Illumination Levels: Then and Now

The following excerpts are from the 1911 and 1925 editions of A Text-Book of Physics by Louis Bevier Spinney, Professor of Physics and Illuminating Engineering at Iowa State College (now Iowa State University) in Ames, Iowa.

From the 1911 edition…

ILLUMINATION

516. The intensity of illumination of any surface is defined as the ratio of the light received by the surface to the area of the surface upon which the light falls.  A unit of intensity which is oftentimes employed is known as the foot candle, and is defined as the intensity of illumination which would be present upon a screen placed at a distance of one foot from a standard candle.  The meter candle is a unit of intensity which is employed to some extent.

The table below gives a number of values of illumination such as are commonly observed, the intensity of illumination being expressed in foot candles.

Suitable for drafting table    .    .    .    .    .    5 to 10

Suitable for library table   .    .    .    .    .   .    3 to 4

Suitable for reading table   .    .    .    .    .   .  1 to 2

Required for street lighting   .    .    .    .    .  0.05 to 0.60

Moonlight (full moon)    .    .    .    .    .    .   .  0.025 to 0.03

 

And from the 1925 edition…

ILLUMINATION

532.  The eye has a remarkable power of adaptation.  In strong light the pupil contracts and in weak light expands, so that we are able to use our eyes throughout a range of illumination which is really quite astonishing.  However, the continued use of the eyes under conditions of unfavorable illumination causes discomfort, fatigue, and even permanent injury.  Experiment and experience show that eye comfort, efficiency, and health considerations demand for each kind of eye work a certain minimum illumination.  Some of these illumination values taken from tables recently compiled are given below.

FOOT-CANDLES

Streets    .    .    .    .    .    .    .    .    .     .    .    .    .    .    1/20 to 1/4

Living rooms; Halls and passageways    .    .    1 to 2

Auditoriums; Stairways and exits;
Machine shops, rough work    .     .    .    .    .    .  2 to 5

Classrooms; Laboratories; Offices;
Libraries; Machine shops, close work    .    .    5 to 10

Engraving; Fine repairing work; Drafting;
Sewing and weaving, dark goods  .    .    .    .     10 to 20

 

By comparing the 1911 and 1925 data with the illumination levels recommended today by IESNA, we can see that recommended light levels for streetlighting have increased anywhere from 40% to 380% since 1925.  A cynic might say that we need more light than our ancestors did to see well at night.  As you may have noticed, light levels have been steadily creeping upward, everywhere, over the last few decades.

Recommended Illumination Levels for Streetlighting

Year        Minimum    Average    Maximum

1911             0.05                ???               0.60

1925           0.05               0.25               ???

1996          0.07                1.20               ???

Have you ever noticed how well you can see at night when the full moon is lighting the ground?  The full moon provides surprisingly adequate non-glaring and uniform illumination at just 0.03 footcandles!  For inspiration, take a look at the following text from an Ames, Iowa city ordinance, dated July 8, 1895:

“The said grantees shall keep said lamps in good condition and repair, and have the same lighted every night in the year from dark until midnight, and from 5:00 a.m. until daylight, except such moonlight nights or fractions of the same as are not obscured by clouds, and as afford sufficient natural light to light the streets of said city.”

This was originally published as IDA Information Sheet 114 in November 1996, and authored by David Oesper.

What is a Vacuum?

A vacuum is not nothing.    It is only a region of three-dimensional space that is entirely devoid of matter, entirely devoid of particles.

The best laboratory vacuum contains about 25 particles (molecules, atoms) per cubic centimeter (cm3).

The atmosphere on the surface of the Moon (if you can call it that) contains a lot more particles than the best laboratory vacuum: about 40,000 particles per cm3.  This extremely tenuous lunar atmosphere is mostly made up of the “noble” gases argon, helium, and neon.

The vacuum of interplanetary space contains about 11 particles per cm3.

The vacuum of interstellar space contains about 1 particle per cm3.

The vacuum of intergalactic space contains about 10-6 particles per cm3.  That’s just 10 particles per cubic meter of space.

But what if we could remove all of the particles in a parcel of space?  And somehow shield that empty parcel of space from any external electromagnetic fields?  What would we have then?

It appears that even completely empty space has some inherent energy associated with it.  The vacuum is constantly “seething” with electromagnetic waves of all possible wavelengths, popping into and out of existence on unimaginably short time scales—allowed by Heisenberg’s energy-time uncertainly principle.  These “quantum flourishes” may be a intrinsic property of space—as is dark energy.  Dark matter, on the other hand, is some weird form of matter that exists within space, exerting gravitational influence but not interacting with normal matter or electromagnetic waves in any other way.

Is there any evidence of this vacuum energy, or is it all theoretical?  There are at least three phenomena that point to the intrinsic energy of empty space.  (1) The Casimir effect; (2) Spontaneous emission; and (3) The Lamb shift.

The Casimir effect
Take two uncharged conductive plates and put them very close to each other, just a few nanometers apart.  Only the shortest wavelengths will be able to exist between the plates, but all wavelengths will exist on the other side of the two plates.  Under normal circumstances, this will cause a net force or pressure that pushes the two plates towards one another.

Spontaneous emission
An example of spontaneous emission is an electron transitioning from an excited state to the ground state, emitting a photon.  What causes this transition to occur when it does?

The Lamb shift
The Lamb shift is a tiny shift in the energy levels of electrons in hydrogen and other atoms that can’t be explained without considering the interaction of the atom with “empty” space.

References
Reucroft, S. and Swain, J., “What is the Casimir effect?”, Scientific American, https://www.scientificamerican.com/article/what-is-the-casimir-effec/.  Accessed 20 Feb 2018.

Koks,D. and Gibbs, P., “What is the Casimir effect?”, http://math.ucr.edu/home/baez/physics/Quantum/casimir.html.  Accessed 20 Feb 2018.