1991) aboard Yohkoh (Ogawara et al. 1991) has a better temporal coverage and resolution than previous X-ray images, and et al. (1992) and Strong et al. (1992) discovered the jet phenomenon in SXT images called ““ X-ray jet œœ (Fig. 1). Shimojo et al.
CITATION STYLE
Shimojo, M., & Shibata, K. (2000). Physical Parameters of Solar X‐Ray Jets. The Astrophysical Journal, 542(2), 1100–1108. https://doi.org/10.1086/317024
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