Results 21 to 30 of about 1,700,755 (212)
The Soft X-Ray and EUV Spectra of Solar Flares [PDF]
International Astronomical Union Colloquium, 1984 The Japanese solar maximum satellite HINOTORI was launched on 21 February 1981, and so far 720 Solar flares were detected including many large flares; the largest observed was a X12 class flare occurred on June 6, 1982. Unfortunately, the data recorder malfunctioned in June, 1982, since then the real time basis observation has been possible to continue.
K. Nishi, K. Tanaka
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Solar flare particle acceleration in collapsing magnetic traps [PDF]
, 2012 Electronic redacted version excludes material for which permission has not been granted by the rights holderThe topic of this thesis is a detailed investigation of different aspects of the particle acceleration mechanisms operating in Collapsing Magnetic
Grady, Keith J.
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The Astrophysical Journal, 2023 Solar flares are complex phenomena emitting all types of electromagnetic radiation and accelerating particles on timescales of minutes, converting magnetic energy to thermal, radiative, and kinetic energy through magnetic reconnections.
Crisel Suarez, Christopher S. Moore
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Characteristics of energetic solar flare electron spectra
The Astrophysical Journal, 1989 A 55 event survey of energy spectra of 0.1-100 MeV interplanetary electrons originating from solar flares as measured by two spectrometers onboard the ISEE 3 (ICE) spacecraft for the years 1978-1982 has been completed. Spectra generated using the maximum flux of a given event in each energy channel were restricted to events with a well-defined flux ...
Dan Moses +3 more
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Extreme ultraviolet imaging of three-dimensional magnetic reconnection in a solar eruption [PDF]
, 2015 X.C., J.Q.S., M.D.D., Y.G., P.F.C. and C.F. are supported by NSFC through grants 11303016, 11373023, 11203014 and 11025314, and by NKBRSF through grants 2011CB811402 and 2014CB744203. C.E.P. and S.J.E. are supported by the UK STFC. J.Z.
Sun, J.Q. +9 more
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Geophysical Research Letters, 2008 Photoelectrons are the main energy source of airglow used to diagnose the state of the ionosphereâthermosphere system. Because of measurement uncertainties and substantial gaps in the historical record, parameterized models of the EUV irradiance and ...
W. K. Peterson +3 more
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Three-dimensional spatial structures of solar wind turbulence from 10 000-km to 100-km scales [PDF]
, 2011 Using the four Cluster spacecraft, we have determined the three-dimensional wave-vector spectra of fluctuating magnetic fields in the solar wind. Three different solar wind intervals of Cluster data are investigated for this purpose, representing ...
Narita, Y. +15 more
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Time distributions of solar energetic particle events: Are SEPEs really random?
, 2009 Solar energetic particle events (SEPEs) can exhibit flux increases of several orders of magnitude over background levels and have always been considered to be random innature in statistical models with no dependence of any one event on the occurrence of ...
Jiggens, P.T.A., Gabriel, S.B.
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The investigation of quasi-separatrix layers in solar magnetic fields [PDF]
, 2011 The structure of the magnetic field is often an important factor in many energetic processes in the solar corona. To determine the topology of the magnetic field features such as null points, separatrix surfaces, and separators must be found.
Restante, Anna Lisa
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Particle acceleration in the presence of weak turbulence at an X-type neutral point [PDF]
, 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
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