-
appear more
stable and
evolve over
longer times.
Images taken in
typical chromospheric lines show the
presence of
brighter cells,
usually referred to as the...
- both
composed of thin
threads that
trace the
magnetic field similar to
chromospheric fibrils. The cool
prominence material that
makes up
spines and barbs—the...
-
observed in
coronal and
chromospheric temperatures are
sometimes referred to as
coronal jets and
chromospheric jets (or
chromospheric surges), respectively...
-
referred to as
bright flocculi, in
contrast to dark flocculi, and as
chromospheric faculae, in
contrast to
photospheric faculae. The term
plage is often...
- Bibcode:1996SoPh..165..115L. De Pontieu, B., Erdélyi, R. and James, S:
Solar chromospheric ****ules from the
leakage of
photospheric oscillations and
flows In:...
- at a well-defined altitude. Rather, it
forms a kind of
nimbus around chromospheric features such as ****ules and filaments, and is in constant, chaotic...
- it is
defined as
chromospheric evaporation. When the
plasma rapidly cools and
falls toward the photosphere, it is
called chromospheric condensation. There...
- A
Moreton wave,
Solar Tsunami, or Moreton-Ramsey wave is the
chromospheric signature of a large-scale
solar corona shock wave.
Described as a kind of...
- -P.; Perdelwitz, V.; Jack, D.; Schmitt, J. H. M. M. (January 2023). "
Chromospheric activity and
photospheric variation of $\alpha$ Ori
during the great...
- Vial, Jean-Claude; Wilhelm,
Klaus (1999). "Solar Wind
Outflow and the
Chromospheric Magnetic Network". Science. 283 (5403): 810–813. Bibcode:1999Sci...283...
