Results 11 to 20 of about 53,020 (220)

Behaviour of electron content in the ionospheric d-region during solar x-ray flares [PDF]

open access: yes, 2016
One of the most important parameters in ionospheric plasma research also having a wide practical application in wireless satellite telecommunications is the total electron content (TEC) representing the columnal electron number density. The F region with
M. Drakul   +5 more
semanticscholar   +1 more source

Some studies on low-frequency signal in relation to X-ray flares and climatic conditions [PDF]

open access: yesAnnales Geophysicae, 1994
The statistical behaviour of the sudden enhancement in signal strength (SES) in relation to solar X-ray flares has been studied for the near east-west propagation of 40 kHz radio waves from Sanwa (36°11'N; 139°51'E) in Japan to Calcutta (22°34'N; 88 ...
S. K. Sarkar, B. K. De
doaj   +1 more source

The existence of hot X-ray onsets in solar flares [PDF]

open access: yesAstronomy & Astrophysics, 2023
It is well known among the scientific community that solar flare activity often begins well before the main impulsive energy release. Our aim is to investigate the earliest phase of four distinct flares observed by Solar Orbiter/STIX and determine the ...
A. Battaglia   +11 more
semanticscholar   +1 more source

Solar X-ray flare hazards on the surface of Mars [PDF]

open access: yesPlanetary and Space Science, 2007
Putative organisms on the Martian surface would be exposed to potentially high doses of ionizing radiation during strong solar X-ray flares. We extrapolate the observed flare frequency-energy release scaling relation to releases much larger than seen so far for the sun, an assumption supported by observations of flares on other solar- and subsolar-mass
Smith, David S., Scalo, John M.
openaire   +2 more sources

The Periodic and Temporal Behaviors of Solar X-Ray Flares in Solar Cycles 23 and 24

open access: yesAstrophysical Journal, 2019
The recent solar cycles 23 and 24 are thought to be unusually quiet with more prolonged periods. Both sunspot groups and solar soft X-ray (SXR) flares show a decline in numbers comparable to cycles 21 and 22.
Jacob Oloketuyi, Yu Liu, Mingyu Zhao
semanticscholar   +1 more source

X-Ray Polarization of Solar Flares Measured with Rhessi [PDF]

open access: yesSolar Physics, 2006
The degree of linear polarization in solar flares has not yet been precisely determined despite multiple attempts to measure it with different missions. The high energy range in particular has very rarely been explored, due to its greater instrumental difficulties.
Suarez-Garcia, E.   +6 more
openaire   +3 more sources

The First AGILE Solar Flare Catalog

open access: yesThe Astrophysical Journal Supplement Series, 2023
We report the Astro-rivelatore Gamma a Immagini LEggero (AGILE) observations of solar flares, detected by the onboard anticoincidence system in the 80–200 keV energy range, from 2007 May 1 to 2022 August 31. In more than 15 yr, AGILE detected 5003 X-ray,
A. Ursi   +11 more
doaj   +1 more source

Detection of Solar Flares from the Analysis of Signal-to-Noise Ratio Recorded by Digisonde at Mid-Latitudes

open access: yesRemote Sensing, 2022
This work proposes a new indirect method to detect the impact of solar flares on ionospheric sounding measurements, i.e., on the signal-to-noise ratio of ionospheric reflected radio signals. The method allows us to detect and characterize the ionospheric
Victor de Paula   +4 more
doaj   +1 more source

Examining the Potential of the Super Dual Auroral Radar Network for Monitoring the Space Weather Impact of Solar X‐Ray Flares

open access: yesSpace Weather, 2018
Increased electron density in the ionosphere due to photoionization by radiation emitted during a solar X‐ray flare impacts high‐frequency (HF) radio wave propagation.
R. Fiori   +6 more
semanticscholar   +1 more source

Strong influence of solar X-ray flares on low-frequency electromagnetic signals in middle latitudes

open access: yesAnnals of Geophysics, 2019
. In this paper we analysed sudden phase anomalies (SPAs) of VLF–LF signals recorded at Graz (Austria), Birr (Ireland) and Moscow (Russia) stations during two strong solar flares in September 2017.
A. Rozhnoi   +7 more
semanticscholar   +1 more source

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