Results 51 to 60 of about 3,640 (192)

On Flux Rope Stability and Atmospheric Stratification in Models of Coronal Mass Ejections Triggered by Flux Emergence [PDF]

open access: yes, 2014
Flux emergence is widely recognized to play an important role in the initiation of coronal mass ejections. The Chen-Shibata (2000) model, which addresses the connection between emerging flux and flux rope eruptions, can be implemented numerically to ...
Lee, E., Linton, M. G., Lukin, V. S.
core   +1 more source

The Patient‐Centred Interdental Cleaning Concept—Consensus Based on a Round Table

open access: yesInternational Journal of Dental Hygiene, EarlyView.
ABSTRACT Aim To consolidate clinical and scientific evidence and develop personalised recommendations for the optimal use of interdental devices, addressing the diverse needs of patients with varying oral health conditions based on the outcomes of an expert meeting.
Tim M. J. A. Thomassen   +9 more
wiley   +1 more source

Simultaneous Optical and Radio Observations of a Large Stellar Flare on EV Lac

open access: yesThe Astrophysical Journal Letters
We present simultaneous optical and radio observations of a large stellar flare on the M dwarf EV Lac, captured between 12:00 and 15:00 UT on 2022 October 25.
Hong-Peng Lu   +10 more
doaj   +1 more source

Comparing SSN Index to X-ray Flare and Coronal Mass Ejection Rates from Solar Cycles 22-24

open access: yes, 2016
The newly revised sunspot number series allows for placing historical geoeffective storms in the context of several hundred years of solar activity.
Balasubramaniam, K. S.   +2 more
core   +1 more source

A synoptic view of solar transient evolution in the inner heliosphere using the Heliospheric Imagers on STEREO [PDF]

open access: yes, 2009
By exploiting data from the STEREO/heliospheric imagers (HI) we extend a well-established technique developed for coronal analysis by producing time-elongation plots that reveal the nature of solar transient activity over a far more extensive region of ...
A. P. Rouillard   +23 more
core   +1 more source

Solar and Stellar Coronal Mass Ejections - a review of the Cool Stars 21 splinter session

open access: yes, 2023
Coronal mass ejections (CMEs) are the most energetic phenomena related to magnetic activity and, by impacting the interplanetary space, they can be the source of severe planetary disturbances. Solar CMEs and their sources, such as flares and filament/prominence eruptions, have been intensively observed and studied over decades.
Chifu, Iulia   +3 more
openaire   +1 more source

The state of knowledge on four families of Syngnathoidei fishes (Teleostei: Syngnathiformes): Aulostomidae, Centriscidae, Fistulariidae and Solenostomidae

open access: yesJournal of Fish Biology, EarlyView.
Abstract Knowledge on the ecology and life‐history traits of coastal marine species is vital to inform their conservation and management, especially as their coastal habitats come under increasing threats. However, such data have never been collated for four of the five families in the suborder Syngnathoidei—the close relatives of the better‐studied ...
Syd J. Ascione   +3 more
wiley   +1 more source

An Extreme Stellar Prominence Eruption Observed by LAMOST Time-domain Spectroscopy

open access: yesThe Astrophysical Journal Letters
We report the detection of an extreme stellar prominence eruption on the M dwarf Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) J044431.62+235627.9, observed through time-domain H α spectroscopy with the LAMOST.
Hong-Peng Lu   +8 more
doaj   +1 more source

Two Energy Release Processes for CMEs: MHD Catastrophe and Magnetic Reconnection

open access: yes, 2007
It remains an open question how magnetic energy is rapidly released in the solar corona so as to create solar explosions such as solar flares and coronal mass ejections (CMEs).
Aly   +33 more
core   +1 more source

Ultra-Wideband Detection of 22 Coherent Radio Bursts on M Dwarfs [PDF]

open access: yes, 2018
Coherent radio bursts detected from M dwarfs have some analogy with solar radio bursts, but reach orders of magnitude higher luminosities. These events trace particle acceleration, powered by magnetic reconnection, shock fronts (such as formed by coronal
Hallinan, Gregg, Villadsen, Jackie
core   +3 more sources

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