Results 51 to 60 of about 959 (179)
Abstract We introduce a new solar feed for the PEPSI nighttime spectrograph of the LBT. It enables spectroscopy of the Sun‐as‐a‐star in circular polarization (CP) and linear polarization (LP) with a spectral resolution of 250,000 (≈0.025Å or 600ms−1$$ 600\kern0.1em \mathrm{m}\kern0.1em {\mathrm{s}}^{-1} $$) for the wavelength range 383–907 nm.
Klaus G. Strassmeier +13 more
wiley +1 more source
Atomic Scale Structure of Self‐Assembled Lipidated Peptide Nanomaterials
A bottom‐up theoretical approach is reported to produce the first atomically resolved experimentally consistent model of lipidated β‐peptide nanomaterials. The β‐peptide materials possess long‐term mechanical and chemical stability in vivo, and may be easily decorated with combinations of different biological cues. This unique combination of properties
Billy J. Williams‐Noonan +8 more
wiley +1 more source
We analyze near-infrared integral field spectropolarimetry of the AB Aurigae protoplanetary disk and protoplanet (AB Aur b), obtained with SCExAO/CHARIS in 22 wavelength channels covering the J , H , and K passbands ( λ _0 = 1.1–2.4 μ m) over angular ...
Erica Dykes +23 more
doaj +1 more source
Spiropyran‐Based Photoisomerizable α‐Amino Acid for Membrane‐Active Peptide Modification
A spiropyran‐derived α‐amino acid was carefully designed for the synthesis of photocontrollable bioactive peptides. Dramatic changes in structure and polarity occurring upon light exposure or dark adaptation of the spiropyran side chain can cause changes in the behavior of peptides in lipid membranes and living cells, as demonstrated on spiropyran ...
Andrii Hrebonkin +12 more
wiley +1 more source
The CHARA Array Polarization Model and Prospects for Spectropolarimetry
Polarimetric data provide key insights into infrared emission mechanisms in the inner disks of young stellar objects (YSOs) and the details of dust formation around asymptotic giant branch (AGB) stars. While polarization measurements are well-established
Linling Shuai +7 more
doaj +1 more source
Full-disk measurements of the solar magnetic field by the Helioseismic and Magnetic Imager (HMI) are often used for magnetic field extrapolations, but its limited spatial and spectral resolution can lead to significant errors.
C. Beck +5 more
doaj +1 more source
Spectropolarimetry and the Study of Circumstellar Disks [PDF]
Circumstellar disks play an important role in many stages of the evolution of stars. However, it is only possible to directly image circumstellar disks for a few of the nearest stars. For massive stars, the situation is even more difficult, as they are on average further away than the more numerous low mass stars.
openaire +2 more sources
We present high-resolution observations of a C4.1-class solar flare (SOL2023-05-03T20:53) in AR 13293 from the Visible Spectro-Polarimeter (ViSP) and Visible Broadband Imager (VBI) instruments at the DKIST.
Rahul Yadav +4 more
doaj +1 more source
Spectropolarimetry of Fraunhofer Lines in Local Upper Solar Atmosphere
Spectropolarimetric results of Fraunhofer lines between 516.3 and 532.6 nm are presented in local upper solar chromosphere and inner corona below a height of about 0.04 solar radius above the solar limb. The data were acquired on 2013 November 3 during a
Z. Q. Qu +8 more
doaj +1 more source
Infrared spectropolarimetry of a C-class solar flare footpoint plasma
We performed high-spatial-resolution spectropolarimetric observations of the active region NOAA 13363 during a C-class flare with the Gregor Infrared Spectrograph (GRIS) on 16 July 2023.
Vashalomidze Z. +12 more
doaj +1 more source

