| Spacecraft | Researcher - Institute | Main Results of the Study | Reference |
|---|---|---|---|
| CRRES | N. P. Meredith (MSSL) R. B. Horne (NERC) R. M. Thorne (ATMOS) D. Summers (MATH-MUN) R. R. Anderson (DPA-UI) | Variability of plasmaspheric hiss (0.1 < f < 2kHz) with respect to spatial location and to substorm activity measured by AE*, defined as the maximum value of the AE index in the previous 3 hours. |
J. Geophys. Res., 109, A06209, doi:10.1029/2004JA010387, 2004 |
| CRRES | N. P. Meredith (MSSL) R. B. Horne (NERC) R. M. Thorne (ATMOS) R. R. Anderson (DPA-UI) | Global maps of the lower-band chorus magnetic field wave intensities observed by CRRES and the important ratio fpe/fce as a function of L, MLT and magnetic activity and also as a function of x, GSM z, and MLT region for active conditions (AE > 300 nT). |
Geophys. Res. Lett., 30, 16, SSC 7, 1871, doi:10.1029/2003GL017698, 2003 |
| Viking | F. Darrouzet (BIRA-IASB) J. Lemaire (BIRA-IASB) W. Spjeldvik (WSU) G. Gustafsson (IRF-U) C. Dyck (BIRA-IASB) C. Hann (BIRA-IASB) | Data-based model of the electromagnetic power spectral density in the VLF band (10-46 kHz) as surveyed onboard the Swedish Viking spacecraft in the high-latitude region in the northern hemisphere. |
Adv. Space Res., 32/3, 323-328, 2003 |
| Dynamics Explorer 1 | R. André (LPCE) F. Lefeuvre (LPCE) F. Simonet (CEA) U.S. Inan (STAR-DEE-US) | Model of the average spectrum amplitude of waves in the 1Hz-500kHz frequency band, as a function of the spatial position and the magnetic activity with magnetic field data. | Ann. Geophysicae, 20, 981-996, 2002 |
| CRRES | B. J. Fraser (CRCSS) T. S. Nguyen (CRCSS) | The occurrence of electromagnetic ion cyclotron (EMIC) waves over L = 3.5-8 by the CRRES spacecraft in the equatorial middle magnetosphere as a function of MLT and MLat. | J. Atmos. Solar-Terr. Phys., 63, 1225-1247, 2001 |
| EXOS-D | Y. Kasahara (GSEC-UK) T. Hosoda (GSEC-UK) T. Mukai (ISAS) S. Watanabe (ISAS) I. Kimura (RASC) H. Kojima (RASC) R. Niitsu (GSEC-UK) | A Kp-dependent statistical study on the spatial and temporal distribution of the conituous broadband noise measured by EXOS-D (Akebono) as a function of MLT and invariant latitude. | J. Geophys. Res., 106, 21123-21136, 2001 |
| CRRES | N. P. Meredith (MSSL) R. B. Horne (NERC) R. R. Anderson (DPA-UI) | The spatial dependence of whistler-mode chorus amplitudes as a function of substorm activity (as measured by AE) using data from the Plasma Wave Experiment on board the CRRES spacecraft. |
J. Geophys. Res., 106, 13165-13178, 2001 |
| Dynamics Explorer 1 | R. E. Erlandson (APL) A. J. Ukhorskiy (APL) | The occurrence of low-L (3.5 < L < 5) electromagnetic ion cyclotron (EMIC) waves during magnetic storms between 1981 and 1991. | J. Geophys. Res., 106, 3883-3895, 2001 |
| Geotail Polar FAST | G. S. Lakhina (IIGM) B. T. Tsurutani (JPL) H. Kojima (RASC) H. Matsumoto (RASC) | The main characteristics and the possible generation mechanisms of the broadband plasma waves (with frequency of > 1 Hz) observed in different boundary layers (magnetopause, plasma sheet and polar cap) are described. | J. Geophys. Res., 105, 27791-27831, 2000 |
| CRRES | N. P. Meredith (MSSL) R. B. Horne (NERC) A. D. Johnstone (MSSL) R. R. Anderson (DPA-UI) | The electron cyclotron harmonic wave amplitudes are observed in 2 regions (region 3.8 < L < 6 with 22 < MLT < 02 and region 6 < L < 7 with 02 < MLT < 06) and are enhanced during substorm particle injections. |
J. Geophys. Res., 105, 12907-12917, 2000 |
| Geotail | Y. Zhang (RASC) H. Matsumoto (RASC) H. Kojima (RASC) | The whistler mode waves in the magnetotail have an average frequency of 0.21 times the electron cyclotron frequency, and they propagate predominantly in a direction parallel or antiparallel to the ambient magnetic field. | J. Geophys. Res., 104, 28633-28644, 1999 |
| Hawkeye 1 | J. L. Green (NASA-GSFC) S. A. Boardsen (NASA-GSFC) | The nonthermal continuum radiation (5-110 kHz) are primarily confined to low latitudes and infrequently observed over the high-altitude polar cap. | J. Geophys. Res., 104, 10307-10316,1999 |
| Freja | R. E. Erlandson (APL) L. J. Zanetti (APL) | The number of auroral electromagnetic ion cyclotron waves (5-250 Hz) peaked in the premidnight sector (18-01 MLT) at auroral latitudes (68° - 72° invariant latitude). | J. Geophys. Res., 103, 4627-4636, 1998 |
| Aureol 3 | M. Parrot (LPCE) | ELF hiss is maximum between 6 and 20 MLT and in the invariant latitude range 50° - 70°, but are intensified in region of man-made waves (VLF transmitters and South Atlantic Anomaly). | Ann. Geophyicae, 8, 135-146, 1990 |
| ISIS 1 ISIS 2 | H. Saito (NIPR) T. Yoshino (NIPR) N. Sato (NIPR) | Narrow-banded ELF emissions (100-500 Hz) mostly occured in the evening 17-24 MLT sector and in the region of 65° - 75° invariant latitude. | Planet. Spa. Sci., 35, 745-752, 1987 |
| OGO 5 | B. T. Tsurutani (JPL) E. J. Smith (JPL) | ELF chorus (10-1500 Hz) occurs principally near the equator (06-12 MLT) and at magnitude latitudes above 15° (08-16 MLT). | J. Geophys. Res., 82, 5112-5128, 1977 |
| Ariel 3 | A. R. W. Hughes (NU) T. R. Kaiser (deceased) and K. Bullough (deceased) | VLF radio emissions (at 3.2 and 9.6 kHz) occur at all magnetic local times but are most frequently observed at midnight and in the early afternoon. | Space Research, XI, 1323-1330, Akademie-Verlag, Berlin 1971 |
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