Storm-time related mass density anomalies in the polar cap as observed by CHAMP

Strong and localized thermospheric mass den- sity events are observed in the polar cap region by the CHAMP satellites at about 400 km altitude during geomag- netic storms. During the 4 years considered (2002-2005) 29 storms with Dst< 100 nT occurred, in 90% of them polar cap density anomalies were detected. Based on the altogether 56 anomaly events a statistical analysis was performed. The anomalies are of medium scale (500-1500 km) and seem to have a short dwell-time (<1.5 h) in the polar cap. The rela- tive density enhancement is found to range around 2 in both hemispheres. The peak density is in the Northern Hemi- sphere by a factor of 1.4 larger than in the southern. Also the number of detected events in the north is twice as large as that in the south (37 vs. 19). Mass density anomalies in the polar cap occur under all interplanetary magnetic field (IMF) directions. Numerous strong anomalies have been detected in positive and negative IMF Bz conditions when the mag- netic field strength is above 5 nT. Rather few events occurred for small |Bz| (<5 nT) or for positive Bz combined with van- ishing By. Some of the density anomalies are accompanied by intensive small-scale field-aligned currents (FACs). But about as many show no relation to FACs. If FACs are present there, the current density is believed to be correlated with the strength of the IMF Bz. Although this paper concentrates on the presentation of the observations, we show for one event that the ion outflow mechanism could be responsible for the mass density anomalies in the polar cap.

[1]  J. Forbes,et al.  Thermosphere density variations due to the 15–24 April 2002 solar events from CHAMP/STAR accelerometer measurements , 2005 .

[2]  Hermann Lühr,et al.  Zonal winds in the equatorial upper thermosphere: Decomposing the solar flux, geomagnetic activity, and seasonal dependencies , 2006 .

[3]  Jeffrey M. Forbes,et al.  Global thermospheric neutral density and wind response to the severe 2003 geomagnetic storms from CHAMP accelerometer data , 2005 .

[4]  Hermann Lühr,et al.  Average thermospheric wind patterns over the polar regions, as observed by CHAMP , 2007 .

[5]  Hermann Lühr,et al.  Global distribution of the thermospheric total mass density derived from CHAMP , 2004 .

[6]  Richard Biancale,et al.  Atmospheric densities derived from CHAMP/STAR accelerometer observations , 2004 .

[7]  D. Cooke,et al.  Ion Drift-Meter Status and Calibration , 2003 .

[8]  T. Killeen,et al.  Large enhancements in the O/N2 ratio in the evening sector of the winter hemisphere during geomagnetic storms , 1995 .

[9]  Jie Zhang,et al.  Solar and Interplanetary Sources of Major Geomagnetic Storms (Dst less than or equal to -100 nT) During 1996 - 2005 , 2007 .

[10]  S. Bruinsma,et al.  Global observation of traveling atmospheric disturbances (TADs) in the thermosphere , 2007 .

[11]  H. Lühr,et al.  SWMF simulation of field-aligned currents for a varying northward and duskward IMF with nonzero dipole tilt , 2008 .

[12]  Jie Zhang,et al.  Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005 , 2007 .

[13]  J. Forbes,et al.  Magnetic storm response of lower thermosphere density , 1996 .

[14]  M. Acuna,et al.  The ACE Magnetic Fields Experiment , 1998 .

[15]  L. Grunwaldt,et al.  Thermospheric up‐welling in the cusp region: Evidence from CHAMP observations , 2004 .

[16]  B. Reinisch,et al.  Comparison of CHAMP and Digisonde plasma frequencies at Jicamarca, Peru , 2007 .

[17]  N. Maynard,et al.  Empirical high‐latitude electric field models , 1987 .

[18]  H. Lühr,et al.  Strong disturbance of the upper thermospheric density due to magnetic storms: CHAMP observations , 2005 .

[19]  H. Lühr,et al.  Observing the north polar ionosphere on 30 October 2003 by GPS imaging and IS radars , 2006 .

[20]  G. Crowley,et al.  Effect of IMF BY on thermospheric composition at high and middle latitudes: 1. Numerical experiments , 2006 .

[21]  Stein Haaland,et al.  IMF dependence of high-latitude thermospheric wind pattern derived from CHAMP cross-track measurements , 2008 .

[22]  A. Richmond Ionospheric Electrodynamics Using Magnetic Apex Coordinates. , 1995 .

[23]  Hermann Lühr,et al.  Climatology of the equatorial thermospheric mass density anomaly , 2007 .

[24]  J. W. Griffee,et al.  Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer , 1998 .

[25]  D. Gurnett,et al.  A survey of upwelling ion event characteristics , 1990 .

[26]  Hermann Lühr,et al.  Solar and magnetospheric forcing of the low latitude thermospheric mass density as observed by CHAMP , 2009 .

[27]  W. J. Burke,et al.  Interplanetary control of thermospheric densities during large magnetic storms , 2007 .

[28]  Hong Wang,et al.  Solar zenith angle and merging electric field control of field‐aligned currents: A statistical study of the Southern Hemisphere , 2005 .

[29]  H. Lühr,et al.  CHAMP observation of intense kilometer-scale field-aligned currents, evidence for an ionospheric Alfvén resonator , 2007 .

[30]  N. Olsen,et al.  Field-aligned currents in the dayside cusp and polar cap region during northward IMF , 2002 .

[31]  D. Mccomas,et al.  Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique , 2003 .

[32]  G. Crowley,et al.  Thermospheric density structures over the polar regions observed with CHAMP , 2005 .

[33]  H. Lühr,et al.  Climatology of the cusp-related thermospheric mass density anomaly, as derived from CHAMP observations , 2008 .

[34]  R. Nerem,et al.  Thermosphere density response to the 20-21 November 2003 solar and geomagnetic storm from CHAMP and GRACE accelerometer data , 2006 .

[35]  J. Forbes,et al.  Dependence of the high-latitude thermospheric densities on the interplanetary magnetic field , 2009 .