activity
20102024
most citedThe Mount Wilson Observatory S-index of the Sun

139 citations · 986 across the 53 of their papers we have counts for

collaborators
Showing 2013Show all

8 papers · 1 filter

astro-ph.IM2013

Camera Gap Removal in SOLIS/VSM Images

Andrew R. Marble, Lorraine Callahan, Alexei A. Pevtsov

The Vector Spectromagnetograph (VSM) instrument on the Synoptic Optical Longterm Investigations of the Sun (SOLIS) telescope is capable of obtaining spectropolarimetry for the full…

astro-ph.SR2013

Zeemanfit: Use and Development of the solis_vms_zeemanfit code

Anna L. H. Hughes, Jack Harvey, Andrew R. Marble +1

The purpose of the SOLIS Zeemanfit Code is to provide a straight-forward, easily checked measure of the total magnetic-field strength in the high-strength umbral regions of the sol…

astro-ph.SR2013★ 14 cited

Global Solar Free Magnetic Energy and Electric Current Density Distribution of Carrington Rotation 2124

Tilaye Tadesse, T. Wiegelmann, Pevtsov A Alexei +2

Solar eruptive phenomena, like flares and coronal mass ejections(CMEs) are governed by magnetic fields. To describe the structure of these phenomena one needs information on the ma…

astro-ph.SR2013★ 32 cited

First use of synoptic vector magnetograms for global nonlinear force free coronal magnetic field models

Tilaye Tadesse, T. Wiegelmann, S. Gosain +2

The magnetic field permeating the solar atmosphere is generally thought to provide the energy for much of the activity seen in the solar corona, such as flares, coronal mass ejecti…

astro-ph.SR2013★ 65 cited

Bimodal Distribution of Magnetic Fields and Areas of Sunspots

Andrey G. Tlatov, Alexei A. Pevtsov

We applied automatic identification of sunspot umbrae and penumbrae to daily observations from the Helioseismic Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO)…

astro-ph.SR2013★ 5 cited

Properties of Magnetic Neutral Line Gradients and Formation of Filaments

Nina V. Karachik, Alexei A. Pevtsov

We investigate gradient of magnetic field across neutral lines (NLs), and compare their properties for NLs with and without the chromospheric filaments. Our results show that there…