9 research outputs found
Bridging the Gap: Capturing the Ly Counterpart of a Type-II Spicule and its Heating Evolution with VAULT2.0 and IRIS Observations
We present results from an observing campaign in support of the VAULT2.0
sounding rocket launch on September 30, 2014. VAULT2.0 is a Ly (1216
\AA) spectroheliograph capable of providing spectroheliograms at high cadence.
Ly observations are highly complementary to the IRIS observations of
the upper chromosphere and the low transition region (TR) but have previously
been unavailable. The VAULT2.0 data provide new constraints on
upper-chromospheric conditions for numerical models. The observing campaign was
closely coordinated with the IRIS mission. Taking advantage of this
simultaneous multi-wavelength coverage of target AR 12172 and by using
state-of-the-art radiative-MHD simulations of spicules, we investigate in
detail a type-II spicule associated with a fast (300 km s) network jet
recorded in the campaign observations. Our analysis suggests that spicular
material exists suspended high in the atmosphere but in lower temperatures
(seen in Ly) until it is heated and becomes visible in TR temperatures
as a network jet. The heating begins lower in the spicule and propagates
upwards as a rapidly propagating thermal front. The front is then observed as
fast, plane-of-the-sky motion typical of a network jet, but contained inside
the pre-existing spicule. This work supports that the high speeds reported in
network jets should not be taken as real mass upflows but only as apparent
speeds of a rapidly propagating heating front along the pre-existing spicule.Comment: 15 pages, 5 figures and one online movie. Accepted for publication in
the Astrophysical Journa