Results 171 to 180 of about 1,069,804 (194)

Solar prominences: theory and models: Fleshing out the magnetic skeleton. [PDF]

Living Rev Sol Phys, 2018
Gibson SE.
europepmc   +1 more source

Characterization of the Micro-Morphology and Compositional Distribution of Chang'e-5 Lunar Soil Mineral Surfaces Using TOF-SIMS. [PDF]

Adv Sci (Weinh)
Song T, Liu J, Zhang C, Yang X, Chen T, Jiang S, Xu F, Li N, Zhu M, Li S, Zou M.   +10 more
europepmc   +1 more source

Mass and Magnetic Field of Eruptive Solar Filaments

, 2016
openaire   +2 more sources

Re-Os geochronology for sulfides and organic-rich sediments. [PDF]

Natl Sci Rev
Li Y, Glorie S, Selby D.
europepmc   +1 more source

Apollo Next Generation Sample Analysis (ANGSA): an Apollo Participating Scientist Program to Prepare the Lunar Sample Community for Artemis. [PDF]

Space Sci Rev
Shearer CK, McCubbin FM, Eckley S, Simon SB, Meshik A, McDonald F, Schmitt HH, Zeigler RA, Gross J, Mitchell J, Krysher C, Morris RV, Parai R, Jolliff BL, Gillis-Davis JJ, Joy KH, Bell SK, Lucey PG, Sun L, Sharp ZD, Dukes C, Sehlke A, Mosie A, Allton J, Amick C, Simon JI, Erickson TM, Barnes JJ, Dyar MD, Burgess K, Petro N, Moriarty D, Curran NM, Elsila JE, Colina-Ruiz RA, Kroll T, Sokaras D, Ishii HA, Bradley JP, Sears D, Cohen B, Pravdivseva O, Thompson MS, Neal CR, Hana R, Ketcham R, Welten K, ANGSA science team.   +47 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Interplanetary shocks preceded by solar filament eruptions

Journal of Geophysical Research, 1986
We discuss the solar and interplanetary characteristics of six interplanetary shock and energetic particle events associated with the eruptions of solar filaments lying outside active regions. The events are characterized by the familiar double‐ribbon Hα brightenings observed with large flares, but only very weak soft X ray and microwave bursts.
H. V. Cane, S. W. Kahler, N. R. Sheeley
exaly   +2 more sources

Low-energy particle events and solar filament eruptions

Advances in Space Research, 1986
Over the period from August 1978 to October 1982, several large low-energy (E < 1.6 Mev) proton events associated with interplanetary travelling disturbances observed at 1 AU by ISEE-3, appeared not to be triggered by solar flares. Six of them can be associated with filament eruptions as the source of the disturbances.
B Sanahuja, V Domingo
exaly   +2 more sources

Eruption of a Bifurcated Solar Filament

Solar Physics, 2013
We study the partial eruption of a solar filament observed by the Solar Dynamics Observatory (SDO) and the Solar TErrestrial RElations Observatory-Ahead (STEREO-A) spacecraft on 9 May 2012. This filament was located in Active Region NOAA 11475 and consisted of two distinct branches, separated in height above the active region’s primary polarity ...
Chunming Zhu, David Alexander
openaire   +1 more source

Failed Eruptions of Solar Filaments

Astronomy Reports, 2020
Solar filaments (prominences), which suddenly and swiftly ascend, i.e., become eruptive, sometimes decelerate and stop at comparatively low altitudes. Causes of failed eruptions generally remain uncertain. The present study analyzes two eruptive phenomena with very similar initial geometries and configurations of external magnetic fields; one of these ...
openaire   +1 more source

The two types of flare-associated filament eruptions [PDF]

Solar Physics, 1986
Using years of high resolution solar footage obtained at Big Bear Solar Observatory flare associated filament eruptions were studied. In addition to the classical type eruption consisting of expansion and breakup, evidence was found of another type where
Tang, F.
exaly   +1 more source