The Facts of the Jellyfish's sting and the treatment
How do we treat a jellyfish sting? This is a full explanation about it.
Cari Tahu Kecerdasan Apa Yang Anda Kuasai
Pada dasarnya, manusia memiliki 9 kecerdasan utama sesuai dengan pembagian kecerdasan pada otak kita. Hanya saja kemampuan yang sangat dominan pada setiap orang berbeda. Cari tau disini kecerdasan apa yang lebih dominan pada diri anda.
4 Trend Masa Depan Berkaitan dengan Teknologi Ramah Lingkungan
Menyelamatkan planet ini dan mengurangi emisi adalah hal yang baik, tapi siapa yang mengatakan bahwa Anda tidak bisa bersenang-senang sedikit ketika melakukan hal itu?
Mempercantik Tampilan Rumah dengan 'Vertical Garden'
Pada masa sekarang, Vertical garden masih belum familiar di kalangan masyarakat Indonesia. Jauh sebelum dikenal di Indonesia, masyarakat dari negara-negara yang memiliki lahan terbatas sudah memanfaatkan solusi ini.
Nokia X2-02, Musik Murah Dengan Easy Swap
Nokia sebagai raja ponsel dunia kembali luncurkan ponsel musik murah meriah. Kali ini dalam balutan Nokia X2-02, dedengkot asal asal Finlandia ini mengusung konsep dual SIM dengan easy swap.
Kamis, 29 Agustus 2013
Be Careful with Fraud Using the Name of UMM
Selasa, 24 April 2012
Crunching the Big Bang With the Greatest Supercomputer Ever Built
Popsci.com - A little more than a decade from now, one of the world’s great arid plains will become a bustling intersection of high-resolution astronomy and high-powered computing. Scrub land in either South Africa or Australia will host the biggest telescope ever, the Square Kilometer Array (SKA), designed to listen to the oldest birth pangs of the universe. And the brains of the operation will likely be the world’s most powerful supercomputer.
The next generation of major scientific instruments will require a whole new information architecture, both for processing and data transfer and for storage. So the future of astronomy is closely tied to the future of computing. To interlace these futures even more tightly, IBM today announced a new $43 million (€32 million) center connected to its research base in Zurich, where computer scientists hope to design and build the first low-power exascale computer systems.
The Square Kilometer Array will consist of thousands of radio antennas spread across an area the size of a continent, with a collecting area equivalent to one square kilometer. It will study dark energy, search for black holes, look for complex organic molecules in interstellar space, and look back to the cosmic Dark Ages — the time before the formation of the first stars. Along with a massive virtual field of view, all this work requires lots of computing power.
Take the current global daily Internet traffic and multiply it by two, and you start to approach the stupendous scales of data the Square Kilometre Array will churn out daily — about an exabyte per day. This vastly outpaces the state of the art in computing, notes Ton Engbersen of IBM Research in Zurich. “The area you would need for PCs is larger than the SKA,” he said.
Depending on how the SKA is designed and how data transfer questions are solved, it will require between two and 30 exaflops, he said. The design parameters are still being hammered out, but the first phases of construction are scheduled to start in 2016. The site in either Australia or Africa (with most of the dishes in South Africa, and others scattered in different countries from Botswana to Zambia) is expected to be announced later this month. The $2 billion project is not planned to be completed until 2024.
Australian SKA Concept: Artist's impression of dishes that would make up the SKA radio telescope if it is built in Australia. Swinburne Astronomy Productions/SKA Program Development Office
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Data from something as enormous as SKA is a challenge on several levels, and aside from industry efforts, researchers like Andreas Wicenec are trying to figure it out in pieces. Wicenec is head of computing at the International Centre for Radio Astronomy Research in the state of Western Australia and part of his job is figuring out how to store all of the SKA’s data. It’s equivalent to 15 million iPods a day, he noted.
“You have to plan for the whole thing in one go. What is currently called exascale computing is not just an exaflop computer; that is the storage flow, too,” he said. “They have to be built up in parallel.”
He is researching how to increase bandwidth among GPUs to transfer data more quickly, and how to keep these monstrous computers cool to lower power needs. This will be especially important in the deserts of South Africa or Western Australia.
