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N3.5 KTN - Opticon
N3.5 KTN - Opticon

... Nasmyth platform ...
Workshop Summary & Discussion
Workshop Summary & Discussion

Powerpoint file as used in presentation
Powerpoint file as used in presentation

... A stripped-down version for only one baseline or otherwise simplified could be easily and relatively cheaply built and tested on the sky, for further verification. ...
Document
Document

... (http://science.hq.nasa.gov/missions/phase.html) have been enabled by improvements in detectors. Beyond 2007, advances are expected in detectors, readout electronics, and other technologies, particularly those enabling polarimetry and large format imaging arrays for the visible, near IR, IR and far ...
Lesson 0: What is progress
Lesson 0: What is progress

... Brahe was one of the best observational astronomers that ever lived. He made the most precise observations that had yet been made by devising the best instruments available before the invention of the telescope, and His observations of planetary motion, particularly that of Mars, provided the crucia ...
1 km
1 km

... atmospheric winds Extending the DMI technique to measuring of tropospheric winds is challenging ─ Observing absorption feature in presence of large background flux reduces sensitivity of interferogram to wind signal (higher SNR is required) ─ Pressure dependence of line shape and position ─ Aerosols ...
Telescopes
Telescopes

WWT Web Client - WorldWide Telescope
WWT Web Client - WorldWide Telescope

... HTML5 SDK OVERVIEW • Essentially WWT – Light. Designed to render most common WWT features within the browser. ...
Personal Digital Assistants
Personal Digital Assistants

Meade Instruments Corporation Instruction Manual
Meade Instruments Corporation Instruction Manual

... The Speed/? key also accesses the "Help" file. "Help" provides on-screen information on how to accomplish whatever task is currently active. TIP: Pressing the Speed/? key very briefly changes the slew speed. Holding down the Speed/? key longer (one to two seconds) accesses the Help function. Hold do ...
ppt presentaion - Akamai Workforce Initiative
ppt presentaion - Akamai Workforce Initiative

Increased Thermal Background for the post-NCS NICMOS
Increased Thermal Background for the post-NCS NICMOS

First All-Sky Measurement of Muon Flux with IceCube
First All-Sky Measurement of Muon Flux with IceCube

...  Buried beneath roughly 1.5 km of ice, extending down to 2.5 km. ...
Architecture for in-space robotic assembly of a modular space
Architecture for in-space robotic assembly of a modular space

... 2. © 2016 Society of Photo-Optical Instrumentation Engineers (SPIE) [DOI: 10.1117/1.JATIS.2.4.041207] Keywords: space telescope; robotic assembly; modular structure; segmented mirror. Paper 15078SS received Nov. 14, 2015; accepted for publication Jun. 6, 2016; published online Jul. 11, 2016. ...
Grade-6 Final Holidays Homework - MRIS Sector
Grade-6 Final Holidays Homework - MRIS Sector

... Eat healthy food and drink lots of water and health drinks during summer. Revise all the work done in the class. Revise tables 2 to 20. Integrating curriculum helps students deepen their understanding of the subject matter and comprehend relationship between different areas of study. This year’s hol ...
Speckle Imaging through the Atmosphere
Speckle Imaging through the Atmosphere

... Fig. 1-The division of the telescope aperture into N effective subapertures. The image results from two independent terms with different dependences on N. The first term describes the superposition of the intensities of al/ the individual subaperlures, and the second term describes the interference ...
Solar modulation of cosmic rays in the energy range
Solar modulation of cosmic rays in the energy range

... The neutron monitor data were kindly provided through the on-line databases of the Polar Geophysical Institute of the Russian Academy of Sciences (Apatity, geomagnetic cut-off 0.6 GV), the Sodankyl Geophysical Observatory of the University of Oulu, Finland (0.8 GV), the Solar-Terrestrial Physics Div ...
MEASURING LIGHT POLLUTION ON LA PALMA
MEASURING LIGHT POLLUTION ON LA PALMA

... spectral line from street lamps is that of sodium at 5890/6 Å, and this increases the wavelength-averaged brightness of the La Palma night sky in the affected imaging bands (V and R filters) by  7%. The effect in other bands is much smaller. The La Palma night sky is as dark as at other prime obser ...
Orion capsules will take astronauts out of low
Orion capsules will take astronauts out of low

... producing energy-absorbing helicopter seats. Orion will be equipped with crew seats that slide a few inches along the axis of the astronaut’s spine. “When Orion hits the water, there will be forces in several different directions,” says Tony Herrmann, subsystems manager for the Orion Crew Impact Att ...
Introduction to Astrophotography
Introduction to Astrophotography

Optical instability of the earth`s atmosphere
Optical instability of the earth`s atmosphere

... expands northward; in December–February, it contracts from the north. It is worth noting that it does not expand southward. Thus, the distribution depends on the season and latitude. The southern hemisphere in low latitudes has smaller values than the northern one there. Figure 3 also shows that loc ...
Introduction to Occultations and How to Observe and Record Them
Introduction to Occultations and How to Observe and Record Them

... who had a Criterion RV6. At 6" I soon developed a severe case of “aperture envy"...I just had to get a bigger scope! I worked at a Worth Ranch Boy Scout camp the summer of 1970 where one of my duties was teaching Astronomy Merit Badge. While working around the camp I found the remains of an 8" refle ...
The Poor Man`s Telescope - Royal Astronomical Society of Canada
The Poor Man`s Telescope - Royal Astronomical Society of Canada

... Not less than an hour and a half, or better still, two hours, should be spent on this final grinding. The result should be a satin-like finish through which large print can be read at three inches distance. It is absolutely essential that the mirror and tool be in perfect contact at the finish as it ...
Deployment of the Hobby-Eberly Telescope wide
Deployment of the Hobby-Eberly Telescope wide

... Downloaded From: http://proceedings.spiedigitallibrary.org/ on 08/16/2016 Terms of Use: http://spiedigitallibrary.org/ss/termsofuse.aspx ...
Brown University PHYS 0060 Physics Department LAB A
Brown University PHYS 0060 Physics Department LAB A

... They are the radius (or mass) and the attached charge of the individual drops. That is because the terminal velocity depends upon both - and as your write up explained. The little latex spheres, each one almost precisely 1/1000 mm (from the write-up), more often than not stick together and so your s ...
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CfA 1.2 m Millimeter-Wave Telescope

The 1.2 meter Millimeter-Wave Telescope at the Harvard-Smithsonian Center for Astrophysics and its twin instrument at CTIO in Chile have been studying the distribution and properties of molecular clouds in our Galaxy and its nearest neighbours since the 1970s. The telescope is nicknamed ""The Mini"" because of its unusually small size. At the time it was built, it was the smallest radio telescope in the world. Together, ""The Mini"" and its twin in Chile have obtained what is by far the most extensive, uniform, and widely used Galactic survey of interstellar carbon monoxide (CO). ""The Mini"" is currently in operation from October to May each year.
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