ライフサイエンスコーパス: far-ultraviolet

1 The wake is visible only in the far ultraviolet and is consistent with an unusual emissi

2 Far-ultraviolet and near-ultraviolet circular dichroism

3 Far-ultraviolet aurora morphology reveals the influence

4 Irradiation at far ultraviolet C (far-UVC) 222 nm by krypton chloride (

5 Far-ultraviolet C (Far-UVC) radiation, with a wavelength

6 Far-ultraviolet-C (far-UVC) irradiation has emerged as a

7 Far ultraviolet-CD spectra for r-NTP and r-PRG B at pH 7

8 Far ultraviolet circular dichroism spectroscopy is used

9 l with the unfolding transition monitored by far ultraviolet circular dichroism.

10 In addition, cryptophycin-52 perturbed the far-ultraviolet circular dichroic spectrum of tubulin an

11 Far-ultraviolet circular dichroism (UV CD) spectra revea

12 Structural studies using far-ultraviolet circular dichroism (UV--CD) and thermal

13 initiated by manual mixing were monitored by far-ultraviolet circular dichroism and fluorescence spec

14 equilibrium unfolding of OPH as monitored by far-ultraviolet circular dichroism and intrinsic tryptop

15 structurally nonintrusive in solution using far-ultraviolet circular dichroism and unraveled the pre

16 Far-ultraviolet circular dichroism spectra show that [19

17 Far-ultraviolet circular dichroism spectra showed that [

18 t absorption and circular dichroism spectra, far-ultraviolet circular dichroism spectra, and infrared

19 hermal denaturation experiments monitored by far-ultraviolet circular dichroism, limited trypsin dige

20 the corresponding change in conformation by far-ultraviolet circular dichroism.

21 here is residual structure left as probed by far-ultraviolet circular dichroism.

22 Here we report persistent, faint, far-ultraviolet emission from the jovian footprints of G

23 the plume generated by the LCROSS impact as far-ultraviolet emissions from the fluorescence of sunli

24 If the surface were irradiated by a far-ultraviolet flux approximately 10(3) times that of t

25 C-labeled and unlabeled aerosol generated by far ultraviolet (FUV) photochemistry of gas mixtures con

26 Here we report the observation of excess far-ultraviolet (FUV) emission in the outer regions of 1

27 contain massive stars, which are sources of far-ultraviolet (FUV) radiation.

28 A red point source in the far-ultraviolet is identified in deep, high-resolution i

29 major features of Jupiter's aurora (based on far-ultraviolet, near-infrared and visible-wavelength ob

30 We report far-ultraviolet observations of Jupiter's moon Europa ta

31 Here we report far-ultraviolet observations of the nearby low-mass star

32 ious attempts to detect N2 absorption in the far-ultraviolet or infrared (ice features) have hitherto

33 We present the first analysis of far-ultraviolet reflectance spectra of regions on Rhea's

34 s a decrease in ellipticity over most of the far-ultraviolet region of the spectrum (between 205-240

35 produce a significant dichroic signal in the far-ultraviolet region.

36 h the wild-type and the W139F enzymes in the far-ultraviolet show about the same degree of ellipticit

37 The far-ultraviolet space telescope (FAUST) was flown on Spa

38 cted in a spectrum of Mars observed with the Far Ultraviolet Spectroscopic Explorer.

39 We present Far-Ultraviolet Spectroscopic Explorer observations of t

40 Well-resolved far-ultraviolet spectroscopic images of O I, S I, and pr

41 platform for on-demand drug delivery using a far ultraviolet (UV) light-degradable polymer, which all

42 cture elements leads to intense bands in the far-ultraviolet (UV).

43 ze 6 years' worth of Earth disk emissions at far ultraviolet wavelengths acquired by the Global Ultra

44 e report the detection of interstellar N2 at far-ultraviolet wavelengths towards the moderately redde