Open image in new window Fig. 3 UV Visible spectrum of temperature-dependent synthesis of Ag NPs by a A. cepa extract and b M. acuminata extract.
Temperature variation in natural environment was conducted in order to predict the action spectrum of temperature under natural environment by substituting the model to the segmented fitting method.
This phase is required not only to solve the flatness and horizon problems plagued in the big-bang cosmology but also to explain a nearly flat spectrum of temperature anisotropies observed in cosmic microwave background (CMB).
Assuming a Raymond-Smith type spectrum of temperature 0.3-1.2 0.3-1.2 a β-model density distribution for the X-ray halo, the central plasma density N0 and core radius Rc for the β model was constrained as [ N010−3cm−3]2 [Rc100keV] ≤ 5.80×10−3.
Figure 2 Spectra of temperature-dependent PL.
From these data, the first horizontal wavenumber spectra of temperature in the middle stratosphere are derived.
The climate action spectrums of temperature and relative humidity are built based on meteorological data of the temperature and the relative humidity variations.
Figure 9a shows an example of frequency spectra of temperature at the surface and near the tropopause observed by radiosondes launched three hourly from both sides of a coastline near Bengkulu, southwestern Sumatera.
The development of non-thermal atmospheric plasmas displaying spectra of temperature within or just above physiological ranges, i.e. tissue tolerable plasmas (TTP), has made the use of plasmas possible for biological or medical applications [ 8, 9].
The energy spectrum of low-temperature quantum oscillations of two interacting vertical Bloch lines in a domain wall of magnetic stripe domain was determined.
