Results 31 to 40 of about 15,087 (215)
The Effect of Helio-Geomagnetic Activity in the Geo-Environment and by Extension to Human Health
AtmosphereSolar activity encompasses various phenomena within the solar atmosphere, notably including eruptive events like solar flares and coronal mass ejections (CMEs) [...]
Panagiota Preka-Papadema +1 more
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Coalescence of Magnetic Flux Ropes Within Interplanetary Coronal Mass Ejections: Multi-cases Studies
Frontiers in Physics, 2019 Coronal mass ejections (CMEs) are intense solar explosive eruptions and have significant impact on geomagnetic activities. It is important to understand how CMEs evolve as they propagate in the solar-terrestrial space.
Yan Zhao +7 more
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The Astrophysical Journal, 2023 In situ measurements from spacecraft typically provide a time series at a single location through coronal mass ejections (CMEs), and they have been one of the main methods to investigate CMEs.
F. Regnault +7 more
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Rotation of a Stealth CME on 2012 October 5 Observed in the Inner Heliosphere
The Astrophysical Journal, 2023 Coronal mass ejections (CMEs) are subject to changes in their direction of propagation, tilt, and other properties. This is because CMEs interact with the ambient solar wind and other large-scale magnetic field structures.
Sandeep Kumar +5 more
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Short term Variability of the Sun Earth System: An Overview of Progress Made during the CAWSES II Period [PDF]
, 2015 This paper presents an overview of results obtained during the CAWSES II period on the short term variability of the Sun and how it affects the near Earth space environment. CAWSES II was planned to examine the behavior of the solar terrestrial system as
Gopalswamy, Nat +2 more
core +2 more sources
Radio Physics and Radio Astronomy, 2017 Purpose: Description of the solar wind investigation technique based on interplanetary scintillation observations of the decameter radio emission of space radio sources.
N. N. Kalinichenko +7 more
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Proton Temperature Anisotropy within the Interplanetary Coronal Mass Ejections Sheath at 1 au
The Astrophysical Journal Letters, 2023 The sheath plasma of interplanetary coronal mass ejections (ICMEs) is highly compressed, heated, turbulent, and magnetically intense relative to the ambient solar wind.
Zubair I. Shaikh +2 more
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Coronal Mass Ejections and Solar Polarity Reversal
The Astrophysical Journal, 2003 We report on a close relationship between the solar polarity reversal and the cessation of high-latitude coronal mass ejections (CMEs). This result holds good for individual poles of the Sun for cycles 21 and 23, for which CME data are available. The high-latitude CMEs provide a natural explanation for the disappearance of the polar crown filaments ...
N. Gopalswamy +3 more
openaire +1 more source
Energetics of a Solar Flare and a Coronal Mass Ejection Generated by a Hot Channel Eruption
The Astrophysical Journal, 2023 Hot channels (HCs) are prevalent in the solar corona and play a critical role in driving flares and coronal mass ejections (CMEs). In this paper, we estimate the energy content of an X1.4 eruptive flare with a fast CME generated by an HC eruption on 2011
Qingmin Zhang +4 more
doaj +1 more source
, 2009 Observations of the quiet solar corona in the 171A (~1MK) passband of the Transition Region and Coronal Explorer (TRACE) often show disruptions of the coronal part of small-scale ephemeral bipolar regions that resemble the phenomena associated with ...
Aschwanden +11 more
core +1 more source