activity
20142017
most citedThe Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs -- Space-weather HMI Active Region Patches

758 citations · 1.8k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201741 cited

Evaluating (and Improving) Estimates of the Solar Radial Magnetic Field Component from Line-of-Sight Magnetograms

K. D. Leka, G. Barnes, E. L. Wagner

Although for many solar physics problems the desirable or meaningful boundary is the radial component of the magnetic field , the most readily available measurement is t…

astro-ph.SR201619 cited

A Fixed-point Scheme for the Numerical Construction of Magnetohydrostatic Atmospheres in Three Dimensions

S. A. Gilchrist, D. C. Braun, G. Barnes

Magnetohydrostatic models of the solar atmosphere are often based on idealized analytic solutions because the underlying equations are too difficult to solve in full generality. Nu…

astro-ph.SR2016228 cited

A Comparison of Flare Forecasting Methods, I: Results from the "All-Clear" Workshop

G. Barnes, K. D. Leka, C. J. Schrijver +15

Solar flares produce radiation which can have an almost immediate effect on the near-Earth environment, making it crucial to forecast flares in order to mitigate their negative eff…

astro-ph.SR2014608 cited

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance

J. Todd Hoeksema, Yang Liu, Keiji Hayashi +9

The Helioseismic and Magnetic Imager (HMI) began near-continuous full-disk solar measurements on 1 May 2010 from the Solar Dynamics Observatory (SDO). An automated processing pipel…

astro-ph.SR2014758 cited

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs -- Space-weather HMI Active Region Patches

Monica G. Bobra, Xudong Sun, J. Todd Hoeksema +5

A new data product from the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) called Space-weather HMI Active Region Patches (SHARPs) is now avail…

astro-ph.SR2014110 cited

The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Optimization of the Spectral Line Inversion Code

R. Centeno, J. Schou, K. Hayashi +5

The Very Fast Inversion of the Stokes Vector (VFISV) is a Milne-Eddington spectral line inversion code used to determine the magnetic and thermodynamic parameters of the solar phot…