Extension of coronal structure into interplanetary space

Geophysical Research Letters

Volumn 24, Issue 10, 1997, Pages 1159-1162

  Woo, Richard ^a   Habbal, Shadia Rifai ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ELECTRON DENSITY MEASUREMENT; LIGHT MEASUREMENT; SCINTILLATION; SOLAR RADIATION; SUN; VELOCITY MEASUREMENT; VOLUME FRACTION;

CORONAL STRUCTURE; INTERPLANETARY SPACE; K CORONAMETER; POLAR CORONAL HOLES; RADIO OCCULTATION MEASUREMENTS; RAYLIKE PLETHORA STRUCTURES; SOLAR WIND; STREAMERS; WHITE LIGHT MEASUREMENTS;

ASTROPHYSICS;

EID: 0031143931     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/97GL01156     Document Type: Article

References (18)

1. Bavassano, B., Woo, R., and Bruno, R., Heliospheric plasma sheet and coronal streamers, Geophys. Res. Lett., 1997, submitted.
2. Fisher, R.R., Lee, R.H., MacQueen, R.M., and Poland, A.I., New Mauna Loa coronagraph systems, Appl. Opt., 20, 1094, 1981.
3. Gosling, J.T., et al., The band of solar wind variability at low helioctraphic latitudes near solar activity minimum: Plasma results from the Ulysses rapid latitude scan, Geophys. Res. Lett., 22, 3329-3332, 1995.
4. Grall, R.R., et al., Rapid acceleration of the polar solar wind, Nature, 379, 429-432, 1996.
5. Guhathakurta, M., Fisher, R., and Woo, R., Radial profile of electron density in a coronal hole from white light coronagraph observations and Ulysses in situ and radio ranging measurements and its solar wind consequences, EOS, 77, F586, 1996.
6. Habbal, S.R., Esser, R., Guhathakurta, M., and Fisher, R.R., Flow properties of the solar wind derived from a two-fluid model with constraints from white light and in situ interplanetary observations, Geophys. Res. Lett., 22, 1465-1468, 1995.
7. Hansteen, V.H., Solar wind theory and modeling, in Solar Wind Eight, eds. D. Winterhalter, J. Gosling, S. Habbal, W. Kurth and M. Neugebauer, AIP Conference Proc., 382, New York, 44-49, 1996.
8. Huddleston, D.E., Woo, R., and Neugebauer, M., Density fluctuations in different types of solar wind flow at 1 AU and comparison with results from Doppler scintillation measurements near the Sun, J. Geophys. Res., 100, 19951-19956, 1995.
9. Koutchmy, S., Study of the June 30, 1973 trans-polar coronal hole, Solar Phys., 51, 399-407, 1977.
10. o, Ap. J., 213, 874-886, 1977.
11. Parker, E.N., Dynamics of the interplanetary gas and magnetic fields, Ap. J., 128, 664-676, 1958.
12. Pätzold, M., Bird, M.K., Edenhofer, P., Asmar, S.W., and McElrath, T.P., Dual-frequency radio sounding of the solar corona during the 1995 conjunction of the Ulysses spacecraft, Geophys. Res. Lett., 22, 3313-3316, 1995.
13. Schwenn, R., Large-scale structure in the interplanetary medium, in Physics of the Inneer Heliosphere I, eds. R. Schwenn and E. Marsch, Springer-Verlag, Berlin, 99-181, 1990.
14. Suess, S. T, et al., The solar wind - Inner heliosphere, in Cosmic Rays in the Heliosphere, eds. L. Fisk, R. Jokipii, G. Simnett, and R. von Steiger, Kluwer, 1997, in press.
15. Woo, R., Kilometre-scale structures in the Sun's corona, Nature, 379, 321-322, 1996a.
16. Woo, R., Detection of low-latitude plumes in the outer corona by Ulysses radio ranging measurements, Ap. J., 464, L95-L98, 1996b.
17. Woo, R., and Habbal, S.R., Finest filamentary structures of the corona in the slow and fast solar wind, Ap. J., 474, L139-L142, 1997.
18. Woo, R., Armstrong, J.W., Bird, M.K., and Pätzold, M., Fine-scale filamentary structure in coronal streamers, Ap. J., 449, L91-L94, 1995.