Galaxy Morphological Classification with Zernike Moments and Machine Learning Approaches

Identification of the asymmetric spectral profiles in the solar transition region

Solar Rotation and Activity for Cycle 24 from SDO/AIA Observations

Complex Network View of the Sun’s Magnetic Patches. I. Identification

Signature of High-amplitude Pulsations in Seven δ Sct Stars via TESS Observations

Asymmetry of the spectral lines of the coronal hole and quiet Sun in the transition region

TESS Cycle 2 observations of roAp stars with 2-min cadence data

Daily and annual modulation rate of low mass dark matter in silicon detectors

Zernike moments description of solar and astronomical features: Python code

Complex Network of sunspots

Behavior of the solar coronal holes around the maximum activity of the cycle 24

Large Power Grid Hazards From Geomagnetic Storms Caused by Solar Activity

Effect of geomagnetic storms on a power network at mid latitudes

The role of the cell shapes on the characteristics of a complex earthquake network

Evidence of self‑organized criticality in time series by the horizontal visibility graph approach

Do Cellular Automaton Avalanche Models Simulate the Quasi-periodic Pulsations of Solar Flares?

Automatic detection of small-scale EUV brightenings observed by the Solar Orbiter/EUI?

Complex Network view to Solar Flare Asymmetric Activity

Temperature Analysis of Flaring (AR 11283) and Non-flaring (AR 12194) Coronal Loops

Synchronization of Small-scale Magnetic Features, Blinkers, and Coronal Bright Points

Investigation of Orbital Decay and Global Modeling of the Planet WASP-43b

Empirical Scaling Relations for the Photospheric Magnetic Elements of the Flaring and Non-Flaring Active Regions

Solar neutrinos and dark matter detection with diurnal modulation

Relations between the asteroseismic indices and stellar parameters of δ Scuti stars for two years of TESS mission

Complex Network for Solar Protons and Correlations with flares

Energetics of Solar Coronal Bright Points

Ultraviolet solar flare signatures in the framework of complex network

Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi

The star formation history of the M31 2 galaxy derived from Long-Period-Variable 3 star counts

The first view of δ Scuti and γ Doradus stars with the TESS mission

Energy Balance in Avalanche Models for Solar Flares

Kappa-Maxwellian Electrons and Bi-Maxwellian Protons in a Two-fluid Model for Fast Solar Wind

Prediction of Flares within 10 Days before They Occur on the Sun

Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2

Statistics of photospheric supergranular cells observed by SDO/HMI

First day-time seeing observations at the Observatory of University of Zanjan in Iran

Magnetoacoustic and Alfvénic black holes

Principle of Minimum Energy in Magnetic Reconnection in a Self-organized Critical Model for Solar Flares

The application of Bayesian spectral analysis in photometric time series

PREDICTION OF SOLAR FLARES USING UNIQUE SIGNATURES OF MAGNETIC FIELD IMAGES

The effects of near-core convective shells on the gravity modes of the subdwarf B pulsator KIC 10553698A

Torsional wave propagation in solar tornadoes

Wave function properties of a single and a system of magnetic flux tube(s) oscillations

Classification of mini-dimmings associated with extreme ultraviolet eruptions by using graph theory

Extraction of Active Regions and Coronal Holes from EUV Images Using the Unsupervised Segmentation Method in the Bayesian Framework

Motion and Magnetic Flux Changes of Coronal Bright Points Relative to Supergranular Cell Boundaries

STATISTICAL PROPERTIES OF SOLAR CORONAL BRIGHT POINTS

Reconstruction of Solar Coronal Linear Force-Free Magnetic Field

Segmentation of Photospheric Solar Images by Using c-Means, k-Means, and FCM Algorithms

A hybrid algorithm for feature subset selection in high-dimensional datasets using FICA and IWSSr algorithm

Automatic Method for Identifying Photospheric Bright Points and Granules Observed by Sunrise

