The Formation of a Sunspot Penumbra Sector in Active Region NOAA 12574

2018 ◽  
Vol 857 (1) ◽  
pp. 21 ◽  
Author(s):  
Qiaoling Li ◽  
Xiaoli Yan ◽  
Jincheng Wang ◽  
DeFang Kong ◽  
Zhike Xue ◽  
...  
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.


2014 ◽  
pp. 335-348 ◽  
Author(s):  
A. Elmhamdi ◽  
P. Romano ◽  
A. S. Kordi ◽  
H. A. Al-trabulsy

2017 ◽  
Vol 57 (8) ◽  
pp. 978-987 ◽  
Author(s):  
V. E. Abramov-Maximov ◽  
V. N. Borovik ◽  
L. V. Opeikina ◽  
A. G. Tlatov ◽  
L. V. Yasnov

1989 ◽  
Vol 104 (2) ◽  
pp. 215-218
Author(s):  
Lin Yuanzhang ◽  
Zhang Hongqi ◽  
Han Feng ◽  
Liu Kening

AbstractIn this paper are described the simultaneously observational results of filtergrams, Dopplergrams and vector magnetograms for a solar flare in the active region NOAA/USAF -1862 on 7 Oct. 1987 with the solar telescope-magnctograph of Beijing Astronomical Observatory. From the analyses of these data, some conclusions were obtained.


2010 ◽  
Vol 720 (2) ◽  
pp. 1102-1107 ◽  
Author(s):  
Sung-Hong Park ◽  
Jongchul Chae ◽  
Ju Jing ◽  
Changyi Tan ◽  
Haimin Wang

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