INTERNATIONAL JOURNAL OF GEOMAGNETISM AND AERONOMY VOL. 5, GI2011, doi:10.1029/2004GI000069, 2004

References

Benevolenskaya, E. A., A. G. Kosovichev, and P. H. Sherer (2001), Detection of high-latitude waves of solar coronal activity in extreme-ultraviolet data from the Solar and Heliospheric Observatory EUV imaging telescope, Astrophys. J., 554, L107.

Bohlin, J. D. (1970), Solar coronal streamers. I: Observed locations, general evolution and classification, Sol. Phys., 12, 240.

Hoeksema, J. T. (1984), Structure and evolution of the large scale solar and heliospheric magnetic fields, Ph.D. dissertation, Stanford Univ., Stanford, Calif..

Eselevich, V. G., and M. V. Eselevich (2002), Study of the nonradial directional property of the rays of the streamer belt and chains in the solar corona, Sol. Phys., 208, 5.

Koutchmy, S., and M. Loucif (1984), Empirical model of the solar corona using solar-cycle related parameters, in: Hydromagnetics of the Sun, Proceedings of the 4th European Meeting Solar Physics, p. 265-267, European Space Agency, Noordwijk, Netherlands.

Loucif, M., and S. Koutchmy (1989), Solar cycle variations of coronal structures, Astron. Astrophys. Suppl. Ser., R77, 45.

Makarov, V. I. (1994), Global magnetic activity in 22-year solar cycle, Sol. Phys., 150, 359.

Nesmianovich, A. F. (1965),, Solar Corona and Corpuscular Radiation in the Interplanetary Space (in Russian), Naukova dumka, Kiev, Ukraine.

Tlatov, A. G., and V. I. Makarov (2002), Features of the corona distribution at altitudes of 1.15R-2.0R according to the data of the Mark-3 coronagraph, in: Solar Activity and Cosmic Rays, edited by V. I. Makarov and V. N. Obridko (in Russian), p. 531, GAO, St. Petersburg, Russia.

Tlatov, A. G., and V. I. Makarov (2003), Variations of corona brightness with the height in the observations of SOHO/EIT-171A in 1996-2002, in: Actual Problems of Physics of Solar and Star Activity (in Russian), p. 181, IPFAN, Nizhny Novgorod, Russia.

Wang, Y.-M., and N. R. Sheeley, Jr. (1992), On potential field models of the solar corona, Astrophys. J., 392, 310.

Zhao, X., and J. T. Hoeksema (1995), Predicting the heliospheric magnetic field using the current sheet-source surface model, Adv. Space Res., 16, (9), 181.



AGU

Citation: Kim, Gun-Der, V. I. Makarov, and A. G. Tlatov (2004), Measurements of brightness and nonradial direction of coronal streamers according to data of SOHO/Large Angle and Spectrometric Coronagraph Experiment (LASCO)-C2, Int. J. Geomagn. Aeron., 5, GI2011, doi:10.1029/2004GI000069.

Copyright 2004 by the American Geophysical Union

Powered by TeXWeb (Win32, v.1.5).