Results 11 to 20 of about 9,915 (239)

Statistical studies of low-power solar flares. Distribution of flares by area, brightness, and classes [PDF]

open access: yesSolar-Terrestrial Physics, 2017
An electronic database has been created for 123801 solar flares that occurred on the Sun over the period from 1972 to 2010. It is based on catalogs of the Solar Geophysical Data (SGD) and Quarterly Bulletin on Solar Activity.
Borovik A.V., Zhdanov A.A.
doaj   +4 more sources

Images of solar flares in HMI continuum

open access: yes, 2021
This dataset contains solar flares in classes B, C, M, and X at HMI Continuum. The images were obtained from the Solar Dynamics Observatory by the Atmospheric Imaging Assembly instrument.
Gradvohl, André Leon Sampaio   +2 more
core   +1 more source

Images of solar flares in 1700 Angstrom wavelength

open access: yes, 2021
This dataset contains solar flares in classes B, C, M, and X at 1700 Angstrom (Å) wavelength. The images were obtained from the Solar Dynamics Observatory by the Atmospheric Imaging Assembly instrument.
Gradvohl, André Leon Sampaio   +2 more
core   +1 more source

THE PROCESSES OF ENERGY RELEASE IN LOW-POWER SOLAR FLARES

open access: yesSolar-Terrestrial Physics, 2019
Using flare patrol data for 1972–2010 [http://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-flares/], we have conducted statistical studies of small solar flares.
Borovik A.V., Zhdanov A.A.
doaj   +1 more source

Solar Flares [PDF]

open access: yesInternational Astronomical Union Colloquium, 1995
AbstractThere are many types of solar flare, but the classic type is a two-ribbon flare with three phases — a preflare phase, a rise phase and a main phase. The properties of these phases are described, together with some recent observational advances in understanding the conditions for solar flares.
openaire   +1 more source

On the classifications of the solar active regions (ARs); Case study for solar cycles 23 and 24

open access: yesEgyptian Journal of Remote Sensing and Space Sciences, 2018
The declining phase of solar cycle 23 is an important case of study. Many high energetic solar flares occurred in 2003. The occurrence of high energetic solar X-ray flares (X-type) is related to solar cycle’s phases and the state of the active regions ...
Wael Mohamed   +2 more
doaj   +1 more source

Comparison of VLF Signal Responses to Solar Flares along Daytime and Nighttime Propagation Paths

open access: yesRemote Sensing, 2023
Solar flares have a severe impact on the near-earth space environment, during which the VLF signals observed by the ground-based instrument exhibit abnormal changes.
Xudong Gu   +9 more
doaj   +1 more source

Measurements and Modeling of the Responses of VLF Transmitter Signals to X‐Class Solar Flares at the Great Wall Station in Antarctica

open access: yesSpace Weather, 2023
Solar flares can severely disturb the Earth's ionosphere, leading to changes of atmospheric chemistry and degradation of Global Navigation Satellite System (GNSS) signals. The key to better assess these effects is to more accurately quantify the electron
Wei Xu   +11 more
doaj   +1 more source

Particle acceleration in the presence of weak turbulence at an X-type neutral point [PDF]

open access: yes, 2012
We simulate the likely noisy situation near a reconnection region by superposing many 2D linear reconnection eigenmodes. The superposition of modes on the steady state X-type magnetic field creates multiple X- and O-type neutral points close to the ...
Petkaki, P.   +4 more
core   +1 more source

Statistical studies of duration of low-power solar flares

open access: yesSolar-Terrestrial Physics, 2018
This paper is a sequel to papers dealing with time parameters of solar flares in the Hα line. Using data from the international flare patrol for 1972–2010, we have determined the mean duration of flares of different importance and classes of area.
Borovik A.V., Zhdanov A.A.
doaj   +1 more source

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