Ivan Zimovets

Dr. Ivan Zimovets

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Research Focus & Metrics

Academic Career Length

20Years (2007-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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19 July 2021 in Space Science Reviews
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Journal Article
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IZIvan Zimovets
Ivan Zimovets
JMJ. A. McLaughlin
J. A. McLaughlin
ASAbhishek Kumar Srivastava
Abhishek Kumar Srivastava
Dmitrii KolotkovDmitrii Kolotkov
Dmitrii Kolotkov
AKA. A. Kuznetsov
A. A. Kuznetsov
Qingmin ZhangQingmin Zhang
Qingmin Zhang

2 February 2016 in Space Science Reviews
Verified
Journal Article
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VNValery Nakariakov
Valery Nakariakov
VPV. Pilipenko
V. Pilipenko
BHB. Heilig
B. Heilig
PJP. Jelínek
P. Jelínek
MKMarian Karlický
Marian Karlický
IZIvan Zimovets
Ivan Zimovets

11 January 2016 in Astronomy & Astrophysics
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Journal Article
Closed access
CGC. R. Goddard
C. R. Goddard
GNGiuseppe Nistico
Giuseppe Nistico
VNV. M. Nakariakov
V. M. Nakariakov
IZIvan Zimovets
Ivan Zimovets
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

22 April 2015 in Astronomy & Astrophysics
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Journal Article
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IZIvan Zimovets
Ivan Zimovets
VNValery Nakariakov
Valery Nakariakov
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

1 April 2019 in The Astrophysical Journal Supplement Series
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Journal Article
Closed access
ANAlena Nechaeva
Alena Nechaeva
IZIvan Zimovets
Ivan Zimovets
VNValery Nakariakov
Valery Nakariakov
CGC. R. Goddard
C. R. Goddard
A catalog of kink oscillations of solar coronal loops, which spans during almost all of solar cycle 24, is presented. The catalog is based on the observations made in the extreme ultraviolet band at 171 Å with Solar Dynamics Observatory/Atmospheric Imaging Assembly and includes parameters of 223 oscillating loops in 96 oscillation events. The catalog provides the information about the oscillation locations, time, and dates of the events, associated flare, initial displacement, oscillation period, exponential damping time, and apparent amplitude. The vast majority of the oscillation detections, 84%, were made in the loops situated near or off the solar limb. The oscillation periods are found to range from 1 to 28 minutes, with 74% of the events that have the period in the range of 2–10 minutes. About 90% of the oscillations have the apparent amplitude in the range of 1–10 Mm. The oscillating loop lengths are 70–600 Mm. The typical apparent amplitude is about 1% of the loop length. The oscillation period scales linearly with the loop length, and the damping time scales linearly with the period, which confirm previous findings. The oscillation quality factor scales with the amplitude to the power of minus 0.7. No statistically significant evidence of correlation was found between both the oscillation period and the mean sunspot number, and the loop length and mean sunspot number. The catalog provides the research community with the foundation for the further statistical study of kink oscillations and their use for coronal seismology.

9 March 2011 in The Astrophysical Journal Letters
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Journal Article
Closed access
VNV. M. Nakariakov
V. M. Nakariakov
IZIvan Zimovets
Ivan Zimovets