Shaik, Shaheda Begum, and Gary, Dale E. Implications of Flat Optically Thick Microwave Spectra in Solar Flares for Source Size and Morphology. Retrieved from https://par.nsf.gov/biblio/10321094. The Astrophysical Journal 919.1 Web. doi:10.3847/1538-4357/ac0fdb.
Shaik, Shaheda Begum, & Gary, Dale E. Implications of Flat Optically Thick Microwave Spectra in Solar Flares for Source Size and Morphology. The Astrophysical Journal, 919 (1). Retrieved from https://par.nsf.gov/biblio/10321094. https://doi.org/10.3847/1538-4357/ac0fdb
@article{osti_10321094,
place = {Country unknown/Code not available},
title = {Implications of Flat Optically Thick Microwave Spectra in Solar Flares for Source Size and Morphology},
url = {https://par.nsf.gov/biblio/10321094},
DOI = {10.3847/1538-4357/ac0fdb},
abstractNote = {},
journal = {The Astrophysical Journal},
volume = {919},
number = {1},
author = {Shaik, Shaheda Begum and Gary, Dale E.},
}
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