Friday, January 03, 2014



Grid Computing

            In the 1980s “internetworking protocols” allowed us to link any two computers, and a vast network called the internet exploded around the globe. In the 1990s the “hypertext transfer protocol” allowed us to link any two documents, and a vast, online library-cum-shopping-mall called the World Wide Web exploded across the Internet. Now, fast-emerging “grid protocols” might allow us to link almost anything else: databases, simulation and visualization tools, even the number-crunching power of the computers themselves. And we might soon find ourselves in the midst of the biggest explosion yet.
            “We’re moving into a future in which the location of [computational] resources doesn’t really matter,” says Argonne National Laboratory’s Ian Foster. Foster and Carl Kesselman of the University of Southern California’s Information Sciences Institute pioneered this concept, which they call grid computing in analogy to the electric grid, and built a community to support it. Foster and Kesselman, along with Argonne’s Steven Tuecke, have led development of the Globus Toolkit, an open-source implementation of grid protocols that has become the de facto standard. Such protocols promise to give home and office machines the ability to reach into cyberspace, find resources wherever they may be, and assemble them on the fly into whatever applications are needed.
            Imagine, says Kesselman, that you’re the head of an emergency response team that’s trying to deal with a major chemical spill. “You’ll probably want to know things like, What chemicals are involved? What’s the weather forecast, and how will that affect the pattern of dispersal? What’s the current traffic situation, and how will that affect the evacuation routes?” If you tried to find answers on today’s internet, says Kesselman, you’d get bogged down in arcane log-in procedures and incompatible software. But with grid computing it would be easy: the grid protocols provide standard mechanisms for discovering, accessing, and invoking just about any online resource, simultaneously building in all requisite safeguards for security and authentication.
            Construction is under way on dozens of distributed grid computers around the world-virtually all of them employing Globus Toolkit. They’ll have unprecedented computing power and applications ranging from genetics to particle physics to earthquake engineering. The $88 million TeraGrid of the U.S. National Science Foundation will be one of the largest. When it’s completed later this year,  the general-purpose, distributed supercomputer will be capable of some 21 trillion floating-point operations per second, making it one of the fastest computational systems on Earth. And grid computing is experiencing an upsurge of support from industry heavyweights such as IBM, Sun Microsystems, and Microsoft. IBM, which is a primary partner in the TeraGrid and several other grid projects, is beginning to market an enhanced commercial version of the Globus Toolkit.

Others in Grid Computing
RESEARCHER
PROJECT
Andrew Chien
Entropia
Peer-to-Peer Working Group
Andrew Grimshaw
Avakii University of Virginia
Commercial grid software
Miron Livny
University of Wisconsin, Madison
Open-source system to harness idle workstations
Steven Tuecke
Argonne National Laboratory
Globus Toolkit

            Out of Foster and Kesselman work’s on protocols and standards, which began in 1995, “this entire grid movement emerged,” says Larry Smarr, director of the California Institute for Telecommunications and Information Technology. What’s more, Smarr and others say, Foster and Kesselman have been instrumental in building a community around grid computing and in advocating its integration which two related approaches: peer-to-peer computing, which brings to bear the power of idle desktop computers on big problems in the manner made famous by SETI@home, and Web services, in which access to far-flung computational resources is provided through enhancements to the Web’s hypertext protocol. By helping to merge these three powerful movements, Foster and Kessleman are bringing the grid revolution much closer to reality. And that could mean seamless and ubiquitous access to unfathomable computer power.


Name                           : Marta Asri Dewi
Student Number         : 12315244009
Study Program            : Science Education
Class                            : International

1. Microscope and its parts


 






















































































2. Function of each part of microscope
a.       Eyepiece: The lens the viewer looks through to see the specimen.
b.      Diopter Adjustment: Useful as a means to change focus on one eyepiece so as to correct for any difference in vision between your two eyes.
c.       Body tube (Head): The body tube connects the eyepiece to the objective lenses.
d.      Arm: The arm connects the body tube to the base of the microscope.
e.       Coarse adjustment: Brings the specimen into general focus.
f.       Fine adjustment: Fine tunes the focus and increases the detail of the specimen.
g.      Nosepiece: A rotating turret that houses the objective lenses. The viewer spins the nosepiece to select different objective lenses.
h.      Objective lenses: One of the most important parts of a compound microscope, as they are the lenses closest to the specimen.
i.        Mechanical Stage: The flat platform where the slide is placed.
j.        Stage clips: Metal clips that hold the slide in place.
k.      Stage height adjustment (Stage Control): These knobs move the stage left and right or up and down.
l.        Aperture: The hole in the middle of the stage that allows light from the illuminator to reach the specimen.
m.    On/off switch (Light Switch): This switch on the base of the microscope turns the illuminator off and on.
n.      Illumination: The light source for a microscope. Older microscopes used mirrors to reflect light from an external source up through the bottom of the stage; however, most microscopes now use a low-voltage bulb.
o.      Brightness Adjustment: Adjusts the amount of light that reaches the specimen.
p.      Condenser: Gathers and focuses light from the illuminator onto the specimen being viewed.
q.      Base: The base supports the microscope and it’s where illuminator is located.