Results 1 to 10 of about 413,287 (118)

ACTIVITY-BRIGHTNESS CORRELATIONS FOR THE SUN AND SUN-LIKE STARS [PDF]

open access: yesThe Astrophysical Journal, 2011
We analyze the effect of solar features on the variability of the solar irradiance in three different spectral ranges. Our study is based on two solar-cycles' worth of full-disk photometric images from the San Fernando Observatory, obtained with red, blue and Ca II K-line filters.
Preminger, Dora   +2 more
openaire   +2 more sources

Active Latitude Oscillations Observed on the Sun [PDF]

open access: yesSolar Physics, 2016
Accepted for publication by Solar ...
Kilcik, Ali   +4 more
openaire   +4 more sources

THE ORIGIN OF ENHANCED ACTIVITY IN THE SUNS OF M67 [PDF]

open access: yesThe Astrophysical Journal, 2009
We report the results of the analysis of high resolution photospheric line spectra obtained with the UVES instrument on the VLT for a sample of 15 solar-type stars selected from a recent survey of the distribution of H and K chromospheric line strengths in the solar-age open cluster M67.
Reiners, Ansgar, Giampapa, Mark S.
openaire   +3 more sources

Solar neutrinos as indicators of the Sun’s activity [PDF]

open access: yesInternational Journal of Modern Physics A, 2019
Opportunity of the solar flares (SFs) prediction observing the solar neutrino fluxes is investigated. In three neutrino generations, the evolution of the neutrino flux traveling the coupled sunspots (CSs) which are the SF source is considered. It is assumed that the neutrinos possess both the dipole magnetic moment and the anapole moment while the ...
O. M. Boyarkin, I. O. Boyarkina
openaire   +4 more sources

Faculae Cancel out on the Surfaces of Active Suns

open access: yesThe Astrophysical Journal Letters, 2022
Abstract Surfaces of the Sun and other cool stars are filled with magnetic fields, which are either seen as dark compact spots or more diffuse bright structures like faculae. Both hamper detection and characterization of exoplanets, affecting stellar brightness and spectra, as well as transmission spectra.
Nèmec, N.-E.   +15 more
openaire   +6 more sources

MAGNETO-ACTIVE LONGITUDES IN THE SUN AND STARS

open access: yesBulletin of Taras Shevchenko National University of Kyiv. Astronomy, 2023
An overview of studies of long-term increased magnetic activity in two discrete longitudinal intervals observed on the Sun and on the surface of stars of certain types is reviewed. Active longitudes on the Sun were first discovered at the end of the 19th century.
openaire   +2 more sources

The active sun

open access: yesSpace Science Reviews, 1981
A brief summary is given of observations which will be required to investigate further the structure and energy balance of active regions.
openaire   +2 more sources

The EUV spectrum of the Sun: Quiet- and active-Sun irradiances and chemical composition [PDF]

open access: yesAstronomy & Astrophysics, 2019
We benchmark new atomic data against a selection of irradiances obtained from medium-resolution quiet-Sun spectra in the extreme ultraviolet (EUV), from 60 to 1040 Å. We used as a baseline the irradiances measured during solar minimum on 2008 April 14 by the prototype (PEVE) of the Solar Dynamics Observatory Extreme ultraviolet Variability Experiment ...
openaire   +2 more sources

CMEs and active regions on the sun [PDF]

open access: yesAdvances in Space Research, 2013
The relationship between active regions (ARs) and coronal mass ejections (CMEs) is studied. For this purpose a statistical analysis of 694 CMEs associated with ARs was carried out. We considered the relationship between properties of the CMEs and ARs characterized using the McIntosh classification.
Michałek, Grzegorz, Yashiro, Seiji
openaire   +2 more sources

Millimeter and Microwave Activity of the Sun [PDF]

open access: yesSymposium - International Astronomical Union, 1990
The emission of solar flares at millimeter wavelengths is of great interest both in its own right and because it is generated by the energetic electrons which also emit gamma rays. Since high-resolution imaging at gamma-ray energies is not presently possible, millimeter observations can act as a substitute.
M. R. Kundu, S. M. White
openaire   +1 more source

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