Results 111 to 120 of about 15,087 (215)

CORONAL MASS EJECTIONS AND SUNSPOTS—SOLAR CYCLE PERSPECTIVE

The Astrophysical Journal, 2010
Recent studies have indicated that the occurrence of the maxima of coronal mass ejection (CME) rate and sunspot number (SSN) were nearly two years apart. We find that the two-year lag of CME rate manifests only when the SSN index is considered and the lag is minimal (two-three months) when the sunspot area is considered.
openaire   +1 more source

Transport in the interplanetary medium of coronal mass ejections [PDF]

Geofísica Internacional, 2008
Coronal mass ejections (CMEs) are large scale structures of plasma and magnetic field expelled from the Sun to the interplanetary medium and generally observed in white light coronagraphs.
A. Ventura, A. Lara, A. Borgazzi
doaj  

Workshop on Solar Activity, Solar Wind, Terrestrial Effects, and Solar Acceleration [PDF]

A summary of the proceedings from the workshop are presented. The areas covered were solar activity, solar wind, terrestrial effects, and solar acceleration.

core   +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

Comparative Analysis of Properties of Coronal Mass Ejections at High and Low Apparent Latitudes in 1996–2025

The Astrophysical Journal
This study examines the statistical properties of coronal mass ejections (CMEs) over two and a half solar cycles (1996–2025) using coronal observations from the SOHO LASCO CDAW and CACTus catalogs, supplemented by sunspot number records and in situ ...
Olga Khabarova, Nuran Samara, Noam Tishler, Hadar Reshef, Colin Price   +4 more
doaj   +1 more source

Modeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory. [PDF]

Space Weather, 2017
Möstl C, Isavnin A, Boakes PD, Kilpua EKJ, Davies JA, Harrison RA, Barnes D, Krupar V, Eastwood JP, Good SW, Forsyth RJ, Bothmer V, Reiss MA, Amerstorfer T, Winslow RM, Anderson BJ, Philpott LC, Rodriguez L, Rouillard AP, Gallagher P, Nieves-Chinchilla T, Zhang TL.   +21 more
europepmc   +1 more source

Observing Solar Coronal Mass Ejections from Space

5 pages, 2 figures.
openaire   +3 more sources

Characterizing Coronal Mass Ejections in Solar Cycle Analysis

, 2018
The Sun is the major source of heat and light in our solar system. The solar cycle is the 11-year cycle of solar activity that can be determined by the rise and fall in the numbers and surface area of sunspots. Solar activity is associated with several factors including radio flux, solar irradiance, magnetic field, solar flares, coronal mass ejections,
openaire   +2 more sources