۱۳۸۹ بهمن ۲۸, پنجشنبه

نقشه تراوایی - نفوذپذیری- گوی زمین Map of Permeability



The map above (click to enlarge) is the first-ever global survey of Earth's permeability: essentially, how leaky it is. It shows how easily water passes through surface rocks, which will help us understand the planet's water cycle and predict the sustainability of underground water sources.

Crucially, it could help reveal the hidden underground movements of 99 per cent of unfrozen fresh water - water which is not taken into account in computer models used to predict the climate.

The map was put together by Tom Gleeson of the University of British Columbia in Vancouver, Canada, and his colleagues. They assembled data on the kinds of rocks found in different regions, and, using information on how permeable each type of rock is, calculated how leaky different regions are.

Permeability varies over 13 orders of magnitude, so the figures are not very precise, but they offer a rough picture. Gleeson says the map should help hydrologists to work out how much groundwater moves from one basin or aquifer to another, which is important if the water is to be managed sustainably.

At the moment we don't know how much water is hiding underground, or where it is. As a result, groundwater gets left out of climate models. Gleeson says that is a significant omission, as the movements of groundwater could well affect regional climate:

۱۳۸۹ بهمن ۲۴, یکشنبه

فوران شعله های خورشیدی و پرتاب توده های بهم تنیدهSolar Flare and Coronal Mass Ejection


On March 20, 2010, which is the spring equinox, NASA also celebrates Sun-Earth Day. The day is comprised of educational events and activities, including a live web cast with NASA solar scientists and space weather experts. In 2010, Sun-Earth Day focuses on magnetic storms, which bombard Earth with charged particles that can interfere with electronics systems and satellites. This image, captured by NASA’s Solar Terrestrial Relations Observatory (STEREO) Ahead spacecraft on February 12, 2010, shows one such storm (albeit a very small one) brewing in two active areas of the Sun.

Two active regions glow brightly in this ultraviolet image of the Sun. A small flare rises from the active area on the left. Flares are intense explosions on the Sun that blast radiation into space. This one paints a white line across the left horizon of the Sun.

The active area on the right churns with magnetic loops. Arcs of charged particles rise from the surface and are drawn back down again in the magnetic field. A video showing a sequence of STEREO observations, including this one, reveals that a small coronal mass ejection (CME) burst from this region a short time after this image was taken. Like a flare, a CME sends charged particles and energy into space, but CMEs are larger solar storms that both last longer and carry a larger cloud of particles and magnetic field into space than do flares.

Both flares and coronal mass ejections can create space weather if aimed at Earth. The charged particles from large storms blast Earth’s magnetic field, which acts as a shield. The charged particles interacting with Earth’s magnetic field generate intense and beautiful aurora, but they can also be destructive. Solar storms in the past have damaged power grids, causing blackouts, and harmed and destroyed satellites.

STEREO is one of several NASA missions studying the Sun. STEREO was launched to help scientists better understand coronal mass ejections. An improved understanding of solar storms will improve space weather forecasts, which will help limit the damage they cause on Earth.

To learn more about the Sun’s magnetic storms and how they affect Earth, watch NASA’s live web cast on March 20, 2010.

  1. References
  2. NASA STEREO. (2010, March 9). Valentine Flare and CME. Accessed March 19, 2010.
Odenwald, S. (2010). The great solar superstorm of 1859. Technology Through टाइम

در عکس به تماشا آمده ، دو منطقه ی درخشان ِ فرابنفش نمایان است ؛در سمت چپ، شعله ای کوچک از ناحیه ای جنبا بر می خیزد که نشان از انفجاری است سهمگین در رویه ی خورشید؛ موج های رادیو اکتیو از آن در فضا پراکنده می شود . این خطی است سفید در سمت ِ چپ افق ِ خورشید .
قوس هایی از ذرات تغییر یافته، بگونه ی حلقه های مغناطیسی از رویه ی خورشید بر خاسته و در حال فرود آمدن به میدان مغناطیسی است । این ، منطقه است جنبا ،که در سمت راست تصویردید ه می شود .
" فضا"، می تواند بسبب این شعله ها و توده های تاجی شکل ، اگر به سوی زمین پرتاب شوند بشدت تحت تاثیر قرار گیرد . ذرات بارور شده بسبب توفان های سهمگین ، جریان ِ دیو بادهای ترسناک ، با توجه به میدان ّ مغناطیسی زمین که چون سپری محافظ عمل می کند را باعث می گردد .
ذرات بارور شده و تغییر یافته، بر یکدیگر تاثیر گذاشته و در هماهنگی با میدان مغناطیسی زمین ، سپیده د م بامدادی را سبب می گردد . این ذرات می توانند زیان های فراوان را نیز سبب شوند .
خسارت های وارده بر شبکه های فشار قوی و قطع کامل برق و از کار افتادن ِ ماهواره ها در فضا، یکی از زیان های توفان های خورشیدی است.
افزون بر آنچه بیان شد، بررسی فوران های خورشیدی ، در دریافت ِ شرایط آبهوایی ،و پیش بینی توفان های خانه بر انداز ،را نمی توان نادیده انگاشت .

