output
19972026
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations

Showing 2017Show all

34 papers · 1 filter

astro-ph.EP2017★ 42 cited

Dependence of the Martian radiation environment on atmospheric depth: Modeling and measurement

Jingnan Guo, Tony C. Slaba, Cary Zeitlin +9

The energetic particle environment on the Martian surface is influenced by solar and heliospheric modulation and changes in the local atmospheric pressure (or column depth). The Ra…

astro-ph.SR2017★ 41 cited

Persistent magnetic vortex flow at a supergranular vertex

Iker S. Requerey, Basilio Ruiz Cobo, Milan Gošić +1

Photospheric vortex flows are thought to play a key role in the evolution of magnetic fields. Recent studies show that these swirling motions are ubiquitous in the solar surface co…

cs.IT2017★ 2 cited

Nonparametric Composite Hypothesis Testing in an Asymptotic Regime

Qunwei Li, Tiexing Wang, Donald J. Bucci +3

We investigate the nonparametric, composite hypothesis testing problem for arbitrary unknown distributions in the asymptotic regime where both the sample size and the number of hyp…

astro-ph.SR2017★ 57 cited

3He-Rich Solar Energetic Particles in Helical Jets on the Sun

Radoslav Bucik, Davina E. Innes, Glenn M. Mason +3

Particle acceleration in stellar flares is ubiquitous in the Universe, however, our Sun is the only astrophysical object where energetic particles and their source flares can both…

astro-ph.SR2017★ 35 cited

First analysis of solar structures in 1.21 mm full-disc ALMA image of the Sun

R. Brajša, D. Sudar, A. O. Benz +11

Various solar features can be seen on maps of the Sun in the mm and sub-mm wavelength range. The recently installed Atacama Large Millimeter/submillimeter Array (ALMA) is capable o…

astro-ph.SR2017★ 91 cited

Intermittent reconnection and plasmoids in UV bursts in the low solar atmosphere

L. Rouppe van der Voort, B. De Pontieu, G. B. Scharmer +9

Magnetic reconnection is thought to drive a wide variety of dynamic phenomena in the solar atmosphere. Yet the detailed physical mechanisms driving reconnection are difficult to di…