“We have to decrease power consumption by a factor of 10 to 100 to be able to pay the power bill for such a machine,” he said.
IBM researchers have some ideas, according to Engbersen. The company wants to build on its prior research using phase-change memory, which you can read more about here, and its work on 3-D chip architectures, which can transfer data more efficiently and keep things cool. He envisions a stack of 100 chips, nestled one on top of each other — with such an architecture, the SKA could theoretically have supercomputers the size of sugar cubes.
Data downloads can be made more efficient, too — Engbersen notes that when you open a document, you normally look at the first few pages before you scroll down all the way. This can work for astronomers too, perhaps, downloading a few “pages” or bits of data at a time.
IBM’s research center will be located in the Netherlands, in collaboration with ASTRON, which is planning the SKA, and the Netherlands Institute for Radio Astronomy.
New system designs stemming from the SKA effort could translate to other Big Data fields, Engbersen said. But the real payoff will be huge for astronomy.
With SKA, astronomers will have a constant, real-time all-sky radio survey, which could help uncover some of the strangest phenomena in the cosmos. Current radio astronomy is powerful, but a full-sky survey is still limited to about 10 arc seconds. That’s a tiny slice of sky — for comparison, this month the planet Venus, at its super-bright huge disc, is between 25 and 37 arc seconds in diameter. Optical sky surveys, which started in the early 20th century with photographic plates, are fairly high-resolution, more like 1 arc second. “If you want a similar resolution with radio telescopes, you have to go to the SKA scale,” Wicenec said.
The SKA’s lengthy construction timeframe will help the telescopes, computers and storage facilities grow together, Wicenec said.
“It is really relying on the fact that technology is improving at a certain rate,” he said.
Senin, 23 April 2012
Where Is The Center of the Universe?
Popsci.com - First, it’s important to know that the big bang wasn’t an explosion of matter into empty space—it was the rapid expansion of space itself. This means that every single point in the universe appears to be at the center. Think of the universe as an empty balloon with dots on it. Those dots represent clusters of galaxies. As the balloon inflates, every dot moves farther away from every other dot. The space between clusters of galaxies expands, like the rest of the universe, at an accelerating rate. (Gravity keeps the clusters themselves the same size.)
Edwin Hubble first observed this phenomenon in 1929, when he noticed that the light from distant galaxies shifted to the red end of the spectrum, as though it had been stretched as it traveled through space. By measuring the wavelengths of the light, Hubble observed that galaxies were expanding away from each other at a rate proportional to their distance from one another.
In the beginning, the universe was a single point. Where was that? It was, and still is, everywhere. Scientists even have proof: Light from the big bang, in the form of cosmic radiation, fills the sky in every direction
Rabu, 18 April 2012
Bima Sakti Tampaknya Kosong Dari Materi Gelap
Sebuah studi baru yang dibawa oleh tim astronom di Chile telah menemukan bahwa teori yang telah diterima secara luas itu tidak sesuai dengan hasil fakta-fakta pengamatan. Ini mungkin berarti bahwa usaha yang selama ini di lakukan untuk langsung mendeteksi partikel materi gelap di bumi tidak mungkin berhasil.
Segolongan tim astronom menggunakan teleskop MPG / ESO 2,2 meter di LA Silla Observatory bersama dengan teleskop observasi lainnya telah menemukan dan berhasil memetakan gerakan lebih dari 400 bintang sampai sejauh 13.000 tahun cahaya dari Matahari. Dari data ini mereka telah menghitung massa materi-materi di sekitar Matahari dalam volume empat kali lebih besar dari yang sebelumnya diperhitungkan.
Kata ketua tim Kristen Moni Bidin (Departamento de Astronomía, Universidad de Concepción, Chili) "Jumlah massa yang kita peroleh sangat cocok dengan apa yang kita lihat - bintang, debu dan gas - di wilayah sekitar Matahari. Penilitian ini tidak meninggalkan observasi tentang materi gelap tetapi malah tertuju kesana yaitu kita tau sekarang bahwa menurut pengukuran kami di sekitar Matahari tidak terdapat materi gelap."
