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Nuclear Physics: Exploring the Heart of Matter
Detection of spike-like structures near the front of type-II bursts. Geophysical Research Letters, Volume 46, Issue 1, pp. Relation between solar flares and halo coronal mass ejections. Journal of Astrophysics and Astronomy, Volume 40, Issue 1, article id. A4, 21 pp.
Study of some characteristics of solar energetic particles and associated solar activities during New Astronomy, Volume 69, p. Small-scale motions in solar filaments as the precursors of eruptions.
The Heliosphere through the Solar Activity Cycle
Study of reconnection rates and light curves in solar flares from low and mid chromosphere. The extreme space weather event in September Is the enhancement of type II radio bursts during CME interactions related to the associated solar energetic particle event? Research in Astronomy and Astrophysics , Volume 19, Issue 1, article id.
Solar Physics, Volume , Issue 1, article id. Solar Physics, Volume , Issue 2, article id. Space Weather, Volume 17, Issue 1, pp. The Astrophysical Journal, Volume , Issue 1, article id. L2, 8 pp.
The Astrophysical Journal, Volume , Issue 2, article id. Pre-eruption processes: heating, particle acceleration and the formation of a hot channel before the October 20 M9. Accepted for publication in The Astrophysical Journal. Formation and eruption of sigmoidal structure from a weak field region of NOAA Accepted for Publication in The Astrophysical journal on 19 February, Properties and relationship between solar eruptive flares and Coronal Mass Ejections during rising phase of Solar Cycles 23 and Advances in Space Research, Volume 61, Issue 1, p.
Solar flares, CMEs and solar energetic particle events during solar cycle Advances in Space Research, Volume 61, Issue 2, p. Effects of space weather on the ionosphere and LEO satellites' orbital trajectory in equatorial, low and middle latitude. Advances in Space Research, Volume 61, Issue 7, p. Advances in Space Research, Volume 61, Issue 9, p. Advances in Space Research, Volume 62, Issue 2, p. A statistical study of CME-Preflare associated events. Ionospheric and thermospheric response to the February geomagnetic storm over north Africa. Annales Geophysicae, Volume 36, Issue 4, , pp.
A, 6 pp. Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test. A25, 12 pp.
The Heliosphere Through the Solar Activity Cycle Springer Praxis Books
Very narrow coronal mass ejections producing solar energetic particles. A34, 6 pp. Association of solar flares with coronal mass ejections accompanied by Deca-Hectometric type II radio burst for two solar cycles 23 and Astrophysics and Space Science, Volume , Issue 5, article id. Astrophysics and Space Science, Volume , Issue 6, article id. Solar radio bursts as a tool for space weather forecasting. Klein, K.
Comptes rendus — Physique, Volume 19, Issue , p Earth, Moon, and Planets, Online First. Geomagnetism and Aeronomy, Volume 58, Issue 1, pp. Geomagnetism and Aeronomy, Volume 58, Issue 4, pp. Geomagnetism and Aeronomy, Volume 58, Issue 8, pp. Geophysical Research Letters, Volume 45, Issue 2, pp. Higher-speed coronal mass ejections and their geoeffectiveness. Journal of Astrophysics and Astronomy, Volume 39, Issue 3, article id.
Signature of a possible relationship between the maximum CME speed index and the critical frequencies of the F1 and F2 ionospheric layers: Data analysis for a mid-latitude ionospheric station during the solar cycles 23 and Type II solar radio burst band-splitting: Measure of coronal magnetic field strength. Multi-instrument view on solar eruptive events observed with the Siberian Radioheliograph: From detection of small jets up to development of a shock wave and CME. Periodic behaviour of coronal mass ejections, eruptive events, and solar activity proxies during solar cycles 23 and On the relationship between filaments and solar energetic particles.
Sun-to-earth propagation of the June 21 coronal mass ejection revealed by optical, EUV, and radio observations.
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- Solar activity catalogue en ligne.
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Comparative analysis of the proton generation efficiency during 17 March and 11 April solar flares. Solar energetic particle catalogs: Assumptions, uncertainties and validity of reports. Coronal flux ropes and their interplanetary counterparts. Extreme solar storms based on solar magnetic field. Solar wind diamagnetic structures as a source of substorm-like disturbances.
Understanding the twist distribution inside magnetic flux ropes by anatomizing an interplanetary magnetic cloud. Halo Coronal Mass Ejections during Solar Cycle reconstruction of the global scenario and geoeffectiveness. A probabilistic approach to the drag-based model. A11, 10 pp.
A37, 14 pp. An operational solar wind prediction system transitioning fundamental science to operations. A39, 21 pp. A40, 32 pp. Flux rope breaking and formation of a rotating blowout jet.
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Dispersively formed quasi-periodic fast magnetosonic wavefronts due to the eruption of a nearby mini-filament. Magnetic evolution linked to the interrelated activity complexes involving transequatorial coronal holes. Formation and dynamics of a solar eruptive flux tube. Nature Communications, Volume 9, id. Kink-induced full and failed eruptions of two coupled flux tubes of the same filament.
New Astronomy, Volume 59, p. Solar flares associated coronal mass ejection accompanied with DH type II radio burst in relation with interplanetary magnetic field, geomagnetic storms and cosmic ray intensity. New Astronomy, Volume 60, p. On some characteristics of large kinetic energy coronal mass ejections during New Astronomy, Volume 63, p. Physical Review Letters, Volume , Issue 13, id.
Space weather at planet Venus during the forthcoming BepiColombo flybys. Planetary and Space Science, Volume , p. Coronal mass ejection hits mercury: A. Flares before and after coronal mass ejections. Disintegration of an eruptive filament via interactions with quasi-separatrix layers. Solar Physics, Volume , Issue 3, article id. Couldn't find your answer? Select a query type below and message the shop directly. Your message was sent successfully. You can expect a response within 2 business days which will be displayed in your Message Centre. Ask a question: 0 Answers.
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