First-authored, refereed papers of Roberto Lionello, ordered by citations


A list of first-authored, refereed publications of Roberto Lionello, derived from the SAO/NASA Astrophysics Data System (ADS) and ordered by the numbers of citations.

Orcid ID: 0000-0001-9231-045X

Number of papers: 19
No. of citations: 1203

363 Multispectral Emission of the Sun During the First Whole Sun Month: Magnetohydrodynamic Simulations
Lionello, Roberto, Linker, Jon A. & Mikić, Zoran, 2009, ApJ, 690, 902
110 Including the Transition Region in Models of the Large-Scale Solar Corona
Lionello, Roberto, Linker, Jon A. & Mikić, Zoran, 2001, ApJ, 546, 542
92 Validating a Time-dependent Turbulence-driven Model of the Solar Wind
Lionello, Roberto, Velli, Marco, Downs, Cooper, Linker, Jon A., Mikić, Zoran & Verdini, Andrea, 2014, ApJ, 784, 120
78 Magnetohydrodynamic Simulations of Interplanetary Coronal Mass Ejections
Lionello, Roberto, Downs, Cooper, Linker, Jon A., Török, Tibor, Riley, Pete & Mikić, Zoran, 2013, ApJ, 777, 76
75 Magnetic Field Topology in Prominences
Lionello, Roberto, Mikić, Zoran, Linker, Jon A. & Amari, Tahar, 2002, ApJ, 581, 718
74 The Effects of Differential Rotation on the Magnetic Structure of the Solar Corona: Magnetohydrodynamic Simulations
Lionello, Roberto, Riley, Pete, Linker, Jon A. & Mikić, Zoran, 2005, ApJ, 625, 463
69 Nonlinear Magnetohydrodynamic Evolution of Line-tied Coronal Loops
Lionello, Roberto, Velli, Marco, Einaudi, Giorgio & Mikić, Zoran, 1998, ApJ, 494, 840
57 Stability of Algorithms for Waves with Large Flows
Lionello, Roberto, Mikić, Zoran & Linker, Jon A., 1999, Journal of Computational Physics, 152, 346
49 Thermal Non-equilibrium Revisited: A Heating Model for Coronal Loops
Lionello, Roberto, Winebarger, Amy R., Mok, Yung, Linker, Jon A. & Mikić, Zoran, 2013, ApJ, 773, 134
47 Application of a Solar Wind Model Driven by Turbulence Dissipation to a 2D Magnetic Field Configuration
Lionello, Roberto, Velli, Marco, Downs, Cooper, Linker, Jon A. & Mikić, Zoran, 2014, ApJ, 796, 111
38 Magnetohydrodynamics of solar coronal plasmas in cylindrical geometry.
Lionello, R., Mikic, Z. & Schnack, D. D., 1998, Journal of Computational Physics, 140, 172
35 The Latitudinal Excursion of Coronal Magnetic Field Lines in Response to Differential Rotation: MHD Simulations
Lionello, Roberto, Linker, Jon A., Mikić, Zoran & Riley, Pete, 2006, ApJ, 642, L69
26 The Contribution of Coronal Jets to the Solar Wind
Lionello, R., Török, T., Titov, V. S., Leake, J. E., Mikić, Z., Linker, J. A. & Linton, M. G., 2016, ApJ, 831, L2
23 Can Large Time Delays Observed in Light Curves of Coronal Loops Be Explained in Impulsive Heating?
Lionello, Roberto, Alexander, Caroline E., Winebarger, Amy R., Linker, Jon A. & Mikić, Zoran, 2016, ApJ, 818, 129
22 Ion Charge States in a Time-Dependent Wave-Turbulence-Driven Model of the Solar Wind
Lionello, Roberto, Downs, Cooper, Linker, Jon A., Mikić, Zoran, Raymond, John, Shen, Chengcai & Velli, Marco, 2019, Solar Physics, 294, 13
20 Global MHD Simulations of the Time-dependent Corona
Lionello, Roberto, Downs, Cooper, Mason, Emily I., Linker, Jon A., Caplan, Ronald M., Riley, Pete, Titov, Viacheslav S. & DeRosa, Marc L., 2023, ApJ, 959, 77
15 Current sheet formation due to nonlinear kink modes in periodic and line-tied configurations
Lionello, Roberto, Schnack, Dalton D., Einaudi, Giorgio & Velli, Marco, 1998, Physics of Plasmas, 5, 3722
6 Integrating physics-based coronal heating and solar wind acceleration in a global MHD model
Lionello, Roberto, Velli, Marco, Linker, Jon A. & Mikić, Zoran, 2013, Solar Wind 13 (Editors: Zank, Gary P., Borovsky, Joe, Bruno, Roberto, Cirtain, Jonathan, Cranmer, Steve, Elliott, Heather, Giacalone, Joe, Gonzalez, Walter, Li, Gang, Marsch, Eckart, Moebius, Ebehard, Pogorelov, Nick, Spann, Jim & Verkhoglyadova, Olga), American Institute of Physics Conference Series, 1539, p. 30
4 Slip-back Mapping as a Tracker of Topological Changes in Evolving Magnetic Configurations
Lionello, R., Titov, V. S., Mikić, Z. & Linker, J. A., 2020, ApJ, 891, 14


Created on Wed Apr 8 04:31:42 2026.