Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Vasili Lobzin"'
Publikováno v:
Space Weather. 15:1151-1164
In the present paper, solar magnetograms provided by the Helioseismic and Magnetic Imager (HMI) on-board Solar Dynamics Observatory (SDO) spacecraft are used to identify active regions automatically by thresholding the line-of-sight component of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e1ba4ee754c755463db46281d26be40f
https://doi.org/10.1002/2017sw001595
https://doi.org/10.1002/2017sw001595
Autor:
Vasili Lobzin, Graham Steward, J. T. Gosling, David M. Malaspina, Bo Li, D. Neudegg, Iver H. Cairns
Publikováno v:
Journal of Geophysical Research: Space Physics. 121:6141-6156
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cd4d48a36493fd6816eb02c00d814be5
https://doi.org/10.1002/2016ja022756
https://doi.org/10.1002/2016ja022756
Autor:
V.R. Chechetkin, Vasili Lobzin
Publikováno v:
Journal of theoretical biology. 426
Using state-of-the-art techniques combining imaging methods and high-throughput genomic mapping tools leaded to the significant progress in detailing chromosome architecture of various organisms. However, a gap still remains between the rapidly growi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b831b4cbb936d369ccb258a24a056b49
https://pubmed.ncbi.nlm.nih.gov/28552553
https://pubmed.ncbi.nlm.nih.gov/28552553
Publikováno v:
Journal of Geophysical Research: Space Physics. 119:6042-6061
Type II solar radio bursts are often indicators for impending space weather events at Earth. They are consequences of shock waves driven by coronal mass ejections (CMEs) that move outward from the Sun. We simulate such type II radio bursts by combini
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::68382042717b1454ab8e8dcaeafe3e27
https://doi.org/10.1002/2014ja019950
https://doi.org/10.1002/2014ja019950
Publikováno v:
Journal of Geophysical Research: Space Physics. 121
Large-scale magnetic field configurations are important for the transport of solar wind strahl electrons, which are suprathermal and directed along the field outward from the Sun. Strahl electrons are routinely used to infer not only the field config
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92a67363d521a84718419ab5d01545d6
https://doi.org/10.1002/2016ja023023
https://doi.org/10.1002/2016ja023023
Autor:
Vasili Lobzin, V.R. Chechetkin
Publikováno v:
Journal of Theoretical Biology. 269:57-63
The standard genetic code is known to be much more efficient in minimizing adverse effects of misreading errors and one-point mutations in comparison with a random code having the same structure, i.e. the same number of codons coding for each particu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b54dce8613ab2e935d6662ec9dc33d2
https://doi.org/10.1016/j.jtbi.2010.10.015
https://doi.org/10.1016/j.jtbi.2010.10.015
Autor:
Roman V. Gorgutsa, Alexander Warmuth, G. Mann, Vasili Lobzin, Iver H. Cairns, Peter A. Robinson, Valery V. Fomichev
Publikováno v:
The Astrophysical Journal. 724:1099-1107
Type III radio bursts are produced near the local electron plasma frequency fp and near its harmonic 2fp by fast electrons ejected from the solar active regions and moving through the corona and solar wind. The coronal bursts have dynamic spectra wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1c5409590fa628384d3b94685e40ef17
https://doi.org/10.1088/0004-637x/724/2/1099
https://doi.org/10.1088/0004-637x/724/2/1099
Publikováno v:
The Astrophysical Journal. 710:L58-L62
Major space weather events such as solar flares and coronal mass ejections are usually accompanied by solar radio bursts, which can potentially be used for real-time space weather forecasts. Type II radio bursts are produced near the local plasma fre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::75000f6360528ddda202bfc604f4f262
https://doi.org/10.1088/2041-8205/710/1/l58
https://doi.org/10.1088/2041-8205/710/1/l58
Publikováno v:
The Astrophysical Journal. 706:L265-L269
The Sun's electron number density profile ne (r) is vital for solar physics but not well measured or understood within a few solar radii RS . Here, a new technique extracts ne (r) directly from coronal type III radio bursts for 40 ≤ f ≤ 180 MHz.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bad8dbaab66e72a3e04ab29382e8e738
https://doi.org/10.1088/0004-637x/706/2/l265
https://doi.org/10.1088/0004-637x/706/2/l265
Publikováno v:
The Astrophysical Journal. 677:L129-L132
Type II radio bursts are produced near the local plasma frequency fp and near 2fp by shocks moving through the corona and solar wind. In the present Letter eight well-defined coronal type II radio bursts (30-300 MHz) are analyzed. Three results are p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::53d99ee48f0a9cd1561f48073ca84905
https://doi.org/10.1086/587980
https://doi.org/10.1086/587980