Data for: Abundance Measurements of Titan’s Stratospheric HCN, HC3N, C3H4, and CH3CN from ALMA Observations

Name: Data for: Abundance Measurements of Titan’s Stratospheric HCN, HC3N, C3H4, and CH3CN from ALMA Observations
Creator: Thelen, Alexander
Keywords: 13. Climate action, Planetary Sciences, Radio Astronomy

Thelen, Alexander

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Mendeley Dataarrow_drop_down

Mendeley Data

Dataset . 2018

License: CC BY

Data sources: Datacite

Mendeley Data

Dataset . 2018

License: CC BY

Data sources: Datacite

Mendeley Data

Dataset . 2018

License: CC BY

Data sources: Mendeley Data

Mendeley Data

Dataset . 2018

License: CC BY

Data sources: Mendeley Data

Data for: Abundance Measurements of Titan’s Stratospheric HCN, HC3N, C3H4, and CH3CN from ALMA Observations

Research datakeyboard_double_arrow_right Dataset 05 Oct 2018Publisher:Mendeley

Authors: Thelen, Alexander;

doi: 10.17632/2ychd8nnr3.1 , 10.17632/2ychd8nnr3

Data for: Abundance Measurements of Titan’s Stratospheric HCN, HC3N, C3H4, and CH3CN from ALMA Observations

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Abstract

Data files each contain a single abundance profile of HC3N, C3H4, CH3CN, or one of the two HCN isotopes: HC15N or H13CN; the latter two profiles have not been scaled by an isotope ratio value to represent HCN, as in the manuscript. Each file corresponds to either disk-averaged (_da) results, or spatially resolved profiles from North (48 N), Center (21 N), or South (16 S) retrievals (_n, _c, and _s, respectively). Abundance profiles cover the approximate altitudes where ALMA sensitivity allows for accurate retrievals: 50-550 km for HC3N, C3H4, and HCN isotopes, and 150-550 km for CH3CN. File column format is as follows: altitude (km), pressure (mbar), abundance.

Keywords

Planetary Sciences, Radio Astronomy

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Abundance measurements of Titan’s stratospheric HCN, HC3N, C3H4, and CH3CN from ALMA observations
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