Vladimir Airapetian

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Research Professor

American University

United States

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About

Vladimir Airapetian is a Research Professor at American University in the United States. His research primarily focuses on solar and stellar phenomena, including the study of flares, magnetic fields, and the evolution of solar extreme-ultraviolet radiation. Recent articles co-authored by Dr. Airapetian explore the dynamics of young stellar energetic flares and the observational characteristics of solar-type stars.

Recent Grants

Grant: Close

USING A VERSION OF THE FOKKER-PLANCK (FP) CODE DEVELOPED BY DR. V. AIRAPETIAN SPECIFICALLY TO TREAT SUPRATHERMAL ELECTRONS IN THE SOLAR CORONA, WE PROPOSE TO INVESTIGATE THE EVOLUTION OF THE ELECTRON DISTRIBUTION FUNCTION IN THE SOLAR CORONA AND THE SOLAR

Open Date: 2011-06-02

Close Date: 2012-06-01

Grant: Close

WE PROPOSE TO CONSISTENTLY ANALYZE THE SPECTRAL LINE PROFILES INCLUDING CRR, CJ, CM, CLY, OVI EMISSION LINES USING DATA FROM GHRSIHST, STISIHST, FUSE AND CHANDRA TO DEDUCE THE PROPERTIES OF ATMOSPHERIC PLASMA IN A TAU. WE THEN WILL DEVELOP AND SUBMIT A PR

Open Date: 2010-04-06

Close Date: 2011-04-05

Articles (18)

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Collaborators (21)

Sven Wedemeyer

Professor

University of Oslo

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Vladimir Airapetian

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Recent Grants

Articles (18)

A Semiempirical Estimate of Solar Extreme-ultraviolet Evolution from 10 Myr to 10 Gyr

Multi-observatory Study of Young Stellar Energetic Flares (MORYSEF): No Evidence for Abnormally Strong Stellar Magnetic Fields after Powerful X-Ray Flares

Role of Nonthermal Processes in the Quiescent and Active Millimeter Spectrum of a Young M Dwarf

Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares

Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-driven Modeling and Observed Magnetic Environment

Multi-Observatory Research of Young Stellar Energetic Flares (MORYSEF): X-Ray-flare-related Phenomena and Multi-epoch Behavior

Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun

Heating of the Magnetically Closed Corona and Physical Models of Solar and Stellar Spectral Irradiances

Reconstructing the XUV Spectra of Active Sun-like Stars Using Solar Scaling Relations with Magnetic Flux

Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers)

Nonthermal Motions and Atmospheric Heating of Cool Stars

The Advanced Spectral Library: The Evolution of Chromospheric Wind Characteristics from Noncoronal to Hybrid Giant Stars*

Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers)

Delayed Development of Cool Plasmas in X-Ray Flares from the Young Sun-like Star κ 1 Ceti

Multiverse Predictions for Habitability: Origin of Life Scenarios

Understanding the Duration of Solar and Stellar Flares at Various Wavelengths

Energetic Superflare from a Young Solar Analog, DS Tucanae A, Observed with NICER

Multiverse Predictions for Habitability: Planetary Characteristics

Collaborators (21)

Sven Wedemeyer

Jan Forbrich

Ofer Cohen

Meng Jin

Eric Feigelson

Joel Coley

Kimitaka Kawamura

L. Ilsedore Cleeves

Peter Hauschildt

Paola Testa

Julien Morin

Kyoko Watanabe

Craig D Johnston

Aline Vidotto

Kai Ikuta

KEVIN FRANCE

ALEXANDER BROWN

Patrick Antolin

Kensei Kobayashi

Yoko Kebukawa

Sudeshna Boro Saikia

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