with Simbol-X. - High Energy Astrophysics
... Simbol-X is a broad-band focusing hard-X-ray telescope that operates from 0.5 to 80 keV. The mission is sponsored jointly by CNES (French Space Agency) and ASI (Italian Space Agency). Its single optics module contains a set of nested nickel shells coated with special multilayers to boost high-energy ...
... Simbol-X is a broad-band focusing hard-X-ray telescope that operates from 0.5 to 80 keV. The mission is sponsored jointly by CNES (French Space Agency) and ASI (Italian Space Agency). Its single optics module contains a set of nested nickel shells coated with special multilayers to boost high-energy ...
Measuring Magnitudes
... surrounding the object you wish to measure. For example if you're trying to determine the magnitude of a star buried in nebulosity you would select a background area with roughly the same brightness as the nebulosity surrounding the star. If you are trying to measure the surface brightness of a gala ...
... surrounding the object you wish to measure. For example if you're trying to determine the magnitude of a star buried in nebulosity you would select a background area with roughly the same brightness as the nebulosity surrounding the star. If you are trying to measure the surface brightness of a gala ...
celt mthr spectrometer
... full 20 arc-minute TMT field of view and/or from AO-corrected fields. This multi-object mode could be fed from a wide variety of fiber inputs and fiber-based d-IFU’s. Though not likely to be funded at first-light (it requires the equivalent of an entirely separate fiber-positioner instrument to feed ...
... full 20 arc-minute TMT field of view and/or from AO-corrected fields. This multi-object mode could be fed from a wide variety of fiber inputs and fiber-based d-IFU’s. Though not likely to be funded at first-light (it requires the equivalent of an entirely separate fiber-positioner instrument to feed ...
Do It Yourself Telescopes
... On the celestial sphere, astronomers use lines similar to those of latitude and longitude on the Earth. The astronomical equivalent of latitude is declination, measured in degrees (°) of arc, positive for north and negative for south. Each degree is divided into sixty minutes ('), and each minute is ...
... On the celestial sphere, astronomers use lines similar to those of latitude and longitude on the Earth. The astronomical equivalent of latitude is declination, measured in degrees (°) of arc, positive for north and negative for south. Each degree is divided into sixty minutes ('), and each minute is ...
Chapter 18 OPTICAL ELEMENTS - Doane College Physics Web
... incident wave energy. At other kinds of surfaces, the fraction of energy reflected depends on the angle of incidence and on the index of refraction of the two media defining the interface. The index of refraction of a material is defined in Equation 18.2. The index of refraction plays the analogous ...
... incident wave energy. At other kinds of surfaces, the fraction of energy reflected depends on the angle of incidence and on the index of refraction of the two media defining the interface. The index of refraction of a material is defined in Equation 18.2. The index of refraction plays the analogous ...
Science Requirements
... “The National Solar Observatory's proposed Advanced Technology Solar Telescope (ATST) can provide critical observations not possible with SDO, such as simultaneous measurements of the coronal magnetic fields directly responsible for the heating and activity. The scientific payoff that would be gaine ...
... “The National Solar Observatory's proposed Advanced Technology Solar Telescope (ATST) can provide critical observations not possible with SDO, such as simultaneous measurements of the coronal magnetic fields directly responsible for the heating and activity. The scientific payoff that would be gaine ...
PPT
... see principle rays (ones you’d use to raytrace) see marginal rays use a light source and screen see the effect of two sources ...
... see principle rays (ones you’d use to raytrace) see marginal rays use a light source and screen see the effect of two sources ...
SPIE - Twinkle Space Mission
... have a science payload consisting of a 450mm diameter telescope, visible spectrometer, fine guidance system and Near Infrared Spectrometer. This paper describes the opto-mechanical design of the NIR spectrometer and how the challenging requirements on stability, both radiometric and spectroscopic, a ...
... have a science payload consisting of a 450mm diameter telescope, visible spectrometer, fine guidance system and Near Infrared Spectrometer. This paper describes the opto-mechanical design of the NIR spectrometer and how the challenging requirements on stability, both radiometric and spectroscopic, a ...
Gov Aker Telescope Operators Manual
... time, useful for showing large number of person the same object. The telescope is protected by a dome made by the Ash Manufacturing company of Plainfield, Illinois. The purpose of the dome is to protect the telescope from weather when not in use. The shutter is an “up and over” dual shutter design. ...
... time, useful for showing large number of person the same object. The telescope is protected by a dome made by the Ash Manufacturing company of Plainfield, Illinois. The purpose of the dome is to protect the telescope from weather when not in use. The shutter is an “up and over” dual shutter design. ...
Playdoh Electronics Activity
... AnnMarie Thomas that described how to use home-made dough to make circuits! We have since experimented with regular play-doh, and found it to be quite conductive as well. What’s the Activity About? We couldn’t have robotic telescopes without electric circuits and sensors that close the telescope dom ...
... AnnMarie Thomas that described how to use home-made dough to make circuits! We have since experimented with regular play-doh, and found it to be quite conductive as well. What’s the Activity About? We couldn’t have robotic telescopes without electric circuits and sensors that close the telescope dom ...
AstroMaster Series Telescopes
... insert the chrome barrel of the eyepieces into the focus tube (remove the plug up cap of the focuser first) and tighten the thumbscrews – see Figure 2-20. The 20mm eyepiece is called an erecting eyepiece since it corrects the image so it is right side up and corrected left to right. This makes the t ...
