A ray may be thought of as each of the lines in which light (and heat or other radiation) may seem to stream from the Sun or any luminous (radiative) body, or pass through a small opening.
Def. a "beam of light or radiation" is called a ray.
Def. an action or process of throwing or sending out a traveling ray in a line, beam, or stream of small cross section is called radiation.
The term radiation is often used to refer to the ray itself.
Def. “[t]he shooting forth of anything from a point or surface, like the diverging rays of light; as, the radiation of heat” is called radiation.
Rays may have a temporal, spectral, or spatial distribution.
They may also be dependent on other variables as yet unknown.
"A delta ray is characterized by very fast electrons produced in quantity by alpha particles or other fast energetic charged particles knocking orbiting electrons out of atoms. Collectively, these electrons are defined as delta radiation when they have sufficient energy to ionize further atoms through subsequent interactions on their own."
"Epsilon radiation is tertiary radiation caused by secondary radiation (e.g., delta radiation). Epsilon rays are a form of particle radiation and are composed of electrons. The term is very rarely used today." Bold added.
Optical astronomy includes those portions of ultraviolet, visual, and infrared astronomy that benefit from the use of quartz crystal or silica glass telescope components."Fused quartz is manufactured by fusing (melting) naturally occurring quartz crystals of high purity at approximately 2000 °C, using either an electrically heated furnace (electrically fused) or a gas/oxygen-fuelled furnace (flame fused). Fused quartz is normally transparent. The optical and thermal properties of fused quartz are superior to those of other types of glass due to its purity. For these reasons, it finds use in situations such as semiconductor fabrication and laboratory equipment. It has better ultraviolet transmission than most other glasses, and so is used to make lenses and other optics for the ultraviolet spectrum."
"Fused silica is produced using high-purity silica sand as the feedstock, and is normally melted using an electric furnace, resulting in a material that is translucent or opaque. (This opacity is caused by very small air bubbles trapped within the material.)"
"Synthetic fused silica is made from a silicon-rich chemical precursor usually using a continuous flame hydrolysis process which involves chemical gasification of silicon, oxidation of this gas to silicon dioxide, and thermal fusion of the resulting dust (although there are alternative processes). This results in a transparent glass with an ultra-high purity and improved optical transmission in the deep ultraviolet."
""UV grade" synthetic fused silica (sold under various tradenames including "HPFS", "Spectrosil" and "Suprasil") has a very low metallic impurity content making it transparent deeper into the ultraviolet. An optic with a thickness of 1 cm will have a transmittance of about 50% at a wavelength of 170 nm, which drops to only a few percent at 160 nm. However, its infrared transmission is limited by strong water absorptions at 2.2 μm and 2.7 μm. "Infrared grade" fused quartz (tradenames "Infrasil", "Vitreosil IR" and others) which is electrically fused, has a greater presence of metallic impurities, limiting its UV transmittance wavelength to around 250 nm, but a much lower water content, leading to excellent infrared transmission up to 3.6 μm wavelength. All grades of transparent fused quartz/fused silica have nearly identical physical properties. The water content (and therefore infrared transmission of fused quartz and fused silica) is determined by the manufacturing process. Flame fused material always has a higher water content due to the combination of the hydrocarbons and oxygen fuelling the furnace forming hydroxyl [OH] groups within the material. An IR grade material typically has an [OH] content of <10 parts per million."
"The optical dispersion of fused silica can be approximated by the following Sellmeier equation:
where the wavelength '"`UNIQ--postMath-00000002-QINU`"' is measured in micrometers."
"This equation is valid between 0.21 and 3.71 micrometers and at 20 °C. Its validity was confirmed for wavelengths up to 6.7 '"`UNIQ--postMath-00000003-QINU`"'m. Experimental data for the real (refractive index) and imaginary (absorption index) parts of the complex refractive index of fused quartz [is available] over the spectral range from 30 nm to 1000 '"`UNIQ--postMath-00000004-QINU`"'m ... online."
"For the case of a [double-convex] lens of thickness d in air, and surfaces with radii of curvature R1 and R2, the effective focal length f is given by:
where n is the refractive index of the lens medium. The quantity 1/f is also known as the optical power of the lens."
"In most photography and all telescopy, where the subject is essentially infinitely far away, longer focal length (lower optical power) leads to higher magnification and a narrower angle of view; conversely, shorter focal length or higher optical power is associated with a wider angle of view."
