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Table 4. Space observatories and instruments used for the relevant observations within the “Sun in Time” project (Güdel, 2007).

From: Variability of solar/stellar activity and magnetic field and its influence on planetary atmosphere evolution

Space observatory

λ [Å ]

E [keV]

XMM-Newton [CCDs]

0.83–83

0.15–15

XMM-Newton [gratings]

6–38

0.33–2.1

ASCA [CCDs]

1.2–31

0.4–10

ROSAT

5.2–124

0.1–2.4

EUVE [gratings]

80–760

0.016–0.15

FUSE [gratings]

920–1180

HST [gratings]

1150–1730

IUE [gratings]

1150–1950

UBVRI [photometry]

3500–8300