Storm-enhanced plasma density features investigated during the Bastille Day Superstorm

Mathematics – Logic

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2

Ionosphere: Ionospheric Storms (7949), Ionosphere: Ionospheric Disturbances, Ionosphere: Ionosphere/Magnetosphere Interactions (2736), Ionosphere: Topside Ionosphere, Ionosphere: Midlatitude Ionosphere

Scientific paper

Field-aligned passes track true profiles. Such Defense Meteorological Satellite Program passes permitted investigating storm-enhanced plasma density (SED) feature development during the Bastille Day Superstorm in a comprehensive way. We tracked equatorial ionization anomaly (EIA) and SED features and their underlying forward fountain circulation and downward SED plume plasma flows, respectively. Northward subauroral polarization stream E fields detaching plasma and producing SED plumes were also detected. We assessed the effects of South Atlantic Magnetic Anomaly and summer-to-winter interhemispheric plasma flows on the EIA and found a southward dipping gradient in drift/flow when no storm/evening-related fountain strengthening occurred. We investigated the relative importance of different plasma sources in SED development. An extremely large plasma enhancement seen over Florida at 2200 UT on 15 July 2000 was a SED feature that was tracked by many GPS total electron content (TEC) maps as a 200 TEC unit (TECU) enhancement. We tracked its equally large conjugate pair over Trelew (Argentine Patagonia) and unraveled their development. Their underlying SED plume supplied most of the plasma. Appearing between these two SED features, a small and highly asymmetrical EIA offered on each side a low baseline upon which the downward streaming SED plume plasma piled up. Contradicting a currently accepted explanation, there was no enhanced fountain action detected to contribute 150 TECU to the 200 TECU. Later (˜2400 UT), there was enhanced fountain action, but SED plume contribution still dominated. Proven by observational evidence, SED development is a complex process of SED plume plasma flows and equatorward wind effects that cannot be described by one single explanation.

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

Storm-enhanced plasma density features investigated during the Bastille Day Superstorm 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 Storm-enhanced plasma density features investigated during the Bastille Day Superstorm, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Storm-enhanced plasma density features investigated during the Bastille Day Superstorm will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1578355

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