Results 91 to 100 of about 1,141,583 (297)

Long‐Term Real‐World Effectiveness of Rupatadine in Chronic Urticaria: A Retrospective Observational Study

open access: yesJEADV Clinical Practice, EarlyView.
This retrospective observational study analyzed a cohort of chronic urticaria (CU) patients to provide insight into the clinical practice of CU with second‐generation antihistamines (SgAHs) and to evaluate the long‐term real‐world effectiveness of rupatadine in CU. Patients with chronic spontaneous urticaria (CSU) and chronic inducible urticaria (CIndU)
A. M. Giménez‐Arnau   +5 more
wiley   +1 more source

PREDICTION OF SOLAR FLARES USING UNIQUE SIGNATURES OF MAGNETIC FIELD IMAGES [PDF]

open access: yes, 2016
Prediction of solar flares is an important task in solar physics. The occurrence of solar flares is highly dependent on the structure and topology of solar magnetic fields.
Abbas Raboonik   +3 more
semanticscholar   +1 more source

Solar flares: An overview

open access: yesAdvances in Space Research, 1992
This is a survey of solar phenomena and physical models that may be useful for improving forecasts of solar flares and proton storms in interplanetary space. Knowledge of the physical processes that accelerate protons has advanced because of gamma-ray and X-ray observations from the Solar Maximum Mission telescopes.
openaire   +3 more sources

An Observational Overview of Solar Flares [PDF]

open access: yesSpace Science Reviews, 2011
This is an article for a monograph on the physics of solar flares, inspired by RHESSI observations. The individual articles are to appear in Space Science Reviews (2011)
Brian R. Dennis   +17 more
openaire   +5 more sources

Statistics of Solar White-light Flares. I. Optimization and Application of Identification Methods

open access: yesThe Astrophysical Journal
White-light flares (WLFs) are energetic activity in the stellar atmosphere. However, observed solar WLFs are relatively rare compared to stellar WLFs or solar flares observed at other wavelengths, which limits our further understanding of solar/stellar ...
Yingjie Cai   +3 more
doaj   +1 more source

No Evidence Supporting Flare Driven High-Frequency Global Oscillations

open access: yes, 2012
The underlying physics that generates the excitations in the global low-frequency, < 5.3 mHz, solar acoustic power spectrum is a well known process that is attributed to solar convection; However, a definitive explanation as to what causes excitations in
A. Ambastha   +23 more
core   +1 more source

The impact of gigafire on vegetation structure, terrestrial vertebrate abundance and diel activity

open access: yesOikos, EarlyView.
Fire regimes are shifting around the world due to climate and land‐use change, resulting in an increased frequency of large and severe wildfires. However, the impact of extreme wildfire events on animal species remains poorly understood. Particularly lacking is an understanding of how fire affects animal behaviour.
Grant D. Linley   +6 more
wiley   +1 more source

THE VERTICAL-CURRENT APPROXIMATION NONLINEAR FORCE-FREE FIELD CODE—DESCRIPTION, PERFORMANCE TESTS, AND MEASUREMENTS OF MAGNETIC ENERGIES DISSIPATED IN SOLAR FLARES [PDF]

open access: yes, 2016
In this work we provide an updated description of the Vertical-Current Approximation Nonlinear Force-Free Field (VCA-NLFFF) code, which is designed to measure the evolution of the potential, non-potential, free energies, and the dissipated magnetic ...
M. Aschwanden
semanticscholar   +1 more source

Effects of Galactic Irradiation on Thermal and Electronic Transport in Tungsten

open access: yesphysica status solidi (b), EarlyView.
This atomic‐scale study reveals how low‐to‐mid‐energy space irradiation alters tungsten's thermal and electronic behavior, even at low defect levels. Focusing on vacancy sites in bulk and near grain boundaries, it employs two novel approaches: site‐projected thermal conductivity and the N2$^{2}$ method for the thermal and electronic response analysis ...
Chinonso Ugwumadu   +2 more
wiley   +1 more source

Critical Height of the Torus Instability in Two-ribbon Solar Flares [PDF]

open access: yes, 2017
We studied the background field for 60 two-ribbon flares of M-and-above classes during 2011–2015. These flares are categorized into two groups, i.e., eruptive and confined flares, based on whether a flare is associated with a coronal mass ejection or not.
Dong Wang   +7 more
semanticscholar   +1 more source

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