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

758 citations · 1.7k across the 5 of their papers we have counts for

collaborators

5 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.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…