Results 81 to 90 of about 10,701,163 (203)
Solar UV radiation influence the Earth's climate and upper atmosphere. The UV emission from the Sun modulates with the sunspot cycle with an 11-year periodicity.
(G) Chandrika +2 more
doaj +1 more source
Abstract Accurately predicting fast solar wind conditions is challenging, as uncertainties are large and unquantified by traditional single‐value prediction models. In particular, the risks of high‐speed solar wind streams (HSSs), which can cause damage to technological infrastructure, cannot be reliably assessed without probabilistic forecasts.
Daniel Collin +5 more
wiley +1 more source
On the Magnetic Field Evolution of Interplanetary Coronal Mass Ejections from 0.07 to 5.4 au
A central question for understanding interplanetary coronal mass ejection (ICME) physics and improving space weather forecasting is how ICMEs evolve in interplanetary space.
Christian Möstl +10 more
doaj +1 more source
Dynamical Solar Wind Forecasting Using In Situ Solar Wind Speed Observations
Abstract Accurate prediction of the ambient solar wind at Earth is a key requirement for space‐weather forecasting but is limited by uncertainties in coronal boundary conditions and, to a lesser extent, heliospheric transport. We present a quantitative assessment of a solar wind forecast that uses near‐Earth in situ solar wind observations to estimate ...
M. J. Owens +3 more
wiley +1 more source
The shape and dynamics of coronal mass ejections (CMEs) vary significantly based on the instrument and wavelength used. This has led to significant debate about the proper definitions of CME/shock fronts, pile-up/compression regions, and core ...
Stepanyuk Oleg, Kozarev Kamen
doaj +1 more source
Radio Sounding Determination of Two‐Dimensional Plasma Structure Velocity
Abstract The Mars spacecraft Tianwen‐1 transmitted radio signals to Earth for its orbit determination. The frequencies of the radio signals exhibited sharp variations when an ICME passed through the Mars‐Earth signal path on 18 June 2021. These sharp variations were observed at different ground stations at different times. This was most probably caused
Qingbao He, Qinghui Liu, Yongzhang Yang
wiley +1 more source
The paper reports the results of calculations of the center-to-limb intensity of optically thin line emission in EUV and FUV wavelength ranges. The calculations employ a multicomponent model for the quiescent solar corona.
Krissinel B.B.
doaj +1 more source
Time-dependent Hinode/EIS Atlas of a Coronal Mass Ejection Containing Cool Material
We report the first time-dependent spectral atlas of a coronal mass ejection (CME) observed by the Hinode/Extreme Ultraviolet Imaging Spectrometer (EIS).
E. M. Wraback +2 more
doaj +1 more source
Use of the Moon to Distinguish the F from the K Corona Using a Rocket Coronagraph During an Eclipse [PDF]
F and K corona observations by rocket coronagraph during solar ...
Mc Cullough, R. E. +3 more
core
Near-Sun observations of an F-corona decrease and K-corona fine structure [PDF]
peer reviewedRemote observations of the solar photospheric light scattered by electrons (the K-corona) and dust (the F-corona or zodiacal light) have been made from the ground during eclipses1 and from space at distances as small as 0.3 astronomical ...
Rouillard, Alexis P. +95 more
core +1 more source

