[HTML][HTML] The solar probe plus mission: humanity's first visit to our star

NJ Fox, MC Velli, SD Bale, R Decker, A Driesman… - Space Science …, 2016 - Springer
Abstract Solar Probe Plus (SPP) will be the first spacecraft to fly into the low solar corona.
SPP's main science goal is to determine the structure and dynamics of the Sun's coronal …

[HTML][HTML] Coronal mass ejections: Observations

DF Webb, TA Howard - Living Reviews in Solar Physics, 2012 - Springer
Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic
particles, and radio bursts. Since the vast majority of these are associated with the eruption …

EUHFORIA: European heliospheric forecasting information asset

J Pomoell, S Poedts - Journal of Space Weather and Space …, 2018 - swsc-journal.org
The implementation and first results of the new space weather forecasting-targeted inner
heliosphere model “European heliospheric forecasting information asset”(EUHFORIA) are …

[HTML][HTML] Ion thrusters for electric propulsion: Scientific issues developing a niche technology into a game changer

K Holste, P Dietz, S Scharmann, K Keil… - Review of Scientific …, 2020 - pubs.aip.org
The transition from old space to new space along with increasing commercialization has a
major impact on space flight, in general, and on electric propulsion (EP) by ion thrusters, in …

[HTML][HTML] Coronal mass ejections: models and their observational basis

PF Chen - Living Reviews in Solar Physics, 2011 - Springer
Coronal mass ejections (CMEs) are the largest-scale eruptive phenomenon in the solar
system, expanding from active region-sized nonpotential magnetic structure to a much larger …

[HTML][HTML] Space weather: The solar perspective

R Schwenn - Living reviews in solar physics, 2006 - Springer
The term space weather refers to conditions on the Sun and in the solar wind,
magnetosphere, ionosphere, and thermosphere that can influence the performance and …

CME–CME interactions as sources of CME geoeffectiveness: The formation of the complex ejecta and intense geomagnetic storm in 2017 early September

C Scolini, E Chané, M Temmer… - The Astrophysical …, 2020 - iopscience.iop.org
Coronal mass ejections (CMEs) are the primary sources of intense disturbances at Earth,
where their geoeffectiveness is largely determined by their dynamic pressure and internal …

[HTML][HTML] Earth-affecting solar transients: a review of progresses in solar cycle 24

J Zhang, M Temmer, N Gopalswamy… - Progress in Earth and …, 2021 - Springer
This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

The thermosphere is a drag: The 2022 Starlink incident and the threat of geomagnetic storms to low earth orbit space operations

TE Berger, M Dominique, G Lucas, M Pilinski… - Space …, 2023 - Wiley Online Library
Abstract On 03 February 2022, SpaceX launched 49 Starlink satellites, 38 of which re‐
entered the atmosphere on or about 07 February 2022 due to unexpectedly high …

[HTML][HTML] Observation-based modelling of magnetised coronal mass ejections with EUHFORIA

C Scolini, L Rodriguez, M Mierla, J Pomoell… - Astronomy & …, 2019 - aanda.org
Context. Coronal mass ejections (CMEs) are the primary source of strong space weather
disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic …