NOTICE: Use the parameters below to customize your search. Regular expressions and bolean "AND" will to match the search. In the case of "Author name", the search is performed using only for the last name.
Found 1 entries in the Bibliography.
Showing entries from 1 through 1
The l = 2 spherical harmonic expansion coefficients of the sky brightness distribution between 0.5 and 7 MHz
Context. The opacity of the ionosphere prevents comprehensive Earth- based surveys of low frequency \ensuremath\nu \ensuremath\lesssim 10 MHz astrophysical radio emissions. The limited available data in this frequency regime show a downturn in the mean sky brightness at \ensuremath\nu \ensuremath\lesssim 3 MHz in a divergence from the synchrotron emission power-law that is observed at higher frequencies. The turning over of the spectrum coincides with a shift in the region of maximum brightness from the Galactic plane to the ...
Page, B.; Bassett, N.; Lecacheux, A.; Pulupa, M.; Rapetti, D.; Bale, S.~D.;
Published by: \aap Published on: dec
YEAR: 2022   DOI: 10.1051/0004-6361/202244621
Parker Data Used; radio continuum: ISM; Galaxy: disk; opacity; methods: data analysis