@Article{HaiderBaAbMuShKu:2015:CoEaIo,
author = "Haider, Syed A. and Batista, Inez Staciarini and Abdu,
Mangalathayil Ali and Muralikrishna, Polinaya and Shah, Siddhi Y.
and Kuroda, T.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Physical Research Laboratory} and {Tohoku
University}",
title = "Dust storm and electron density in the equatorial D region
ionosphere of Mars: Comparison with Earth's ionosphere from rocket
measurements in Brazil",
journal = "Journal of Geophysical Research: Space Physics",
year = "2015",
volume = "120",
number = "10",
pages = "8969--8977",
month = "Oct.",
abstract = "We report the first model result for the dust densities and
electron densities in the D region ionosphere of Mars for aerosol
particles of different sizes during a major dust storm that
occurred in Martian Year (MY) 25 at low latitude. These
calculations are made at latitude 10°S and solar longitudes
(Ls)\ =\ 200°, 220°, 250°, and 280° for high,
medium, low, and absence of dust storms, respectively. Four
corresponding dust layers were found at 50\ km,
50\ km, 38\ km, and 25\ km during these
events. During high dust storm period, the optical depth and dust
density increased by a factor of ~20 from its normal condition.
The electron densities estimated for the D region ionosphere of
Mars for submicron sized dust particles are largest as compared to
that estimated for larger particles. The electron density reduced
by ~2 orders of magnitude during high dust storm. The estimated
electron density in the clear atmosphere of Mars is compared with
measurements of Earth's ionosphere at nearly the same geophysical
condition.",
doi = "10.1002/2015ja021630",
url = "http://dx.doi.org/10.1002/2015ja021630",
issn = "2169-9402",
label = "lattes: 2582665858245251 4 HaiderBaAbMuShKu:2015:CoEaIo",
language = "en",
urlaccessdate = "27 abr. 2024"
}