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101.
Counterstreaming in a Large Polar Crown Filament 总被引:1,自引:0,他引:1
The motion of small-scale structures is well resolved in high-resolution filament images that were observed on 19 June 1998
with the Swedish Vacuum Solar Telescope, La Palma. The filament was between 80 000 and 100 000 km high. The study is based
on two hours of narrow-band observations at three wavelength positions in Hα. Velocities along the line of sight and in the
transverse direction, respectively, V
los and V
tr, were measured for a large number of individual small-scale filament structures. Small features are all moving along nearly
parallel threads, some in one direction along the threads and the remainder in the other direction, a pattern of motion known
as counterstreaming. The net flow velocities in the two directions are about 8 km s−1 and both are tilted by an angle δ≃16° relative to the plane of the sky. This angle is less than expected, by factors between
2.0 and 2.5, relative to the local horizontal plane. We believe that V
los is underestimated by these factors due to a line-shift reducing effect by the underlying Hα absorption line of the chromosphere.
Supplementary material to this paper is available in electronic form at http://dx.doi.org/10.1023/A:1026150809598 相似文献
102.
The EUV Imaging Spectrometer for Hinode 总被引:1,自引:0,他引:1
J. L. Culhane L. K. Harra A. M. James K. Al-Janabi L. J. Bradley R. A. Chaudry K. Rees J. A. Tandy P. Thomas M. C. R. Whillock B. Winter G. A. Doschek C. M. Korendyke C. M. Brown S. Myers J. Mariska J. Seely J. Lang B. J. Kent B. M. Shaughnessy P. R. Young G. M. Simnett C. M. Castelli S. Mahmoud H. Mapson-Menard B. J. Probyn R. J. Thomas J. Davila K. Dere D. Windt J. Shea R. Hagood R. Moye H. Hara T. Watanabe K. Matsuzaki T. Kosugi V. Hansteen Ø. Wikstol 《Solar physics》2007,243(1):19-61
The EUV Imaging Spectrometer (EIS) on Hinode will observe solar corona and upper transition region emission lines in the wavelength ranges 170?–?210 Å and 250?–?290 Å. The line centroid positions and profile widths will allow plasma velocities and turbulent or non-thermal line broadenings to be measured. We will derive local plasma temperatures and densities from the line intensities. The spectra will allow accurate determination of differential emission measure and element abundances within a variety of corona and transition region structures. These powerful spectroscopic diagnostics will allow identification and characterization of magnetic reconnection and wave propagation processes in the upper solar atmosphere. We will also directly study the detailed evolution and heating of coronal loops. The EIS instrument incorporates a unique two element, normal incidence design. The optics are coated with optimized multilayer coatings. We have selected highly efficient, backside-illuminated, thinned CCDs. These design features result in an instrument that has significantly greater effective area than previous orbiting EUV spectrographs with typical active region 2?–?5 s exposure times in the brightest lines. EIS can scan a field of 6×8.5 arc?min with spatial and velocity scales of 1 arc?sec and 25 km?s?1 per pixel. The instrument design, its absolute calibration, and performance are described in detail in this paper. EIS will be used along with the Solar Optical Telescope (SOT) and the X-ray Telescope (XRT) for a wide range of studies of the solar atmosphere. 相似文献
103.
Roy H. ØStensen 《Astrophysics and Space Science》2004,291(3-4):263-266
An interactive database interface to the subdwarf catalogue has been designed and prototyped. The implementation is still under development, but is already fully functional. More than 2300 stars from an updated edition of the subdwarf catalogue have been loaded into the database, and additional photometric data from many other sources have been included. The database tools include advanced search capabilities in coordinate, magnitude and colour space. Output tables can be generated in HTML with hyperlinks to automatically generated finding charts, the SIMBAD database, the Aladin viewer, as well as an internal data sheet generated for each database entry. Search results can be visualised automatically as interactive position, magnitude or colour diagrams. Access to the database is currently restricted to those who wish to contribute to the development of the project. 相似文献
104.
