Results 91 to 100 of about 107,783 (198)
An ICME impact on the Martian hydrogen corona
Earth and Planetary Physics, 2020 The Martian hydrogen exosphere extends out of the bow shock, forming a "hydrogen corona". The solar wind interacts directly with the hydrogen corona. During an ICME event on 7 March 2015, the SWIA instrument onboard Mars Atmosphere and Volatile Evolution
Qi Xu +5 more
doaj +1 more source
Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
, 2008 The heating of the solar chromosphere and corona is a long-standing puzzle in solar physics. Hinode observations show the ubiquitous presence of chromospheric anemone jets outside sunspots in active regions.
A. M. Title +24 more
core +1 more source
ChemistryOpen, Volume 15, Issue 5, May 2026.This review summarizes recent advances in the synthesis and processing of carbon nanotubes and carbon nanocomposites, highlighting structure–property relationships and their applications in energy storage, biomedical systems, and environmental technologies, with emphasis on performance optimization and sustainable material design.
Noor‐ul‐Huda Altaf +9 more
wiley +1 more source
Coordinated observations in support of the solar maximum mission [PDF]
The in-orbit repair of the Solar Maximum Mission satellite has provided an opportunity to continue observations of the Sun's outer corona, transition region, and bolometric flux through the decay phase and minimum of the solar cycle.
Labonte, B.
core +1 more source
Solar Flares, the Solar Corona, and Solar Physics [PDF]
Symposium - International Astronomical Union, 2000 The Sun serves as the local physics laboratory for studying the suprathermal activity phenomena of stars. Scrutiny of the Sun has led to the discovery of a host of previously unknown physical effects, largely within the classical physics of Newton and Maxwell, but including quantum mechanics and lepton physics as well.
openaire +1 more source
Constraining Electron‐Impact Ionization of O2 Through UV Aurora Observations at Ganymede
Journal of Geophysical Research: Space Physics, Volume 131, Issue 5, May 2026.Abstract While photoionization rates of Ganymede's O2 ${\mathrm{O}}_{2}$ dominated atmosphere are well constrained, the contribution of electron‐impact ionization is rather uncertain. Previous quantitative estimates have relied on assumptions about densities and energy distributions of precipitating electrons, or on rare spacecraft measurements that ...
Stefan Duling +5 more
wiley +1 more source
The Astrophysical JournalThe plasma of the solar corona harbors a multitude of coronal wave modes, some of which could be dissipated to provide the required energy and momentum to heat the corona and accelerate the solar wind.
Momchil E. Molnar +6 more
doaj +1 more source
The solar flare environment [PDF]
Solar flare environment - solar atmosphere, photosphere, chromosphere, corona, and solar flare types, model, occurence, prediction, and ...
Roberts, W. T.
core +1 more source
A zone of preferential ion heating extends tens of solar radii from Sun
, 2017 The extreme temperatures and non-thermal nature of the solar corona and solar wind arise from an unidentified physical mechanism that preferentially heats certain ion species relative to others.
Bale, Stuart D. +8 more
core +3 more sources
A Case of Blastomycosis Like Pyoderma Responsive to Intralesional Triamcinolone Acetonide Injections
Australasian Journal of Dermatology, EarlyView.
Dasmesh Sron +3 more
wiley +1 more source