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  2. XMM-Newton - Wikipedia

    en.wikipedia.org/wiki/XMM-Newton

    Animation of XMM-Newton 's trajectory around Earth. XMM-Newton, also known as the High Throughput X-ray Spectroscopy Mission and the X-ray Multi-Mirror Mission, is an X-ray space observatory launched by the European Space Agency in December 1999 on an Ariane 5 rocket. It is the second cornerstone mission of ESA's Horizon 2000 programme.

  3. XMM Cluster Survey - Wikipedia

    en.wikipedia.org/wiki/XMM_Cluster_Survey

    The XMM Cluster Survey (XCS) is a serendipitous X-ray galaxy cluster survey being conducted using archival data taken by ESA’s XMM-Newton satellite. Galaxy clusters trace the large scale structure of the universe, and their number density evolution with redshift provides a way to measure cosmological parameters, independent of cosmic microwave background experiments or supernovae cosmology ...

  4. Interface Region Imaging Spectrograph - Wikipedia

    en.wikipedia.org/wiki/Interface_Region_Imaging...

    The near-ultraviolet channel covers 278.5-283.5 nm with an 0.08 nm resolution and an effective area of 0.3 cm 2 (0.047 sq in). [7] Slit-jaw imaging has four passbands : 133.5 nm and 140.0 nm with a 4 nm bandpass each; and 279.6 nm and 283.1 nm with a 0.4 nm bandpass each.

  5. European Space Agency Science Programme - Wikipedia

    en.wikipedia.org/wiki/European_Space_Agency...

    The Science Programme [1] [2] [a] of the European Space Agency is a long-term programme of space science and space exploration missions. Managed by the agency's Directorate of Science, The programme funds the development, launch, and operation of missions led by European space agencies and institutions through generational campaigns.

  6. Post-Newtonian expansion - Wikipedia

    en.wikipedia.org/wiki/Post-Newtonian_expansion

    Higher-order terms can be added to increase accuracy, but for strong fields sometimes it is preferable to solve the complete equations numerically. This method is a common mark of effective field theories. In the limit, when the small parameters are equal to 0, the post-Newtonian expansion reduces to Newton's law of gravity.

  7. X-ray telescope - Wikipedia

    en.wikipedia.org/wiki/X-ray_telescope

    The instrument consisted of four detectors based on spectroscopic MWPCs, making an effective area of 2,400 cm 2 at 10 keV and 800 cm 2 at 100 keV. The time resolution was 200 microseconds. [25] The X-ray spectrometer aboard ISEE-3 was designed to study both solar flares and cosmic gamma-ray bursts over the energy range 5-228 keV. The experiment ...

  8. Aperture (antenna) - Wikipedia

    en.wikipedia.org/wiki/Aperture_(antenna)

    The effective area of an antenna or aperture is based upon a receiving antenna. However, due to reciprocity , an antenna's directivity in receiving and transmitting are identical, so the power transmitted by an antenna in different directions (the radiation pattern ) is also proportional to the effective area A e {\displaystyle A_{e}} .

  9. Kinetic bombardment - Wikipedia

    en.wikipedia.org/wiki/Kinetic_bombardment

    The larger device is expected to be quite effective at penetrating deeply buried bunkers and other command and control targets. [19] The weapon would be very hard to defend against. It has a very high closing velocity and a small radar cross-section. The launch is difficult to detect. Any infrared launch signature occurs in orbit, at no fixed ...