Results 71 to 80 of about 1,134 (135)

Coronal mass ejections and their geoeffectiveness [PDF]

, 1998
43-46Coronal Mass Ejections (CMEs) which are vast structures of solar plasma and magnetic field expelled from the sun into the heliosphere, produce large inter-planetary and geomagnetic disturbances.
Dubey, S C
core  

DETERMINING THE MAGNETIC FIELD ORIENTATION OF CORONAL MASS EJECTIONS FROM FARADAY ROTATION

, 2007
We describe a method with which to measure the magnetic field orientation of coronal mass ejections (CMEs) using Faraday rotation (FR). Two basic FR profiles, Gaussian-shaped with a single polarity or N-shaped with polarity re-versals, are produced by a ...
J. W. Belcher, J. D. Richardson, J. C. Kasper, Y. Liu, W. B. Manchester Iv   +4 more
core  

A Model for Flux Rope Formation and Disconnection in Pseudostreamer Coronal Mass Ejections

Coronal mass ejections (CMEs) from pseudostreamers represent a significant fraction of large-scale eruptions from the Sun. In some cases, these CMEs take a narrow jet-like form reminiscent of coronal jets; in others, they have a much broader fan-shaped ...
B. J. Lynch, L. K. S. Daldorff, S. K. Antiochos, Wyper, P. F., DeVore, C. R., P. F. Wyper, C. R. DeVore, Lynch, B. J., Kumar, P., Daldorff, L. K. S., Antiochos, S. K., P. Kumar   +11 more
core   +1 more source

Coronal Mass Ejections Near the Sun and in the Interplanetary Medium

, 2012
Coronal mass ejections (CMEs) are the most energetic phenomenon in the heliosphere. During solar eruptions, the released energy flows out from the Sun in the form of magnetized plasma and electromagnetic radiation.
Gopalswamy, Nat
core  

The Relation between Coronal Holes and Coronal Mass Ejections during the Rise, Maximum, and Declining Phases of Solar Cycle 23

, 2012
We study the interaction between coronal holes (CHs) and coronal mass ejections (CMEs) using a resultant force exerted by all the coronal holes present on the disk and is defined as the coronal hole influence parameter (CHIP). The CHIP magnitude for each
Akiyama, S., Mohamed, A. A., Makela, P., Xie, H., Jung, H., Gopalswamy, N, Yashiro, S.   +6 more
core  

Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]

Sol Phys
Martinez Oliveros JC, Krupar V, Ervin T, Krucker S, Pulupa M, Badman ST, Buitrago Casas JC, Mondal S, Bale SD.   +8 more
europepmc   +1 more source

Simulating high-speed solar wind streams from coronal holes using an L5-L1 configuration of lagrangian points. [PDF]

Sci Rep
Podladchikova T, Veronig AM, Temmer M, Hofmeister SJ.   +3 more
europepmc   +1 more source

Observations of a Solar Energetic Particle Event From Inside and Outside the Coma of Comet 67P. [PDF]

J Geophys Res Space Phys, 2022
Wellbrock A, Jones GH, Dresing N, Coates AJ, Simon Wedlund C, Nilsson H, Sanchez-Cano B, Palmerio E, Turc L, Myllys M, Henri P, Goetz C, Witasse O, Nordheim TA, Mandt K.   +14 more
europepmc   +1 more source

FlareDB: A Database of Significant Flares in Solar Cycles 24 and 25 with SDO/HMI and SDO/AIA Observations. [PDF]

Sci Data
Liu N, Abduallah Y, Kapure TS, Li Q, Wang H, Wang JTL.   +5 more
europepmc   +1 more source

Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]

Space Sci Rev
Kubyshkina D, Way MJ, Dandouras I, Lammer H, Lanza AF, Lingam M, Nakamura R, Persson M, Scherf M, Seki K.   +9 more
europepmc   +1 more source