25 citations as recorded by crossref.

1. INNER HELIOSPHERIC EVOLUTION OF A “STEALTH” CME DERIVED FROM MULTI-VIEW IMAGING AND MULTIPOINT IN SITU OBSERVATIONS. I. PROPAGATION TO 1 AU T. Nieves-Chinchilla et al. 10.1088/0004-637X/779/1/55
2. The Need for Near-Earth Multi-Spacecraft Heliospheric Measurements and an Explorer Mission to Investigate Interplanetary Structures and Transients in the Near-Earth Heliosphere N. Lugaz et al. 10.1007/s11214-024-01108-8
3. Observations of ICMEs and ICME-like Solar Wind Structures from 2007 – 2010 Using Near-Earth and STEREO Observations E. Kilpua et al. 10.1007/s11207-012-9957-0
4. On the relationship between magnetic cloud field polarity and geoeffectiveness E. Kilpua et al. 10.5194/angeo-30-1037-2012
5. The Width of Magnetic Ejecta Measured near 1 au: Lessons from STEREO-A Measurements in 2021–2022 N. Lugaz et al. 10.3847/1538-4357/ad17b9
6. Magnetic Field Configuration Models and Reconstruction Methods for Interplanetary Coronal Mass Ejections N. Al-Haddad et al. 10.1007/s11207-013-0244-5
7. Studying the relationship of localization parameters of solar sources of magnetic clouds with their characteristics and substorm activity Н. Бархатов et al. 10.12737/stp-53201907
8. Studying the relationship of localization parameters of solar sources of magnetic clouds with their characteristics and substorm activity Н. Бархатов et al. 10.12737/szf-53201907
9. Analysis of the Internal Structure of the Streamer Blowout Observed by the Parker Solar Probe During the First Solar Encounter T. Nieves-Chinchilla et al. 10.3847/1538-4365/ab61f5
10. A Quarter Century ofWindSpacecraft Discoveries L. Wilson et al. 10.1029/2020RG000714
11. Polytropic Behavior in the Structures of Interplanetary Coronal Mass Ejections M. Dayeh & G. Livadiotis 10.3847/2041-8213/aca673
12. Investigating Coronal Mass Ejections through Multispacecraft Measurements: STEREO-A and L1 in 2022–2023 S. Banu et al. 10.3847/1538-4357/adb60c
13. Testing the Effects of Cosmic Ray Flux Intensity Modulation on Solar Emission Characteristics C. Onah et al. 10.1088/1674-4527/adb135
14. Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum E. Kilpua et al. 10.1007/s11207-014-0552-4
15. Why have geomagnetic storms been so weak during the recent solar minimum and the rising phase of cycle 24? E. Kilpua et al. 10.1016/j.jastp.2013.11.001
16. Models and data analysis tools for the Solar Orbiter mission A. Rouillard et al. 10.1051/0004-6361/201935305
17. Statistical Study of ICMEs and Their Sheaths During Solar Cycle 23 (1996 – 2008) E. Mitsakou & X. Moussas 10.1007/s11207-014-0505-y
18. Analysis of the substructure within a complex magnetic cloud on 3–4 September 2008 K. Andreeova et al. 10.5194/angeo-31-555-2013
19. Estimating Travel Times of Coronal Mass Ejections to 1 AU Using Multi-spacecraft Coronagraph Data E. Kilpua et al. 10.1007/s11207-012-0005-x
20. A CIRCULAR-CYLINDRICAL FLUX-ROPE ANALYTICAL MODEL FOR MAGNETIC CLOUDS T. Nieves-Chinchilla et al. 10.3847/0004-637X/823/1/27
21. Prediction of the In Situ Coronal Mass Ejection Rate for Solar Cycle 25: Implications for Parker Solar Probe In Situ Observations C. Möstl et al. 10.3847/1538-4357/abb9a1
22. Sources of the Slow Solar Wind During the Solar Cycle 23/24 Minimum E. Kilpua et al. 10.1007/s11207-016-0979-x
23. Elliptic-cylindrical Analytical Flux Rope Model for Magnetic Clouds T. Nieves-Chinchilla et al. 10.3847/1538-4357/aac951
24. Modeling the Geoefficiency of Solar Wind in Solar Activity Minima V. Degtyarev & G. Popov 10.17150/2411-6262.2022.13(1).17
25. Understanding the Internal Magnetic Field Configurations of ICMEs Using More than 20 Years of Wind Observations T. Nieves-Chinchilla et al. 10.1007/s11207-018-1247-z