bright ...
Ana Cristina Cadavid, Mari Paz Miralles
doaj +1 more source
Properties of Forbush Decreases with AMS-02 Daily Proton Flux Data
A Forbush decrease (FD) is a sudden reduction of Galactic Cosmic Rays (GCRs) that is usually caused by intense solar wind transients, such as Interplanetary Coronal Mass Ejections (ICMEs) and Corotating Interaction Regions (CIRs).
Siqi Wang +6 more
doaj +1 more source
On the importance of investigating CME complexity evolution during interplanetary propagation
This perspective paper brings to light the need for comprehensive studies on the evolution of interplanetary coronal mass ejection (ICME) complexity during propagation. To date, few studies of ICME complexity exist.
Réka M. Winslow +29 more
doaj +1 more source
Five-minute Periodicities in the Population of Solar Coronal Brightenings
The population of small-scale brightenings observed across broad regions of the quiet-Sun (QS) corona shows coherent strong periodicities of ≈5 minutes and amplitudes of 20% to 30% of the mean.
Huw Morgan +4 more
doaj +1 more source
Solar-MACH: An open-source tool to analyze solar magnetic connection configurations
The Solar MAgnetic Connection HAUS1 tool (Solar-MACH) is an open-source tool completely written in Python that derives and visualizes the spatial configuration and solar magnetic connection of different observers (i.e., spacecraft or planets) in the ...
Jan Gieseler +13 more
doaj +1 more source

