Received: 2021-09-22
Accepted: 2021-11-08
Published Online: 2021-12-13
© 2021 Qiang Li et al., published by De Gruyter
Articles in the same Issue
- Regular articles
- On the plausible origins of the spiral character of galaxies
- Astrometry and photometry of digitized plates of Baldone Schmidt telescope
- The atmospheric model of neural networks based on the improved Levenberg-Marquardt algorithm
- The New Ephemeris and Light Curve Analysis of V870 Ara by the Ground-Based and TESS Data
- The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition
- Machine Learning for the Relationship of High-Energy Electron Flux between GEO and MEO with Application to Missing Values Imputation for Beidou MEO Data
- Optimal attitude control for solar array orientation
- An orbit determination method of spacecraft based on distribution regression
- Special Issue: The Global Space Exploration Conference (GLEX) 2021
- Introduction to the Special Issue “The Global Space Exploration Conference (GLEX) 2021”
- Prevention of NEO hazard: the Russian approach
- Gravity assists maneuver in the problem of extension accessible landing areas on the Venus surface
- The use of radiation-resistant materials in gas semiconductor Fourier spectroscopy for express analysis of rocket fuel in the production process on the Moon / Mars / asteroids
- Special Issue: Modern Stellar Astronomy
- On the forms of accretion of interstellar gas and dust during the formation of single stars and their planetary systems
- Analysis and modeling of the dynamics of the glow of calcium and hydrogen lines in solar and stellar flares
- PRESTALINE: a package for simulation and analysis of molecular spectra of star forming regions
- Observations of the gamma-ray pulsar J1836+5925 at 111 MHz
- Future of the General Catalogue of Variable Stars from the Experience of Recent Name-lists
- Biermann battery as a source of astrophysical magnetic fields
- A possible nonthermal X-ray emission from γ Cas analogues stars
- Nonlinear cosmogony of the spiral galaxy bulges
- Solar activity and COVID-19 pandemic
- Fitting procedure for estimating interstellar extinction at high galactic latitudes
- The fine structure of the rotational periods of the solar mean magnetic field
- On the direction of the velocity and magnetic field fluctuations in undisturbed solar wind
- Application of clustering algorithm to wide stellar pairs for unsupervised search of parts of disrupting clusters
- Possibilities of velocity field analysis from Hinode SOT/SP data
- Absolute magnitudes of white dwarfs and discovery of new white dwarfs from FBS Blue Stellar Objects by means of Gaia EDR3 data
- Flare energy release and avalanche ionization of plasma by runaway electrons in lower solar atmosphere
- Probing the rotation rate of solar active regions: the comparison of methods
- The near-infrared observations at the Tower Solar Telescope TST-2 of the Crimean Astrophysical Observatory
Creative Commons
BY 4.0
Articles in the same Issue
- Regular articles
- On the plausible origins of the spiral character of galaxies
- Astrometry and photometry of digitized plates of Baldone Schmidt telescope
- The atmospheric model of neural networks based on the improved Levenberg-Marquardt algorithm
- The New Ephemeris and Light Curve Analysis of V870 Ara by the Ground-Based and TESS Data
- The Mg/Fe ratio of silicate minerals in the meteoritic materials and in the circumstellar environment: A case study for the chondritic-like composition
- Machine Learning for the Relationship of High-Energy Electron Flux between GEO and MEO with Application to Missing Values Imputation for Beidou MEO Data
- Optimal attitude control for solar array orientation
- An orbit determination method of spacecraft based on distribution regression
- Special Issue: The Global Space Exploration Conference (GLEX) 2021
- Introduction to the Special Issue “The Global Space Exploration Conference (GLEX) 2021”
- Prevention of NEO hazard: the Russian approach
- Gravity assists maneuver in the problem of extension accessible landing areas on the Venus surface
- The use of radiation-resistant materials in gas semiconductor Fourier spectroscopy for express analysis of rocket fuel in the production process on the Moon / Mars / asteroids
- Special Issue: Modern Stellar Astronomy
- On the forms of accretion of interstellar gas and dust during the formation of single stars and their planetary systems
- Analysis and modeling of the dynamics of the glow of calcium and hydrogen lines in solar and stellar flares
- PRESTALINE: a package for simulation and analysis of molecular spectra of star forming regions
- Observations of the gamma-ray pulsar J1836+5925 at 111 MHz
- Future of the General Catalogue of Variable Stars from the Experience of Recent Name-lists
- Biermann battery as a source of astrophysical magnetic fields
- A possible nonthermal X-ray emission from γ Cas analogues stars
- Nonlinear cosmogony of the spiral galaxy bulges
- Solar activity and COVID-19 pandemic
- Fitting procedure for estimating interstellar extinction at high galactic latitudes
- The fine structure of the rotational periods of the solar mean magnetic field
- On the direction of the velocity and magnetic field fluctuations in undisturbed solar wind
- Application of clustering algorithm to wide stellar pairs for unsupervised search of parts of disrupting clusters
- Possibilities of velocity field analysis from Hinode SOT/SP data
- Absolute magnitudes of white dwarfs and discovery of new white dwarfs from FBS Blue Stellar Objects by means of Gaia EDR3 data
- Flare energy release and avalanche ionization of plasma by runaway electrons in lower solar atmosphere
- Probing the rotation rate of solar active regions: the comparison of methods
- The near-infrared observations at the Tower Solar Telescope TST-2 of the Crimean Astrophysical Observatory