Space Physics: The solar corona is a very hot atmosphere surrounding the visible surface of the sun. X-ray emissions from the corona show that its temperature is about 2 × 106 K. The gas pressure in the corona is about 0.03 Pa. Estimate the number density of particles in the solar corona with units of particles per cubic meter.
Space Physics: The solar corona is a very hot atmosphere surrounding the visible surface of the sun. X-ray emissions from the corona show that its temperature is about 2 × 106 K. The gas pressure in the corona is about 0.03 Pa. Estimate the number density of particles in the solar corona with units of particles per cubic meter.
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![Space Physics: The solar corona is a very hot atmosphere surrounding the visible surface of the sun.
X-ray emissions from the corona show that its temperature is about 2 × 106 K. The gas pressure in
the corona is about 0.03 Pa. Estimate the number density of particles in the solar corona with units
of particles per cubic meter.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F0ee67c44-0754-41fd-9006-bdc882dbaccb%2F519f1067-31a9-4a4f-ad9c-67c94c45d2fa%2Fyew76rh.jpeg&w=3840&q=75)
Transcribed Image Text:Space Physics: The solar corona is a very hot atmosphere surrounding the visible surface of the sun.
X-ray emissions from the corona show that its temperature is about 2 × 106 K. The gas pressure in
the corona is about 0.03 Pa. Estimate the number density of particles in the solar corona with units
of particles per cubic meter.
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