Up: Magnetosphere on May 11,
- Bol'shakova and Troitskaya, 1968
Bol'shakova, O. V., and V. A. Troitskaya, Relation of the IMF direction
to the system of stable oscillations, Dokl. Akad.Nauk. SSSR, 180,
- Greenstadt et al., 1980
Greenstadt, E. W., C. T. Russell, and M. M. Hoppe, Magnetic field
orientation and suprathermal ion streams in the Earth's foreshock,
, 85, 3473, 1980.
- Greenstadt and Olson, 1977
Greenstadt, E. W., and J. V. Olson, A contribution to ULF activity
in the Pc 3-4 range correlated with IMF radial orientation,
J. Geophys. Res., 82, 4991, 1977.
- Gul'elmi, 1974
Gul'elmi, A. V., Diagnostics of the magnetosphere and interplanetary
medium by means of pulsations, Space Sci. Rev., 16, 331, 1974.
- Hoppe et al., 1981
Hoppe, M. M., C. T. Russell, L. A. Frank, T. E. Eastman, and E. W.
Greenstadt, Upstream hydromagnetic waves and their association with
backstreaming ion population: ISEE 1 and 2 observations, J. Geophys.
Res., 86, 4471, 1981.
- Le, 1991
Le, G., Generation of upstream ULF waves in the Earth's foreshock,
Ph.D. dissertation, 230 pp., University of California, Los Angeles,
CA, June 1991.
- Le and Russell, 1990
Le, G., and C. T. Russell, Observations of the magnetic fluctuation
enhancement in the Earth's foreshock region, Geophys. Res. Lett.,
17, 905, 1990.
- Le and Russell, 1992
Le, G., and C. T. Russell, A study of ULF wave foreshock morphology,
I. ULF foreshock boundary, Planet. Space Sci., 40, 1203, 1992.
- Le et al., 1999
Le, G., C. T. Russell, and S. M. Petrinec, The magnetosphere on May 11,
1999, the day the solar wind almost disappeared: I. Current systems,
Geophys. Res. Lett., submitted, 1999.
- Lepping et al., 1995
Lepping, R. P., et al., The Wind magnetic field investigation,
Space Sci. Rev., 71, 207, 1995.
- Luhmann et al., 1986
Luhmann, J. G., C. T. Russell, and R. C. Elphic, Spatial distribution
of magnetic field fluctuations in the dayside magnetospheath, J.
Geophys. Res., 91, 1711, 1986.
- Odera, 1986
Odera, T. J., Solar wind controlled pulsations: A review,
it Rev. Geophys., 24, 55, 1986.
- Russell et al., 1995
Russell, C. T., R. C. Snare, J. D. Means, D. Pierce, D. Dearborn, M.
Larson, G. Barr, and G. Le, The GGS/Polar magnetic fields investigation,
it Space Sci. Rev., 71, 563, 1995.
- Singer et al., 1977
Singer, H. J., C, T. Russell, M. G. Kivelson, E. W. Greenstadt, and
J. V. Olson, Evidence of the control of Pc 3, 4 magnetic pulsation
by the solar wind velocity, Geophys. Res. Lett., 4, 377, 1977.
- Troitskaya, 1994
Troitskaya, V. A., History of the study of upstream sources of ULF waves,
in Solar Wind Sources of Magnetospheric Ultra-Low-Frequency
Waves, edited by M. Engebretson, K. Takahashi and M. Scholer,
Geophys. Monogr. Ser. 81, pp. 45, American Geophysics Union,
Washington, D. C., 1994.
- Troitskaya et al., 1971
Troitskaya, V. A., T. A. Plyasova-Bakunina, and A. V. Gul'elmi,
Relationship between Pc 2-4 pulsations and the interplanetary field,
Dokl. Aka. Nauk. SSSR, 197, 1313, 1971.
Schematic of foreshock geometry and spacecraft
locations in the V-B plane (the plane that contains the solar
wind velocity and the IMF) for 01-11 UT, May 11.
Simultaneous observed magnetic field data in the foreshock
(red) and in the undisturbed solar wind (blue) on May 11. The top
panels are time series of the magnetic field. The bottom panels are
corresponding power spectra (the sum of power in all
Dynamic power spectra of Polar magnetic field data in By
GSM component from 07 to 10 UT on May 11 (top) and May 14 (bottom).
Dynamic power spectra of the H-component of ground-based
magnetic field from IGPP/LANL mid-latitudes stations AFA, LAL,
Up: Magnetosphere on May 11,