Abstract
The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) has observed the extended solar corona between 1 and 10 R· for more than two years. We review spectroscopic and polarimetric measurements made in coronal holes, equatorial streamers, and coronal mass ejections, as well as selected non-solar targets. UVCS/SOHO has provided a great amount of empirical information about the physical processes that heat and accelerate the solar wind, and about detailed coronal structure and evolution.
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Allen, L. A., Habbal, S. R., and Hu, Y. Q.: 1998, J. Geophys. Res. 103, 6551.
Antonucci, E., et al.: 1997a, Ap. J. Letters 490, L183.
Antonucci, E., Giordano, S., Benna, C., Kohl, J. L., Noci, G., Michels, J., and Fineschi, S.: 1997b, in The Corona and Solar Wind Near Minimum Activity, Fifth SOHO Workshop, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-404, 175.
Ciaravella, A., et al.: 1997a, Ap. J. Letters 491, L59.
Ciaravella, A., et al.: 1997b, in Correlated Phenomena at the Sun, in the Heliosphere and in Geospace, 31st ESLAB Symposium, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-415, 543.
Ciaravella, A., et al.: 1998, in preparation.
Collier, M. R., Hamilton, D. C., Gloeckler, G., Bochsler, P., and Sheldon, R. B.: 1996, Geophys. Res. Letters 23, 1191.
Corti, G., Poletto, G., Romoli, M., Michels, J., Kohl, J., and Noci, G.: 1997, in The Corona and Solar Wind Near Minimum Activity, Fifth SOHO Workshop, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-404, 289.
Cranmer, S. R.: 1998, Ap. J. 508, in press (1 Dec 1998).
Cranmer, S. R., et al.: 1999, Ap. J. 511, in press (20 Jan 1999).
Davila, J. M.: 1994, Ap. J. 423, 871.
Dobrzycka, D., Cranmer, S. R., Panasyuk, A. V., Strachan, L., and Kohl, J. L.: 1998, J. Geophys. Res., submitted.
Esser, R., Fineschi, S., Dobrzycka, D., Habbal, S. R., Edgar, R. J., Raymond, J. C., Kohl, J. L., and Guhathakurta, M.: 1998, Ap. J., submitted.
Feldman, W. C., and Marsch, E.: 1997, in Cosmic Winds and the Heliosphere, ed. J. R. Jokipii, C. P. Sonett, and M. S. Giampapa (Tucson: University of Arizona Press), 617.
Fineschi, S., Kohl, J. L., Strachan, L., Gardner, L. D., Romoli, M., Huber, M. C. E., and Noci, G.: 1997, presented at The Corona and Solar Wind Near Minimum Activity, Fifth SOHO Workshop, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-404.
Fleck, B., Domingo, V., and Poland, A., eds.: 1995, The SOHO Mission, Solar Phys. 162, 1–531.
Giordano, S., Antonucci, E., Benna, C., Romoli, M., Noci, G., Kohl, J. L., Fineschi, S., Michels, J., and Naletto, G.: 1997a, in The Corona and Solar Wind Near Minimum Activity, Fifth SOHO Workshop, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-404, 413.
Giordano, S., Antonucci, E., Benna, C., Kohl, J. L., Noci, G., Michels, J., and Fineschi, S.: 1997b, in Correlated Phenomena at the Sun, in the Heliosphere and in Geospace, 31st ESLAB Symposium, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-415, 327.
Habbal, S. R., Woo, R., Fineschi, S., O'Neal, R., Kohl, J., and Korendyke, C.: 1997, Ap. J. Letters 489, L103.
Kohl, J. L., et al.: 1995, Solar Phys. 162, 313.
Kohl, J. L., Strachan, L., and Gardner, L. D.: 1996, Ap. J. Letters 465, L141.
Kohl, J. L., et al.: 1997a, Solar Phys. 175, 613.
Kohl, J. L., et al.: 1997b, Adv. Space Res. 20,no. 1, 3.
Kohl, J. L., et al.: 1998a, Ap. J. Letters 501, L127.
Kohl, J. L., et al.: 1998b, Ap. J. Letters, submitted.
Li, J., Raymond, J. C., Acton, L. W., Kohl, J. L., Romoli, M., Noci, G., and Naletto, G.: 1998b, Ap. J., submitted.
Li, X., Habbal, S. R., Kohl, J. L., and Noci, G.: 1998a, Ap. J. Letters 501, L133.
Maccari, L., et al.: 1997, presented at Correlated Phenomena at the Sun, in the Heliosphere and in Geospace, 31st ESLAB Symposium, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-415.
Noci, G., Kohl, J. L., and Withbroe, G. L.: 1987, Ap. J. 315, 706.
Noci, G., et al.: 1997a, Adv. Space Res. 20,no. 12, 2219.
Noci, G., et al.: 1997b, in The Corona and Solar Wind Near Minimum Activity, Fifth SOHO Workshop, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-404, 75.
Ofman, L., Romoli, M., Poletto, G., Noci, G., and Kohl, J. L.: 1997, Ap. J. Letters 491, L111.
Olsen, E. L., Leer, E., and Holzer, T. E.: 1994, Ap. J. 420, 913.
Panasyuk, A. V.: 1998, J. Geophys. Res., in press.
Raymond, J. C., et al.: 1997, Solar Phys. 175, 645.
Raymond, J. C., Suleiman, R., Kohl, J. L., and Noci, G.: 1998a, Space Sci. Rev., this volume.
Raymond, J. C., et al.: 1998b, Ap. J., in press.
Raymond, J. C., et al.: 1998c, in preparation.
Romoli, M., et al.: 1997, in The Corona and Solar Wind Near Minimum Activity, Fifth SOHO Workshop, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-404, 633.
Strachan, L., Kohl, J. L., Weiser, H., Withbroe, G. L., and Munro, R. H.: 1993, Ap. J. 412, 410.
Strachan, L., et al.: 1997, in The Corona and Solar Wind Near Minimum Activity, Fifth SOHO Workshop, ed. A. Wilson (Noordwijk, The Netherlands: ESA), ESA SP-404, 691.
Wang, Y.-M.: 1994, Ap. J. Letters 435, L153.
Wang, Y.-M.: 1998, Ap. J. Letters 501, L145.
Withbroe, G. L., Kohl, J. L., Weiser, H., and Munro, R. H.: 1982, Space Sci. Rev. 33, 17.
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Cranmer, S.R., Kohl, J.L. & Noci, G. UVCS/SOHO: The First Two Years. Space Science Reviews 85, 341–348 (1998). https://doi.org/10.1023/A:1005175106042
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DOI: https://doi.org/10.1023/A:1005175106042