Physics
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006georl..3317801s&link_type=abstract
Geophysical Research Letters, Volume 33, Issue 17, CiteID L17801
Physics
19
Atmospheric Composition And Structure: Cloud Physics And Chemistry, Atmospheric Composition And Structure: Aerosols And Particles (0345, 4801, 4906), Atmospheric Processes: Clouds And Aerosols
Scientific paper
Under conditions commonly found in Earth's atmosphere, water can form two solid phases; hexagonal ice (Ih) and cubic ice (Ic). Recent reports have suggested that Ic may form in the atmosphere under a wider range of conditions than previously believed. In light of these reports, the formation of Ic has been suggested as one contributing factor for in-situ observations of persistent in-cloud supersaturations in cold cirrus. However, an accurate evaluation of the contribution of Ic formation to the observed supersaturations requires knowledge of the saturation vapor pressure of Ic, which has not been measured. In this manuscript, we report direct measurements of the vapor pressure of Ic over the temperature range 180-190 K. Over this temperature range, the vapor pressure of the cubic phase is 10.5 +/- 2.5% higher than that of the hexagonal phase. Field measurements of in-cloud supersaturations made during CRYSTAL-FACE are also re-analyzed and discussed.
Bertram Allan K.
Jensen Eric J.
Murray John B.
Shilling John E.
Tolbert Margaret A.
No associations
LandOfFree
Measurements of the vapor pressure of cubic ice and their implications for atmospheric ice clouds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Measurements of the vapor pressure of cubic ice and their implications for atmospheric ice clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measurements of the vapor pressure of cubic ice and their implications for atmospheric ice clouds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1079264