| Issue |
EPJ Web of Conferences
Volume 47, 2013
Hot Planets and Cool Stars
|
|
|---|---|---|
| Article Number | 12002 | |
| Number of page(s) | 4 | |
| Section | Model Atmospheres | |
| DOI | https://doi.org/10.1051/epjconf/20134712002 | |
| Published online | 25 April 2013 | |
https://doi.org/10.1051/epjconf/20134712002
Modelling of the Earth's transmission spectrum in the framework of one-slab model
1 Main Astronomical Observatory of the National Academy of Sciences of Ukraine
2 University of Hertfordshire
3 INTA-CSIC Centro de Astrobiologia, Madrid, Spain
a e-mail: greg@mao.kiev.ua
b e-mail: yp@mao.kiev.ua
We discuss the possibility of using the transmission spectrum of the Earth in the measurements of the molecules abundance ratios. We use optical and near infrared transmission spectrum of the Earth obtained during observations of a lunar eclipse in 2008 by Enric Palle and others (E. Pallé et al., 2009). This task is interesting in terms of estimation of the chemical composition of the Earth-like planets around other stars during their transits. We use one-slab model approach for modelling transmission spectra using HITRAN line database. Comparison with observational data gives us clues to our problem.
© Owned by the authors, published by EDP Sciences, 2013
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.