First Stereo Image of Entire Sun and Solar Flares نخستین عکس استریو ارخورشید و زبانه های آن


First Stereo Images of Entire Sun and Solar Flares
February 11, 2011 | NASA

“On February 6th, 2011 NASA’s twin STEREO probes moved into position on opposite sides of the sun, and they are now beaming back uninterrupted images of the entire star—front and back. “For the first time ever, we can watch solar activity in its full 3-dimensional glory,” says Angelos Vourlidas, a member of the STEREO science team at the Naval Research Lab in Washington, DC. Quoted from the NASA press रिलीज़

وقتی کاوشگر ِ دوقلو، در سویی از خورشید قرار گرفت که تا اکنون از دید ِ ما زمینیان پنهان بود ، برای نخستین بار بی مانع و مزاحم، تصاویری سرتاسری از رو و پشت آن به زمین فرستاده شد که فعالیت های خورشید و فوران ِ شعله های بیرون پریده از جانش رابه زیبایی و شکوه در سه جهت ،نمایان ساخت .


۱۳۸۹ بهمن ۱۶, شنبه

تابان ابرهای شبانه ، تابناک تر می شوند Night -Shining Clouds are Getting Brighter

Night-Shining Clouds are Getting Brighter

Polar Mesospheric Clouds, 1979–2010 image acquired January 1, 1979 - December 31, 2010


After the Sun sets on a summer evening and the sky fades to black, you may be lucky enough to see thin, wavy clouds illuminating the night, such as these seen over Billund, Denmark, on July 15, 2010. Noctilucent or polar mesospheric clouds, form at very high altitudes—between 80 and 85 kilometers (50–53 miles)—which positions them to reflect light long after the Sun has dropped below the horizon. These “night-shining” clouds are rare—rare enough that Matthew DeLand, who has been studying them for 11 years, has only seen them once in person. But the chances of seeing these elusive clouds are increasing.

DeLand, an atmospheric scientist with Science Systems and Applications Inc. and NASA's Goddard Space Flight Center, has found that polar mesospheric clouds are forming more frequently and becoming brighter. He has been observing the clouds in data from Solar Backscatter Ultraviolet instruments that have been flown on satellites since 1978. The graph above shows how the brightness of the clouds has changed in the Northern Hemisphere. For reasons no one fully understands, the brightness wiggles up and down in step with solar activity, with fewer clouds forming when the Sun is most active. The biggest variability is in the far north. Underlying the changes caused by the Sun, however, is a trend toward brighter clouds. The upward trend in brightness, says DeLand, reveals subtle changes in the atmosphere that may be linked to greenhouse gases.

Polar mesospheric clouds are extremely sensitive to changes in atmospheric water vapor and temperature. The clouds form only when temperatures drop below -130 degrees Celsius (-200 Fahrenheit), when the scant amount of water high in the atmosphere freezes into ice clouds. This happens most often in far northern and southern latitudes (above 50 degrees) in the summer when, counter-intuitively, the mesosphere is coldest.

Changes in temperature or humidity in the mesosphere make the clouds brighter and more frequent. Colder temperatures allow more water to freeze, while an increase in water vapor allows more ice clouds to form. Increased water vapor also leads to the formation of larger ice particles that reflect more light.

The fact that polar mesospheric clouds are getting brighter suggests that the mesosphere is getting colder and more humid, says DeLand. Increasing greenhouse gases in the atmosphere could account for both phenomena. In the mesosphere, carbon dioxide radiates heat into space, causing cooling. More methane, on the other hand, puts more water vapor into the atmosphere because sunlight breaks methane into water molecules at high altitudes.

