Richard J. Edgar

TL;DR: In this article, a series of models for the plasma properties along open magnetic flux tubes rooted in solar coronal holes, streamers, and active regions are presented, which represent the first self-consistent solutions that combine chromospheric heating driven by an empirically guided acoustic wave spectrum; coronal heating from Alfven waves that have been partially reflected, then damped by anisotropic turbulent cascade; and solar wind acceleration from gradients of gas pressure, acoustic wave pressure, and Alfven wave pressure.

TL;DR: The newly discovered supernova remnant G266.2-1.2 (RX J0852.0-4622) was observed with ASCA for 120 ks as mentioned in this paper.

TL;DR: In this paper, a limit on the turbulent wave motion of the background plasma and the thermal motions of the protons and Mg+9 and O+5 ions is estimated from the measured line widths and electron densities derived from white light coronagraph observations, assuming WKB approximation at radial distances covered by the observations.

TL;DR: In this paper, Chandra ACIS-S3 was used to model the diffuse component of the cosmic X-ray background (CXB) in the 0.3-7 keV band for four directions at high Galactic latitudes.

TL;DR: The newly discovered supernova remnant G266.2-1.2 (RX J0852.0--0462) was observed with ASCA for 120 ks as mentioned in this paper.