![SOLVED: Let uS suppose that the photon spectral flux density (# of photons cm-2s-'eV-!) in the solar spectrum can be approximated by the following function: n(E) = 0 (E < a) n(E) = SOLVED: Let uS suppose that the photon spectral flux density (# of photons cm-2s-'eV-!) in the solar spectrum can be approximated by the following function: n(E) = 0 (E < a) n(E) =](https://cdn.numerade.com/ask_images/3a865103fbe8456682666204ab41a074.jpg)
SOLVED: Let uS suppose that the photon spectral flux density (# of photons cm-2s-'eV-!) in the solar spectrum can be approximated by the following function: n(E) = 0 (E < a) n(E) =
➢Lamp Power Density - The simplest method of calculation ➢Total power consumed by lamps, excluding ballasts, etc ➢Total =
![Achieving ultrahigh instantaneous power density of 10 MW/m2 by leveraging the opposite-charge-enhanced transistor-like triboelectric nanogenerator (OCT-TENG) | Nature Communications Achieving ultrahigh instantaneous power density of 10 MW/m2 by leveraging the opposite-charge-enhanced transistor-like triboelectric nanogenerator (OCT-TENG) | Nature Communications](https://media.springernature.com/m685/springer-static/image/art%3A10.1038%2Fs41467-021-25753-7/MediaObjects/41467_2021_25753_Fig1_HTML.png)
Achieving ultrahigh instantaneous power density of 10 MW/m2 by leveraging the opposite-charge-enhanced transistor-like triboelectric nanogenerator (OCT-TENG) | Nature Communications
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