So far, it’s not clear which factor—water vapor or cooling—is causing polar mesospheric clouds to change. It’s likely that both are contributing, says DeLand, but the question is the focus of current research.

  1. References
  2. DeLand, M.T., Shettle, E.P., Thomas, G.E., and Olivero, J.J. (2007, May 30). Latitude-dependent long-term variations in polar mesospheric clouds from SBUV version 3 PMC data. Journal of Geophysical Research, 112, D10315.
  3. Shettle, E.P., DeLand, M.T., Thomas, G.E., and Olivero, J.J. (2009, January 17). Long term variations in the frequency of polar mesospheric clouds in the Northern Hemisphere from SBUV. Geophysical Research Letters, 36, L02803.

Photograph ©2010 Jan Erik Paulsen. Graph by Robert Simmon, adapted from Latitude-dependent long-term variations in polar mesospheric clouds from SBUV version 3 PMC data. Caption by Holli Riebeek.

nstrumentI:



download large Increase of Polar Mesospheric Clouds, 1979–2010 image (75 KB, PDF) acquired Night-Shining Clouds are Getting BrighterJanuary 1, 1979 - December 31, 2010

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After the Sun sets on a summer evening and the sky fades to black, you may be lucky enough to see thin, wavy clouds illuminating the night, such as these seen over Billund, Denmark, on July 15, 2010. Noctilucent or polar mesospheric clouds, form at very high altitudes—between 80 and 85 kilometers (50–53 miles)—which positions them to reflect light long after the Sun has dropped below the horizon. These “night-shining” clouds are rare—rare enough that Matthew DeLand, who has been studying them for 11 years, has only seen them once in person. But the chances of seeing these elusive clouds are increasing.

DeLand, an atmospheric scientist with Science Systems and Applications Inc. and NASA's Goddard Space Flight Center, has found that polar mesospheric clouds are forming more frequently and becoming brighter. He has been observing the clouds in data from Solar Backscatter Ultraviolet instruments that have been flown on satellites since 1978. The graph above shows how the brightness of the clouds has changed in the Northern Hemisphere. For reasons no one fully understands, the brightness wiggles up and down in step with solar activity, with fewer clouds forming when the Sun is most active. The biggest variability is in the far north. Underlying the changes caused by the Sun, however, is a trend toward brighter clouds. The upward trend in brightness, says DeLand, reveals subtle changes in the atmosphere that may be linked to greenhouse gases.

Polar mesospheric clouds are extremely sensitive to changes in atmospheric water vapor and temperature. The clouds form only when temperatures drop below -130 degrees Celsius (-200 Fahrenheit), when the scant amount of water high in the atmosphere freezes into ice clouds. This happens most often in far northern and southern latitudes (above 50 degrees) in the summer when, counter-intuitively, the mesosphere is coldest.

Changes in temperature or humidity in the mesosphere make the clouds brighter and more frequent. Colder temperatures allow more water to freeze, while an increase in water vapor allows more ice clouds to form. Increased water vapor also leads to the formation of larger ice particles that reflect more light.

The fact that polar mesospheric clouds are getting brighter suggests that the mesosphere is getting colder and more humid, says DeLand. Increasing greenhouse gases in the atmosphere could account for both phenomena. In the mesosphere, carbon dioxide radiates heat into space, causing cooling. More methane, on the other hand, puts more water vapor into the atmosphere because sunlight breaks methane into water molecules at high altitudes.

So far, it’s not clear which factor—water vapor or cooling—is causing polar mesospheric clouds to change. It’s likely that both are contributing, says DeLand, but the question is the focus of current research.

  1. References
  2. DeLand, M.T., Shettle, E.P., Thomas, G.E., and Olivero, J.J. (2007, May 30). Latitude-dependent long-term variations in polar mesospheric clouds from SBUV version 3 PMC data. Journal of Geophysical Research, 112, D10315.
  3. Shettle, E.P., DeLand, M.T., Thomas, G.E., and Olivero, J.J. (2009, January 17). Long term variations in the frequency of polar mesospheric clouds in the Northern Hemisphere from SBUV. Geophysical Research Letters, 36, L02803.

Photograph ©2010 Jan Erik Paulsen. Graph by Robert Simmon, adapted from Latitude-dependent long-term variations in polar mesospheric clouds from SBUV version 3 PMC data. Caption by Holli Riebeek.

Instrument: