Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Patricia R. Jibben"'
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 3 (2016)
Coronal cavities are regions of low coronal emission that usually sit above solar prominences. These systems can exist for days or months before erupting. The magnetic structure of the prominence-cavity system during the quiescent period is important
Externí odkaz:
https://doaj.org/article/519973d7dfee42f5b24037a761816ab9
Autor:
Yingjie Zhu, Yu Liang, Jingwen Zhang, Zhong Yue, Patricia R. Jibben, Zihao Yang, Yingna Su, Linhua Deng, Tanmoy Samanta, Yajie Chen, Hui Tian, Linghua Wang, Zhongquan Qu, Jiansen He
We present an investigation of a coronal cavity observed above the western limb in the coronal red line Fe X 6374 {\AA} using a telescope of Peking University and in the green line Fe XIV 5303 {\AA} using a telescope of Yunnan Observatories, Chinese
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::079b9bdc324219d6eb27325251520aac
http://arxiv.org/abs/1802.04432
http://arxiv.org/abs/1802.04432
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 3 (2016)
Coronal cavities are regions of low coronal emission that usually sit above solar prominences. These systems can exist for days or months before erupting. The magnetic structure of the prominence-cavity system during the quiescent period is important
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6d2db75ee4924d55cea95ae075f9983
http://journal.frontiersin.org/Journal/10.3389/fspas.2016.00010/full
http://journal.frontiersin.org/Journal/10.3389/fspas.2016.00010/full
Autor:
Kiyoto Shibasaki, Patricia R. Jibben, Alphonse C. Sterling, Thomas E. Berger, David Alan Myers, Ryohei Kano, Taro Sakao, Richard A. Shine, Monica G. Bobra, Loraine L. Lundquist, John M. Davis, Noriyuki Narukage, Theodore D. Tarbell, Ronald L. Moore, Mark Weber
Publikováno v:
PASJ: Publications of the Astronomical Society of Japan. 59(SP3):823-829
著者人数：15名
Accepted: 2007-09-11
資料番号: SA1000268000
Accepted: 2007-09-11
資料番号: SA1000268000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2f3a7654e202f9bd74ac52940db0bed
http://id.nii.ac.jp/1696/00023589/
http://id.nii.ac.jp/1696/00023589/
Publikováno v:
The Astrophysical Journal. 807:97
In this paper we study the soft X-ray (SXR) signatures of one particular prominence. The X-ray observations used here were made by the Hinode/XRT instrument using two different filters. Both of them have a pronounced peak of the response function aro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4b2e80012899f76082ef727d19bebb7
https://doi.org/10.1088/0004-637x/807/1/97
https://doi.org/10.1088/0004-637x/807/1/97
Autor:
Yajie Chen, Hui Tian, Yingna Su, Zhongquan Qu, Linhua Deng, Patricia R. Jibben, Zihao Yang, Jingwen Zhang, Tanmoy Samanta, Jiansen He, Linghua Wang, Yingjie Zhu, Yue Zhong, Yu Liang
Publikováno v:
Astrophysical Journal; 3/20/2018, Vol. 856 Issue 1, p1-1, 1p