Results 111 to 120 of about 1,069,804 (194)

The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field

The Astrophysical Journal
Kinematics of solar eruptive filaments is one of the important diagnostic parameters for predicting whether solar eruptions would induce geomagnetic storms.
Ye Qiu, Yang Guo, Mingde Ding, Chuan Li, Linggao Kong, Zhen Li   +5 more
doaj   +1 more source

Ultra-high-resolution observations of persistent null-point reconnection in the solar corona. [PDF]

Nat Commun, 2023
Cheng X, Priest ER, Li HT, Chen J, Aulanier G, Chitta LP, Wang YL, Peter H, Zhu XS, Xing C, Ding MD, Solanki SK, Berghmans D, Teriaca L, Aznar Cuadrado R, Zhukov AN, Guo Y, Long D, Harra L, Smith PJ, Rodriguez L, Verbeeck C, Barczynski K, Parenti S.   +23 more
europepmc   +1 more source

Large-scale Coronal Dimming Foreshadowing a Solar Eruption on 2011 October 1

The Astrophysical Journal
Understanding large-scale solar eruptions requires detailed investigation of the entire system’s evolution, including the magnetic environment enveloping the source region and searches for precursor activity prior to event onset.
Chunming Zhu, C. Richard DeVore, Joel T. Dahlin, Jiong Qiu, Maria D. Kazachenko, Vadim M. Uritsky, Jackson S. Vandervelde   +6 more
doaj   +1 more source

Diverse glasses revealed from Chang'E-5 lunar regolith. [PDF]

Natl Sci Rev, 2023
Zhao R, Shen L, Xiao D, Chang C, Huang Y, Yu J, Zhang H, Liu M, Zhao S, Yao W, Lu Z, Sun B, Bai H, Zou Z, Yang M, Wang W.   +15 more
europepmc   +1 more source

Data-driven modeling of solar coronal magnetic field evolution and eruptions. [PDF]

Innovation (Camb), 2022
Jiang C, Feng X, Guo Y, Hu Q.
europepmc   +1 more source

Flux Cancelation: The Key to Solar Eruptions [PDF]

, 2017
Solar coronal jets are magnetically channeled eruptions that occur in all types of solar environments (e.g. active regions, quiet-Sun regions and coronal holes).
Panesar, Navdeep K., Chakrapani, Prithi, Moore, Ronald, Sterling, Alphonse, Schmit, Don, Tiwari, Sanjiv, Innes, Davina   +6 more
core  

Defining the Middle Corona. [PDF]

Sol Phys, 2023
West MJ, Seaton DB, Wexler DB, Raymond JC, Del Zanna G, Rivera YJ, Kobelski AR, Chen B, DeForest C, Golub L, Caspi A, Gilly CR, Kooi JE, Meyer KA, Alterman BL, Alzate N, Andretta V, Auchère F, Banerjee D, Berghmans D, Chamberlin P, Chitta LP, Downs C, Giordano S, Harra L, Higginson A, Howard RA, Kumar P, Mason E, Mason JP, Morton RJ, Nykyri K, Patel R, Rachmeler L, Reardon KP, Reeves KK, Savage S, Thompson BJ, Van Kooten SJ, Viall NM, Vourlidas A, Zhukov AN.   +41 more
europepmc   +1 more source

Fracture mechanics of volcanic eruptions [PDF]

, 2009
Seismology is a key tool in the forecasting of volcanic eruptions. The onset of an eruption is often preceded and accompanied by an increase in local seismic activity, driven by fracturing within the edifice.
Matthews, C., Matthews, C
core  

High-resolution Observation and Magnetic Modeling of a Solar Minifilament: The Formation, Eruption, and Failing Mechanisms

The Astrophysical Journal
Minifilaments are widespread small-scale structures in the solar atmosphere. To better understand their formation and eruption mechanisms, we investigate the entire life of a sigmoidal minifilament located below a large quiescent filament observed by Big
Weilin Teng, Yingna Su, Rui Liu, Jialin Chen, Yanjie Liu, Jun Dai, Wenda Cao, Jinhua Shen, Haisheng Ji   +8 more
doaj   +1 more source

The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images. [PDF]

Sol Phys, 2023
Seaton DB, Berghmans D, Bloomfield DS, De Groof A, D'Huys E, Nicula B, Rachmeler LA, West MJ.   +7 more
europepmc   +1 more source