Coronal and Interplanetary Propagation of CME/Shocks from Radio, In Situ and White‐Light Observations

2007 ◽  
Vol 663 (2) ◽  
pp. 1369-1385 ◽  
Author(s):  
M. J. Reiner ◽  
M. L. Kaiser ◽  
J.‐L. Bougeret
2018 ◽  
Vol 868 (2) ◽  
pp. 137 ◽  
Author(s):  
Ming Xiong ◽  
Jackie A. Davies ◽  
Xueshang Feng ◽  
Bo Li ◽  
Liping Yang ◽  
...  

2021 ◽  
Author(s):  
Manuela Temmer ◽  
Lukas Holzknecht ◽  
Mateja Dumbovic ◽  
Bojan Vrsnak ◽  
Nishtha Sachdeva ◽  
...  

<p>Using combined STEREO-SOHO white-light data, we present a method to determine the volume and density of a coronal mass ejection (CME) by applying the graduated cylindrical shell model (GCS) and deprojected mass derivation. Under the assumption that the CME  mass is roughly equally distributed within a specific volume, we expand the CME self-similarly and calculate the CME density for distances close to the Sun (15–30 Rs) and at 1 AU. The procedure is applied on a sample of 29 well-observed CMEs and compared to their interplanetary counterparts (ICMEs). Specific trends are derived comparing calculated and in-situ measured proton densities at 1 AU, though large uncertainties are revealed due to the unknown mass and geometry evolution: i) a moderate correlation for the magnetic structure having a mass that stays rather constant and ii) a weak correlation for the sheath density by assuming the sheath region is an extra mass - as expected for a mass pile-up process - that is in its amount comparable to the initial CME deprojected mass. High correlations are derived between in-situ measured sheath density and the solar wind density and solar wind speed as measured 24 hours ahead of the arrival of the disturbance. This gives additional confirmation that the sheath-plasma indeed stems from piled-up solar wind material. While the CME interplanetary propagation speed is not related to the sheath density, the size of the CME may play some role in how much material is piled up.</p>


1994 ◽  
Vol 1 (2) ◽  
pp. 75-78 ◽  
Author(s):  
S. Lam ◽  
C. Macaulay ◽  
J. C. Leriche ◽  
N. Ikeda ◽  
B. Palcic

The performance of a fluorescence imaging device was compared with conventional white-light bronchoscopy in 100 patients with lung cancer, 46 patients with resected stage I non-small cell lung cancer, 10 patients with head and neck cancer, and 67 volunteers who had smoked at least 1 pack of cigarettes per day for 25 years or more. Using differences in tissue autofluorescence between premalignant, malignant, and normal tissues, fluorescence bronchoscopy was found to detect significantly more areas with moderate/severe dysplasia or carcinoma in situ than conventional white-light bronchoscopy with a similar specificity. Multiple foci of dysplasia or cancer were found in 13–24% of these individuals. Fluorescence bronchoscopy may be an important adjunct to conventional bronchoscopic examination to improve our ability to detect and localize premalignant and early lung cancer lesions.


2012 ◽  
Vol 22 (3) ◽  
pp. 824-826 ◽  
Author(s):  
Zhi-yong Mao ◽  
Ying-chun Zhu ◽  
Lin Gan ◽  
Fang-fang Xu ◽  
Yang Wang ◽  
...  

2016 ◽  
Vol 4 (14) ◽  
pp. 2748-2751 ◽  
Author(s):  
Ankit Jain ◽  
Amritroop Achari ◽  
Muthuswamy Eswaramoorthy ◽  
Subi J. George

In this study, soft clay chromophore hybrids were used to demonstrate a photo-modification strategy, in which one white light standard can be converted into another via in situ generation of a blue emitting chromophore.


2005 ◽  
Vol 44 (22) ◽  
pp. 4693 ◽  
Author(s):  
Alexei Kiselev ◽  
Heike Wex ◽  
Frank Stratmann ◽  
Alexandre Nadeev ◽  
Dmitry Karpushenko

2016 ◽  
Vol 4 (7) ◽  
pp. 1134-1134
Author(s):  
Youssef Oulad-Zian ◽  
Juan Ramon Sanchez-Valencia ◽  
Manuel Oliva ◽  
Julian Parra-Barranco ◽  
Maria Alcaire ◽  
...  

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