Menurut teori saat ini, materi gelap diperkirakan merupakan 83% dari isi alam semesta dengan 17% sisanya adalah bentuk materi normal. Sebuah jumlah yang jauh lebih besar dari energi gelap tampaknya juga hadir di alam semesta namun tidak diharapkan mempengaruhi gerakan bintang-bintang di dalam Bima Sakti. Semua upaya sejauh ini untuk mendeteksi materi gelap laboratorium di Bumi telah gagal.
Para astronom yang ada masih bingung mengenai bagaimana galaksi terbentuk dan berputar serta bahwa Bima Sakti dikelilingi oleh lingkaran materi gelap. Mereka tidak mampu secara tepat memprediksi bagaimana bentuk HALO (Bentuk cincin yang melingkari Bima sakti) ini. Walaupun penelitian ini memakan waktu yang sangat lama tetapi mereka berharap dapat menemukan jumlah yang signifikan di wilayah sekitar Matahari. Hanya bentuk yang sangat sulit dan tidak mungkin untuk menjelaskan HALO dari materi gelap.
"Meskipun hasilnya baru, materi yang terlihat sendiri saja sudah dapat menunjukkan bahwa Bima Sakti berputar jauh lebih cepat. Jadi, jika materi gelap tidak terdapat di daerah yang seperti kita harapkan, solusi baru untuk masalah hilangnya massa di luar angkasa harus ditemukan. Hasil kami bertentangan dengan teori saat ini yang diterima. Misteri materi gelap baru saja menjadi lebih misterius. Survei masa mendatang, seperti misi Gaia ESA, akan sangat penting untuk bergerak melampaui titik ini ". Kristen Moni Bidin menyimpulkan.
Minggu, 15 April 2012
'Worm Hole' Mesin Waktu Yang Akan Segera Ditemukan
Inspired by : www.kompasiana.com
Jumat, 13 April 2012
The Facts of the Jellyfish's sting and the treatment
The victim may suffer immediate burning pain, skin rash, blistering, allergic reaction, or a number of systemic symptoms, including neurological sydromes, low blood pressure, abnormal heart rhythms, difficulty breathing, abdominal pain, nausea and vomiting, diarrhea, muscle cramping, and many others.
Treatment should be swift in order to minimize the clinical syndrome.
- Rinse the wound with seawater or concentrated salt solution if possible. A gentle fresh water rinse may cause more stinging cells to discharge their venom.
- There is growing support for hot water immersion therapy (113 degrees Fahrenheit or 45 degrees Centigrade), similar to that for a stingray or scorpionfish envenomation, for treatment of certain jellyfish stings. This recommendation emanates from experts in Australia. It is not known if this therapy is effective against North American, European, and non-Australian (Indo-Pacific) jellyfish species.
- Anticipate an allergic reaction and be prepared to treat with injectable epinephrine and/or oral antihistamines.
- Do not rub the wound.
- Wear protective gloves (double thickness of a surgical glove or a thick dishwashing glove preferred).
- If the sting is from the box jellyfish Chironex fleckeri, flood the area with topical acetic acid 5% (vinegar) immediately and with a continuous application for a minimum of 30 minutes.
- Remove large tentacle fragments with forceps.
- DO NOT apply the pressure immobilization technique.
- Other topical decontaminants that may work, depending on the jellyfish species, include isopropyl (rubbing) alcohol, dilute ammonium hydroxide (household ammonia), powdered bicarbonate (baking soda), unseasoned meat tenderizer (papain), papaya fruit or juice, or lime or lemon (citrus) juice.
- After decontamination, remove adherent nematocysts by applying shaving cream or a paste of baking soda and shaving with a sharp edge, such as a safety razor.
- For a mild skin reaction, apply a topical corticosteroid (“steroid”) cream, ointment or lotion.
- If the reaction is moderate to severe, a physician may prescribe a systemic steroid or administer a steroid injection.
- Anti-tetanus immunization is standard.
- Observe closely for development of a wound infection.
- If the sting is from the box jellyfish Chironex fleckeri, there is an antivenom available in certain locales. The true efficacy of this therapy is currently under scrutin.
Senin, 19 Maret 2012
Your brain is older than you think, say researchers from Stanford and the University of Chicago