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  2. Minute and second of arc - Wikipedia

    en.wikipedia.org/wiki/Minute_and_second_of_arc

    A second of arc, arcsecond (arcsec), or arc second, denoted by the symbol ″, [2] is ⁠ 1 / 60 ⁠ of an arcminute, ⁠ 1 / 3600 ⁠ of a degree, [1] ⁠ 1 / 1 296 000 ⁠ of a turn, and ⁠ π / 648 000 ⁠ (about ⁠ 1 / 206 264.8 ⁠) of a radian.

  3. Inverse trigonometric functions - Wikipedia

    en.wikipedia.org/wiki/Inverse_trigonometric...

    2.2.1 Detailed example and explanation of the "plus or minus" symbol ... Principal values of the arcsec(x) and arccsc(x) functions graphed on the cartesian plane.

  4. Bortle scale - Wikipedia

    en.wikipedia.org/wiki/Bortle_scale

    mag/arcsec 2 Description 1 Excellent dark-sky site 7.6–8.0 21.76 - 22.0 the zodiacal light is visible and colorful; the gegenschein is readily visible; the zodiacal band is visible; airglow is readily visible; the Scorpius and Sagittarius regions of the Milky Way cast obvious shadows

  5. List of integrals of inverse trigonometric functions - Wikipedia

    en.wikipedia.org/wiki/List_of_integrals_of...

    The following is a list of indefinite integrals (antiderivatives) of expressions involving the inverse trigonometric functions.For a complete list of integral formulas, see lists of integrals.

  6. Surface brightness - Wikipedia

    en.wikipedia.org/wiki/Surface_brightness

    A truly dark sky has a surface brightness of 2 × 10 −4 cd m −2 or 21.8 mag arcsec2. [9] [clarification needed] The peak surface brightness of the central region of the Orion Nebula is about 17 Mag/arcsec 2 (about 14 milli nits) and the outer bluish glow has a peak surface brightness of 21.3 Mag/arcsec 2 (about 0.27 millinits). [10]

  7. List of trigonometric identities - Wikipedia

    en.wikipedia.org/wiki/List_of_trigonometric...

    For the above isosceles triangle with unit sides and angle , the area ⁠ 1 / 2 ⁠ × base × height is calculated in two orientations. When upright, the area is sin ⁡ θ cos ⁡ θ {\displaystyle \sin \theta \cos \theta } .

  8. Sky brightness - Wikipedia

    en.wikipedia.org/wiki/Sky_brightness

    (The S 10 unit is defined as the surface brightness of a star whose V-magnitude is 10 and whose light is smeared over one square degree, or 27.78 mag arcsec2.) The total sky brightness in zenith is therefore ~220 S 10 or 21.9 mag/arcsec² in the V-band. Note that the contributions from Airglow and Zodiacal light vary with the time of year ...

  9. Hinode (satellite) - Wikipedia

    en.wikipedia.org/wiki/Hinode_(satellite)

    Spatial resolution is around 2 arcsec, and the field of view is up to 560 x 512 arcsec 2. The emission lines in the EIS wavelength bands are emitted at temperatures ranging from 50,000 K to 20 million K. EIS is used to identify the physical processes involved in heating the solar corona .