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High-cadence, synchronized, multiwavelength optical observations of a solar active region (NOAA 10794) are presented. The data were obtained with the Dunn Solar Telescope at the National Solar Observatory/Sacramento Peak using a newly…

天体物理学 · 物理学 2009-11-13 D. B. Jess , A. Andic , M. Mathioudakis , D. S. Bloomfield , F. P. Keenan

We analyse the multiwavelength observations of an M2.9/1N flare that occurred in the active region (AR) NOAA 11112 in the vicinity of a huge filament system on 16 October 2010. SDO/HMI magnetograms reveal the emergence of a bipole (within…

太阳与恒星天体物理 · 物理学 2015-06-11 Pankaj Kumar , Sung-Hong Park , K. -S. Cho , S. -C. Bong

We report the detection of oscillatory phenomena associated with a large bright-point group that is 430,000 square kilometers in area and located near the solar disk center. Wavelet analysis reveals full-width half-maximum oscillations with…

太阳与恒星天体物理 · 物理学 2009-11-13 D. B. Jess , M. Mathioudakis , R. Erdelyi , P. J. Crockett , F. P. Keenan , D. J. Christian

Magnetic flux tubes in the solar wind can be twisted as they are transported from the solar surface, where the tubes are twisted owing to photospheric motions. It is suggested that the twisted magnetic tubes can be detected as the variation…

太阳与恒星天体物理 · 物理学 2015-06-18 Teimuraz Zaqarashvili , Zoltán Vörös , Yasuhito Narita , Roberto Bruno

Sunspot proper motions and flares of a super active region NOAA 5395, which was the biggest and the most flare-active region in the 22nd sunspot cycle, were analyzed in details. We measured sunspot proper motions by using the H-alpha - 5.0…

天体物理学 · 物理学 2009-10-30 Takako T. Ishii , Hiroki Kurokawa , Tsutomu T. Takeuchi

Combining the Solar Dynamics Observatory and the New Vacuum Solar Telescope observations, we study a confined flare triggered by a rising flux rope within the trailing sunspots of active region 12733. The flux rope lying above the sheared…

太阳与恒星天体物理 · 物理学 2019-06-19 Shuhong Yang , Jun Zhang , Qiao Song , Yi Bi , Ting Li

We present an analysis of twisting motions in penumbral filaments in sunspots located at heliocentric angles from $30^\circ$ to $48^\circ$ using three time series of blue continuum images obtained by the Broadband Filter Imager (BFI)…

太阳与恒星天体物理 · 物理学 2015-05-19 Lokesh Bharti , Sami K. Solanki , Johann Hirzberger

In this study, we investigate motions in the hot plasma above the flare loops during the 2017 September 10 X8.2 flare event. We examine the region to the south of the main flare arcade, where there is data from the Interface Region Imaging…

太阳与恒星天体物理 · 物理学 2021-01-06 Katharine K. Reeves , Vanessa Polito , Bin Chen , Giselle Galan , Sijie Yu , Wei Liu , Gang Li

A broad jet was observed in a weak magnetic field area at the edge of active region NOAA 11106. The peculiar shape and magnetic environment of the broad jet raised the question of whether it was created by the same physical processes of…

We aim to ascertain the physical parameters of a propagating wave over the solar disk detected by the Interface Region Imaging Spectrograph (IRIS). Using imaging data from the IRIS and the Solar Dynamic Observatory (SDO), we tracked bright…

太阳与恒星天体物理 · 物理学 2018-03-21 B. Zhang , Y. J. Hou , J. Zhang

We present the first observations of chromospheric swirls using the Hydrogen-alpha Rapid Dynamics camera and Rapid Oscillations in the Solar Atmosphere imaging instruments at the Dunn Solar Telescope. These vortices contribute to heating…

太阳与恒星天体物理 · 物理学 2025-09-18 Oana Vesa , Juie Shetye , Erwin Verwichte

Using high-resolution observations from the 1.6 m New Solar Telescope (NST) operating at the Big Bear Solar Observatory (BBSO), we report direct evidence of merging/reconnection of cool H$\alpha$ loops in the chromosphere during two…

太阳与恒星天体物理 · 物理学 2017-07-05 Pankaj Kumar , Vasyl Yurchyshyn , Kyung-Suk Cho , Haimin Wang

Hot flow anomalies (HFAs) are studied using observations of the RAPID suprathermal charged particle detector, the FGM magnetometer, and the CIS plasma detector aboard the four Cluster spacecraft. Previously, we studied several specific…

We firstly report the simultaneous activities of a slipping motion of flare loops and a slipping eruption of a flux rope in 131 {\AA} and 94 {\AA} channels on 2014 February 02. The east hook-like flare ribbon propagated slippingly at a…

太阳与恒星天体物理 · 物理学 2015-06-22 Ting Li , Jun Zhang

Multi-wavelength observations of an M 2.0 flare event on 2000 March 23 in NOAA active region 8910 provide us a good chance to study the detailed structure and dynamics of the magnetic reconnection region. In the process of the flare,…

太阳与恒星天体物理 · 物理学 2015-05-13 Leping Li , Jun Zhang

The high spatial and time resolution data obtained with SDO/AIA for the sunspot in active region NOAA 11131 on 08 December 2010 were analysed with the time-distance plot technique and the pixelised wavelet filtering method. Oscillations in…

太阳与恒星天体物理 · 物理学 2014-09-17 R. Sych , V. M. Nakariakov

We analyse multiwavelength observations of a western limb flare (C3.9) occurred in AR NOAA 111465 on 30 April 2012. The high resolution images recorded by SDO/AIA 304, 1600 \AA\ and Hinode/SOT H$\alpha$ show the activation of a…

太阳与恒星天体物理 · 物理学 2014-12-03 Pankaj Kumar , Kyung-Suk Cho

A small flare ribbon above a sunspot umbra in active region 12205 was observed on November 7, 2014, at 12:00 UT in the blue imaging channel of the 1.5 m GREGOR telescope, using a 1 A Ca II H interference filter. Context observations from…

With the high tempo-spatial \emph{Interface Region Imaging Spectrograph} 1330 {\AA} images, we find that many bright structures are rooted in the light bridge of NOAA 12192, forming a \emph{light wall}. The light wall is brighter than the…

太阳与恒星天体物理 · 物理学 2015-05-20 Shuhong Yang , Jun Zhang , Fayu Jiang , Yongyuan Xiang

We analyse the 30 October, 2004, X1.2/SF solar event that occurred in AR 10691 (N13 W18) at around 11:44 UT. Observations at 212 and 405 GHz of the Solar Submillimeter Telescope (SST), with high time resolution (5 ms), show an intense…

天体物理学 · 物理学 2008-11-26 G. Cristiani , C. G. Giménez de Castro , M. L. Luoni , C. H. Mandrini , M. G. Rovira , P. Kaufmann
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