... insert the chrome barrel of the eyepieces into the focus tube (remove the plug up cap of the focuser first) and tighten the thumbscrews – see Figure 2-20. The 20mm eyepiece is called an erecting eyepiece since it corrects the image so it is right side up and corrected left to right. This makes the t ...
microscope project
... magnifying glass and optical instruments derived from it, such as the telescope. Just for this reason, some historians attribute the invention of the microscope to Galileo, who in 1624 would have come up with a small telescope, called a lorgnette. The model of Flanders. Other scholars, however, beli ...
... magnifying glass and optical instruments derived from it, such as the telescope. Just for this reason, some historians attribute the invention of the microscope to Galileo, who in 1624 would have come up with a small telescope, called a lorgnette. The model of Flanders. Other scholars, however, beli ...
Zeeman Effect - UCI Physics and Astronomy
... field --known as the Zeeman effect--was first explored by Faraday. However, because of the low resolution of his instrument, he was unable to detect any spectral line splitting. It was later successfully observed by Zeeman, for whom the effect was named. This advanced laboratory employs a Fabry-Pero ...
... field --known as the Zeeman effect--was first explored by Faraday. However, because of the low resolution of his instrument, he was unable to detect any spectral line splitting. It was later successfully observed by Zeeman, for whom the effect was named. This advanced laboratory employs a Fabry-Pero ...
airborne survey instrument - Portable Spectrometer FTIR
... for optimal signal to noise. The rotary interferometer lends itself more to airborne applications where high speed and freezing of motion are required. Either design can be used in an imaging type spectrometer, but so far only the rotary type has been built for imaging. Both types typically have a 1 ...
... for optimal signal to noise. The rotary interferometer lends itself more to airborne applications where high speed and freezing of motion are required. Either design can be used in an imaging type spectrometer, but so far only the rotary type has been built for imaging. Both types typically have a 1 ...
The Laser Beacon
... The system consists of a master clock that provides a common clock signal to many slave clocks. A designated calibration signal is distributed through the same clock system and returned by the slave clocks. The relative time offsets are measured on shore by recording the propagation delays of the ca ...
... The system consists of a master clock that provides a common clock signal to many slave clocks. A designated calibration signal is distributed through the same clock system and returned by the slave clocks. The relative time offsets are measured on shore by recording the propagation delays of the ca ...
Sample pages 1 PDF
... The full range of wavelengths when plotted on a diagram is known as the electromagnetic spectrum (Fig. 2.1). The shorter the wavelength of electromagnetic radiation, the higher its energy and the greater its danger to humans and other living matter. Thus radiation with the shortest wavelengths and h ...
... The full range of wavelengths when plotted on a diagram is known as the electromagnetic spectrum (Fig. 2.1). The shorter the wavelength of electromagnetic radiation, the higher its energy and the greater its danger to humans and other living matter. Thus radiation with the shortest wavelengths and h ...
Total Reflection X-Ray Fluorescence Spectrometer
... The application of focusing optics to increase the primary beam intensity at the sample position of total reflection x-ray fluorescence (TXRF) spectrometers is always associated with the increase in the angular divergence, which is tolerable for TXRF to a limited extent only. The possibility to impr ...
... The application of focusing optics to increase the primary beam intensity at the sample position of total reflection x-ray fluorescence (TXRF) spectrometers is always associated with the increase in the angular divergence, which is tolerable for TXRF to a limited extent only. The possibility to impr ...
Heat Through The Ages
... 4. Brainstorm and draft a plan to show the events on your list in order of discoveryearliest to most recent. 5. Once you have worked out a regular date scale and decided on your ten events of discovery, get a large paper from Mrs. Horton and begin the good copy of your timeline. (Use a ruler, work i ...
... 4. Brainstorm and draft a plan to show the events on your list in order of discoveryearliest to most recent. 5. Once you have worked out a regular date scale and decided on your ten events of discovery, get a large paper from Mrs. Horton and begin the good copy of your timeline. (Use a ruler, work i ...
juandiego
... What did Galileo contribute to society? • He built one of the first telescopes • He found out that Jupiter had 4 moons • His idea that maybe the Earth was moving around the sun www.barometers.com/ galileo.jpg ...
... What did Galileo contribute to society? • He built one of the first telescopes • He found out that Jupiter had 4 moons • His idea that maybe the Earth was moving around the sun www.barometers.com/ galileo.jpg ...
STARTRACKER SYSTEM - Galileo Telescope Makers
... or more evenly illuminated, concentric rings of light. The angular size of the central disc and the spacing of the rings are functions of the telescope's aperture and central obstruction, if any. The visible extent of the disc as well as the number of the rings visible varies from a given instrument ...
... or more evenly illuminated, concentric rings of light. The angular size of the central disc and the spacing of the rings are functions of the telescope's aperture and central obstruction, if any. The visible extent of the disc as well as the number of the rings visible varies from a given instrument ...
Reflecting telescope
A reflecting telescope (also called a reflector) is an optical telescope which uses a single or combination of curved mirrors that reflect light and form an image. The reflecting telescope was invented in the 17th century as an alternative to the refracting telescope which, at that time, was a design that suffered from severe chromatic aberration. Although reflecting telescopes produce other types of optical aberrations, it is a design that allows for very large diameter objectives. Almost all of the major telescopes used in astronomy research are reflectors. Reflecting telescopes come in many design variations and may employ extra optical elements to improve image quality or place the image in a mechanically advantageous position. Since reflecting telescopes use mirrors, the design is sometimes referred to as a ""catoptric"" telescope.