SOTSP: HOP277 (polarimetry w/DST)
2015-03-06T15:18:38 to 2015-03-06T16:45:57
Science Goal: Imaging Spectropolarimetry in He I 1083.0 nm at the DST
Program: Fast deep map 250x165", 1 side, Q65
Target: Active Region
xcen=-408 ycen=-77
Instrument: SOTSP
HOP/JOP: 277
Description:
Magnetism in the solar chromosphere is structured on all spatial scales. EUV imagery from the Solar Dynamics Observatory (SDO) show clearly the complex interconnectivity of the magnetic field over large distances between active regions and the quiet-Sun net- work. The ChroMag full-disk imaging polarimeter is designed to diagnose chromospheric magnetic field in a synoptic fashion. At the very finest resolution, we find dynamic features such as spicules, mottles, and fibrils (for a review see, e.g., Tsiropoula et al. 2012). High-resolution instruments like the Interferometric Bidimensional Spectrometer (IBIS) on the Dunn Solar Telescope (DST) are shedding light on the complex environment of the chromosphere. These instruments typically observe the H? line at 656.3 nm and the Ca ii line at 854.2 nm. The He i line at 1083.0 nm has been largely neglected by imaging polarimeters. However, this line is known to be a powerful diagnostic of chromospheric magnetic field (see recent works by,e.g.,Orozco Suaand#769
rez et al. 2014, Schad et al. 2013, Kuckein et al. 2012, Centeno et al. 2010). It is often observed using traditional spectrographs such as SPINOR and FIRS at the DST that must sacrifice spatial information and temporal cadence to achieve high spectral resolution and signal to noise. We propose to address the lack of polarimetric observations with high cadence and high spatial resolution in the He i line at 1083.0 nm by using the ChroMag Lyot filter-polarimeter that has an operating wavelength range of 580 nm to 1100 nm at the DST. Our goals are to observe active regions, filaments, prominences, and spicules at the diffraction limit of the DST with high cadence and signal-to-noise adequate for the application of spectro-polarimetric inversion codes. In addition to providing data for studies of chromospheric magnetism, these obser- vations will function as a proof-of-concept for future instruments such as the planned Japanese SOLAR-C mission that is to have a filter-polarimeter with specifications not dissimilar from the ChroMag Lyot filter.
Magnetism in the solar chromosphere is structured on all spatial scales. EUV imagery from the Solar Dynamics Observatory (SDO) show clearly the complex interconnectivity of the magnetic field over large distances between active regions and the quiet-Sun net- work. The ChroMag full-disk imaging polarimeter is designed to diagnose chromospheric magnetic field in a synoptic fashion. At the very finest resolution, we find dynamic features such as spicules, mottles, and fibrils (for a review see, e.g., Tsiropoula et al. 2012). High-resolution instruments like the Interferometric Bidimensional Spectrometer (IBIS) on the Dunn Solar Telescope (DST) are shedding light on the complex environment of the chromosphere. These instruments typically observe the H? line at 656.3 nm and the Ca ii line at 854.2 nm. The He i line at 1083.0 nm has been largely neglected by imaging polarimeters. However, this line is known to be a powerful diagnostic of chromospheric magnetic field (see recent works by,e.g.,Orozco Suaand#769
rez et al. 2014, Schad et al. 2013, Kuckein et al. 2012, Centeno et al. 2010). It is often observed using traditional spectrographs such as SPINOR and FIRS at the DST that must sacrifice spatial information and temporal cadence to achieve high spectral resolution and signal to noise. We propose to address the lack of polarimetric observations with high cadence and high spatial resolution in the He i line at 1083.0 nm by using the ChroMag Lyot filter-polarimeter that has an operating wavelength range of 580 nm to 1100 nm at the DST. Our goals are to observe active regions, filaments, prominences, and spicules at the diffraction limit of the DST with high cadence and signal-to-noise adequate for the application of spectro-polarimetric inversion codes. In addition to providing data for studies of chromospheric magnetism, these obser- vations will function as a proof-of-concept for future instruments such as the planned Japanese SOLAR-C mission that is to have a filter-polarimeter with specifications not dissimilar from the ChroMag Lyot filter.
wavelength: 6302A Continuum Intensity cadence: 0 min fov: 236,162 images: 749 JavaScript Landing Page
