Author name code: hashimoto
ADS astronomy entries on 2022-09-14
=author:"Hashimoto, Yuki" 
------------------------------------------------------------------------  

Title: Internal Fine Structure of Ellerman Bombs
Authors: Hashimoto, Yuki; Kitai, Reizaburo; Ichimoto, Kiyoshi; Ueno,
   Satoru; Nagata, Shin'ichi; Ishii, Takako T.; Hagino, Masaoki; Komori,
   Hiroyuki; Nishida, Keisuke; Matsumoto, Takuma; Otsuji, Kenichi;
   Nakamura, Tahei; Kawate, Tomoko; Watanabe, Hiroko; Shibata, Kazunari
Bibcode: 2010PASJ...62..879H
Altcode:
  We conducted coordinated observations of Ellerman bombs (EBs) between
  Hinode Satellite and Hida Observatory (HOP12). CaII H broad-band
  filter images of NOAA 10966 on 2007 August 9 and 10 were obtained
  with the Solar Optical Telescope (SOT) aboard the Hinode Satellite,
  and many bright points were observed. We identified a total of 4
  bright points as EBs, and studied the temporal variation of their
  morphological fine structures and spectroscopic characteristics. With
  high-resolution CaII H images of SOT, we found that the EBs, thus far
  thought of as single bright features, are composed of a few of fine
  subcomponents. Also, by using Stokes I/V filtergrams with Hinode/SOT,
  and CaII H spectroheliograms with Hida/Domeless Solar Telescope (DST),
  our observation showed: (1) The mean duration, the mean width, the
  mean length, and the mean aspect ratio of the subcomponents were
  390 s, 170 km, 450 km, and 2.7, respectively. (2) Subcomponents
  started to appear on the magnetic neutral lines, and extended their
  lengths from the original locations. (3) When the CaII H line of EBs
  showed the characteristic blue asymmetry, they are associated with the
  appearance or re-brightening of subcomponents. Summarizing our results,
  we obtained an observational view that elementary magnetic reconnections
  take place one by one successively and intermittently in EBs, and that
  their manifestation is the fine subcomponents of the EB phenomena.