All Tables

Table 1: Slow and Fast Solar Wind Parameters. Cross sections for CX between SW heavy ions and H and He are based on theoretical and experimental work of (Beijers et al. 1994; Bliman et al. 1992; Bonnet et al. 1985; Dijkkamp et al. 1985a,b; Fritsch et al. 1996; Greenwood et al. 2001; Harel et al. 1992, 1998; Ishii et al. 2004; Iwai et al. 1982; Lee et al. 2004; Liu et al. 2005; Phaneuf et al. 1987; Richter et al. 1993; Shimakura et al. 1992; Suraud et al. 1991; Wu et al. 1994).
Table 2: Contribution of the Outer Heliosphere, up to $\sim$ 170 AU UW, $\sim$ 300 AU CW and $\sim$ 3000 AU DW, to the X-ray intensity due to CX between heavy SW ions and IS H atoms and to the total directional X-ray intensity (H+He) within 100 AU.
Table 3: Parameters of XMM-Newton observation of HDFN on June 1, 2001.