Open Access
Table 1
Symbols and abbreviations used repeatedly.
Abbreviation | Description | Example unit |
---|---|---|
Physical parameters in the gas parcel | ||
t | Simulation integration time | yr, s |
Tgas | Gas temperature | K |
NH | Hydrogen atom column density | cm−2 |
NH | Hydrogen atom number density | cm−3 |
n(H2) | Hydrogen molecule number density | cm−3 |
ζ | Cosmic-ray ionisation rate | s−1 |
Granular parameters | ||
ng | Number density of interstellar grains | cm−3 |
Td | Dust grain temperature | K |
a | Dust grain radius | μm |
b | Ice mantle thickness on grains | μm, MLs |
X:H2O | Icy species’ X abundance relative to that of water ice | % |
ML | Monolayer –ice layer with the thickness of a single molecule | |
Desorption energy parameters | ||
ED | Surface molecule desorption (binding) energy | K |
Ediff | Surface molecule diffusion energy; 0.5ED | K |
ED,pol | Default base ED value, on H2O ice surface | K |
ED,np | ED on hyper-volatile (CO) ice surface | K |
ED,bare | ED for molecules on completely bare grains | K |
ED,np/ED,pol | Factor for ED,pol change in CO ices | |
ED,pol-ED,bare | Energy value of a H-bond. | K |
EA | Reaction activation energy | K |
Xdes | Fitting parameter for ED on mixed ice, Eq. (3) | |
H-bond rule | Bare grain surface does not form hydrogen bonds. | |
Hyper-volatiles | Icy species with ED lower than ≈1300 K | |
Efficiency parameters for desorption mechanisms | ||
fCRD | Frequency of cosmic-ray induced heating of whole grains | s−1 |
Ypd | UV photodesorption yield. | molecule photon−1 |
fCD | Probability for surface reaction product desorption |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.