Composite infrared spectrometer (CIRS) on Cassini: publisher's note.

Applied Optics Optica Publishing Group 56:21 (2017) 5897

Authors:

DE Jennings, FM Flasar, VG Kunde, CA Nixon, ME Segura, PN Romani, N Gorius, S Albright, JC Brasunas, RC Carlson, AA Mamoutkine, E Guandique, MS Kaelberer, S Aslam, RK Achterberg, GL Bjoraker, CM Anderson, V Cottini, JC Pearl, MD Smith, BE Hesman, RD Barney, S Calcutt, TJ Vellacott, LJ Spilker, SG Edgington, SM Brooks, P Ade, PJ Schinder, A Coustenis, R Courtin, G Michel, R Fettig, S Pilorz, C Ferrari

Mountain glaciers as paleoclimate proxies

Annual Review of Earth and Planetary Sciences Annual Reviews 49 (2017) 649-680

Authors:

Andrew N Mackintosh, Brian M Anderson, Raymond Pierrehumbert

Abstract:

Glaciers offer the potential to reconstruct past climate over timescales from decades to millennia. They are found on nearly every continent, and at the Last Glacial Maximum, glaciers were larger in all regions on Earth. The physics of glacier-climate interaction is relatively well understood, and glacier models can be used to reconstruct past climate from geological evidence of past glacier extent. This can lead to significant insights regarding past, present and future climate. For example, glacier modelling has demonstrated that the near ubiquitous global pattern of glacier retreat during the last few centuries resulted from a global-scale climate warming of ~1°C, consistent with instrumental data and climate proxy records. Climate reconstructions from glaciers also demonstrated that the tropics were colder at the Last Glacial Maximum than was originally inferred from sea surface temperature reconstructions. Future efforts to reconstruct climate from glaciers may provide new constraints on climate sensitivity to CO2 forcing, polar amplification of climate change, and more.

The PanCam Instrument for the ExoMars Rover

ASTROBIOLOGY 17:6-7 (2017) 511-541

Authors:

AJ Coates, R Jaumann, AD Griffiths, CE Leff, N Schmitz, J-L Josset, G Paar, M Gunn, E Hauber, CR Cousins, RE Cross, P Grindrod, JC Bridges, M Balme, S Gupta, IA Crawford, P Irwin, R Stabbins, D Tirsch, JL Vago, T Theodorou, M Caballo-Perucha, GR Osinski, P Team

Rayleigh scattering in the transmission spectrum of HAT-P-18b

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 468:4 (2017) 3907-3916

Authors:

J Kirk, PJ Wheatley, T Louden, AP Doyle, I Skillen, J McCormac, PGJ Irwin, R Karjalainen

Composite infrared spectrometer (CIRS) on Cassini

Applied Optics 56:18 (2017) 5274-5294

Authors:

DE Jennings, FM Flasar, VG Kunde, CA Nixon, ME Segura, PN Romani, N Gorius, S Albright, JC Brasunas, RC Carlson, AA Mamoutkine, E Guandique, MS Kaelberer, S Aslam, RK Achterberg, GL Bjoraker, CM Anderson, V Cottini, JC Pearl, MD Smith, BE Hesman, RD Barney, S Calcutt, TJ Vellacott, LJ Spilker, SG Edgington, SM Brooks, P Ade, PJ Schinder, A Coustenis, R Courtin, G Michel, R Fettig, S Pilorz, C Ferrari

Abstract:

© 2017 Optical Society of America. The Cassini spacecraft orbiting Saturn carries the composite infrared spectrometer (CIRS) designed to study thermal emission from Saturn and its rings and moons. CIRS, a Fourier transform spectrometer, is an indispensable part of the payload providing unique measurements and important synergies with the other instruments. It takes full advantage of Cassini's 13-year-long mission and surpasses the capabilities of previous spectrometers on Voyager 1 and 2. The instrument, consisting of two interferometers sharing a telescope and a scan mechanism, covers over a factor of 100 in wavelength in the mid and far infrared. It is used to study temperature, composition, structure, and dynamics of the atmospheres of Jupiter, Saturn, and Titan, the rings of Saturn, and surfaces of the icy moons. CIRS has returned a large volume of scientific results, the culmination of over 30 years of instrument development, operation, data calibration, and analysis. As Cassini and CIRS reach the end of their mission in 2017, we expect that archived spectra will be used by scientists for many years to come.