... Астронет | ... рда.) область сантиметровых волн (длин волн) . ... рда.) сантиметровый диапазон (длин волн) . ... рда.) область декаметровых волн (длин волн) . ... рда.) декаметровыи диапазон (длин волн) . ... рда.) область дециметровых волн (длин волн) . ... рда.) дециметровый диапазон (длин волн) . ... рда.) область метровых волн (длин волн) . ... рда.) метровый диапазон (длин волн) . ... рда.) область миллиметровых волн (длин волн) . ... рда.) область субмиллиметровых волн (длин волн) . ...

Еще в разделе: (Показать все результаты (>4849) - www.astronet.ru/ )

• Journal "Peremennye Zvezdy"
• Астронет > Страница 25
• Астронет > NGC 1512: A Panchromatic View

The Cosmic Microwave Background Radiation Temperature Work in groups of 2-4. ... Due 1999 April 15 In this laboratory exercise, you will use the radio telescope on the roof of Science B to measure the intensity of the Cosmic Microwave Background Radiation (CMBR). ... The output of the telescope when pointing at the sky will then be 2 Tsys = Trec + Tsky : The temperature of the sky can in principle arise from two sources, radiation from the atmosphere and radiation from outer space (the CMBR). ...

Еще в разделе: (Показать все результаты (>532) - www.naic.edu/ )

• http://www.naic.edu/vscience/schedule/tpfiles/CampbelltagR2022tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/CampbelltagR2102tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/CampbelltagR2955tp.pdf

... Future seminars . ... Relativistic magneto-active laser plasmas " . ... Generation of super-strong magnetic fields. ... This method is based on the observation of resonance interaction between the Landau levels in magnetic field and energy levels of plasma ions. ... The important peculiarity of the energy distribution of fast ions is their slow decreasing up to the energy of 1.4 MeV at the laser intensity of 2 10 18 W/cm 2 ; the effective temperature of fast ions is of the order of 350 keV. ...

Еще в разделе: (Показать все результаты (>179) - www.cosmos.ru/ )

• (Q-3) Atomic Energy Levels

... Bionic eyes. If our eyes could see in different wavelength bands, this is what the Sun would look like. ... Visible light, crucial to photosynthesis, is a type of radiation. ... At the heart of this revolution is the recognition that light travels as a wave. ... Dreams of Fields . ... By the time the fields go from strong to weak and back to strong, the wave has moved a certain distance, known as the wavelength. ... Red light, blue light, infrared light, ultraviolet light, radio waves, x-rays ? ...

Еще в разделе: (Показать все результаты (>61) - www.astrosociety.org/ )

• ASP: Black Holes to Blackboards: Seeing the Light

Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...

Еще в разделе: (Показать все результаты (>126) - www.stecf.org/ )

• stecf.slitless - a Slitless Spectroscopy Quick-look Tool
• The Photometric Performance of the NICMOS Grisms
• GOODS

Optical Communication Experiment using Very Small Optical transmitter with SLR station National Institute of Information and Communications Technology, Japan Space Communications System Laboratory Hiroo Kunimori and VSOTA TEAM Sep 24, 2012 WPLTN Technical Workshop@St.Petersburg, Russia Table of Contents Backgound:HODOYOSHI Project JapaneseHODOYOHI= Reasonable Reliability Engineering to develop series of 50kg Satellite. ... How to share wavelength communication beam and ranging beams. ...

Еще в разделе: (Показать все результаты (>50) - www.ipa.nw.ru/ )

• http://www.ipa.nw.ru/conference/wpltn2012/docs/25/1600%20koltsov.pdf

... Resolution - 1.5-2.0 km . Swath - 450 km . ... Swath - 550 km . ... Resolution - 370 km . ... Spectral bands - 0.6-0.7 um; 0.8-1.1 um . ... Kondor - system for collection and transmission of data from sea and ice stations . ... Downlinking to ground stations (main centers) . ... Satellite's information system operates in both direct transmission mode and recording to on-board recorder mode with later downlink to ground station. ... For more information send a mail to: info@sputnik.infospace.ru . ...

Еще в разделе: (Показать все результаты (>3) - sputnik.infospace.ru/ )

alpha(2000) = 05h 05m 30.62s , delta(2000) = +52d 49' 54.0'' . V = 11.78, B-V = -0.33, Spectral type: DA0 . Field is 10.0 x 10.0 arcmin . Oke (1990) data (1A steps 3200-4700A; 2A steps 4702-9200A); Bohlin et al. (1995) FOS data + WD model atmosphere . ftp access to visible wavelength data files for this standard ftp access to UV+visible wavelength data files for this standard . jwalsh@eso.org

Еще в разделе: (Показать все результаты (>202) - www.apo.nmsu.edu/ )

• Tolerances
• Feige 66
• Feige 67

... Bad Astronomy . ... Mad Science . ... How fast must an object be travelling so the sound I perceive as it directly passes me will drop in pitch exactly one octave? ... When an object is moving past another object, any sound emitted by the first object is changed in pitch due to the relative motion. ... wl(emitted)" is the wavelength of sound emitted by the object at rest, "wl(heard)" is the wavelength you hear from the object, "v" is the velocity of the object, and "c" is the speed of sound. ...

Еще в разделе: (Показать все результаты (>14) - www.badastronomy.com/ )

If you already know the catalogue abbreviation or numbering, enter it below : . Alternatively you can find the catalogue by selecting wavelength or mission or other keys: (More on how to select catalogues) . ... Mission . ... A preliminary list of catalogues available in VizieR (still growing). The acronyms and symbols in use to designate astronomical catalogues in the literature are explained in the Dictionary of Nomenclature of Celestial Objects . Location : CDS Strasbourg, France . ...

Еще в разделе: (Показать все результаты (>37) - www.asc.rssi.ru/ )

• Results of measurements of SRT antenna parameters in Pushchino
• MILLIMETRON

Astronotes Armagh Planetarium's Stellar Blog! ... Colin Johnston . ... This submillimetre-wavelength image of the region surrounding the reflection nebula M78 made with the Atacama Pathfinder Experiment (APEX) telescope (overlaid on a view of the same region in visible light) shows the position of interstellar dust grains (orange) to show where new stars are being formed.( ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...

Еще в разделе: (Показать все результаты (>845) - www.armaghplanet.com/ )

• What is light? - The electromagnetic spectrum made easy | Astronotes

... OH, = 18 cm Nancay Radio Telescope, OH 18-cm line observations , since 1969 F, Jy 6 4 2 0 0 -1 -2 0 -1 -2 0 -2 -4 -6 30 40 50 1612 MHz I HU Pup August 5, 2009 1665 MHz 4 2 0 0.5 0.0 - 0.5 -1.0 -1.5 1.0 0.5 0.0 - 0.5 4 3 2 1 0 -1 1667 MHz I I 1.0 0.5 0.0 0.5 0.0 22-meter telescope, Pushchino Radio Astronomy Observatory H2O F, Jy 1.0 0.5 0.0 0.4 0.2 0.0 -0.2 -0.4 0.4 0.2 0.0 -0.2 -0.4 -0.6 0.6 0.4 0.2 0.0 -0.2 -0.4 -70 -60 -50 -40 -30 -20 -10 0 Mira-type star R Leo. ...