THE ROLE OF ATMOSPHERIC CIRCULATION PATTERNS IN AGROCLIMATE VARIABILITY IN FINLAND, 1961–2011
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MASOUD IRANNEZHAD DELIANG CHEN BJØRN KLØVE 《Geografiska Annaler: Series A, Physical Geography》2016,98(4):287-301
This study evaluates interannual variations and trends in growing season daily temperature sum and daily precipitation sum in Finland during 1961–2011, and their connections to well known atmospheric circulation patterns. Changes in summer (June–August) climate partially explain changes in growing season daily temperature sum and daily precipitation sum over Finland, which naturally decreased from south to north. On a national scale, growing season warmed and became wetter during 1961–2011, as growing season daily temperature sum and daily precipitation sum significantly (p < 0.05) increased by 5.01 ± 3.17°C year–1 and 1.39 ± 0.91 mm year–1, respectively. The East Atlantic pattern was the most influential atmospheric circulation pattern for variations in growing season daily temperature sum (rho = 0.40) across Finland and the East Atlantic/West Russia pattern was most influential for growing season daily precipitation sum variability (rho = –0.54). There were significant (p < 0.05) increasing trends in growing season daily temperature sum and daily precipitation sum throughout Finland during 1961–2011. Increased growing season daily temperature sum was mainly observed in northern, central, western, eastern and coastal areas of south‐western Finland. This warming was positively associated with the East Atlantic pattern in the north, centre and south, but negatively associated with the East Atlantic/West Russia pattern in eastern Finland. Increased GSP mostly occurred in southern, eastern, western, central, northern and north‐western Finland. These wetting trends were positively correlated with the East Atlantic pattern in the north and negatively correlated with the Polar pattern in the south and the East Atlantic/West Russia pattern in the east, west, centre and north‐east of Finland. The overall agroclimatic year‐to‐year variability in Finland between 1961 and 2011 was mostly linked to variations in the East Atlantic and East Atlantic/West Russia patterns. 相似文献
105.
Human adaptation to climate change is gaining increasing academic as well as political attention. Understanding how and what people around the world adapt to is, however, difficult. Climate change is often, if not always, only one of a multiplicity of exposures perforating local communities. In Biidi 2, a small Sahelian village in northern Burkina Faso, climate variability have had a great influence on inhabitants’ lives since the major droughts of the early 1970s and 1980s. Tracing the intertwinement of drought, diminishing agricultural production and the need to buy food, this article explores how villagers attempt to attract development projects and negotiate with political parties in order to negate the impact of the global food crisis on their livelihoods. In doing so the article attempts to show how adaptation to climate variability is related to multiple, intersecting processes, and in this specific case is a matter of navigating changing socioeconomic factors. Using recent theory from social anthropology, adaptation is explored as a matter of social navigation. It is suggested that this theoretical approach might help nuance and elucidate how, and to what, local people around the world adapt. 相似文献
106.
Christakos Konstantinos Furevik Birgitte R. Aarnes Ole Johan Breivik Øyvind Tuomi Laura Byrkjedal Øyvind 《Ocean Dynamics》2020,70(1):57-75
Ocean Dynamics - Accurate predictions of surface ocean waves in coastal areas are important for a number of marine activities. In complex coastlines with islands and fjords, the quality of wind... 相似文献
107.
