- 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...
- 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...
-
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...
- Lockyer, is
credited with
discovering the
gaseous nature of the
solar chromosphere, but
there is no
justification for the
conclusion that he
deserves credit...
-
Microturbulence Oscillations Radiation zone
Atmosphere Photosphere Starspot Chromosphere Stellar corona Alfvén
surface Stellar wind
Bubble Bipolar outflow Accretion...
-
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...
-
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...
-
evidence of a hot
chromosphere above the
photosphere of red giants,
where investigating the
heating mechanisms for the
chromospheres to form
requires 3D...
- of 273°, an
orbit that
would potentially place it
within the star's
chromosphere. The more
distant companion was at 0.51″±0.01″ (≈77 AU) with a position...
