SOTSP: HOP 320 w/IRIS, BBSO @ AR12578
2016-08-19T16:00:34 to 2016-08-19T16:44:02
Science Goal: Small-scale solar activities and their spectroscopic property
Program: Normal map 82"x82", Q65/Q75, 1 side
Target: MicroFlare
xcen=-262 ycen=9
Instrument: SOTSP
HOP/JOP: 320
Description:
abstract of observational proposal It is well accepted that the small-scale solar activities play important roles in heating the upper solar atmosphere, including the solar chromosphere and the solar corona (Li et al. 2007
Schmieder et al. 2013
Wang et al. 2014). Detailed study of the response of the upper solar atmosphere to small-scale flux emergence and the related changes of physical parameters will open a new window to investigate the heating mechanisms of the upper solar atmosphere. In this proposal, we would like to observe small-scale solar activities, such as small-scale emerging flux region (SEFR), Ellerman Bombs (EBs), jets, coronal bright points (CBPs) with the Interface Region Imaging Spectrometer (IRIS) together with Hinode and New Solar Telescope (NST) at Big Bear Solar Observatory (BBSO) in order to investigate the physical properties, spectroscopic characteristics and evolutions of these activities. request to SOT SP, Normal map mode FOV: 82"?82" Time cadence: 43 min Duration: 7 hours Data volume: 2833 Mbits
abstract of observational proposal It is well accepted that the small-scale solar activities play important roles in heating the upper solar atmosphere, including the solar chromosphere and the solar corona (Li et al. 2007
Schmieder et al. 2013
Wang et al. 2014). Detailed study of the response of the upper solar atmosphere to small-scale flux emergence and the related changes of physical parameters will open a new window to investigate the heating mechanisms of the upper solar atmosphere. In this proposal, we would like to observe small-scale solar activities, such as small-scale emerging flux region (SEFR), Ellerman Bombs (EBs), jets, coronal bright points (CBPs) with the Interface Region Imaging Spectrometer (IRIS) together with Hinode and New Solar Telescope (NST) at Big Bear Solar Observatory (BBSO) in order to investigate the physical properties, spectroscopic characteristics and evolutions of these activities. request to SOT SP, Normal map mode FOV: 82"?82" Time cadence: 43 min Duration: 7 hours Data volume: 2833 Mbits
wavelength: 6302A Continuum Intensity cadence: -1 min fov: 80,81 images: 510 JavaScript Landing Page
