High resolution observation of H? solar flares and temporal relation between H? and X-ray, microwave emission

1986 ◽  
Vol 118 (1-2) ◽  
pp. 149-152 ◽  
Author(s):  
H. Kurokawa ◽  
T. Kitahara ◽  
Y. Nakai ◽  
Y. Funakoshi ◽  
K. Ichimoto
Keyword(s):  
High Resolution ◽  
Solar Flares ◽  
Temporal Relation ◽  
Microwave Emission ◽  
X Ray ◽  
Resolution Observation ◽  
High Resolution Observation

scholarly journals High-resolution Observation of Steel Using X-ray Tomography Technique

2012 ◽  
Vol 52 (3) ◽  
pp. 516-521 ◽  
Author(s):  
Hiroyuki Toda ◽  
Fukuto Tomizato ◽  
Frank Zeismann ◽  
Yasuko Motoyashiki-Besel ◽  
Kentaro Uesugi ◽  
...  
Keyword(s):  
High Resolution ◽  
X Ray ◽  
Resolution Observation ◽  
High Resolution Observation

scholarly journals Hydrodynamic Models of Solar and Stellar Flares

1989 ◽  
Vol 104 (1) ◽  
pp. 289-298
Author(s):  
Giovanni Peres
Keyword(s):  
High Resolution ◽  
Light Curve ◽  
Solar Flares ◽  
Impulsive Phase ◽  
Light Curves ◽  
Physical Parameters ◽  
The Sun ◽  
Hydrodynamic Models ◽  
X Ray ◽  
Stellar Flares

AbstractThis paper discusses the hydrodynamic modeling of flaring plasma confined in magnetic loops and its objectives within the broader scope of flare physics. In particular, the Palermo-Harvard model is discussed along with its applications to the detailed fitting of X-ray light curves of solar flares and to the simulation of high-resolution Caxix spectra in the impulsive phase. These two approaches provide complementary constraints on the relevant features of solar flares. The extension to the stellar case, with the fitting of the light curve of an X-ray flare which occurred on Proxima Centauri, demonstrates the feasibility of using this kind of model for stars too. Although the stellar observations do not provide the wealth of details available for the Sun, and, therefore, constrain the model more loosely, there are strong motivations to pursue this line of research: the wider range of physical parameters in stellar flares and the possibility of studying further the solar-stellar connection.

Application of K-FADOF in Solar High-Resolution Observation

2012 ◽  
Vol 39 (8) ◽  
pp. 0808003
Author(s):  
张俊 Zhang Jun ◽  
杨勇 Yang Yong ◽  
程学武 Cheng Xuewu ◽  
杨尚斌 Yang Shangbin ◽  
龚威 Gong Wei
Keyword(s):  
High Resolution ◽  
Resolution Observation ◽  
High Resolution Observation

High resolution observation of 3C 66B

1992 ◽  
Author(s):  
W. B. Sparks ◽  
F. Macchetto ◽  
N. J. Jackson ◽  
G. K. Miley
Keyword(s):  
High Resolution ◽  
Resolution Observation ◽  
High Resolution Observation

In Situ High-Resolution Observation for Decomposition of NaAlH4

2007 ◽  
pp. 1621-1624
Author(s):  
Hiroshi Kawasaki ◽  
Somei Ohnuki ◽  
Takanori Suda ◽  
Naoyuki Hashimoto ◽  
Yoshitsugu Kojima
Keyword(s):  
High Resolution ◽  
Resolution Observation ◽  
High Resolution Observation

Iue high-resolution observation of the Venus dayglow spectrum 1280-1380 Å

1981 ◽  
Vol 8 (1) ◽  
pp. 111-112 ◽  
Author(s):  
Samuel T. Durrance ◽  
Robert R. Conway ◽  
Charles A. Barth ◽  
A. L. Lane
Keyword(s):  
High Resolution ◽  
Resolution Observation ◽  
High Resolution Observation
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