676 research outputs found
Temporal evolution of multiple evaporating ribbon sources in a solar flare
We present new results from the Interface Region Imaging Spectrograph showing
the dynamic evolution of chromospheric evaporation and condensation in a flare
ribbon, with the highest temporal and spatial resolution to date. IRIS observed
the entire impulsive phase of the X-class flare SOL2014-09-10T17:45 using a 9.4
second cadence `sit-and-stare' mode. As the ribbon brightened successively at
new positions along the slit, a unique impulsive phase evolution was observed
for many tens of individual pixels in both coronal and chromospheric lines.
Each activation of a new footpoint displays the same initial coronal up-flows
of up to ~300 km/s, and chromospheric downflows up to 40 km/s. Although the
coronal flows can be delayed by over 1 minute with respect to those in the
chromosphere, the temporal evolution of flows is strikingly similar between all
pixels, and consistent with predictions from hydrodynamic flare models. Given
the large sample of independent footpoints, we conclude that each flaring pixel
can be considered a prototypical, `elementary' flare kernel.Comment: Accepted for publication - ApJ letter
Optical Spectral Observations of a Flickering White-Light Kernel in a C1 Solar Flare
We analyze optical spectra of a two-ribbon, long duration C1.1 flare that
occurred on 18 Aug 2011 within AR 11271 (SOL2011-08-18T15:15). The impulsive
phase of the flare was observed with a comprehensive set of space-borne and
ground-based instruments, which provide a range of unique diagnostics of the
lower flaring atmosphere. Here we report the detection of enhanced continuum
emission, observed in low-resolution spectra from 3600 \AA\ to 4550 \AA\
acquired with the Horizontal Spectrograph at the Dunn Solar Telescope. A small,
0''.5 ( cm) penumbral/umbral kernel brightens repeatedly in
the optical continuum and chromospheric emission lines, similar to the temporal
characteristics of the hard X-ray variation as detected by the Gamma-ray Burst
Monitor (GBM) on the Fermi spacecraft. Radiative-hydrodynamic flare models that
employ a nonthermal electron beam energy flux high enough to produce the
optical contrast in our flare spectra would predict a large Balmer jump in
emission, indicative of hydrogen recombination radiation from the upper flare
chromosphere. However, we find no evidence of such a Balmer jump in the
bluemost spectral region of the continuum excess. Just redward of the expected
Balmer jump, we find evidence of a "blue continuum bump" in the excess emission
which may be indicative of the merging of the higher order Balmer lines. The
large number of observational constraints provides a springboard for modeling
the blue/optical emission for this particular flare with radiative-hydrodynamic
codes, which are necessary to understand the opacity effects for the continuum
and emission line radiation at these wavelengths.Comment: 54 pages, 13 figures, accepted for publication in the Astrophysical
Journa
New technique to measure the cavity defects of Fabry-Perot interferometers
(Abridged):
We define and test a new technique to accurately measure the cavity defects
of air-spaced FPIs, including distortions due to the spectral tuning process
typical of astronomical observations. We further develop a correction technique
to maintain the shape of the cavity as constant as possible during the spectral
scan. These are necessary steps to optimize the spectral transmission profile
of a two-dimensional spectrograph using one or more FPIs.
We devise a generalization of the techniques developed for the so-called
phase-shifting interferometry to the case of FPIs. The technique is applicable
to any FPI that can be tuned via changing the cavity spacing (-axis), and
can be used for any etalon regardless of the coating' reflectivity. The major
strength of our method is the ability to fully characterize the cavity during a
spectral scan, allowing for the determination of scan-dependent modifications
of the plates. As a test, we have applied this technique to three 50 mm
diameter interferometers, with cavity gaps ranging between 600 micron and 3 mm,
coated for use in the visible range.
We obtain accurate and reliable measures of the cavity defects of air-spaced
FPIs, and of their evolution during the entire spectral scan. Our main, and
unexpected, result is that the relative tilt between the two FPI plates varies
significantly during the spectral scan, and can dominate the cavity defects; in
particular, we observe that the tilt component at the extremes of the scan is
sensibly larger than at the center of the scan. Exploiting the capability of
the electronic controllers to set the reference plane at any given spectral
step, we develop a correction technique that allows the minimization of the
tilt during a complete spectral scan. The correction remains highly stable over
long periods, well beyond the typical duration of astronomical observations.Comment: 15 pages, 20+ figures, accepted for publication in A&A. Two
additional movies are available in the online version of the pape
1D and 2D site amplification effects at Tarcento (Friuli, NE Italy), 30years later
A temporary accelerometer network has been installed in Tarcento (Friuli, NE Italy), a small town heavily hit by the 1976-1977 Friuli earthquake sequence, as a part of an ongoing research project aimed at ground motion simulation and generation of shakemaps in the near-field of an earthquake. The network operated from October 2008 to April 2010 and consisted of three K2 accelerographs with internal Episensor, distributed over a linear array of about 1.5km length. Tarcento town had been chosen, at the end of the 1970s, as the ideal site for a pilot microzonation study, the first of this kind in Italy, in which a substantial number of field (and laboratory) tests were carried out in order to assess the mechanical properties of local alluvium deposits and their complex (3D) geometrical configuration. The data from the temporary network, illustrated herein, allow for proper verification and review of some of the quantitative predictions formulated in the 1980 study. As argued in the discussion section, we also believe that the data are apt to provide valuable information of more general interest on the complex seismic response of alluvium-filled valleys, and we show therein how the observations can be interpreted in the light of presently available parametric simulation studies and simplified criteria for handling basin amplification effect
Small-scale structure and dynamics of the lower solar atmosphere
The chromosphere of the quiet Sun is a highly intermittent and dynamic
phenomenon. Three-dimensional radiation (magneto-)hydrodynamic simulations
exhibit a mesh-like pattern of hot shock fronts and cool expanding post-shock
regions in the sub-canopy part of the inter-network. This domain might be
called "fluctosphere". The pattern is produced by propagating shock waves,
which are excited at the top of the convection zone and in the photospheric
overshoot layer. New high-resolution observations reveal a ubiquitous
small-scale pattern of bright structures and dark regions in-between. Although
it qualitatively resembles the picture seen in models, more observations - e.g.
with the future ALMA - are needed for thorough comparisons with present and
future models. Quantitative comparisons demand for synthetic intensity maps and
spectra for the three-dimensional (magneto-)hydrodynamic simulations. The
necessary radiative transfer calculations, which have to take into account
deviations from local thermodynamic equilibrium, are computationally very
involved so that no reliable results have been produced so far. Until this task
becomes feasible, we have to rely on careful qualitative comparisons of
simulations and observations. Here we discuss what effects have to be
considered for such a comparison. Nevertheless we are now on the verge of
assembling a comprehensive picture of the solar chromosphere in inter-network
regions as dynamic interplay of shock waves and structuring and guiding
magnetic fields.Comment: 8 pages, 2 figures, to appear in the proceedings of the IAU Symposium
No. 247, Waves & Oscillations in the Solar Atmosphere: Heating and
Magneto-Seismology (Venezuela 2007
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