DMSP observations of equatorial plasma bubbles in the topside ionosphere near solar maximum

Mathematics – Logic

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

60

Ionosphere: Electric Fields, Ionosphere: Equatorial Ionosphere, Ionosphere: Ionosphere/Magnetosphere Interactions, Ionosphere: Ionospheric Irregularities

Scientific paper

The Defense Meteorological Satellite Program (DMSP) flights F9 and F10 crossed postsunset local time sectors approximately 14 times per day in Sun-synchronous orbits at an altitude of ~840 km. We have examined a large database of postsunset plasma density measurements acquired during ~15,000 equatorial crossings made by DMSP F9 in 1989 and 1991 and DMSP F10 in 1991. On 2086 of these crossings equatorial plasma bubbles (EPBs) were observed as intervals of depleted and irregular plasma densities. We have analyzed these EPB events to determine their distributions with season, longitude (S/L), and levels of geomagnetic activity. The global S/L distributions of EPBs observed by the DMSP satellites are shown to be in general agreement with results from discrete ground-based measurements. That is, the seasonal variations detected at 840 km in longitude bins hosting radar/scintillation observatories appear similar to those reported from the ground. Over the Atlantic sector where EPBs occur frequently, we found good agreement with predictions of a simple model proposed by Tsunoda [1985]. In the Pacific sector the frequency of EPB occurrence is considerably lower, and poor counting statistics preclude confident predictions regarding the absolute value of seasonal variations. We suggest that relatively large equatorial magnetic fields at F layer altitudes in the Pacific (~0.34 G) sector more strongly inhibit the growth of the Rayleigh-Taylor instability than at Atlantic (~0.25 G) longitudes. Contrary to general belief, we found that EPBs occurred regularly during geomagnetic storms, especially in the initial and main phases. EPB activity appears to have been suppressed from many hours to days during storm recovery phases.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

DMSP observations of equatorial plasma bubbles in the topside ionosphere near solar maximum does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with DMSP observations of equatorial plasma bubbles in the topside ionosphere near solar maximum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and DMSP observations of equatorial plasma bubbles in the topside ionosphere near solar maximum will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-941978

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.