Publications of Denis Rodkin

A list of publications authored or co-authored by Denis Rodkin, 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: 0000-0002-5874-4737

List of publications ordered by citations
Number of papers: 16 (refereed: 13)
No. of citations: 116
First author papers: 5 (refereed: 3)

2022

1. Formation of Coronal Mass Ejection and Posteruption Flow of Solar Wind on 2010 August 18 Event [2]
   Slemzin, Vladimir, Goryaev, Farid & Rodkin, Denis, ApJ, 929, 146

2020

1. Identification of Hot Plasma Anomalies in Solar Wind Using Fe Ion Charge Distributions [5]
   Goryaev, Farid F., Slemzin, Vladimir & Rodkin, Denis, ApJ, 905, L17
2. Geomagnetic Storms and Forbush-Decreases Related to Single and Complex Transient Structures of Solar Wind [3]
   Rodkin, D. G., Slemzin, V. A. & Shugay, Yu. S., Bulletin of the Lebedev Physics Institute, 47, 92
3. Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance [11]
   Yermolaev, Y. I., Lodkina, I. G., Yermolaev, M. Y., Riazantseva, M. O., Rakhmanova, L. S., Borodkova, N. L., Shugay, Y. S., Slemzin, V. A., Veselovsky, I. S. & Rodkin, D. G., Journal of Geophysical Research (Space Physics), 125, e27878

2019

1. Development of a Fast CME and Properties of a Related Interplanetary Transient [15]
   Grechnev, V. V., Kochanov, A. A., Uralov, A. M., Slemzin, V. A., Rodkin, D. G., Goryaev, F. F., Kiselev, V. I. & Myshyakov, I. I., Solar Physics, 294, 139
2. Large-Scale and Small-Scale Solar Wind Structures Formed during Interaction of Streams in the Heliosphere [1]
   Rodkin, D. G., Kaportseva, K. B., Lukashenko, A. T., Veselovsky, I. S., Slemzin, V. A. & Shugay, Yu. S., Cosmic Research, 57, 18
3. Formation of Coronal Mass Ejections in the Solar Corona and Propagation of the Resulting Plasma Streams in the Heliosphere [7]
   Slemzin, V. A., Goryaev, F. F., Rodkin, D. G., Shugay, Yu. S. & Kuzin, S. V., Plasma Physics Reports, 45, 889

2018

1. Brightening and Darkening of the Extended Solar Corona during the Superflares of September 2017 [8]
   Goryaev, Farid F., Slemzin, Vladimir A., Rodkin, Denis G., D'Huys, Elke, Podladchikova, O. & West, Matthew J., ApJ, 856, L38
2. Single ICMEs and Complex Transient Structures in the Solar Wind in 2010 - 2011 [14]
   Rodkin, D., Slemzin, V., Zhukov, A. N., Goryaev, F., Shugay, Y. & Veselovsky, I., Solar Physics, 293, 78
3. Influence of coronal mass ejections on parameters of high-speed solar wind: a case study [8]
   Shugay, Yulia, Slemzin, Vladimir, Rodkin, Denis, Yermolaev, Yuri & Veselovsky, Igor, Journal of Space Weather and Space Climate, 8, A28

2017

1. Origin and Ion Charge State Evolution of Solar Wind Transients during 4 - 7 August 2011 [24]
   Rodkin, D., Goryaev, F., Pagano, P., Gibb, G., Slemzin, V., Shugay, Y., Veselovsky, I. & Mackay, D. H., Solar Physics, 292, 90
2. Features of solar wind streams on June 21-28, 2015 as a result of interactions between coronal mass ejections and recurrent streams from coronal holes [1]
   Shugay, Yu. S., Slemzin, V. A. & Rod'kin, D. G., Cosmic Research, 55, 389
3. Possible causes of the discrepancy between the predicted and observed parameters of high-speed solar wind streams [7]
   Shugay, Yu. S., Veselovsky, I. S., Slemzin, V. A., Yermolaev, Yu. I. & Rodkin, D. G., Cosmic Research, 55, 20
4. Prediction of geoeffective solar wind streams near earth according to solar observational data [0]
   Shugay, Yu. S., Slemzin, V. A., Rodkin, D. G. & Veselovsky, I. S., Bulletin of the Lebedev Physics Institute, 44, 303

2016

1. The effect of solar activity on the evolution of solar wind parameters during the rise of the 24th cycle [5]
   Rod'kin, D. G., Shugay, Yu. S., Slemzin, V. A. & Veselovskii, I. S., Solar System Research, 50, 44
2. Interaction of high-speed and transient fluxes of solar wind at the maximum of solar cycle 24 [5]
   Rodkin, D. G., Shugai, Yu. S., Slemzin, V. A. & Veselovskii, V. A., Bulletin of the Lebedev Physics Institute, 43, 287