| The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches MG Bobra, X Sun, JT Hoeksema, M Turmon, Y Liu, K Hayashi, G Barnes, ... Solar Physics 289, 3549-3578, 2014 | 528 | 2014 |
| The Helioseismic and Magnetic Imager (HMI) vector magnetic field pipeline: overview and performance JT Hoeksema, Y Liu, K Hayashi, X Sun, J Schou, S Couvidat, A Norton, ... Solar Physics 289, 3483-3530, 2014 | 498 | 2014 |
| Evolution of magnetic field and energy in a major eruptive active region based on SDO/HMI observation X Sun, JT Hoeksema, Y Liu, T Wiegelmann, K Hayashi, Q Chen, ... The Astrophysical Journal 748 (2), 77, 2012 | 351 | 2012 |
| Comparison of line-of-sight magnetograms taken by the solar dynamics observatory/helioseismic and magnetic imager and solar and heliospheric observatory/Michelson Doppler imager Y Liu, JT Hoeksema, PH Scherrer, J Schou, S Couvidat, RI Bush, ... Solar Physics 279, 295-316, 2012 | 209 | 2012 |
| How should one optimize nonlinear force-free coronal magnetic field extrapolations from SDO/HMI vector magnetograms? T Wiegelmann, JK Thalmann, B Inhester, T Tadesse, X Sun, ... Solar Physics 281, 37-51, 2012 | 164 | 2012 |
| Hot spine loops and the nature of a late-phase solar flare X Sun, JT Hoeksema, Y Liu, G Aulanier, Y Su, IG Hannah, RA Hock The Astrophysical Journal 778 (2), 139, 2013 | 153 | 2013 |
| On polar magnetic field reversal and surface flux transport during solar cycle 24 X Sun, JT Hoeksema, Y Liu, J Zhao The Astrophysical Journal 798 (2), 114, 2015 | 133 | 2015 |
| Why is the great solar active region 12192 flare-rich but CME-poor? X Sun, MG Bobra, JT Hoeksema, Y Liu, Y Li, C Shen, S Couvidat, ... The Astrophysical Journal Letters 804 (2), L28, 2015 | 129 | 2015 |
| Formation of a double-decker magnetic flux rope in the sigmoidal solar active region 11520 X Cheng, MD Ding, J Zhang, XD Sun, Y Guo, YM Wang, B Kliem, ... The Astrophysical Journal 789 (2), 93, 2014 | 118 | 2014 |
| A database of flare ribbon properties from the Solar Dynamics Observatory. I. Reconnection flux MD Kazachenko, BJ Lynch, BT Welsch, X Sun The Astrophysical Journal 845 (1), 49, 2017 | 101 | 2017 |
| Coronal field opens at lower height during the solar cycles 22 and 23 minimum periods: IMF comparison suggests the source surface should be lowered CO Lee, JG Luhmann, JT Hoeksema, X Sun, CN Arge, I de Pater Solar Physics 269, 367-388, 2011 | 90 | 2011 |
| The influence of spatial resolution on nonlinear force-free modeling ML DeRosa, MS Wheatland, KD Leka, G Barnes, T Amari, A Canou, ... The Astrophysical Journal 811 (2), 107, 2015 | 86 | 2015 |
| A non-radial eruption in a quadrupolar magnetic configuration with a coronal null X Sun, JT Hoeksema, Y Liu, Q Chen, K Hayashi The Astrophysical Journal 757 (2), 149, 2012 | 76 | 2012 |
| A new method for polar field interpolation X Sun, Y Liu, JT Hoeksema, K Hayashi, X Zhao Solar Physics 270, 9-22, 2011 | 74 | 2011 |
| Magnetic energy partition between the coronal mass ejection and flare from AR 11283 L Feng, T Wiegelmann, Y Su, B Inhester, YP Li, XD Sun, WQ Gan The Astrophysical Journal 765 (1), 37, 2013 | 72 | 2013 |
| Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST) MP Rast, N Bello González, L Bellot Rubio, W Cao, G Cauzzi, E DeLuca, ... Solar Physics 296 (4), 70, 2021 | 63 | 2021 |
| Investigating the magnetic imprints of major solar eruptions with SDO/HMI high-cadence vector magnetograms X Sun, JT Hoeksema, Y Liu, M Kazachenko, R Chen The Astrophysical Journal 839 (1), 67, 2017 | 62 | 2017 |
| The role of erupting sigmoid in triggering a flare with parallel and large-scale quasi-circular ribbons NC Joshi, C Liu, X Sun, H Wang, T Magara, YJ Moon The Astrophysical Journal 812 (1), 50, 2015 | 58 | 2015 |
| Numerical simulations of coronal mass ejection on 2011 March 7: one-temperature and two-temperature model comparison M Jin, WB Manchester, B Van Der Holst, R Oran, I Sokolov, G Toth, Y Liu, ... The Astrophysical Journal 773 (1), 50, 2013 | 57 | 2013 |
| Super-flaring active region 12673 has one of the fastest magnetic flux emergence ever observed X Sun, AA Norton arXiv preprint arXiv:1711.08383, 2017 | 56 | 2017 |
Jon Todd HoeksemaStanford UniversityBestätigte E-Mail-Adresse bei sun.stanford.edu
