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  2. Solar constant - Wikipedia

    en.wikipedia.org/wiki/Solar_constant

    The solar constant includes radiation over the entire electromagnetic spectrum. It is measured by satellite as being 1.361 kilo watts per square meter (kW/m 2) at solar minimum (the time in the 11-year solar cycle when the number of sunspots is minimal) and approximately 0.1% greater (roughly 1.362 kW/m 2) at solar maximum. [1]

  3. Solar irradiance - Wikipedia

    en.wikipedia.org/wiki/Solar_irradiance

    It is measured facing (pointing at / parallel to) the incoming sunlight (i.e. the flux through a surface perpendicular to the incoming sunlight; other angles would not be TSI and be reduced by the dot product). [3] The solar constant is a conventional measure of mean TSI at a distance of one astronomical unit (AU).

  4. Solar flux unit - Wikipedia

    en.wikipedia.org/wiki/Solar_flux_unit

    The solar flux unit (sfu) is a convenient measure of spectral flux density often used in solar radio observations, such as the F10.7 solar activity index: [1]. 1 sfu = 10 4 Jy = 10 −22 W⋅m −2 ⋅Hz −1 = 10 −19 erg⋅s −1cm −2 ⋅Hz −1.

  5. Coronal radiative losses - Wikipedia

    en.wikipedia.org/wiki/Coronal_radiative_losses

    In active regions the energy flux is about 10 7 erg cm −2 sec −1, in the quiet Sun it is roughly 8 10 5 – 10 6 erg cm −2 sec −1, and in coronal holes 5 10 5 - 8 10 5 erg cm −2 sec −1, including the losses due to the solar wind. [1] The required power is a small fraction of the total flux irradiated from the Sun, but this energy is ...

  6. Jansky - Wikipedia

    en.wikipedia.org/wiki/Jansky

    Radio-frequency interference from a GSM telephone transmitting 0.5 W at 1.8 GHz at a distance of 1 km (RSSI of −70 dBm) [9] 20 000 000: Disturbed Sun at 20 MHz (Karl Guthe Jansky's initial discovery, published in 1933) 4 000 000: Sun at 10 GHz 1 600 000: Sun at 1.4 GHz: 1 000 000: Milky Way at 20 MHz 10 000: 1 solar flux unit: 2 000: Milky ...

  7. Radiative flux - Wikipedia

    en.wikipedia.org/wiki/Radiative_flux

    Radiant flux emitted, reflected, transmitted or received, per unit solid angle. This is a directional quantity. Spectral intensity: I e,Ω,ν [nb 3] watt per steradian per hertz W⋅sr −1 ⋅Hz −1: M⋅L 2 ⋅T −2: Radiant intensity per unit frequency or wavelength. The latter is commonly measured in W⋅sr −1 ⋅nm −1. This is a ...

  8. Today's Wordle Hint, Answer for #1273 on Friday, December 13 ...

    www.aol.com/todays-wordle-hint-answer-1273...

    Today's Wordle Answer for #1273 on Friday, December 13, 2024. Today's Wordle answer on Friday, December 13, 2024, is BOXER. How'd you do? Next: Catch up on other Wordle answers from this week.

  9. Irradiance - Wikipedia

    en.wikipedia.org/wiki/Irradiance

    In radiometry, irradiance is the radiant flux received by a surface per unit area. The SI unit of irradiance is the watt per square metre (W⋅m −2).The CGS unit erg per square centimetre per second (erg⋅cm −2 ⋅s −1) is often used in astronomy.