PHIRE is a goniometer/reflectometer experiment. It is designed to measure the reflected radiance from a surface as a function of the angles of incidence and emission and the phase angle (i, e, and g, respectively, see figure). The concept for the experiment is similar to the Bloomsburg University Goniometer (BUG; run by Michael Shepard) and the Spectro-gonio-radiometer developed at the IPAG/University of Grenoble by Bernard Schmitt. Slightly different systems are used at JPL and the Astronomy Group (including Karri Muinonen) of the University of Helsinki also work in this field.
It is possible to infer the properties of a surface from the way it scatters light. Surfaces that are quite rough tend to show a surge in the reflected radiance as the angles of emission and incidence reach zero. The sizes of the particles that make up the surface also play a role. The scattering is complicated but in recent years several theoretical developments have been made (notably by Bruce Hapke and Michael Mischenko), which we can now test by experiments. The results can be used to test model of the scattering properties of surfaces on, for example, Mars, Mercury and the Moon.
We are interested in the scattering properties of surfaces for several reasons. Firstly, we have been using the experiment to study the reflectance behaviour of simulants of the Mercury surface. This will be important for calculating signal to noise ratios for the BepiColombo Laser Altimeter (BELA). Secondly, the reflectance properties of Martian surface materials have been of interest to us in the past, particularly for Mars Pathfinder and for the MER missions. We are also interested in measuring photometric properties of icy samples containing impurities, analogues to cometary surfaces or icy satellites, in support of the ROSETTA (VIRTIS, OSIRIS) and JUICE missions (GALA). Finally, the surface of Titan may have some rather bizarre surface materials. PHIRE-1 and -2 can be used to study whether the scattering properties of these materials are unusual.
The first version of the instrument was fully described by Gunderson et al. in a paper in Planetary and Space Science in 2006. The system is sufficiently simple that students can use it in the advanced practicum at the University.
A second version of the instrument was built to permit measurements at sub-zero temperatures and hence to study the photometry of samples containing ice. We have also applied a series of modifications to improve the general performances of the instrument (in particular the measurement speed) and to make the measurement procedure fully automatic, allowing the user to concentrate on the sample preparation and characterisation.
Both the hardware and the software parts of the PHIRE-2 instrument were entirely designed and developed at the Physikalisches Institut in Bern. The PHIRE-2 instrument shares some characteristics with the PHIRE-1 instrument, the BUG instrument operated at Bloomsburg University by M. Shepard and the Spectro-gonio-radiometer operated at Grenoble University by B. Schmitt.
The PHIRE-2 instrument is the central part of the Planetary Ice laboratory where analogue samples are characterised using different complementary methods: photometry, microscopy, electric and thermal properties etc.
Bernhard Jost, Antoine Pommerol, Olivier Poch, Yann Brouet, Sonia Fornasier, Nathalie Carrasco, Cyril Szopa, Nicolas Thomas (2017b) Bidirectional reflectance of laboratory cometary analogues to interpret the spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko, Planetary and Space Science, Volume 148.
Bernhard Jost, Antoine Pommerol, Olivier Poch, Zuriñe Yoldi, Sonia Fornasier, Pedro Henrique Hasselmann, Clément Feller, Nathalie Carrasco, Cyril Szopa and Nicolas Thomas (2017a) Bidirectional reflectance and VIS-NIR spectroscopy of cometary analogues under simulated space conditions, Planetary and Space Science, Volume 145, 14-27.
B. Jost, A. Pommerol, O. Poch, B. Gundlach, M. Leboeuf, M. Dadras, J. Blum and N. Thomas (2016). Experimental characterization of the opposition surge in fine-grained water–ice and high albedo ice analogs, Icarus, Volume 264.
Yoldi, Z., Pommerol, A., Jost, B., Poch, O., Gouman, J., & Thomas, N. (2015). VIS‐NIR reflectance of water ice/regolith analogue mixtures and implications for the detectability of ice mixed within planetary regoliths. Geophysical Research Letters, 42(15), 6205-6212.
Pommerol, A., N. Thomas, B. Jost, P. Beck, C. Okubo, and A.S. McEwen, (2013) Photometric properties of Mars soils analogs, J. Geophys. Res. 118, 2045-2072.
Jost, B., B. Gundlach, A. Pommerol, J. Oesert, S.N. Gorb, J. Blum, N. Thomas, (2013), Micrometer-sized ice particles for planetary-science experiments - II. Bidirectional reflectance, Icarus 225, 352-366.
Beck, P., A. Pommerol, N. Thomas, B. Schmitt, F. Moynier and J.-A. Barrat, (2012), The Photometry of Meteorites, Icarus, 218, 364-377.
Pommerol, A., N. Thomas, M. Affolter, G. Portyankina, B. Jost, K. Seiferlin, and K.-M. Aye, (2011), Photometry and bulk physical properties of Solar System surfaces icy analogs: the Planetary Ice Laboratory at University of Bern, Planetary and Space Science, 59, 1601-1612.
Gunderson, K.and N.Thomas, (2008) Polarimetric NIR reflectance measurements of regolith simulants at zero phase angle, Planetary and Space Science, 56, 1925-1938.
Gunderson, K., B.S. Lüthi, P. Russell, and N. Thomas, (2007) Visible/NIR photometric signatures of liquid water in Martian regolith simulant, Planetary and Space Science, 55, 1272-1282.
Gunderson, K., N.Thomas, and J.A.Whitby, (2006) First measurements with the Physikalisches Institut Radiometric Experiment (PHIRE), Planetary and Space Science, 54, 1046-1056.