Automated tracking of solar coronal loops and detection of their oscillations

Identification of solar coronal loops based on moments of image

Classification of Galaxies from Morphological Structures Using Zernike Moments

Earthquake Magnitude Relationships using the Markov Chain Monte Carlo (MCMC) Method

A picture of nano flare model of solar coronal emission

Identification of flares for TIC 150359500 star observed by TESS space telescope

A Network Analysis Perspective on The Sun’s Magnetic Patches

Directional effects in detection of dark matter with ultra-low threshold solid state detectors

Correlation of solar activity and its rotation during cycle 24 from SDO/AIA observations

Magnetic sources of solar short wavelength radiation

Identification of the asymmetric spectral profiles in the solar transition region

Daily and annual modulation rates of solar neutrino reaction in solid state detector

Galaxies classification from Hubble image features based on the k-nearest neighbors' algorithm

Activity of small-scale coronal events and magnetic photospheric patches in the northern and southern hemispheres in cycle 24

Reconstruction of solar coronal magnetic field using linear and nonlinear methods

Investigation of Threshold Power-Law Behavior in Solar Flare Network

Daily and annual modulation rates of dark matter reaction in solid state detector (Ge & Si)

Evidences of Chaotic Behavior in the Quiet Sun

Characteristics of the Complex Network for Solar Active Regions

Daily and annual modulation rates of dark matter reaction in solid state detector (Ge & Si)

Prediction of X, M, and large C flares associated with coronal mass ejections

Investigation of Omori Law in the Solar Flare Network

The Role of Small Scale Events in Heating the Sun’s Corona

Automatic detection of corona bright points based on SDO observation in 24 cycle

Ephemeris Refinement of K2-30 b with MCMC Method

‫‪Evolution‬‬ of the Parameters for Networks of Iran Earthquakes

Complex Network for Solar Proton Flux

The prediction of flares associated with coronal mass ejections using the machine learning and Zernike moments

Study of the Cellular Automaton Avalanche Models for Solar Flares Based on a Probabilistic Approach

Photometry of v1644cyg Variable Star

Forecasting of solar eruptive phenomena using the machine learning method

Thermal Evolution and Estimation of the Thermal Energy for a Solar Coronal Mass Ejection

Complex Network of Solar Coronal Index

Damping and oscillations of Coronal Loops

Prediction of solar flares associated with coronal mass ejection before their

Physical Parameters of Solar Coronal Bright Points by Differential Emission Measure Function

Do solar active regions form a scale-free network

Physical Parameters of Solar Coronal Bright Points by Differential Emission Measure Function

Do solar active regions form a scale-free network?

Automatic identification of the transitional regions brightenings and their relationship with coronal bright points

Asteroseismic analysis and rotationally split modes of hybrid δ Scuti – γ Doradus pulsating stars

Determination of the initial and boundary conditions corresponds to a simulation of the small scale events in magnetohydrodynamics approach

Investigation of Relationships between Sunspots, Coronal Holes, and El Nino

Comparison between the results obtained by asteroseismology formalism based on modified Helmholtz’s theorem and Rayleigh-Ritz method proposed by Sobouti and GYRE asteroseismology code

Size-Frequency Distributions of Photospheric Suprgranular Cells Extracted from HMI Images by Ball-Tracking Method

Behavior of Eigenfrequencies in a System of Coronal Loops Oscillation: Multi-stranded Loops Interaction Approach”

statistics of Solar Magnetic Elements Observed by SDO/HMI During the year 2011

new segmentation method for investigating coronal bright points

Kink and Sausage Oscillations of a QS Mini Loop

Eigen-Frequencies of MHD Wave Equations in the Presence of Longitudinal Stratification Density

Extracting Kink-like Modes of Multi-Stranded Loops in The Solar Corona

Evolution of solar Coronal Holes (CH) from Extra Ultra Violet (EUV)