@prefix isq: <https://w3id.org/standards/isq/ontologies/core/> .
@prefix smart: <https://example.org/smart-sdu/> .
@prefix rdf: <http://www.w3.org/1999/02/22-rdf-syntax-ns#> .
@prefix dcterms: <http://purl.org/dc/terms/> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .

<isq:t7-16>
  a isq:Entry ;
  rdf:type isq:Quantity ;
  rdf:type smart:TermEntry ;
  dcterms:identifier "7-16" ;
  skosxl:prefLabel "illuminance"@en ;
  skosxl:altLabel "E_\"v\""@en ;
  skosxl:altLabel "(E)"@en ;
  skos:definition "density of incident luminous flux with respect to area at a point on a real or imaginary surface, expressed by\n\n[stem%unnumbered]\n++++\nE_\"v\" = (\"d\"Phi_\"v\")/(\"d\"A)\n++++\n\nwhere stem:[Phi_\"v\"] is luminous flux (<<t7-13>>) and stem:[A] is the area (<<iso80000-3>>) on which the luminous flux is incident\n"@en ;
  smart:hasBindingnessType "bindingness-type:normative" ;
  dcterms:isPartOf <isq:part-7> ;
  isq:hasUnit [
    skos:notation "lx" ;
    skosxl:prefLabel "lux"@en
  ] ;
  isq:hasUnit [
    skos:notation "cd*sr*m^(-2)" ;
    skosxl:prefLabel "candela steradian per square metre"@en
  ] ;
  skos:note "Illuminance can be derived from the spectral irradiance distribution by\n\n[stem%unnumbered]\n++++\nE_\"v\" = K_\"m\" int_0^(oo) E_(\"e\",lambda)(lambda)V(lambda)\"d\"lambda\n++++\n\nwhere stem:[K_\"m\"] is maximum luminous efficacy (<<t7-11.3>>), stem:[E_(\"e\",lambda)(lambda)] is the spectral irradiance (<<t7-7.2>>) at wavelength stem:[lambda] (<<iso80000-3>>), and stem:[V(lambda)] is spectral luminous efficiency (<<t7-10.2>>).\n\nIntegral limits can be confined depending on the spectral sensitivity of the detectors used as a sensor.\n\nThe corresponding radiometric quantity is \"irradiance\" (<<t7-7.1>>). The corresponding quantity for photons is \"photon irradiance\" (<<t7-23>>).\n\nThe quantity \"spherical illuminance\" is defined by the mean value of illuminance on the outer curved surface of a very small (real or imaginary) sphere at a point in space.\n\nIt can be expressed by\n\n[stem%unnumbered]\n++++\nE_(\"v\",0) = int_(4pi)L_\"v\"\"d\"Omega\n++++\n\nwhere stem:[Omega] is solid angle (<<iso80000-3>>) and stem:[L_\"v\"] is luminance (<<t7-15>>).\n\nIt can be expressed by the quotient of the luminous flux (<<t7-13>>) of all the light incident on the outer surface of an infinitely small sphere centred at the given point, and the area (<<iso80000-3>>) of the diametrical cross-section of that sphere.\n"@en ;
  iso:urn <urn:iso:std:iso:80000:-7:ed-2:en:item:7-16> .
