Improving the solar wind density model used in processing of spacecraft ranging observations
Author:
Affiliation:
1. Institute of Applied Astronomy , 191187, St. Petersburg, Kutuzova Embankment, 10, Russia
2. St. Petersburg Electrotechnical University , 197022, St. Petersburg, ul. Professora Popova 5, Russia
Abstract
Funder
NASA
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/article-pdf/514/3/3191/44204489/stac1229.pdf
Reference50 articles.
1. Exploring the Asymmetry of the Solar Corona Electron Density with Very Long Baseline Interferometry
2. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates
3. Solar radio burst and in situ determination of interplanetary electron density
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