Results 121 to 130 of about 16,696 (216)

Slow shocks in coronal mass ejections [PDF]

The possibility that slow-mode shock compression may produce at least some of the increased brightness observed at the leading edge of coronal mass ejections is investigated.
Steinolfson, R. S.
core   +1 more source

MHD Forecasting of Solar Wind With Coronal Mass Ejections

Space Weather
We present a model, implemented as an online service, for predicting the speed and density of solar wind in the inner heliosphere and near Earth. The model is based on a numerical magnetohydrodynamics code PLUTO.
S. Arutyunyan, A. Kodukov, M. Subbotin, D. Pavlov   +3 more
doaj   +1 more source

Interactions Between Coronal Mass Ejections

, 2020
This work is supported by the NSF-REU Solar Physics program at SAO, grant number AGS-1850750.
openaire   +1 more source

3D Non-equilibrium Ionization and Spectroscopic Modeling of Coronal Mass Ejections. II. CME Energy Budget

The Astrophysical Journal
Coronal mass ejections (CMEs) release between ≈10 ^30 and 10 ^33 erg of energy into the corona; however, their detailed energy budget is difficult to constrain.
E. M. Wraback, W. B. Manchester IV, E. Landi, J. Szente   +3 more
doaj   +1 more source

Discrepancies in the Properties of a Coronal Mass Ejection on Scales of 0.03 au as Revealed by Simultaneous Measurements at Solar Orbiter and Wind: The 2021 November 3–5 Event

The Astrophysical Journal
Simultaneous in situ measurements of coronal mass ejections (CMEs), including both plasma and magnetic field, by two spacecraft in radial alignment have been extremely rare.
F. Regnault, N. Al-Haddad, N. Lugaz, C. J. Farrugia, W. Yu, B. Zhuang, E. E. Davies   +6 more
doaj   +1 more source

Driving Dynamical Inner‐Heliosphere Models With In Situ Solar Wind Observations

Space Weather
Accurately reconstructing the solar wind throughout the inner heliosphere is essential for understanding solar–terrestrial interactions and improving space‐weather forecasts.
M. J. Owens, L. A. Barnard, H. Turner, D. Gyeltshen, N. Edward‐Inatimi, J. O’Donoghue, M. Lockwood, S. Watson, M. Rutala, C. M. Jackman, P. Riley   +10 more
doaj   +1 more source

The ap Prediction Tool Implemented by the A.Ne.Mo.S./NKUA Group

Atmosphere
A novel tool utilizing machine learning techniques was designed to forecast ap index values for the next three consecutive days (24 values). The tool employs time series data from the 3 h ap index of solar cycles 23 and 24 to train the Long Short-Term ...
Helen Mavromichalaki, Maria Livada, Argyris Stassinakis, Maria Gerontidou, Maria-Christina Papailiou, Line Drube, Aikaterini Karmi   +6 more
doaj   +1 more source

The source and engine of coronal mass ejections. [PDF]

Philos Trans A Math Phys Eng Sci, 2019
Georgoulis MK, Nindos A, Zhang H.
europepmc   +1 more source

Initiation Route of Coronal Mass Ejections. II. The Role of Filament Mass

The Astrophysical Journal
A thorough understanding of the initiation of coronal mass ejections (CMEs), which is manifested as a slow rise of pre-eruptive structures before the impulsive ejection in kinematics, is key for forecasting solar eruptions.
Chen Xing, Xin Cheng, Guillaume Aulanier, Mingde Ding   +3 more
doaj   +1 more source

Predicting the geoeffective properties of coronal mass ejections: current status, open issues and path forward. [PDF]

Philos Trans A Math Phys Eng Sci, 2019
Vourlidas A, Patsourakos S, Savani NP.
europepmc   +1 more source