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  2. Space Sciences Laboratory - Wikipedia

    en.wikipedia.org/wiki/Space_Sciences_Laboratory

    The Space Sciences Laboratory (SSL) is an Organized Research Unit (ORU) of the University of California, Berkeley. [ 1 ] [ 2 ] Founded in 1959, the laboratory is located in the Berkeley Hills above the university campus.

  3. Head-related transfer function - Wikipedia

    en.wikipedia.org/wiki/Head-related_transfer_function

    HRTF filtering effect. A head-related transfer function (HRTF) is a response that characterizes how an ear receives a sound from a point in space. As sound strikes the listener, the size and shape of the head, ears, ear canal, density of the head, size and shape of nasal and oral cavities, all transform the sound and affect how it is perceived, boosting some frequencies and attenuating others.

  4. Janet Luhmann - Wikipedia

    en.wikipedia.org/wiki/Janet_Luhmann

    Janet G. Luhmann (born 1946) is an American physicist and senior fellow of the Space Sciences Laboratory of the University of California, Berkeley. [1] She has made major contributions to a wide range of topics in planetary, solar, magnetospheric, and heliospheric physics.

  5. Research centers and laboratories at the University of ...

    en.wikipedia.org/wiki/Research_centers_and...

    The Berkeley APEC Study Center (BASC) is an APEC Study Center. It was established in 1996 in response to the Asia-Pacific Economic Cooperation (APEC) Leaders Education Initiative introduced by President Bill Clinton and endorsed by the leaders of the other APEC member nations at their historic meetings on Blake Island, Seattle in November 1993.

  6. Hanbury Brown and Twiss effect - Wikipedia

    en.wikipedia.org/wiki/Hanbury_Brown_and_Twiss_effect

    The HBT effect can, in fact, be predicted solely by treating the incident electromagnetic radiation as a classical wave.Suppose we have a monochromatic wave with frequency on two detectors, with an amplitude () that varies on timescales slower than the wave period /.

  7. SETI@home - Wikipedia

    en.wikipedia.org/wiki/SETI@home

    Berkeley Space Science Lab has found ways of working with small budgets, and the project has received donations allowing it to go well beyond its original planned duration, but it still has to compete for limited funds with other SETI projects and other space sciences projects.

  8. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    A Laplace resonance is a three-body resonance with a 1:2:4 orbital period ratio (equivalent to a 4:2:1 ratio of orbits). The term arose because Pierre-Simon Laplace discovered that such a resonance governed the motions of Jupiter's moons Io , Europa , and Ganymede .

  9. Leuschner Observatory - Wikipedia

    en.wikipedia.org/wiki/Leuschner_Observatory

    The Space Sciences Lab, which operates SETI, began operations in 1960 at Leuschner Observatory until a permanent home in the Berkeley hills was completed in 1966. [ 5 ] In 1965, the observatory was relocated a short distance east of the Berkeley campus in the hills of Lafayette, California , on the 283-acre (1.15 km 2 ) Russell Reservation.