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Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

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Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data. Angela Zalucha MIT Haystack Observatory/ University of Illinois at Urbana Champaign [email protected]. Background Information. - PowerPoint PPT Presentation
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Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data Angela Zalucha MIT Haystack Observatory/ University of Illinois at Urbana Champaign [email protected]
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Page 1: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Empirical Ionospheric Model Based on Saint Santin

Incoherent Scatter Radar Data

Angela Zalucha

MIT Haystack Observatory/

University of Illinois at Urbana Champaign

[email protected]

Page 2: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Background Information

Ionospheric data recorded by the bistatic incoherent scatter radar at St. Santin, France (45-47 N c.f. 54 N for Millstone)

Data obtained from the CEDAR/MADRIGAL database

Data spans the years 1966 through 1987

Model used originally developed for Millstone Hill data

Page 3: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Building a Model

IN IN

OUT

We measured… With the corresponding…

EmpiricalModel

Ne

Te Ti

Alt.LT

F107Day No.

Measurements are binnedaccording to Alt., LT, Day No.

F107 dependence determined through linear least squares fit

Page 4: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Investigating the Data Distribution

Number of points per month

Number of pointsper altitude and LT

Number of points per F107

Check if linear fit is good for F107

F107

Page 5: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Data and Model Profiles• Check how well

measured data and model data match

• Here we plot each parameter vs. LT for Day No. = 184 and Alt. = 275

LT (hours)

log(Ne)

Ti

TeMeasured Data

F107 = 60F107 = 100F107 = 135F107 = 200

Page 6: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Data and Model Profiles

• Here we plot Alt. vs. each parameter for LT = 12 and Day No. = 184

• The limits of the F107 range should be at the edges of the data respectively

Alt

. (km

)

log(Ne) Ti Te

Measured Data

F107 = 60F107 = 100F107 = 135F107 = 200

Page 7: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Millstone Hill Vs. St. Santin

• Each model created using essentially the same software—do they produce similar outputs?

• Models match reasonably well

• St. Santin tends to vary less than Millstone and produce quantitatively higher Ne outputsDay No. = 184

Alt. = 275 kmF107 = 135

LT (hours)

Day No.

log(Ne)

Ti

Te

LT = 12 hoursAlt. = 250 kmF107 = 135

Te

Ti

log(Ne)

Page 8: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Movies allow us to view multiple parameters at once

log(Ne): Alt. vs. LT, progressing over Day No., F107 = 135

Page 9: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Movies allow us to view multiple parameters at once

Ti: Alt. vs. LT, progressing over Day No., F107 = 135

Page 10: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

Movies allow us to view multiple parameters at once

Te: Alt. vs. LT, progressing over Day No., F107 = 135

Page 11: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

The Virtual St. Santin Radar

Calculates predicted ionospheric conditions at the current time

Updated every 15 minuteshttp://www.haystack.mit.edu/madrigal/vssr

Page 12: Empirical Ionospheric Model Based on Saint Santin Incoherent Scatter Radar Data

ConclusionThe Saint Santin Empirical Model produces reasonable results with respect to both the measured data and the Millstone Hill Empirical Model.

Angela [email protected]

University of Illinois/MIT Haystack Observatory

Advisors John Holt Shunrong Zhang

[email protected] [email protected] MIT Haystack Observatory


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