9 research outputs found
Photo-production of Nucleon Resonances and Nucleon Spin Structure Function in the Resonance Region
The photo-production of nucleon resonances is calculated based on a chiral
constituent quark model including both relativistic corrections H{rel} and
two-body exchange currents, and it is shown that these effects play an
important role. We also calculate the first moment of the nucleon spin
structure function g1 (x,Q^2) in the resonance region, and obtain a
sign-changing point around Q^2 ~ 0.27 {GeV}^2 for the proton.Comment: 23 pages, 5 figure
EUV Analysis of a Quasi-Static Coronal Loop Structure
Decaying active region 10942 is investigated from 4:00-16:00 UT on February
24, 2007 using a suite of EUV observing instruments. Results from Hinode/EIS,
STEREO and TRACE show that although the active region has decayed and no
sunspot is present, the physical mechanisms that produce distinguishable loop
structures, spectral line broadening, and plasma flows still occur. A coronal
loop that appears as a blue-shifted structure in Doppler maps is apparent in
intensity images of log(T) = 6.0-6.3 ions. The loop structure is found to be
anti-correlated with spectral line broadening generally attributed to
nonthermal velocities. This coronal loop structure is investigated physically
(temperature, density, geometry) and temporally. Lightcurves created from
imaging instruments show brightening and dimming of the loop structure on two
different time scales; short pulses of 10-20 min and long duration dimming of
2-4 hours until its disappearance. The coronal loop structure, formed from
relatively blue-shifted material that is anti-correlated with spectral line
broadening, shows a density of 10^10 to 10^9.3 cm-3 and is visible for longer
than characteristic cooling times. The maximum nonthermal spectral line
broadenings are found to be adjacent to the footpoint of the coronal loop
structure.Comment: 26 pages, 13 figures; Solar Physics 201
A Coherence-Based Approach for Tracking Waves in the Solar Corona
We consider the problem of automatically (and robustly) isolating and
extracting information about waves and oscillations observed in EUV image
sequences of the solar corona with a view to near real-time application to data
from the Atmospheric Imaging Array (AIA) on the Solar Dynamics Observatory
(SDO). We find that a simple coherence / travel-time based approach detects and
provides a wealth of information on transverse and longitudinal wave phenomena
in the test sequences provided by the Transition Region and Coronal Explorer
(TRACE). The results of the search are "pruned" (based on diagnostic errors) to
minimize false-detections such that the remainder provides robust measurements
of waves in the solar corona, with the calculated propagation speed allowing
automated distinction between various wave modes. In this paper we discuss the
technique, present results on the TRACE test sequences, and describe how our
method can be used to automatically process the enormous flow of data
(~1Tb/day) that will be provided by SDO/AIA after launch in late 2008.Comment: 34 pages, 16 figures - in press Solar Physic
Propagating Disturbances in Coronal Loops: A Detailed Analysis of Propagation Speeds
Quasi-periodic disturbances have been observed in the outer solar atmosphere
for many years now. Although first interpreted as upflows (Schrijver et al.
(1999)), they have been widely regarded as slow magnetoacoustic waves, due to
observed velocities and periods. However, recent observations have questioned
this interpretation, as periodic disturbances in Doppler velocity, line width
and profile asymmetry were found to be in phase with the intensity oscillations
(De Pontieu et al. (2010),Tian1 et al. (2011))}, suggesting the disturbances
could be quasi-periodic upflows. Here we conduct a detailed analysis of the
velocities of these disturbances across several wavelengths using the
Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory
(SDO). We analysed 41 examples, including both sunspot and non sunspot regions
of the Sun. We found that the velocities of propagating disturbances (PDs)
located at sunspots are more likely to be temperature dependent, whereas the
velocities of PDs at non sunspot locations do not show a clear temperature
dependence. We also considered on what scale the underlying driver is affecting
the properties of the PDs. Finally, we found that removing the contribution due
to the cooler ions in the 193 A wavelength suggests that a substantial part of
the 193 emission of sunspot PDs can be contributed to the cool component of
193\AA.Comment: 26 Papges, 15 Figure
Observations of the Sun at Vacuum-Ultraviolet Wavelengths from Space. Part II: Results and Interpretations
Utility of tissue residues for predicting effects of metals on aquatic organisms
As part of a SETAC Pellston Workshop, we evaluated the potential use of metal tissue residues for predicting effects in aquatic organisms. This evaluation included consideration of different conceptual models and then development of several case studies on how tissue residues might be applied for metals, assessing the strengths and weaknesses of these different approaches. We further developed a new conceptual model in which metal tissue concentrations from metal-accumulating organisms (principally invertebrates) that are relatively insensitive to metal toxicity could be used as predictors of effects in metal-sensitive taxa that typically do not accumulate metals to a significant degree. Overall, we conclude that the use of tissue residue assessment for metals other than organometals has not led to the development of a generalized approach as in the case of organic substances. Species-specific and site-specific approaches have been developed for one or more metals (e.g., Ni). The use of gill tissue residues within the biotic ligand model is another successful application. Aquatic organisms contain a diverse array of homeostatic mechanisms that are both metal- and species-specific. As a result, use of whole-body measurements (and often specific organs) for metals does not lead to a defensible position regarding risk to the organism. Rather, we suggest that in the short term, with sufficient validation, species- and site-specific approaches for metals can be developed. In the longer term it may be possible to use metal-accumulating species to predict toxicity to metal-sensitive species with appropriate field validation