Dynamics of atmospheres with a non-dilute condensible component

Proceedings of the Royal Society of London. Series A, Mathematical and physical sciences Royal Society, The 472 (2016) 20160107

Authors:

RT Pierrehumbert, F Ding

ALMA Observations of HCN and its Isotopologues on Titan

(2016)

Authors:

Edward M Molter, Conor A Nixon, Martin A Cordiner, Joseph Serigano, Patrick GJ Irwin, Nicholas A Teanby, Steven B Charnley, Johan E Lindberg

ALMA OBSERVATIONS OF HCN AND ITS ISOTOPOLOGUES ON TITAN

Astronomical Journal American Astronomial Society 152:42 (2016) 1-7

Authors:

EM Molter, CA Nixon, MA Cordiner, J Serigano, Patrick Irwin, NA Teanby, SB Charnley, JE Lindberg

Abstract:

All rights reserved.We present sub-millimeter spectra of HCN isotopologues on Titan, derived from publicly available ALMA flux calibration observations of Titan taken in early 2014. We report the detection of a new HCN isotopologue on Titan, H13C15N, and confirm an earlier report of detection of DCN. We model high signal-to-noise observations of HCN, H13CN, HC15N, DCN, and H13C15N to derive abundances and infer the following isotopic ratios: 12C/13C = 89.8 ±2.8, 14N/15N = 72.3 ±2.2, D/H = (2.5 ± 0.2) ×10-4, and HCN/H13C15N = 5800 ±270 (1σ errors). The carbon and nitrogen ratios are consistent with and improve on the precision of previous results, confirming a factor of ∼2.3 elevation in 14N/15N in HCN compared to N2 and a lack of fractionation in 12C/13C from the protosolar value. This is the first published measurement of D/H in a nitrile species on Titan, and we find evidence for a factor of ∼2 deuterium enrichment in hydrogen cyanide compared to methane. The isotopic ratios we derive may be used as constraints for future models to better understand the fractionation processes occurring in Titan's atmosphere.

Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 458:3 (2016) 2405-2422

Authors:

S Kendrew, S Zieleniewski, RCW Houghton, N Thatte, J Devriendt, M Tecza, F Clarke, K O'Brien, B Haussler

New use of global warming potentials to compare cumulative and short-lived climate pollutants

Nature Climate Change Nature Publishing Group 6:8 (2016) 773-776

Authors:

Myles R Allen, Jan S Fuglestvedt, Keith P Shine, Andy Reisinger, Raymond Pierrehumbert, Piers M Forster

Abstract:

Parties to the United Nations Framework Convention on Climate Change (UNFCCC) have requested guidance on common greenhouse gas metrics in accounting for Nationally determined contributions (NDCs) to emission reductions1. Metric choice can affect the relative emphasis placed on reductions of ‘cumulative climate pollutants’ such as carbon dioxide versus ‘short-lived climate pollutants’ (SLCPs), including methane and black carbon2, 3, 4, 5, 6. Here we show that the widely used 100-year global warming potential (GWP100) effectively measures the relative impact of both cumulative pollutants and SLCPs on realized warming 20–40 years after the time of emission. If the overall goal of climate policy is to limit peak warming, GWP100 therefore overstates the importance of current SLCP emissions unless stringent and immediate reductions of all climate pollutants result in temperatures nearing their peak soon after mid-century7, 8, 9, 10, which may be necessary to limit warming to “well below 2 °C” (ref. 1). The GWP100 can be used to approximately equate a one-off pulse emission of a cumulative pollutant and an indefinitely sustained change in the rate of emission of an SLCP11, 12, 13. The climate implications of traditional CO2-equivalent targets are ambiguous unless contributions from cumulative pollutants and SLCPs are specified separately.