425 research outputs found
A STUDY OF CRYOPUMP CONFIGURATIONS IN FREE MOLECULAR FLOW REGIONS
Monte carlo computer technique applied to focusing of cryopump configurations in free molecular flow regio
Characteristics of Magnetohydrodynamic Oscillations Observed with Michelson Doppler Imager
We report on the spatial distribution of magnetogram oscillatory power and
phase angles between velocity and magnetogram signals as observed with the
Michelson Doppler Imager. The dataset is 151.25 arcsec times 151.25 arcsec
containing sunspot from Dec 2, 1997 with a temporal sampling interval of 60
seconds and spatial sampling of 0.605 arcsec. Simultaneously observed continuum
intensity and surface velocity accompany the magnetic information. We focus on
three frequency regimes: 0.5-1.0, 3.0-3.5 and 5.5-6.0 mHz corresponding roughly
to timescales of magnetic evolution, p-modes and the 3 minute resonant sunspot
oscillation. Significant low frequency magnetogram power is found in lower flux
pixels, 100-300 Gauss, in a striking ring with filamentary structure
surrounding sunspot. Five minute magnetogram power peaks in extended regions of
flux 600-800 Gauss. The 3 minute oscillation is observed in sunspot umbra in
pixels whose flux measures 1300-1500 Gauss. Phase angles of approximately -90
degrees between velocity and magnetic flux in the 3.0-3.5 and 5.5-6.0 mHz
regimes are found in regions of significant cross amplitude.Comment: 4 Pages, 4 Figures -- For better Figure files see:
http://www.astro.ucla.edu/~norton/pub_list.htm
Evidence of Twisting and Mixed-polarity Solar Photospheric Magnetic Field in Large Penumbral Jets: IRIS and Hinode Observations
A recent study using {\it Hinode} (SOT/FG) data of a sunspot revealed some
unusually large penumbral jets that often repeatedly occurred at the same
locations in the penumbra, namely at the tail of a penumbral filament or where
the tails of multiple penumbral filaments converged. These locations had
obvious photospheric mixed-polarity magnetic flux in \NaI\ 5896 Stokes-V images
obtained with SOT/FG. Several other recent investigations have found that
extreme ultraviolet (EUV)/X-ray coronal jets in quiet Sun regions (QRs),
coronal holes (CHs) and near active regions (ARs) have obvious mixed-polarity
fluxes at their base, and that magnetic flux cancellation prepares and triggers
a minifilament flux-rope eruption that drives the jet. Typical QR, CH, and AR
coronal jets are up to a hundred times bigger than large penumbral jets, and in
EUV/X-ray images show clear twisting motion in their spires. Here, using IRIS
\MgII\ k 2796 \AA\ SJ images and spectra in the penumbrae of two sunspots we
characterize large penumbral jets. We find redshift and blueshift next to each
other across several large penumbral jets, and interpret these as untwisting of
the magnetic field in the jet spire. Using Hinode/SOT (FG and SP) data, we also
find mixed-polarity magnetic flux at the base of these jets. Because large
penumbral jets have mixed-polarity field at their base and have twisting motion
in their spires, they might be driven the same way as QR, CH and AR coronal
jets.Comment: 18 pages, 11 figures; to appear in Ap
Proof Loading to Assure Lumber Strength
The control of within-mill variations in the strength distribution of a given structural grade of lumber is of growing concern to the wood industry. Recent studies have proposed the use of on-line proof loading procedures to maintain quality through the elimination of weak pieces.An experiment was conducted on one thousand two hundred pieces of 2 x 4 No. 2 Dense KD Southern pine to determine the effect of both single and reverse bending proof loads on the strength of lumber tested in both bending and tension parallel-to-grain. The specimens were separated into six groups, each containing two hundred pieces. A pair of control groups, single proof load groups, and reverse proof load groups were tested. One group in each pair was failed in bending, the other was in tension. During the testing, no damage due to the proof loading was detected.Probabilistic analysis of the data indicates that the bending strength of the single proof loaded specimens could be reduced by 12% and still remain as reliable as the control. Reverse proof loaded specimens could tolerate a reduction of 33%. The tensile strength for each single proof loaded member could tolerate a reduction of 13%, while reverse proof loaded specimens could face a decrease of 18% and maintain a level of safety equal to the related control. When using a bending proof load to assure lumber strength, it is necessary to use a higher proof load to assure tensile strength than would be needed just to assure bending strength
How can project-based mentorships enhance the dietetics profession?
