Comparison of Solar Wind Speed Estimates from Nearly Simultaneous IPS Observations at 327 and 111 MHz
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s11207-021-01804-6.pdf
Reference22 articles.
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2. Armstrong, J.W., Coles, W.A., Kojima, M., Rickett, B.J.: 1990, Observations of field-aligned density fluctuations in the inner solar wind. Astrophys. J. 358(8), 685. DOI.
3. Chang, O., Bisi, M.M., Aguilar-Rodriguez, E., Fallows, R.A., Gonzalez-Esparza, J.A., Chashei, I., Tyul’bashev, S., Tokumaru, M.: 2019, Single-site IPS power spectra analysis for space-weather products using cross correlation function results from EISCAT and MERLIN IPS data. Space Weather 17(7), 1114. DOI.
4. Chashei, I.V., Kojima, M., Tokumaru, M.: 2000, Anisotropy of magnetosonic turbulence in the solar wind between 0.1 and 0.4 AU. J. Geophys. Res. 105(A12), 27401. DOI.
5. Chashei, I.V., Efimov, A.I., Rudash, V.K., Bird, M.K.: 2000, Anisotropy and velocities of small-scale irregularities in the solar wind acceleration region. Astron. Rep. 77(9), 713. DOI.
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