Cesar Valladares
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Recent Grants
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Collaborative Research: Investigations of the Mid-Latitude Ionosphere during Magnetic Disturbances: Observations, Modeling and Space Weather Impacts
Open Date: 2013-08-15
Close Date: 2016-07-31
Grant: Close
Collaborative Research: The Low-latitude Ionosphere and the Development of Forecasting Techniques Using the Low-latitude Ionosphere Sensor Network (LISN) Distributed Observatory
Open Date: 2012-10-01
Close Date: 2016-09-30
Grant: Close
US-South America Workshop to Foster Space Weather Investigation using the LISN Observatory
Open Date: 2011-09-01
Close Date: 2012-08-31
Grant: Close
Development of the First Distributed Observatory Dedicated to Studies of the Low Latitude Ionosphere and Atmosphere
Open Date: 2005-08-01
Close Date: 2012-07-31
Grant: Close
M-I Coupling: An Observational and Modeling Study Under Conditions of Extreme Forcing
Open Date: 2004-03-01
Close Date: 2008-02-29
Articles (6)
In this case study, we focus on how hemispheric differences in the electric potential distribution in the auroral zones are related to hemispheric differences in the energetic particle precipitation that indicate the presence of field‐aligned potential drops. Utilizing data during the spring and fall equinox in 2013 and 2014 from the Defense Meteorological Satellite Program (DMSP) F16 and F17 satellites, we systematically examine simultaneous measurements of plasma drift velocity and particle precipitation in magnetically conjugate regions across the auroral zone in both hemispheres. This allows us to establish the degree to which the interhemispheric differences in ionospheric electric potential may be accounted for by field‐aligned potential drops. Thirty‐seven eligible cases examined show accelerated electron energy spectra at conjugate locations in the northern and/or southern hemispheres. Of these 37 cases, 23 show conjugate differences in electric potential that agree qualitatively with the observed electron acceleration and average energy of precipitating electrons in each hemisphere. This result suggests that the hemispheric differences in ionospheric electric potential in the auroral zone may be most frequently accounted for by field‐aligned potential drops along the magnetic flux tubes connecting conjugate points to the equatorial plane. The spatial and temporal variability of the potential distribution, electron precipitation, and magnetic field configuration could account for deviations from the normally observed situation in the remaining cases. More magnetically conjugate observations at various altitudes in both hemispheres are needed to investigate this hemispheric coupling in more detail.
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2023
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2023
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2023
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2023
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2023
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2021
Collaborators (4)
Clayton E. Cantrall
Johns Hopkins University Applied Physics Laboratory
John Noto
Chief Scientist
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Qian Wu
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L. A. Navarro
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