- A
chromosphere ("sphere of color", from the
Ancient Gr****
words χρῶμα (khrôma) 'color' and σφαῖρα (sphaîra) 'sphere') is the
second layer of a star's atmosphere...
-
absorption lines. It is
called the
chromosphere from the Gr**** root chroma,
meaning color,
because the
chromosphere is
visible as a
colored flash at the...
-
lowest level of the atmosphere, just
above the photosphere, is the thin
chromosphere region,
where ****ules
appear and
stellar flares begin.
Above this is...
-
evidence of a hot
chromosphere above the
photosphere of red giants,
where investigating the
heating mechanisms for the
chromospheres to form
requires 3D...
- main
objectives of Aditya-L1 are: To
observe the
dynamics of the Sun's
chromosphere and corona: To
study chromospheric and
coronal heating, the
physics of...
-
known as
solar prominences or filaments. The Sun's
corona lies
above the
chromosphere and
extends millions of
kilometres into
outer space.
Coronal light is...
-
known as a
fibril or mottle, is a
dynamic jet of
plasma in the Sun's
chromosphere about 300 km in diameter. They move
upwards with
speeds between 15 and...
-
features in the Sun's atmosphere,
including solar prominences and the
chromosphere.
According to the Bohr
model of the atom,
electrons exist in quantized...
-
magnetic field, lie in the photosphere.
Above the
photosphere lies the
chromosphere. This part of the
atmosphere first cools down and then
starts to heat...
-
environment otherwise known as the MOLsphere, a
gaseous envelope, a
chromosphere, a dust
environment and two
outer s**** (S1 and S2)
composed of carbon...
