Physical Parameters of Solar X-Ray Jets

By M. Shimojo, Kazunari Shibata. 2000

179 citations recorded by the source corpus.

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Citations in the corpus

A MODEL FOR SOLAR POLAR JETS (2009, background): “These observations strongly suggest that impulsive magnetic reconnection, between the closed field of the bipole and the external open field, is the driving mechanism for the jets (Shibata et al. 1997; Shimojo & Shibata 2000a).”
THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS (2010, background): “Shimojo & Shibata (2000) showed that the thermal energy emitted by the jet is related to the magnetic flux at its chromospheric footpoint.”
Characteristics of EUV Coronal Jets Observed with STEREO/SECCHI (2009, background): “Very early observations of coronal jets were provided by Skylab and, in more details, later by Yohkoh in the soft X-rays (Shimojo et al., 1996; Shimojo and Shibata, 2000).”
Magnetic Topology of Impulsive and Gradual Solar Energetic Particle Events (2002, methodology): “This diagram is similar to the ones considered by Kahler et al. (2001) for impulsive SEP events with CMEs and was proposed by Shimojo & Shibata (2000) to describe X-ray jets and the source of the 10–100 keV electrons that produce interplanetary type III radio bursts (Robinson & Benz 1998).”
Coronal Mass Ejections Associated with Impulsive Solar Energetic Particle Events (2001, background): “Shimojo & Shibata (2000) have measured the physical properties of 16 X-ray jets from small Ñares and interpreted them in terms of Figure 7, in which the jets are driven along open Ðeld lines by evaporation Ñows produced by magnetic reconnection.”
The Two Sources of Solar Energetic Particles (2012, background): “…and Mason 2006; Nitta et al. 2006), where reconnection between open and closed field lines takes place (e.g. Shibata, et al. 1992; Heyvaerts, Priest, Rust 1977; Shimojo and Shibata 2000; Aschwanden (2002); Reames 2002), accelerating electrons and ions that have direct acc ss to open field lines.”