By Mario Livio, Keith Noll, Massimo Stiavelli
Precis of the achievements of the Hubble house Telescope in its first decade of operation.
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Extra resources for A Decade of Hubble Space Telescope Science (2003)(en)(270s)
Geophys. , 84, 8415. Slipher E. C. 1962 Mars: The Photographic Story. Sky Publishing Corp. Smith, P. , Bell III, J. , Bridges, N. , Britt, D. , Keller, H. , Herkenhoff, K. , Johnson, J. , Kirk, R. , Maki, J. , Malin, M. C. Murchie, S. L. , Parker, T. , Reid, R. , Soderblom, L. , Tomasko, M. , & Wegryn, E. 1997 Science, 278, 1758. Soderblom, L. , Eliason, E. , Sanchez, E. , & Charette, M. P. 1978 Icarus, 34, 446. Tamppari, L. , Zurek, R. , & Paige, D. A. 2000 J. Geophys. , 105, 4087. Wells, E. , & Thomas, P.
FUV/EUV auroral spectra of the north aurora 36 J. T. Clarke: HST images of Jupiter’s UV aurora Figure 9. Polar projection of Jupiter showing the observed locations of auroral emissions from Io’s magnetic footprint. Overplotted are the 6 RJ auroral ovals from the earlier (O6) and modiﬁed (VIP4) magnetic ﬁeld models, showing the improved ﬁts to the footprint locations. Figure from Clarke et al. 1998. were obtained on the second HUT ﬂight in March 1995 simultaneously with WFPC2 images (Morrissey et al.
Interpreting the highest frequency detected as an electron gyrofrequency implied a maximum ﬁeld strength of 10 Gauss. Jupiter’s ionosphere was ﬁrst detected by radio occultation during the Pioneer 10 ﬂyby in 1974 (Kliore et al. 1974), and ground-based telescopic observations ﬁrst detected the plasma torus in the mid 1970s (Brown & Yung 1976). It was during the Voyager 1 ﬂyby in 1979 that Jupiter’s UV auroral were ﬁrst observed (Broadfoot et al. 1979), and during this and the Voyager 2 encounter the long aperture of the UVS was used to map the equatorward extent of the UV auroral emissions.
A Decade of Hubble Space Telescope Science (2003)(en)(270s) by Mario Livio, Keith Noll, Massimo Stiavelli