Lower photosphere: 2×10−4 kg/m3
Lower chromosphere: 5×10−6 kg/m3
Photosphere is what we see most of the time, but you can also see the Chromosphere during a solar eclipse.
The lower photosphere is hotter than the upper photosphere.
Ag, C, and Tn
Yes
No, they have higher density than non-metals comparatively.
Photosphere is what we see most of the time, but you can also see the Chromosphere during a solar eclipse.
yes
The lower photosphere is hotter than the upper photosphere.
red, due to ionized hydrogen at lower pressure
red, due to ionized hydrogen at lower pressure
red, due to ionized hydrogen at lower pressure.
Ag, C, and Tn
Yes
No
No
R- Selected species have high population densities while k-selected species have lower population densities
The fluids with highest densities form the lowest layers. The fluids with lowest densities form the highest layers.