Research Outcomes: The RD Mentorship Program is designed to provide dietetic students (mentee) with the opportunity to gain one-on-one experience with a Registered Dietitian (mentor). This nationwide program evaluates project-based mentorships. Methods: Potential mentors and mentees completed an initial survey that indicated mentor projects and mentee interests. Mentees (n=378) were matched to a mentor (n=264) based on their project preferences and interests. Matches met virtually monthly from September 2020 to April 2021. A mid-program evaluation was sent out in December 2020. Analysis: Descriptive statistics were used to analyze the data Results: The mid-program evaluation indicated that 96% (n=265) of participants found the application and matching process good to very good. The majority of mentee participants liked the variety of dietitians and projects. Some of the projects were, but not limited to, the following: social media and website development, food photography, grocery store tours, virtually shadowing, recipe development, community involvement projects, meal plans, writing and research, analyzing recipes for allergens, literature reviews, cooking classes, case studies, creating exams, resume building, newsletters, course development, interviewing skills development, public policy task force, community assessments, reviewing needs assessments, menu reviews and development, podcast development and patient education handouts. Conclusion: Through the RD Mentorship Program’s project-based mentorship format, mentees are exposed to a broad range of activities that Registered Dietitians perform across many sectors. These projects help to build relationships and offer valuable experiential learning opportunities in dietetics
Emergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork
We study the emergence of magnetic flux at very small spatial scales (less
than 2 arcsec) in the quiet Sun internetwork. To this aim, a time series of
spectropolarimetric maps was taken at disk center using the instrument SP/SOT
on board Hinode. The LTE inversion of the full Stokes vector measured in the Fe
I 6301 and 6302 A lines allows us to retrieve the magnetic flux and topology in
the region of study. In the example presented here, the magnetic flux emerges
within a granular structure. The horizontal magnetic field appears prior to any
significant amount of vertical field. As time goes on, the traces of the
horizontal field disappear while the the vertical dipoles drift -carried by the
plasma motions- towards the surrounding intergranular lanes. These events take
place within typical granulation timescales.Comment: 9 pages (referee format), 3 figures. Accepted for publication in ApJ
Letter
Formation Process of a Light Bridge Revealed with the Hinode Solar Optical Telescope
The Solar Optical Telescope (SOT) aboard HINODE successfully and continuously
observed a formation process of a light bridge in a matured sunspot of the NOAA
active region 10923 for several days with high spatial resolution. During its
formation, many umbral dots were observed emerging from the leading edges of
penumbral filaments, and intruding into the umbra rapidly. The precursor of the
light bridge formation was also identified as the relatively slow inward motion
of the umbral dots which emerged not near the penumbra, but inside the umbra.
The spectro-polarimeter on SOT provided physical conditions in the photosphere
around the umbral dots and the light bridges. We found the light bridges and
the umbral dots had significantly weaker magnetic fields associated with
upflows relative to the core of the umbra, which implies that there was hot gas
with weak field strength penetrating from subphotosphere to near the visible
surface inside those structures. There needs to be a mechanism to drive the
inward motion of the hot gas along the light bridges. We suggest that the
emergence and the inward motion are triggered by a buoyant penumbral flux tube
as well as the subphotospheric flow crossing the sunspot.Comment: 8 pages, 6 figures, accepted in the PASJ Hinode special issu
Flare Ribbons Observed with G-band and FeI 6302A Filters of the Solar Optical Telescope on Board Hinode
The Solar Optical Telescope (SOT) on board Hinode satellite observed an X3.4
class flare on 2006 December 13. Typical two-ribbon structure was observed, not
only in the chromospheric CaII H line but also in G-band and FeI 6302A line.
The high-resolution, seeing-free images achieved by SOT revealed, for the first
time, the sub-arcsec fine structures of the "white light" flare. The G-band
flare ribbons on sunspot umbrae showed a sharp leading edge followed by a
diffuse inside, as well as previously known core-halo structure. The underlying
structures such as umbral dots, penumbral filaments and granules were visible
in the flare ribbons. Assuming that the sharp leading edge was directly heated
by particle beam and the diffuse parts were heated by radiative back-warming,
we estimate the depth of the diffuse flare emission using the intensity profile
of the flare ribbon. We found that the depth of the diffuse emission is about
100 km or less from the height of the source of radiative back-warming. The
flare ribbons were also visible in the Stokes-V images of FeI 6302A, as a
transient polarity reversal. This is probably related to "magnetic transient"
reported in the literature. The intensity increase in Stokes-I images indicates
that the FeI 6302A line was significantly deformed by the flare, which may
cause such a magnetic transient.Comment: 14 pages, 7 figures, PASJ in pres
A Tale Of Two Spicules: The Impact of Spicules on the Magnetic Chromosphere
We use high-resolution observations of the Sun in Ca II H 3968 A from the
Solar Optical Telescope on Hinode to show that there are at least two types of
spicules that dominate the structure of the magnetic solar chromosphere. Both
types are tied to the relentless magnetoconvective driving in the photosphere,
but have very different dynamic properties. ``Type-I'' spicules are driven by
shock waves that form when global oscillations and convective flows leak into
the upper atmosphere along magnetic field lines on 3-7 minute timescales.
``Type-II'' spicules are much more dynamic: they form rapidly (in ~10s), are
very thin (<200km wide), have lifetimes of 10-150s (at any one height) and seem
to be rapidly heated to (at least) transition region temperatures, sending
material through the chromosphere at speeds of order 50-150 km/s. The
properties of Type II spicules suggest a formation process that is a
consequence of magnetic reconnection, typically in the vicinity of magnetic
flux concentrations in plage and network. Both types of spicules are observed
to carry Alfven waves with significant amplitudes of order 20 km/s.Comment: 8 pages, 5 figures, accepted for Hinode special issue of PAS
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