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Sheeley, N.R.J., Wang, Y.-M., Hawley, S.H., Brueckner, G.E., Dere, K.P., Howard, R.A., Koomen, M.A., Korendyke, C.M., Michels, D.M., Paswaters, S.E., Socker, D.G., Cyr, O.C.S., Wang, D., Lamy, P.L., Llebaria, A., Schwenn, R., Simnett, G.M., Plunkett, S. and Biesecker, D.A. (1997) Measurements of Flow Speeds in the Corona between 2 and 30 R. The Astrophysical Journal, 484, 472-478.
https://doi.org/10.1086/304338

has been cited by the following article:

• TITLE: Validation of Novel Model for Identification of Thermal Conditions in the Low Corona

  AUTHORS: Daniel B. Berdichevsky, Jenny M. Rodríguez Gómez, Luis E. Vieira, Alisson Dal Lago

  KEYWORDS: Solar Corona, Electron Density, Temperature

  JOURNAL NAME: Advances in Aerospace Science and Technology, Vol.7 No.1, March 28, 2022

  ABSTRACT: The electron density and temperature key properties of the neutral-magnetized plasma in the solar corona, which are predicted with a novel model, provide an interesting window along the whole solar cycle. In this work, we test the quantitative validity of the model and prove that the Coronal Density and Temperature (CODET) is reliable. Furthermore, this work contrasts the CODET model results with alternative observational remote and in-situ datasets during the simplest conditions of the quiescent corona near the solar minimum. This successful outcome/validation of the CODET model allowed a good qualitative density and temperature retrieval in the solar corona covering a large portion of time interval from solar cycles 23 and 24.