Seasonal Differences in the Dusk Equatorial Topside Ionosphere Measured by C/NOFS and DMSP

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

[2415] Ionosphere / Equatorial Ionosphere, [2437] Ionosphere / Ionospheric Dynamics, [2481] Ionosphere / Topside Ionosphere, [2494] Ionosphere / Instruments And Techniques

Scientific paper

The C/NOFS spacecraft is in a near-equatorial elliptical orbit with an apogee of about 845 km which precesses through all local times over a period of about 66 days. The four operational DMSP spacecraft are in sun-synchronous circular polar orbits at roughly the same altitude as C/NOFS’s apogee. Thus the C/NOFS apogee overlaps with the DMSP duskside orbits every 66 days for a period of about two weeks. This work will present the analysis of three of these overlap periods during the northern winter (roughly December 30, 2008-January 12, 2009), the northern summer (roughly July 14-31, 2009), and one equinox period (roughly March 6-21, 2009) where we will use the combined C/NOFS and DMSP data to show the seasonal changes in ion density, composition, and temperature in the topside ionosphere. This will allow a further validation of the CINDI plasma instruments on C/NOFS as well as establishing a baseline of these geophysical parameters in the topside ionosphere through all seasons during the current extreme solar minimum conditions.

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

Seasonal Differences in the Dusk Equatorial Topside Ionosphere Measured by C/NOFS and DMSP 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 Seasonal Differences in the Dusk Equatorial Topside Ionosphere Measured by C/NOFS and DMSP, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Seasonal Differences in the Dusk Equatorial Topside Ionosphere Measured by C/NOFS and DMSP will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1780496

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