scholarly journals TIME EVOLUTION OF CORONAL MAGNETIC HELICITY IN THE FLARING ACTIVE REGION NOAA 10930

2010 ◽  
Vol 720 (2) ◽  
pp. 1102-1107 ◽  
Author(s):  
Sung-Hong Park ◽  
Jongchul Chae ◽  
Ju Jing ◽  
Changyi Tan ◽  
Haimin Wang
2003 ◽  
Vol 32 (10) ◽  
pp. 1949-1952 ◽  
Author(s):  
T. Yokoyama ◽  
K. Kusano ◽  
T. Maeshiro ◽  
T. Sakurai

2011 ◽  
Vol 530 ◽  
pp. A36 ◽  
Author(s):  
F. P. Zuccarello ◽  
P. Romano ◽  
F. Zuccarello ◽  
S. Poedts

Solar Physics ◽  
2014 ◽  
Vol 290 (2) ◽  
pp. 491-506 ◽  
Author(s):  
G. Valori ◽  
P. Romano ◽  
A. Malanushenko ◽  
I. Ermolli ◽  
F. Giorgi ◽  
...  

2013 ◽  
Vol 778 (1) ◽  
pp. 13 ◽  
Author(s):  
Sung-Hong Park ◽  
Kanya Kusano ◽  
Kyung-Suk Cho ◽  
Jongchul Chae ◽  
Su-Chan Bong ◽  
...  

2020 ◽  
Vol 36 (3) ◽  
pp. 69-90
Author(s):  
S. N. Chornogor ◽  
◽  
N. N. Kondrashova ◽  

2020 ◽  
Vol 60 (7) ◽  
pp. 936-941
Author(s):  
M. I. Savchenko ◽  
P. V. Vatagin ◽  
P. B. Dmitriev ◽  
M. G. Ogurtsov ◽  
E. M. Kruglov ◽  
...  

2006 ◽  
Vol 50 (8) ◽  
pp. 679-686 ◽  
Author(s):  
N. G. Peterova ◽  
B. V. Agalakov ◽  
T. P. Borisevich ◽  
A. N. Korzhavin ◽  
B. I. Ryabov

2018 ◽  
Vol 13 (S340) ◽  
pp. 155-156
Author(s):  
T. G. Priya ◽  
Jiangtao Su ◽  
Robertus Erd̎elyi

AbstractThe earlier work on the oscillatory phenomena in sunspot structures have supported in validating the detection of long-period oscillations, which are generated by the photospheric umbral response to the five minute p-mode global oscillations. We report here on the events of 3- min umbral oscillations which are detected within a duration of one hour from a single-polarity sunspot of active region NOAA 12132. The umbral oscillations that appear first around umbral boundaries is speculated to be excited by the wavefronts at the umbral-penumbral boundaries due to sub-photospheric or photospheric granular buffetings. The appearance of the wavefronts in spiral structures suggests that the wave guides are twisted. In addition, the newly formed running penumbral waves (RPWs) appears to be connected with the preceding RPWs.


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