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Ionosphere, Magnetosphere and Thermosphere Anthea Coster

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Transport of heavy ionospheric ions into the magnetosphere has long been ... Three dimensional ionospheric tomography of ionization as well as thermal ... – PowerPoint PPT presentation

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Title: Ionosphere, Magnetosphere and Thermosphere Anthea Coster


1
Ionosphere, Magnetosphere and ThermosphereAnthea
Coster
  • Topics -
  • Magnetospheric-Ionospheric Coupling
  • Ion-Neutral Coupling
  • Low-Mid-High Latitude Connections
  • High Latitude and Polar Processes
  • Impacts from Below

2
  • Magnetospheric-Ionospheric Coupling
  • Ionospheric Feedbacks on the Magnetosphere.
  • Ionospheric conductivity controls magnetospheric
    processes.
  • Transport of heavy ionospheric ions into the
    magnetosphere has long been observed but is
    poorly understood.
  • Daytime auroral observations suggest ionospheric
    control of auroral precipitation.
  • Fine-scale measurements are critical - AMISR,
    Satellite, Optical.
  • Daytime optical measurements.

3
  • Penetration Electric Fields
  • During magnetic storms, the high latitude E-field
    maps down to the equator
  • The region 2 field-aligned currents progressively
    shield the low latitudes
  • The mechanisms are poorly understood the role of
    dynamo electric fields, conductivity gradients
    other factors has not been properly modelled.
  • Ionospheric density and scintillation strongly
    depend on this E-field
  • Observations from radars, ionosondes
    magnetometers can provide ground-truth

4
  • High Latitude Processes
  • High-temporal and spatial resolution Total
    Electron Content (TEC) measurements
  • Three dimensional ionospheric tomography of
    ionization as well as thermal structures in the
    polar cap ionosphere using ground based ionosonde
    and GPS TEC measurements
  • Polar cap boundary measurements using the array
    of photometers
  • Coarse information about precipitating particle
    energy in the polar cap ionosphere

5
  • Heliospheric Impacts
  • Studies of the fundamental plasma physical
    processes which mediate energy flow in the
    solar-terrestrial system
  • Studies of naturally occurring processes such as
    the structure and dynamics of auroral arcs,
    proton aurora, ionosphere-thermosphere
    interactions, ion outflow and non-Maxwellian
    plasmas are of critical importance

6
  • Conjugacy
  • Global scale auroras are known to be similar, but
    how about mesoscales (L100-1000 km)?.
  • ASC images The real conjugate point of a station
    can move hundreds (tens) of km in longitude
    (latitude) during one hour.

7
  • Ion-Neutral Coupling
  • Neutral outflow at high-latitudes occurs when an
    energized out-flowing ion undergoes a
    charge-exchange reaction with a background
    neutral atom.
  • Models of the aurora do not include the impact of
    heavy, or light, neutral atoms produced in the
    charge-exchange reactions of energized ions
    out-flowing from the auroral zone.
  • Improved understanding of neutral atom impact on
    the magnetosphere.

8
  • Low-Mid-High Latitude Connections
  • Do we really understand the formation of
    medium-scale TIDs
  • What is the source of mesoscale ionospheric
    structures at tropical latitudes.

9
  • Low-Mid-High Latitude Connections
  • What are the relative roles of storm-time
    magnetospheric electric fields and dynamo
    electric fields from thermospheric winds driven
    by high latitude heating?
  • Do mid-latitude storms have a longitudinal
    dependence perhaps related to the South Atlantic
    Anomaly?
  • Is mass transfer from the ionosphere to the
    magnetosphere significant?

10
  • Low-Mid-High Latitude Connections
  • How is plasma transported from the equatorial
    anomalies poleward
  • Are mid-latitude ionospheric storms the cause of
    polar cap patches.
  • What are the production mechanisms for
    mid-latitude irregularities

11
  • Impacts from Below
  • The response of lower thermosphere (gt100km) to
    stratospheric warming events is not known.
  • Wintertime winds and temperatures in the lower
    thermosphere are much more variable than during
    other seasons.
  • Tidal signatures before major stratospheric
    warming (LTCS-6, Dec 1991) were vastly different
    from other winter campaigns.
  • Pronounced and persistent variability for this
    period was also reported in thermospheric
    parameters in the F-region
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