ライフサイエンスコーパス: far-ultraviolet

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

5 Far ultraviolet circular dichroism spectroscopy is used

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

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

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

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

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

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

12 Far-ultraviolet circular dichroism spectra show that [19

13 Far-ultraviolet circular dichroism spectra showed that [

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

31 We present Far-Ultraviolet Spectroscopic Explorer observations of t

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

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

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

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

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