Publications of L. Linan

A list of publications authored or co-authored by L. Linan, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0002-4014-1815

List of publications ordered by citations
Number of papers: 26 (refereed: 26)
No. of citations: 351
First author papers: 5 (refereed: 5)

2025

  1. Optimization of the FRi3D CME Model in EUHFORIA [0]
    Flossie, M., Maharana, A., Linan, L., Plets, K., Isavnin, A. & Poedts, S., Space Weather, 23, e2025SW004401
  2. Modelling gyrosynchrotron emission from coronal energetic electrons in a CME flux rope [1]
    Husidic, E., Wijsen, N., Jebaraj, I. C., Vourlidas, A., Linan, L., Vainio, R. & Poedts, S., A&A, 701, A53
  3. Prediction of Time-evolving Radial Magnetic Fields on the Solar Surface Using Deep Learning [4]
    Jeong, Hyun-Jin, Poedts, Stefaan, Wang, Haopeng, Dineva, Ekatarina, Gonidakis, Panagiotis, Carella, Francesco, Miloshevich, George, Linan, Luis & Lee, Harim, ApJ, 989, L31
  4. Coronal mass ejection propagation in the dynamically coupled space weather tool: COCONUT + EUHFORIA [9]
    Linan, L., Baratashvili, T., Lani, A., Schmieder, B., Brchnelova, M., Guo, J. H. & Poedts, S., A&A, 693, A229
  5. FoMo white-light tool: Coupling with state-of-the-art numerical models [2]
    Sorokina, D., Van Doorsselaere, T., Lloveras, D. G., Linan, L. & Poedts, S., A&A, 701, A166
  6. Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT [5]
    Wang, H. P., Poedts, S., Lani, A., Linan, L., Baratashvili, T., Zhang, F., Sorokina, D., Jeong, H.-J., Li, Y. C., Najafi-Ziyazi, M. & Schmieder, B., A&A, 702, A37
  7. Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT [8]
    Wang, H. P., Poedts, S., Lani, A., Brchnelova, M., Baratashvili, T., Linan, L., Zhang, F., Hou, D. W. & Zhou, Y. H., A&A, 694, A234
  8. SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections [6]
    Wang, H. P., Guo, J. H., Yang, L. P., Poedts, S., Zhang, F., Lani, A., Baratashvili, T., Linan, L., Lin, R. & Guo, Y., A&A, 693, A257
  9. SIP-IFVM: An Observation-based Magnetohydrodynamic Model of a Coronal Mass Ejection [3]
    Wang, Hao P., Guo, Jin H., Poedts, S., Lani, A., Linan, L., Baratashvili, T., Yang, Li P., Jeong, H.-J., Wei, Wen W., Li, Cai X., Yang, Y., Li, Yu C., Wu, Hao, Guo, Yang & Schmieder, B., ApJS, 281, 43
  10. SIP-IFVM: A Time-evolving Coronal Model with an Extended Magnetic Field Decomposition Strategy [9]
    Wang, Haopeng, Yang, Liping, Poedts, Stefaan, Lani, Andrea, Zhou, Yuhao, Gao, Yuhang, Linan, Luis, Lv, Jiakun, Baratashvili, Tinatin, Guo, Jinhan, Lin, Rong, Su, Zhan, Li, Caixia, Zhang, Man, Wei, Wenwen, Yang, Yun, Li, Yucong, Ma, Xinyi, Husidic, Edin, Jeong, Hyun-Jin, Najafi-Ziyazi, Mahdi, Wang, Juan & Schmieder, Brigitte, ApJS, 278, 59

2024

  1. The operationally ready full 3D magnetohydrodynamic model from the Sun to Earth: COCONUT+Icarus [11]
    Baratashvili, T., Brchnelova, M., Linan, L., Lani, A. & Poedts, S., A&A, 690, A184
  2. Dependence of coronal mass ejections on the morphology and toroidal flux of their source magnetic flux ropes [5]
    Guo, J. H., Linan, L., Poedts, S., Guo, Y., Schmieder, B., Lani, A., Ni, Y. W., Brchnelova, M., Perri, B., Baratashvili, T., Li, S. T. & Chen, P. F., A&A, 690, A189
  3. Modeling the propagation of coronal mass ejections with COCONUT: Implementation of the regularized Biot-Savart law flux rope model [13]
    Guo, J. H., Linan, L., Poedts, S., Guo, Y., Lani, A., Schmieder, B., Brchnelova, M., Perri, B., Baratashvili, T., Ni, Y. W. & Chen, P. F., A&A, 683, A54
  4. Cross-field Diffusion Effects on Particle Transport in a Solar Coronal Flux Rope [6]
    Husidic, Edin, Wijsen, Nicolas, Linan, Luis, Brchnelova, Michaela, Vainio, Rami & Poedts, Stefaan, ApJ, 976, L31
  5. Toroidal Miller-Turner and Soloviev coronal mass ejection models in EUHFORIA. I. Implementation [9]
    Linan, L., Maharana, A., Poedts, S., Schmieder, B. & Keppens, R., A&A, 681, A103
  6. Toroidal modified Miller-Turner CME model in EUHFORIA: Validation and comparison with flux rope and spheromak [4]
    Maharana, A., Linan, L., Poedts, S. & Magdalenić, J., A&A, 691, A146

2023

  1. Self-consistent propagation of flux ropes in realistic coronal simulations [27]
    Linan, L., Regnault, F., Perri, B., Brchnelova, M., Kuzma, B., Lani, A., Poedts, S. & Schmieder, B., A&A, 675, A101
  2. Comparison of magnetic energy and helicity in coronal jet simulations [10]
    Pariat, E., Wyper, P. F. & Linan, L., A&A, 669, A33

2022

  1. Magnetic Helicity Evolution and Eruptive Activity in NOAA Active Region 11158 [7]
    Green, L. M., Thalmann, J. K., Valori, G., Pariat, E., Linan, L. & Moraitis, K., ApJ, 937, 59

2020

  1. Energy and helicity fluxes in line-tied eruptive simulations [9]
    Linan, L., Pariat, É., Aulanier, G., Moraitis, K. & Valori, G., A&A, 636, A41
  2. Additivity of relative magnetic helicity in finite volumes [6]
    Valori, Gherardo, Démoulin, Pascal, Pariat, Etienne, Yeates, Anthony, Moraitis, Kostas & Linan, Luis, A&A, 643, A26

2019

  1. Magnetic helicity and eruptivity in active region 12673 [38]
    Moraitis, K., Sun, X., Pariat, É. & Linan, L., A&A, 628, A50
  2. Magnetic Helicity Budget of Solar Active Regions Prolific of Eruptive and Confined Flares [49]
    Thalmann, Julia K., Moraitis, K., Linan, L., Pariat, E., Valori, G. & Dalmasse, K., ApJ, 887, 64
  3. On the Reliability of Magnetic Energy and Helicity Computations Based on Nonlinear Force-free Coronal Magnetic Field Models [27]
    Thalmann, Julia K., Linan, L., Pariat, E. & Valori, G., ApJ, 880, L6

2018

  1. Time Variations of the Nonpotential and Volume-threading Magnetic Helicities [34]
    Linan, L., Pariat, É., Moraitis, K., Valori, G. & Leake, J., ApJ, 865, 52
  2. Threshold of Non-potential Magnetic Helicity Ratios at the Onset of Solar Eruptions [49]
    Zuccarello, F. P., Pariat, E., Valori, G. & Linan, L., ApJ, 863, 41

Created on Wed Apr 8 04:36:06 2026.