Results 51 to 60 of about 42,046 (150)
Skin Diseases in Long‐Distance Runners
JEADV Clinical Practice, Volume 4, Issue 2, Page 378-388, June 2025.Long‐distance/trails runners often experience various skin manifestations due to prolonged physical activity and environmental exposure (sun, heat, altitude, cold air, etc.). Common issues include blisters, chafing, calluses, nail dystrophy, and sunburn. Acne mechanica and fungal infections are also frequent due to sweat and occlusion. Proper skin care,
Henna Ahomies +3 more
wiley +1 more source
Particle Acceleration in Solar Flares [PDF]
International Astronomical Union Colloquium, 1989 AbstractParticle acceleration during solar flares is a complex process where the main ‘actors’ (Direct (D.C.) or turbulent electric fields) are hidden from us. It is easy to construct a successful particle accelertion model if we are allowed to impose on the flaring region arbitrary conditions (e.g., strength and scale length of the D.C.
openaire +3 more sources
Comparison of UV Ceti Flares with Solar Flares [PDF]
Symposium - International Astronomical Union, 1975 During several intervals totalling 26 h, 84 flares of UV Ceti were observed using a photometer with 1 s time resolution. Using solar flare terminology, all flares of UV Ceti observed here can be characterized by a typical light curve, consisting of a preflare, a flash and a slow phase.
W. Haupt, W. Schlosser
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Earth and Space Science, Volume 12, Issue 6, June 2025.Abstract To explore the hypothesis of a common source of variability in two time series, observers may estimate the magnitude‐squared coherence (MSC), which is a frequency‐domain view of the cross correlation. For time series that do not have uniform observing cadence, MSC can be estimated using Welch's overlapping segment averaging.
Sarah E. Dodson‐Robinson +1 more
wiley +1 more source
Solar-geophysical data number 496, December 1985. Part 2: (Comprehensive reports). Data for June 1985, January-May 1985 and miscellanea [PDF]
Contents include the detailed index for 1985; data for June 1985 (solar flares, solar radio bursts at fixed frequencies, solar X-ray radiation from GOES satellite graphs, mass ejections from the sun, and active prominences and filaments); data for ...
Coffey, H. E.
core +1 more source
Using the Maximum X-ray Flux Ratio and X-ray Background to Predict Solar Flare Class
, 2015 We present the discovery of a relationship between the maximum ratio of the flare flux (namely, 0.5-4 Ang to the 1-8 Ang flux) and non-flare background (namely, the 1-8 Ang background flux), which clearly separates flares into classes by peak flux level.
Balasubramaniam, K., Winter, Lisa M.
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Variation of Model‐Predicted Reconnection Voltages Applied to Uranus' Dayside Magnetosphere
Journal of Geophysical Research: Space Physics, Volume 130, Issue 6, June 2025.Abstract Uranus provides a key missing piece for fundamentally understanding solar wind‐magnetospheric interactions due to its location in the outer solar system. Whether the viscous‐like interaction overtakes global magnetic reconnection as the dominant process at the magnetopause of the outer planets remains unresolved.
S. Zomerdijk‐Russell +2 more
wiley +1 more source
The role of eruption in solar flares [PDF]
Solar Physics, 1989 AbstractThis article focuses on two problems involved in the development of models of solar flares. The first concerns the mechanism responsible for eruptions, such as erupting filaments or coronal mass ejections, that are sometimes involved in the flare process.
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Solar-geophysical data number 489, May 1985. Part 2: (Comprehensive reports). Data for December 1984, March-May 1983 and miscellanea [PDF]
Contents include: detailed index for 1984 to 1985; data for December 1984--(Meudon Carte Synoptique, solar radio bursts at fixed frequencies, solar X-ray radiation from GOES satellite graphs, mass ejections from the sun, active prominences and filaments,
Coffey, H. E.
core +1 more source
Space Weather, Volume 23, Issue 6, June 2025.Abstract In early May 2024 ∼ ${\sim} $6 Coronal Mass Ejections were launched toward the Earth in short succession. This triggered the G5 “Gannon” geomagnetic storm lasting from ∼ ${\sim} $17 UT on 10 May 2024 to ∼ ${\sim} $9 UT on 12 May 2024.
D. H. Mac Manus +9 more
wiley +1 more source