Fig. 10 Map of light pollution’s visual impact on the night sky.

Slides:



Advertisements
Similar presentations
The Eye. Rods and Cones The eye is made of cells that are called Rods and Cones. Cone cells are coned shaped and Rod cells are rod shaped.
Advertisements

© red ©
Color.
Color. -Visual light -An integral part of the sculpture -Creates desired effect -Distinguish items -Strengthen interest.
IPC Notes Light & Color. The colors of light that we see are the colors of light that an object reflects towards our eyes. ex) blue jeans absorb all colors.
Colour Theory.
Is the practical guidance to color mixing and the visual effects of a specific color combination.
Photoreceptors Rods “Blue” Cones “Yellow” Cones –“Green” –“Red”
C o l o u r s Created by – Ganesh Satimeshram.
The new world atlas of artificial night sky brightness by Fabio Falchi, Pierantonio Cinzano, Dan Duriscoe, Christopher C. M. Kyba, Christopher D. Elvidge,
THIS IS NOT YELLOW Philosophy.
Why is the sky blue?.
Colours.
Two ways to discuss color 1) Addition 2) Subtraction
An Overview of the Element of Colour
Surface depiction of cluster II epitopes on the surface of ricin toxin
What Color is it?.
Chapter 14: Light Section 2: Light and Color
COLOURS.
Fig. 4 Pupil shape and image quality in the model sheep eye.
Fig. 5 In vivo MIP imaging of lipid and protein in C. elegans.
Fig. 1 Upward emission functions used to compute the maps.
Fig. 2 Tera-Wasserburg plot of zircon dates from LASS and APM data.
Fig. 4 Estimations of nonlinear functionals of a single-qubit state with the quantum Fredkin gate. Estimations of nonlinear functionals of a single-qubit.
Fig. 4 States of the Antarctic Ice Sheet after 10,000 years.
Fig. 7 LSH database and similarity search example.
Fig. 2 Changes in ice surface elevation, h, of Thwaites Glacier.
Fig. 4 Power and wavelet spectra of benthic δ18O.
Fig. 3 Aβ16–22 can interact with Aβ40 monomers and dimers.
Fig. 1 Map of the trifurcation area of the SJFZ.
Fig. 3 Faculty placement distributions.
Fig. 2 Fluence-dependent emission characteristics of CH3NH3PbI3 recorded at 15 and 300 K. Fluence-dependent emission characteristics of CH3NH3PbI3 recorded.
Fig. 1 Study area and field site setting.
Fig. 3 Controlled phase shift.
Fig. 1 Fastest and simplest paths in primal and dual networks.
Fig. 2 Time series of ice loss from the Amundsen Sea sector for the cases of unperturbed destabilization (black) and mass deposition (colored). Time series.
Fig. 6 External drivers and model response.
Fig. 2 Genetic structure of the three species.
Fig. 2 Images of complex structures formed via sequential folding.
Fig. 2 Spatial distribution of earthquake density derived from a catalog spanning 93 nights of the LB Array data set. Spatial distribution of earthquake.
Fig. 4 Identification of C
Fig. 3 ET dynamics on the control and treatment watersheds during the pretreatment and treatment periods. ET dynamics on the control and treatment watersheds.
Fig. 3 Evolutions of freshwater transport and salinity.
Fig. 4 FRESH printed scaffolds with complex internal and external architectures based on 3D imaging data from whole organs. FRESH printed scaffolds with.
Fig. 5 Maps of Europe’s artificial sky brightness, in twofold increasing steps, as a ratio to the natural sky brightness (assumed to be 174 μcd/m2). Maps.
Fig. 4 Relationships between light and economic parameters.
Fig. 3 Plumage brightness (PC1) for each sex in relation to morphological, ecological, and behavioral traits. Plumage brightness (PC1) for each sex in.
Fig. 1 Fractional coverage of the mapping method used in this study.
Fig. 2 Evolution of seismic source and statistical properties of induced seismicity in response to fluid injection. Evolution of seismic source and statistical.
Fig. 4 City sectors ranked by per-industrial output emissions.
Fig. 3 Maximal energy intake.
Fig. 4 Guided-wave propagation in a single-crystalline KDP hexagonal microstructure. Guided-wave propagation in a single-crystalline KDP hexagonal microstructure.
Fig. 2 Number of years that would have been required for the observed vertebrate species extinctions in the last 114 years to occur under a background.
Fig. 4 The relationship between the total mean absolute momentum disturbance 〈∣p∣〉zB (in units of ℏ/D) and fringe visibility V. The relationship between.
Fig. 2 RVFV causes pathology within the liver, uterus, and placenta of pregnant dams. RVFV causes pathology within the liver, uterus, and placenta of pregnant.
Interpreted seismic reflection image across reactivated fracture zones
Fig. 19 Comparisons between sky brightness NPS CCD observations and atlas predictions. Comparisons between sky brightness NPS CCD observations and atlas.
Fig. 5 Fabrication of origami structures by two-side illuminations.
Fig. 2 Observation of type II Weyl nodes in LaAlGe.
Fig. 2 OH formation and speciation in the PAA – Fe(II) system.
Fig. 1 Distribution of deformation and aqueous alteration in MIL
SEM and TEM images and photoluminescence properties of composites
Fig. 3 Voltage-driven phase switching in a 1T-TaS2 nano-thick crystal.
Fig. 4 Matrix for intersections of differentially expressed transcripts between RNAiAFL transgenic and null kernels. Matrix for intersections of differentially.
Fig. 2 Spatial distribution of five city groups.
Fig. 4 In situ mapping of human patient breast cancer and stroma.
Fig. 5 Spatial resolution of the optogenetic activation achieved with OLED microarrays. Spatial resolution of the optogenetic activation achieved with.
Fig. 3 Genome editing of the MSTN gene.
Fig. 1 Uplift of the Isthmus of Panama and global sea levels over the last 20 My. Uplift of the Isthmus of Panama and global sea levels over the last 20.
Fig. 3 Spatial distribution of the shoot density (high densities are represented in dark green and low ones in bright yellow) in a simulation of a P. oceanica.
Presentation transcript:

Fig. 10 Map of light pollution’s visual impact on the night sky. Map of light pollution’s visual impact on the night sky. The sky brightness levels are those used in the tables and indicate the following: up to 1% above the natural light (0 to 1.7 μcd/m2; black); from 1 to 8% above the natural light (1.7 to 14 μcd/m2; blue); from 8 to 50% above natural nighttime brightness (14 to 87 μcd/m2; green); from 50% above natural to the level of light under which the Milky Way is no longer visible (87 to 688 μcd/m2; yellow); from Milky Way loss to estimated cone stimulation (688 to 3000 μcd/m2; red); and very high nighttime light intensities, with no dark adaption for human eyes (>3000 μcd/m2; white). Fabio Falchi et al. Sci Adv 2016;2:e1600377 Copyright © 2016, The Authors