The 35 mm lens in the image at right has an aperture range of '"`UNIQ--postMath-00000009-QINU`"' to '"`UNIQ--postMath-0000000A-QINU`"'
The lens at right uses "a standard f-stop scale, which is an approximately geometric sequence of numbers that corresponds to the sequence of the powers of the square root of 2: '"`UNIQ--postMath-0000000B-QINU`"' '"`UNIQ--postMath-0000000C-QINU`"' '"`UNIQ--postMath-0000000D-QINU`"' '"`UNIQ--postMath-0000000E-QINU`"' '"`UNIQ--postMath-0000000F-QINU`"' '"`UNIQ--postMath-00000010-QINU`"' '"`UNIQ--postMath-00000011-QINU`"' '"`UNIQ--postMath-00000012-QINU`"' '"`UNIQ--postMath-00000013-QINU`"' [and] '"`UNIQ--postMath-00000014-QINU`"'"
"The sequence above is obtained by approximating the following exact geometric sequence:"
"The Russians have found crystal lenses, perfectly spherical and of great precision, in ancient Egypt, during the African-dominated period."
"There are now 23 ancient lenses on display in the Archaeological Museum at Herakleion and many more are in storage there. They are also made of rock crystal and are of optical quality, with generated plano-convex surfaces."
There is more about lenses more recently from Visby, Gotland. "What intrigues the researchers is that the lenses are of such high quality that they could have been used to make a telescope some 500 years before the first known crude telescopes were constructed in Europe in the last few years of the 16th century." "Made from rock-crystal, the lenses have an accurate shape that betrays the work of a master craftsman. The best example of the lenses measures 50 mm (2 inches) in diameter and 30 mm (1 inch) thick at its centre." "The [Visby] Gotland crystals provide the first evidence that sophisticated lens-making techniques were being used by craftsmen over a 1,000 years ago."
"If one Italian scientist is correct then the telescope was not invented sometime in the 16th century by Dutch spectacle makers, but by ancient Assyrian astronomers nearly three thousand years earlier. According to Professor Giovanni Pettinato of the University of Rome, a rock crystal lens, currently on show in the British museum, could rewrite the history of science. He believes that it could explain why the ancient Assyrians knew so much about astronomy."
|Name (or identification)||Discovery period||Location||Approximate date||Source unless noted otherwise|
|Egyptian lenses||IV/V Dynasties||Egypt, eyes in funerary statues||2620-2400 BC|||
|Evans lenses (plano-convex)||Middle Minoan IIIB||Temple Repositories at Knossos, along with a "royal Draught Board" with ivory and crystal inlays backed with silver foil||1640-1600 BC, Minoan civilization||A. Evans, The Palace of Minos I (London 1921) 469-72; cf. the eye of the steatite bull's-head rhyton from the Little Palace at Knossos: Evans, The Tomb of the Double Axes etc (London 1914) 82.|
|"Three bossed crystal discs" (plano-convex)||Late Minoan II-IIIA||Mavrospelio cemetery||1425-1340 BC||E. J. Forsdyke, "The Mavro Spelio Cemetery at Knossos," BSA 28 (1926-1927) 243-96, esp. 288.|
|Artemision lenses (plano-concave)||Archaic levels||the Artemision of Ephesos||3300-1200 BC||D.G. Hogarth, Excavations at Ephesus: The Archaic Artemisia (London 1908) 210-11, pl. 46.|
|Schliemann lenses (plano-convex)||Troy||Troy||1334-1184 BC||V. Tolstikov and M. Treister, The Gold of Troy: Searching for Homer's Fabled City (London 1996) nos. 176-216, 230.|
|Nimrud lens (plano-convex)||Neo-Assyrian||North West Palace, Room AB||750–710 BC||Austen Henry Layard at the Assyrian palace of Nimrud, in modern-day Iraq.|
|Roman London lens (fragmentary biconvex glass lens of light green color)||Roman London||Roman London||43-50 AD||H. Syer Cuming, "On Spectacles," The Journal of the British Archaeological Association 11 (1855) 144-49.|
|Pompeii lens (plano-convex)||excavations of the Via Stabia||"House of the Engraver"||79 AD||E. Gerspach, L'art de la verrerie (Paris 1885) 41-42.|
|four rock-crystal lentoids (plano-convex)||the historical period||Amathous||Temple of Aphrodite||M.-E Boussac in P. Aupert and A. Hermary, "Travaux de l'Ecole franlaise i Amathonte en 1979," BCH 104 (1980) 809, fig. 12; Aupert and Hermary, "Amathonte: Rapport préliminaire (1975-1979)," RDAC 1980, 237, pl. 32.6|
|Sakellarakis lenses (plano-convex)||historical period||Idaean Cave||historical period|||
Girolamo Cardano (1501-1576) made "a camera obscura with a diverting spectacle ... appears ... to have initiated the use of a convex lens in the aperture."
