Ionospheric Corrections via PIM and Real-Time Data

Details Ionospheric Corrections via PIM and Real-Time Data Ionospheric Corrections via PIM and Real-Time Data

1999-07-29

arxiv.org/abs/astro-ph/9907412v1

New Astron.Rev. 43 (1999) 617-621

Astronomy and Astrophysics

Astrophysics

6 pages, 2 fiugres; LaTeX2e (96/12/01); uses elsart.cls (2.15, 98/07/15); to appear in New Astronomy Reviews

Scientific paper

10.1016/S1387-6473(99)00065-2

We describe a method for removing ionospheric effects from single-frequency radio data a posteriori. This method is based on a theoretical climatological model developed by the USAF, which returns electron density as a function of position and time along the line of sight to the source. Together with a model of the earth's magnetic field, ionospheric delays and Faraday rotation values ensue. If contemoraneous ionospheric data -- GPS TEC observations or ionosonde profiles -- exist, they can be incorporated to update the modeled electron densities.

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