Results 1 to 10 of about 62,110 (306)

Coronal Balance vs. Sagittal Profile in Adolescent Idiopathic Scoliosis, Are They Correlated?

Frontiers in Pediatrics, 2019
Muhammad Ali, Lihua Zhao, Sun Wang
exaly  

Source regions and storm effectiveness of frontside full halo coronal mass ejections

Journal of Geophysical Research, 2003
exaly  

Root surface and coronal caries in adults with type 2 diabetes mellitus

Community Dentistry and Oral Epidemiology, 2007
exaly  

Acceleration of the solar wind as a result of the reconnection of open magnetic flux with coronal loops

Journal of Geophysical Research, 2003
exaly  

Can computed tomography with coronal reconstruction improve the diagnosis of choledocholithiasis?

Journal of Gastroenterology and Hepatology (Australia), 2008
exaly  

Coronal tooth structure in root‐treated teeth prepared for complete and partial coverage restorations

Journal of Oral Rehabilitation, 2009
exaly  

The Birth of A Coronal Mass Ejection [PDF]

Science Advances, 2019
The Sun's atmosphere is frequently disrupted by coronal mass ejections (CMEs), coupled with flares and energetic particles. In the standard picture, the coupling is explained by magnetic reconnection at a vertical current sheet connecting the flare loops
Gou, Tingyu, Kliem, Bernhard, Liu, Rui, Veronig, Astrid M., Wang, Yuming   +4 more
core   +9 more sources

Planar magnetic structures in coronal mass ejection-driven sheath regions [PDF]

Annales Geophysicae, 2016
Planar magnetic structures (PMSs) are periods in the solar wind during which interplanetary magnetic field vectors are nearly parallel to a single plane.
E. Palmerio, E. K. J. Kilpua, N. P. Savani, N. P. Savani   +3 more
doaj   +3 more sources

Reconnection in a slow Coronal Mass Ejection [PDF]

Annales Geophysicae, 2008
Abstract. This paper aims at studying reconnection occurring in the aftermath of the 28 May 2004, CME, first imaged by the LASCO (Large Angle and Spectrometric Coronagraph) C2 at 11:06 UT. The CME was observed in White Light and UV radiation: images acquired by the LASCO C2 and C3 coronagraphs and spectra acquired by UVCS (Ultraviolet Coronagraph ...
G. Poletto, A. Bemporad, F. Landini, ROMOLI, MARCO   +3 more
openaire   +3 more sources

Source Regions of Coronal Mass Ejections [PDF]

Symposium - International Astronomical Union, 2001
Observations of the solar corona with the LASCO and EIT instruments on SOHO provide an unprecedented opportunity to study coronal mass ejections (CMEs) from their initiation through their evolution out to 30 R⊙. The objective of this study is to gain an understanding of the source regions from which the CMEs emanate.
Prasad Subramanian, Prasad Subramanian, Kenneth P. Dere   +2 more
  +8 more sources