"Old Kingdom Egyptian statues from the first to the sixth dynasties had lenses placed in their eyes." "The thickness of the lenses was not intended to duplicate the thickness of the real human eye, but rather to create an effect so that the eye follows the person passing by when looked from other angles." "[T]he illusion of the following eye technique."
"The Archaic or Early Dynastic Period of Egypt immediately follows the unification of Lower and Upper Egypt c. 3100 BC. It [is] generally taken to include the First and Second Dynasties, lasting from the Protodynastic Period of Egypt until about 2686 BC, or the beginning of the Old Kingdom."
The eyes of these statues contain rock-crystals. "These are probably the oldest portrait statues in the world. These people who sit before us side by colored to the life, fresh and glowing as the day they gave the artist his last sitting lived at a time when the great pyramids were not yet built and at a date which is variously calculated as from about 4,000 to 6,300 years from the present day. The princess wears her hair precisely as it is still worn in Nubia and her necklace is of a pattern still favored. The eyes of both statues are inserted. The eyeball which is set in an eyelid of bronze, is made of opaque white quartz with an iris of rock-crystal enclosing a pupil of some kind of brilliant metal. This treatment gives to the eyes a look of intelligence which is almost appalling." Amelia B. Edwards "These incomparable statues are most expressive and stand in vitality to the works of any later age in Egypt. They were found in the tomb chamber- Ra-Ho-tep is entitled a royal son [probably of Seneferu]- The signs carved in these tombs are among the earliest known. Instead of full-length burial with coffins, head rests, vases, and provision for a future life, the more usual method of burial at Medum is lying on the left side with the knees drawn up facing the east and without vases or other objects, showing a diversity of beliefs and probably of races." W.M. Flinders Petrie.
"The composition of these eyes is a lens of polished rock crystal (either alpha silica or fused silica, formerly known as cystalline quartz and fused quartz which had a convex front surface and a near hemispherical concave ground pupil surface in a flat iris plane (normally covered with resin) at the rear of the lens."
"The Prehistory of Egypt spans the period of earliest human settlement to the beginning of the Early Dynastic Period of Egypt in ca. 3100 BC, starting with King Menes/Narmer."
"The Predynastic Period is traditionally equivalent to the Neolithic period, beginning ca. 6000 BC and including the Protodynastic Period (Naqada III)."
"Typical requirements for grinding and polishing a curved mirror ... require the surface to be within a fraction of a wavelength of light of a particular conic shape."
"Telescopes ... use front silvered or first surface mirrors, where the reflecting surface is placed on the front (or first) surface of the glass (this eliminates reflection from glass surface ordinary back mirrors have). Some of them use silver, but most are aluminium, which is more reflective at short wavelengths than silver. All of these coatings are easily damaged and require special handling. They reflect 90% to 95% of the incident light when new. The coatings are typically applied by vacuum deposition. A protective overcoat is usually applied before the mirror is removed from the vacuum, because the coating otherwise begins to corrode as soon as it is exposed to oxygen and humidity in the air. Front silvered mirrors have to be resurfaced occasionally to keep their quality."
"Cold mirrors are dielectric mirrors that reflect the entire visible light spectrum, while efficiently transmitting infrared wavelengths. These are the converse of hot mirrors."
"Hot mirrors reflect infrared light while allowing visible light to pass. These can be used to separate useful light from unneeded infrared to reduce heating of components in an optical device. They can also be used as dichroic beamsplitters. (Hot mirrors are the converse of cold mirrors.)"
“Active optics is a technology used with reflecting telescopes developed in the 1980s, which actively shapes a telescope's mirrors to prevent deformation due to external influences such as wind, temperature, mechanical stress. Without active optics, the construction of 8 metre class telescopes is not possible, nor would telescopes with segmented mirrors be feasible.”
Def. "[a]n optical system in telescopes that reduces atmospheric distortion by dynamically measuring and correcting wavefront aberrations in real time, often by using a deformable mirror" is called adaptive optics.
"Already it has allowed ground-based telescopes to produce images with sharpness rivalling those from the Hubble Space Telescope. The technique is expected to revolutionize the future of ground-based optical astronomy."
The slow-motion simulation at right is typical for adaptive optics operation of a telescope. "The left hand side shows what a point source (e.g. small star) would look like through a ground-based telescope without adaptive optics correction. The right hand side shows what is seen after adaptive optics correction has been applied. Note that the adaptive optics corrected image is normally very compact, but occasionally it "breaks up". If long exposure images are taken, the adaptive optics correction produces a sharp point at the centre of the image, while the uncorrected image is just a large fuzzy blob. Note that the pattern changes much more quickly when adaptive optics correction is applied. This can make it difficult to use adaptive optics corrected telescopes in an astronomical interferometer or for speckle imaging."
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