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Geomagnetism and Aeronomy
ISSN 0016-7932 (Print) ISSN 1555-645X (Online)
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Keywords Auroral Oval Auroral Zone Central Meridian Cutoff Rigidity Flare Geomagnetic Cutoff Rigidity Geomagnetic Field Strength Geomagnetic Latitude Geomagnetic Pulsation Interplanetary Magnetic Field Ionosphere Magnetic Anomaly Magnetic Local Time Magnetic Storm Plasma Sheet Prevailing Wind Proton Flux Solar Proton Solar Wind Substorm Onset Total Electron Content
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Keywords Auroral Oval Auroral Zone Central Meridian Cutoff Rigidity Flare Geomagnetic Cutoff Rigidity Geomagnetic Field Strength Geomagnetic Latitude Geomagnetic Pulsation Interplanetary Magnetic Field Ionosphere Magnetic Anomaly Magnetic Local Time Magnetic Storm Plasma Sheet Prevailing Wind Proton Flux Solar Proton Solar Wind Substorm Onset Total Electron Content
Home > Search > Author Details

Author Details

Kudryavtsev, I. V.

Issue Section Title File
Vol 56, No 7 (2016) Article Reconstructions of the 14С cosmogenic isotope content from natural archives after the last glacial termination
Vol 56, No 8 (2016) Article Reconstructions of the heliospheric modulation potential and Wolf numbers based on the content of the 14C isotope in tree rings during the Maunder and Spörer minimums
Vol 58, No 7 (2018) Article Reconstruction of the Production Rate of Cosmogenic 14C in the Earth’s Atmosphere for 17 000–5000 BC
Vol 58, No 8 (2018) Article Reconstruction of the Wolf Numbers Based on Radiocarbon Data from the Early 11th Century until the Middle of the 19th Century with Respect to Climate Changes
Vol 59, No 7 (2019) Article Dynamics of Fast Electrons in an Inhomogeneous Plasma with Plasma Beam Instability
Vol 59, No 7 (2019) Article Solar Activity from the Mid-Second Millennium B.C. to the First Millennium A.D. Based on Radiocarbon Data
Vol 59, No 8 (2019) Article Solar System Collisions with Dense Interstellar Gas Clouds and Radiocarbon Traces of Periods with “Abnormally Low” Solar Modulation of Cosmic Rays
Vol 59, No 8 (2019) Article Reconstruction of Heliospheric Modulation Potential Based on Radiocarbon Data in the Time Interval 17 000–5000 Years B.C.
 

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