Search results for "183.0"
showing 10 items of 82 documents
Do shifts in life strategies explain microbial community responses to increasing nitrogen in tundra soil?
2016
Subarctic tundra soils store large quantities of the global organic carbon (C) pool as the decomposition of plant litter and soil organic matter is limited by low temperatures and limiting nutrients. Mechanisms that drive organic matter decomposition are still poorly understood due to our limited knowledge of microbial communities and their responses to changing conditions. In subarctic tundra large grazers, in particular reindeer, exert a strong effect on vegetation and nutrient availability causing drastic nutrient pulses in the soils located along the migratory routes. Here we studied the effect of increased nitrogen (N) availability on microbial community structure and activities by lab…
"Table 9" of "Energy dependence of event shapes and of alpha(s) at LEP-2."
1999
Moments of the Small Jet Broadening (BMIN) distributions at cm energies 133, 161, 172 and 183 GeV.
"Table 11" of "Energy dependence of event shapes and of alpha(s) at LEP-2."
1999
Moments of the Jet Broadening Difference (BDIFF) distributions at cm energies 133, 161, 172 and 183 GeV.
"Table 46" of "Energy dependence of event shapes and of alpha(s) at LEP-2."
1999
ALPHAS from the higher energies extrapolated to the Z0 mass. The second systematic (DSYS) error is the scale error.
"Table 5" of "Energy dependence of event shapes and of alpha(s) at LEP-2."
1999
Moments of the Heavy Jet Mass (MH**2/EVIS**2) distributions at cm energies 133, 161, 172 and 183 GeV.
"Table 1" of "Energy dependence of event shapes and of alpha(s) at LEP-2."
1999
Moments of the (1-THRUST) distributions at cm energies 133, 161, 172 and 183 GeV.
"Table 7" of "Energy dependence of event shapes and of alpha(s) at LEP-2."
1999
Moments of the Jet Mass Differences (MDIFF**2/EVIS**2) distributions at cm energies 133, 161, 172 and 183 GeV.
"Table 4" of "Energy dependence of event shapes and of alpha(s) at LEP-2."
1999
Moments of the Oblateness distributions at cm energies 133, 161, 172 and 183 GeV.
"Table 9" of "Measurement of W pair production in e+ e- collisions at centre-of-mass energies from 183-GeV to 209-GeV."
2004
The measured cross section for the final state MU NU Q Q. The DSYS error is the typical systematic error.
"Table 12" of "Measurement of W pair production in e+ e- collisions at centre-of-mass energies from 183-GeV to 209-GeV."
2004
The measured cross section for the final state Q Q Q Q. The DSYS error is the typical systematic error.