activity
20072022
most citedDiscovery of Scattering Polarization in the Hydrogen Lyman- Line of the Solar Disk Radiation

67 citations · 146 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022

Quiet Sun Center to Limb Variation of the Linear Polarization Observed by CLASP2 Across the Mg II h & k Lines

L. A. Rachmeler, J. Trujillo Bueno, D. E. McKenzie +25

The CLASP2 (Chromospheric LAyer SpectroPolarimeter 2) sounding rocket mission was launched on 2019 April 11. CLASP2 measured the four Stokes parameters of the Mg II h & k spectral…

astro-ph.SR2022★ 9 cited

Empirical relations between the intensities of Lyman lines of H and He

M. Gordino, F. Auchère, J. -C. Vial +9

Empirical relations between major UV and extreme UV spectral lines are one of the inputs for models of chromospheric and coronal spectral radiances and irradiances. They are also n…

astro-ph.SR2018★ 3 cited

A Statistical Inference Method for Interpreting the CLASP Observations

J. Stepan, J. Trujillo Bueno, L. Belluzzi +25

On 3rd September 2015, the Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) successfully measured the linear polarization produced by scattering processes in the hydrogen Lyman…

astro-ph.SR2017★ 8 cited

Comparison of Solar Fine Structure Observed Simultaneously in Ly-α and Mg II h

D. J. Schmit, A. V. Sukhorukov, B. De Pontieu +9

The Chromospheric Lyman Alpha Spectropolarimeter (CLASP) observed the Sun in H I Lyman-α during a suborbital rocket flight on September 3, 2015. The Interface Region Imaging Telesc…

astro-ph.SR2017★ 67 cited

Discovery of Scattering Polarization in the Hydrogen Lyman- Line of the Solar Disk Radiation

R. Kano, J. Trujillo Bueno, A. Winebarger +25

There is a thin transition region (TR) in the solar atmosphere where the temperature rises from 10,000 K in the chromosphere to millions of degrees in the corona. Little is known a…

astro-ph2007★ 59 cited

Hinode Calibration for Precise Image Co-alignment between SOT and XRT (November 2006 -- April 2007)

Toshifumi Shimizu, Yukio Katsukawa, Keiichi Matsuzaki +11

To understand the physical mechanisms for activity and heating in the solar atmosphere, the magnetic coupling from the photosphere to the corona is an important piece of informatio…