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Macromolecule conformational shaping for extreme mechanical programming of polymorphic hydrogel fibers | Nature Communications
![SOLVED: QUESTION The temperature and pressure in the Suns atmosphere are 2.8x108 Kand 0.03 Pa. Calculate the rms speed (mls) of free electrons (mass 9.11 x 10-31kg) there, assuming they are an SOLVED: QUESTION The temperature and pressure in the Suns atmosphere are 2.8x108 Kand 0.03 Pa. Calculate the rms speed (mls) of free electrons (mass 9.11 x 10-31kg) there, assuming they are an](https://cdn.numerade.com/ask_images/ecf1b1a1a55e44719a1d7804c4d7d4b0.jpg)
SOLVED: QUESTION The temperature and pressure in the Suns atmosphere are 2.8x108 Kand 0.03 Pa. Calculate the rms speed (mls) of free electrons (mass 9.11 x 10-31kg) there, assuming they are an
![SOLVED: Use Y = 9 in this question Ozone is a colourless and very reactive gas that can be found throughout all layers of our atmosphere Most ozone is found in the SOLVED: Use Y = 9 in this question Ozone is a colourless and very reactive gas that can be found throughout all layers of our atmosphere Most ozone is found in the](https://cdn.numerade.com/ask_images/3aeef7bfb396435980d19d93dc41af14.jpg)