-
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...
- hole or a
compact stellar nucleus, but
sometimes both.
chromosphere chromospheric activity index A
parameter indicating the
magnetic activity in a star's...
-
observed in
coronal and
chromospheric temperatures are
sometimes referred to as
coronal jets and
chromospheric jets (or
chromospheric surges), respectively...
- -P.; Perdelwitz, V.; Jack, D.; Schmitt, J. H. M. M. (January 2023). "
Chromospheric activity and
photospheric variation of $\alpha$ Ori
during the great...
-
molecular clouds and
identified by
their optical variability and
strong chromospheric lines. T
Tauri stars are pre-main-sequence
stars in the
process of contracting...
-
referred to as
bright flocculi, in
contrast to dark flocculi, and as
chromospheric faculae, in
contrast to
photospheric faculae. The term
plage is often...
-
occur at a well-defined altitude, but
forms a kind of
nimbus around chromospheric features such as ****ules and filaments, and is in constant, chaotic...
- Pontieu, Bart; Erdélyi, Robert; James,
Stewart P. (July 2004). "Solar
chromospheric ****ules from the
leakage of
photospheric oscillations and flows". Nature...
- 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...
-
rotation once
every 83.5 days. A
subsequent time
series analysis of
chromospheric indicators in 2002
suggests a
longer rotation period of 116.6±0.7 days...
