most citedSpectral Line Selection for HMI: A Comparison of Fe I 6173 and Ni I 6768

129 citations · 200 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph200645 cited

Radiative transfer effects on Doppler measurements as sources of surface effects in sunspot seismology

S. P. Rajaguru, K. Sankarasubramanian, R. Wachter +1

We show that the use of Doppler shifts of Zeeman sensitive spectral lines to observe wavesn in sunspots is subject to measurement specific phase shifts arising from, (i) altered he…

astro-ph200626 cited

Magnetic field vector retrieval with the Helioseismic and Magnetic Imager

J. M. Borrero, S. Tomczyk, A. Norton +5

We investigate the accuracy to which we can retrieve the solar photospheric magnetic field vector using the Helioseismic and Magnetic Imager (HMI) that will fly onboard of the Sola…

astro-ph2006129 cited

Spectral Line Selection for HMI: A Comparison of Fe I 6173 and Ni I 6768

A. A. Norton, J. Pietarila Graham, R. K. Ulrich +8

We present a study of two spectral lines, Fe I 6173 Angstroms and Ni I 6768 Angstroms, that were candidates to be used in the Helioseismic and Magnetic Imager (HMI) for observing D…

astro-ph2006

Magnetic field vector retrieval with HMI

J. M. Borrero, S. Tomczyk, A. Norton +5

The Helioseismic and Magnetic Imager (HMI), on board the Solar Dynamics Observatory (SDO), will begin data acquisition in 2008. It will provide the first full disk, high temporal c…

astro-ph2005

Magnetic topologies and two-class coronal mass ejections: a numerical magnetohydrodynamic study

W. Liu, X. P. Zhao, S. T. Wu +1

White-light observations of the solar corona show that there are two characteristic types of Coronal Mass Ejections (CMEs) in terms of speed-height profiles: so-called fast CMEs th…