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Fractals, 1995
When a chaotic signal is used to force a switching-type variable which dependent on the momentary magnitude of the chaotic stimulus either shows a damped or an autocatalytic response, a new dynamical phenomenon arises. It is reminiscent of the “flares” observed in astrophysical situations.
Otto E. Rössler, Georg C. Hartmann
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When a chaotic signal is used to force a switching-type variable which dependent on the momentary magnitude of the chaotic stimulus either shows a damped or an autocatalytic response, a new dynamical phenomenon arises. It is reminiscent of the “flares” observed in astrophysical situations.
Otto E. Rössler, Georg C. Hartmann
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Vision-Based Monitoring of Flare Soot
IEEE Transactions on Instrumentation and Measurement, 2020The flare stack is a typical flare gas combustion facility used to guarantee the safe production of petrochemical plants, refineries, and other enterprises.
Ke Gu, Yonghui Zhang, J. Qiao
semanticscholar +1 more source
Auroral flares and solar flares
Space Science Reviews, 1975The morphology of development of auroral flares (magnetospheric substorms) for both electron and proton auroras is summarized, based on ground-based as well as rocket-borne and satellite-borne data with specific reference to the morphology of solar flares.
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A stellar flare−coronal mass ejection event revealed by X-ray plasma motions
Nature Astronomy, 2019Coronal mass ejections (CMEs), often associated with flares1–3, are the most powerful magnetic phenomena occurring on the Sun. Stars show magnetic activity levels up to ten thousand times higher4, and CME effects on stellar physics and circumstellar ...
C. Argiroffi +8 more
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Periodicity of the Flare Frequency of Flare Stars
Astrophysics, 2019Data from the Kepler Orbital Observatory are used in a statistical study of the periodic/cyclical variability of the flare frequency of 76 flare stars. Corresponding periodic functions of the flare frequency are obtained and a possible periodicity of the flare frequency with a period equal to the star’s rotation period is tested.
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Cyclic flaring activity of flare stars
Astrophysics, 2010Methods of detecting probable cycles in the flaring activity of flare stars and determining the cycle durations are examined. A new method of detecting a cycle of flaring activity and determining its duration is proposed assuming periodic flaring activity.
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Poor responders: to flare or not to flare?
Fertility and Sterility, 2023Katherine M, Baker, Jennifer L, Eaton
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Variation of the flare frequency of flare stars
Astrophysics, 1999The question of the possible variation of the flare frequency of flare stars is considered.
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AIP Conference Proceedings, 2007
Solar two ribbon flares are commonly explained by magnetic field reconnections in the high corona. During the reconnection energetic particles (electrons and protons) are accelerated from the reconnection site. These particles are following the magnetic field lines down to the chromosphere.
B. Schmieder +6 more
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Solar two ribbon flares are commonly explained by magnetic field reconnections in the high corona. During the reconnection energetic particles (electrons and protons) are accelerated from the reconnection site. These particles are following the magnetic field lines down to the chromosphere.
B. Schmieder +6 more
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Variation in the Flare Frequency of Flare Stars. III. Flare Stars in the Orion Association
Astrophysics, 2002The possible variation of the flare frequency of flare stars in the Orion association is considered. It is shown that of the 23 chosen stars, each having exhibited four or more flares, a change in flare frequency at the 0.1 significance level can be suspected for 13.
L. A. Sargsyan, A. A. Akopian
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