[HTML][HTML] Magnetospheric accretion in the intermediate-mass T Tauri star HQ Tauri

K Pouilly, J Bouvier, E Alecian, SHP Alencar… - Astronomy & …, 2020 - aanda.org
… Indeed, we verified that the ASAS-SN g-band and V-band … averaged them and computed
the rms dispersion, and then removed the … of the longitudinal component of the magnetic field, …

The rotationally modulated polarization of ξ Boo A

DV Cotton, D Evensberget, SC Marsden… - Monthly Notices of …, 2019 - academic.oup.com
… with the maximum global longitudinal magnetic field (|B ℓ | max ) … nm) is similar to that of the
gband (472.4 nm); however, … estimate only 10–20 are bright enough to be accessible from …

[HTML][HTML] Cavity-enhanced Raman microscopy of individual carbon nanotubes

T Hümmer, J Noe, MS Hofmann, TW Hänsch… - Nature …, 2016 - nature.com
… We observe a 320-times enhanced Raman scattering spectral … at small mirror separation
using a single longitudinal cavity … spectra integrated over the full G ± band, yielding C=6.22.5. …

[HTML][HTML] Dynamics of the photosphere along the solar cycle from SDO/HMI

T Roudier, JM Malherbe, GM Mirouh - Astronomy & Astrophysics, 2017 - aanda.org
… The longitudinal magnetic field and Doppler data were … exhibit quite similar shapes with very
little dispersion (Fig. 6). … (intensity, velocity, and field strength) are constrained by the spatial …

He I spectropolarimetry of a supersonic coronal downflow within a sunspot umbra

TA Schad, GI Dima, T Anan - The Astrophysical Journal, 2021 - iopscience.iop.org
… , we infer longitudinal magnetic field strengths of ∼2.4 kG in … co-registration with a cooperating
G-band context imager and … the absorption lines and bright emission spectra near 10830 Å…

Automatic detection and extraction of ultra-fine bright structure observed with new vacuum solar telescope

L Deng - Eighth International Conference on Graphic and …, 2017 - spiedigitallibrary.org
… elements observed in the absorption band of CN (G-band; 430.5 nm) and CH (UV band-head; …
magnetic bright points may drive Alfven/Kink waves in magnetic field lines within magnetic

Origins of the ambient solar wind: implications for space weather

SR Cranmer, SE Gibson, P Riley - Space Science Reviews, 2017 - Springer
… along magnetic field lines rooted … , bright points, faculae, ephemeral regions) and medium-scale
structures (eg, active regions, filaments) that are associated mainly with closed magnetic

Longitudinally Grafting of Graphene with Iron Phthalocyanine‐based Porous Organic Polymer to Boost Oxygen Electroreduction

L Li, X Tang, S Huang, C Lu… - Angewandte …, 2023 - Wiley Online Library
… at ≈1350 cm −1 and a G band (tangential stretch of sp 2 -… The G-CN yields a higher intensity
ratio of the D to G band (I … of bright spots also demonstrates the atomic-level dispersion of …

[HTML][HTML] Accessible hotspots for single-protein SERS in DNA-origami assembled gold nanorod dimers with tip-to-tip alignment

F Schuknecht, K Kołątaj, M Steinberger, T Liedl… - Nature …, 2023 - nature.com
… , scattering spectra of individual structures were acquired to analyse the longitudinal … D-band
at ≈1350 cm −1 and a stronger G-band at ≈1580 cm −1 that dominate the time-averaged …

Unravelling external perturbation effects on the optical phonon response of graphene

N Bendiab, J Renard, C Schwarz… - Journal of Raman …, 2018 - Wiley Online Library
… important than that of the G band in graphene. As for the … the optical interference with Raman
scattering, we provide a local … route towards inducing strong pseudo-magnetic fields.[2009, …