• The Sky Polarization Observatory (SPOrt) was an Italian instrument planned for launch to the International Space Station in for a planned 2-year mission...
    2 KB (233 words) - 02:15, 29 October 2022
  • Thumbnail for Sky
    John (December 1868). "On the Blue Colour of the Sky, the Polarization of Skylight, and on the Polarization of Light by Cloudy Matter Generally". Proceedings...
    24 KB (2,777 words) - 21:14, 18 March 2025
  • Chandrasekhar polarization Bagnulo, S. (2003). "Observations of magnetic Ap stars at the Pic-du-Midi Observatory: From broadband linear polarization measurements...
    7 KB (757 words) - 21:26, 22 November 2024
  • Sport, an Austrian paraglider design Sky Polarization Observatory (SPOrt), a cancelled Italian space observatory Sportcoat or sports coat, a type of jacket...
    3 KB (440 words) - 20:22, 13 April 2025
  • Thumbnail for Cosmic microwave background
    variation in polarization. The polarisation at each direction in the sky has an orientation described in terms of E-mode and B-mode polarization. The E-mode...
    108 KB (13,202 words) - 17:04, 10 June 2025
  • Thumbnail for Simons Observatory
    constructed. One of the primary goals of the Simons Observatory are polarization maps of the sky with an order of magnitude better sensitivity than the Planck...
    11 KB (1,331 words) - 11:51, 25 May 2025
  • originally consisted of two independent modules, EXPOSE and Sky Polarization Observatory (SPOrt). EXPOSE was a facility holding multiple exobiology experiments...
    5 KB (465 words) - 04:19, 24 February 2023
  • Thumbnail for Airborne observatory
    Photographs helped "to derive coronal brightness and polarization, along with sky brightness and polarization". Several missions were made in 1960s. Three NC-135...
    18 KB (1,808 words) - 16:24, 10 May 2025
  • Thumbnail for Stratospheric Observatory for Infrared Astronomy
    The Stratospheric Observatory For Infrared Astronomy (SOFIA) was an 80/20 joint project of NASA and the German Aerospace Center (DLR) to construct and...
    41 KB (4,162 words) - 04:28, 2 June 2025
  • Thumbnail for Owens Valley Radio Observatory
    Owens Valley Radio Observatory (OVRO) is a radio astronomy observatory located near Big Pine, California (US) in Owens Valley. It lies east of the Sierra...
    15 KB (1,648 words) - 22:06, 18 May 2025
  • Thumbnail for Cosmic Background Imager
    Cosmic Background Imager (category Astronomical observatories in Chile)
    detected fluctuations in the polarization of the microwave background obtaining the first detailed E-mode polarization spectrum providing evidence that...
    4 KB (480 words) - 12:58, 4 April 2025
  • Thumbnail for Planck (spacecraft)
    observatory was launched in May 2009 and reached the Earth/Sun L2 point by July 2009. By February 2010, it had successfully started a second all-sky survey...
    48 KB (3,121 words) - 23:39, 17 May 2025
  • Thumbnail for Gravitational-wave observatory
    A gravitational-wave detector (used in a gravitational-wave observatory) is any device designed to measure tiny distortions of spacetime called gravitational...
    37 KB (4,211 words) - 17:10, 10 May 2025
  • Thumbnail for Polarization (cosmology)
    Monitor (Fermi-GBM) and Neil Gehrels Swift Observatory has pointed to lower gamma-ray burst polarization. But the authors have also stated that those...
    26 KB (3,095 words) - 06:24, 10 June 2025
  • Thumbnail for Antenna (radio)
    vertical polarization; if turned on its side the same antenna's polarization will be horizontal. Reflections generally affect polarization. Radio waves...
    83 KB (10,949 words) - 22:44, 29 April 2025
  • Thumbnail for POLARBEAR
    POLARBEAR (category Astronomical observatories in Chile)
    POLARBEAR (POLARization of the Background Radiation) is a cosmic microwave background polarization experiment located in the Atacama Desert of northern...
    7 KB (590 words) - 07:21, 15 June 2024
  • Thumbnail for Astronomical Observatory of the University of Warsaw
    long-term optical sky surveys: OGLE and ASAS. Both these surveys take sky images using dedicated telescopes located at the Las Campanas Observatory, Chile. Scientific staff...
    9 KB (869 words) - 03:04, 25 March 2025
  • Thumbnail for List of cosmic microwave background experiments
    has produced the highest resolution all-sky map to-date of both the temperature anisotropies and polarization signals. Current scientific goals for CMB...
    44 KB (2,472 words) - 09:52, 10 March 2025
  • the orientation of the incoming electromagnetic waves (polarization) at every point on the sky with an angular resolution of 0.73 degrees. The angular...
    6 KB (635 words) - 20:47, 19 March 2025
  • Thumbnail for LIGO
    Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational...
    90 KB (8,438 words) - 12:08, 10 April 2025
  • Thumbnail for Parkes Observatory
    Parkes Observatory is a radio astronomy observatory, located 20 kilometres (12 mi) north of the town of Parkes, New South Wales, Australia. It hosts Murriyang...
    41 KB (3,841 words) - 05:14, 6 April 2025
  • diagram Skin depth Skin effect Skip distance Skip reentry Sky Polarization Observatory Sky anchor Sky brightness Skyrmion Slack water Slater-type orbital Slater...
    32 KB (3,248 words) - 12:19, 30 July 2024
  • Thumbnail for Skyglow
    Skyglow (redirect from Sky-glow)
    doi:10.1016/j.jqsrt.2013.12.004. Garstang, R. (1989). "Night-Sky Brightness at Observatories and Sites". Publications of the Astronomical Society of the...
    32 KB (3,297 words) - 05:41, 30 December 2024
  • Thumbnail for RX J1856.5−3754
    indications of vacuum birefringence from RX J1856.5−3754. A degree of polarization of about 16% was measured from the visible spectrum being large enough...
    10 KB (962 words) - 18:15, 10 May 2025
  • DSA-2000 (category Gravitational wave observatories)
    Radio Observatory, but located in Nevada USA. Its main goal is a sky survey, acting as a radio camera to produce an archive of images of the entire sky visible...
    7 KB (903 words) - 18:02, 21 May 2025
  • Thumbnail for Cosmology Large Angular Scale Surveyor
    by making precise measurements of the polarization of the Cosmic Microwave Background (CMB) over 65% of the sky at multiple frequencies in the microwave...
    23 KB (2,592 words) - 20:47, 17 May 2025
  • Thumbnail for BICEP and Keck Array
    Extragalactic Polarization) and the Keck Array are a series of cosmic microwave background (CMB) experiments. They aim to measure the polarization of the CMB;...
    25 KB (2,449 words) - 03:19, 6 May 2025
  • Thumbnail for Llano de Chajnantor Observatory
    Llano de Chajnantor Observatory is the name for a group of astronomical observatories located at an altitude of over 4,800 m (15,700 ft) in the Atacama...
    21 KB (2,190 words) - 20:01, 13 February 2025
  • Thumbnail for Coronagraph
    coronagraphs, such as the High Altitude Observatory's Mark IV Coronagraph on top of Mauna Loa, use polarization to distinguish sky brightness from the image of the...
    15 KB (1,803 words) - 14:52, 30 May 2025
  • also operates the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST) and one of the largest radio observatory, the Five-hundred-meter Aperture...
    10 KB (986 words) - 01:20, 30 April 2025