Characteristics of Pi 2 magnetic pulsations observed at the CPMN stations: A review of the STEP results

From analyses of magnetic data from the Circum-pan Pacific Magnetometer Network (CPMN) stations, we can find the following wave characteristics of Pi 2 magnetic pulsations. (1) Pi 2 pulsations observed on the ground are an ensemble of various hydromagnetic modes excited at high, middle, low, and equatorial latitudes. Each mode exhibits its own propagation (timing) and spatial illumination. (2) There are apparent longitudinal propagation and latitudinal time delays of the maximum Pi 2 magnetic energy among the CPMN stations within 100 sec. (3) When a single low-latitude station is located in the sectors of 00–24 hr LT, 20–03 hr local time (LT), and 23-01 hr LT, respectively, 62%, 79%, and 100% of auroral breakups identified by the Polar satellite have associated Pi 2s. 66% of the low-latitude Pi 2s occur within 1 min of the auroral breakups, and 85% within 2 min. Pi 2s are still a good indicator of substorm onsets, but they should be used with care.

[1]  Takao Saito,et al.  Magnetic pulsation Pi2 and substorm onset , 1976 .

[2]  Robert L. McPherron,et al.  Satellite studies of magnetospheric substorms on August 15, 1968. IX - Phenomenological model for substorms. , 1973 .

[3]  T. Yeoman,et al.  Phase and spectral power of mid-latitude Pi2 pulsations: evidence for a plasmaspheric cavity resonance , 1989 .

[4]  J. Chao,et al.  Spectral power of low-latitude Pi 2 pulsations at the 210° magnetic meridian stations and plasmaspheric cavity resonances , 2000 .

[5]  K. Yumoto External and Internal Sources of Low-Frequency MHD Waves in the Magnetosphere-A Review , 1988 .

[6]  David G. Sibeck,et al.  Observation of IMF and seasonal effects in the location of auroral substorm onset , 2001 .

[7]  John V. Olson,et al.  Pi2 pulsations and substorm onsets: A review , 1999 .

[8]  J. Samson,et al.  Latitude‐dependent characteristics of high‐latitude Pc 4 and Pc 5 micropulsations , 1972 .

[9]  R. McPherron Satellite studies of magnetospheric substorms on August 15, 1968. I - State of the magnetosphere. , 1973 .

[10]  C. Meng,et al.  Particle injections with auroral expansions , 2001 .

[11]  C. Meng,et al.  Evaluation of low‐latitude Pi2 pulsations as indicators of substorm onset using Polar ultraviolet imagery , 2000 .

[12]  K. Yumoto,et al.  Generation and propagation mechanisms of low-latitude magnetic pulsations ― A review , 1986 .

[13]  A. Hasegawa,et al.  A theory of long‐period magnetic pulsations: 2. Impulse excitation of surface eigenmode , 1974 .

[14]  M. Freeman,et al.  A comparison of midlatitude Pi 2 pulsations and geostationary orbit particle injections as substorm indicators , 1994 .

[15]  K. Yumoto,et al.  Pi2 magnetic pulsations as response on spatio‐temporal oscillations of auroral arc current system , 2000 .

[16]  K. Yumoto Initial Results from the 210° Magnetic Meridian Project-Review , 1995 .

[17]  B. J. Fraser,et al.  Some aspects of the relation between Pi 1-2 magnetic pulsations observed at L = 1.3-2.1 on the ground and substorm-associated magnetic field variations in the near-Earth magnetotail observed by AMPTE CCE , 1989 .

[18]  K. Yumoto,et al.  On the cavity mode nature of low‐latitude Pi 2 pulsations , 1991 .

[19]  Kiyohumi Yumoto,et al.  The step 210° Magnetic meridian network Project , 1996 .

[20]  K. Yumoto Evidences of Magnetospheric Cavity Pi2 Waves , 1990 .

[21]  J. Olson,et al.  Characteristics of energy transfer of Pi 2 magnetic pulsations: Latitudinal dependence , 2000 .

[22]  A. Hasegawa,et al.  A theory of long period magnetic pulsations 1 , 1974 .

[23]  M. Lester,et al.  Pi 2 pulsations and the substorm current wedge: Low‐latitude polarization , 1989 .

[24]  W. F. Stutart A mechanism of selective enhancement of Pi'2's by the plasmasphere , 1974 .

[25]  B. J. Fraser,et al.  Characteristics of Low-Latitude Pi 2 Pulsations along the 210° Magnetic Meridian , 1996 .

[26]  C. Meng,et al.  A Fresh Look at Substorm Onset Identifiers , 1998 .

[27]  Lou‐Chuang Lee,et al.  Observations of Pi 2 pulsations at a very low latitude (L = 1.06) station and magnetospheric cavity resonances , 1991 .

[28]  B. Anderson,et al.  Upper Atmosphere Research Satellite observation of a Pi2 pulsation , 1999 .

[29]  Y. Koyama,et al.  Magnetic pulsation Pi2 as a sensitive indicator of magnetospheric substorm , 1976 .

[30]  A. Matsuoka,et al.  Pi2 pulsations observed from the Akebono satellite in the plasmasphere , 1998 .

[31]  T. Mukai,et al.  Substorm onset timing: The December 31, 1995, event , 1999 .

[32]  D. Southwood Some features of field line resonances in the magnetosphere , 1974 .

[33]  Takao Saito,et al.  Geomagnetic pulsations , 1969 .

[34]  A. Yoshikawa,et al.  Wave characteristics of daytime and nighttime Pi 2 pulsations at the equatorial and low latitudes , 1997 .

[35]  K. Shiokawa,et al.  Correlation of High- and Low-Latitude Pi 2 Magnetic Pulsations Observed at 210°Magnetic Meridian Chain Stations , 1994 .

[36]  S. Krimigis,et al.  AMPTE CCE Observations of Pi 2 Pulsations in the Inner Magnetosphere (Paper 92GL01283) 1447 , 1992 .

[37]  Brian J. Anderson,et al.  Statistical analysis of Pi 2 pulsations observed by the AMPTE CCE Spacecraft in the inner magnetosphere , 1995 .