B. Rudels R. Meyer E. Fahrbach V. V. Ivanov S. Østerhus D. Quadfasel U. Schauer V. Tverberg R. A. Woodgate 《Annales Geophysicae》2000,18(6):687-705
The water mass distribution in northern Fram Strait and over the Yermak Plateau in summer 1997 is described using CTD data from two cruises in the area. The West Spitsbergen Current was found to split, one part recirculated towards the west, while the other part, on entering the Arctic Ocean separated into two branches. The main inflow of Atlantic Water followed the Svalbard continental slope eastward, while a second, narrower, branch stayed west and north of the Yermak Plateau. The water column above the southeastern flank of the Yermak Plateau was distinctly colder and less saline than the two inflow branches. Immediately west of the outer inflow branch comparatively high temperatures in the Atlantic Layer suggested that a part of the extraordinarily warm Atlantic Water, observed in the boundary current in the Eurasian Basin in the early 1990s, was now returning, within the Eurasian Basin, toward Fram Strait. The upper layer west of the Yermak Plateau was cold, deep and comparably saline, similar to what has recently been observed in the interior Eurasian Basin. Closer to the Greenland continental slope the salinity of the upper layer became much lower, and the temperature maximum of the Atlantic Layer was occasionally below 0.5 °C, indicating water masses mainly derived from the Canadian Basin. This implies that the warm pulse of Atlantic Water had not yet made a complete circuit around the Arctic Ocean. The Atlantic Water of the West Spitsbergen Current recirculating within the strait did not extend as far towards Greenland as in the 1980s, leaving a broader passage for waters from the Atlantic and intermediate layers, exiting the Arctic Ocean. A possible interpretation is that the circulation pattern alternates between a strong recirculation of the West Spitsbergen Current in the strait, and a larger exchange of Atlantic Water between the Nordic Seas and the inner parts of the Arctic Ocean. 相似文献
108.
Øivind Hauge 《Solar physics》1969,10(2):315-318
The solar spectrum at 3261 Å has been studied using the spectrograph at the Oslo Solar Observatory. From analysis of this wavelength region and recent results at 5085 Å, a solar cadmium abundance log N
Cd = 1.86 ± 0.15 is obtained. 相似文献
109.
110.
Øyvind Byrkjedal Nils Gunnar Kvamstø Marius Meland Eystein Jansen 《Climate Dynamics》2006,26(5):473-487
Published reconstructions of last glacial maximum (LGM) sea surface temperatures and sea ice extent differ significantly.
We here test the sensitivity of simulated North Atlantic climates to two different reconstructions by using these reconstructions
as boundary conditions for model experiments. An atmospheric general circulation model has been used to perform two simulations
of the (LGM) and a modern-day control simulation. Standard (CLIMAP) reconstructions of sea ice and sea surface temperatures
have been used for the first simulation, and a set of new reconstructions in the Nordic Seas/Northern Atlantic have been used
for the second experiment. The new reconstruction is based on 158 core samples, and represents ice-free conditions during
summer in the Nordic Seas, with accordingly warmer sea surface temperatures and less extensive sea ice during winter as well.
The simulated glacial climate is globally 5.7 K colder than modern day, with the largest changes at mid and high latitudes.
Due to more intense Hadley circulation, the precipitation at lower latitudes has increased in the simulations of the LGM.
Relative to the simulation with the standard CLIMAP reconstructions, reduction of the sea ice in the North Atlantic gives
positive local responses in temperature, precipitation and reduction of the sea level pressure. Only very weak signatures
of the wintertime Icelandic Low occur when the standard CLIMAP sea surface temperature reconstruction is used as the lower
boundary condition in LGM. With reduced sea ice conditions in the Nordic Seas, the Icelandic Low becomes more intense and
closer to its present structure. This indicates that thermal forcing is an important factor in determining the strength and
position of the Icelandic Low. The Arctic Oscillation is the most dominant large scale variability feature on the Northern
Hemisphere in modern day winter climate. In the simulation of the LGM with extensive sea ice this pattern is significantly
changed and represents no systematic large scale variability over the North Atlantic. Reduction of the North Atlantic sea
ice extent leads to stronger variability in monthly mean sea level pressure in winter. The synoptic variability appears at
a lower level in the simulation when standard reconstructions of the sea surface in the LGM are used. A closer inspection
of storm tracks in this model experiment shows that that the synoptic lows follow a narrow band along the ice edge during
winter. The trajectories of synoptic lows are not constrained to the sea ice edge to the same degree when the sea ice extent
is reduced. Seasonally open waters in the Nordic Seas in the new reconstruction apparently act as a moisture source, consistent
with the current understanding of the rapid growth of the Fennoscandian and Barents Ice Sheets, during the LGM. The signal
from the intensified thermal forcing in the North Atlantic in Boreal winter is carried zonally by upper tropospheric waves,
and thus generates non-local responses to the changed sea ice cover. 相似文献