Abstract
Laboratory results of the optical properties of vapor-deposited water
ice, specifically the refractive index and extinction coefficient, are
available mainly for a selective set of wavelengths and a limited number
of deposition temperatures. Experimental limitations are the main reason
for the lack of broadband data, which is unfortunate as these quantities
are needed to interpret and predict astronomical and planetary
observations. The goal of this work is to address these lacking data,
using an experimental broadband method that is capable of rapidly
providing reliable water ice data across the entire UV-visible range.
This approach combines the simultaneous use of a monochromatic HeNe
laser and a broadband Xe-arc lamp to record interference fringes of
water ice during deposition at astronomically relevant ice temperatures.
The ice thickness is typically more than 20 μm. Analyzing the period
and intensity patterns combining both the monochromatic and broadband
interference patterns allows the determination of the
wavelength-dependent refractive index and extinction coefficient. We
present accurate refractive index and extinction coefficient graphs for
wavelengths between 250 and 750 nm and ices deposited between 30 and 160
K. From our data, we find a possible structural change in the ice in the
110-130 K region that has not been reported before. We also discuss that
the data presented in this paper can be used to interpret astronomical
observations of icy surfaces.
| Original language | English |
|---|---|
| Pages (from-to) | 179 |
| Journal | The Astrophysical Journal |
| Volume | 925 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1 Feb 2022 |
| Externally published | Yes |
Keywords
- Laboratory astrophysics
- Experimental techniques
- Surface ices
- 2004
- 2078
- 2117