Friday, 18 March 2011

Laboratorium Astrofisika

"Anda tidak boleh bernegosiasi dengan impian anda. Bernegosiasilah dengan apa yang harus anda lakukan untuk mencapainya. "

– Mario Teguh -

Astrophysics Laboratory

 


 
Harvard-Smithsonian Center for Astrophysics
60 Garden Street, Cambridge, MA 02138
Study of Galactic Rotation and Molecular Clouds with a CO Telescope
 

Instructors: Thomas Dame and Patrick Thaddeus
 
The 1.2 meter millimeter-wave telescope on the roof of building D at the CfA is ideal in size for the study of large molecular clouds and the kinematics of the Galaxy. Its beamwidth at 115 GHz, the frequency of the fundamental rotational transition of CO, is only 8', which is four times better than the resolution with which the classical Dutch and Australian 21 cm surveys of the Galaxy were conducted. Its cryogenic receiver, with a superconducting SIS mixer (see experiment above) is about as sensitive as that of most large millimeter-wave instruments. The system is quite "user-friendly," and students should be able to master its operation during the first few sessions of the course.

Students will then design more or less from first principles an experiment to determine the rotation curve of the Galaxy with a reasonable amount of observations - one session at the telescope of 4-5 hours should be enough. Analysis of the data will essentially consist of determining the terminal velocity as a function of longitude along the Galactic plane; quite good results can be obtained by classical methods without a great deal of numerical analysis. Students will then use their derived rotation curve with the same data to determine both the molecular mass and the total gravitational mass of the Galaxy, as well as some gross properties of the Galactic molecular cloud distribution. In the process they will obtain a good introduction to the techniques of millimeter-wave astronomy and a liberal education in studies of Galactic structure.



Laboratory Astrophysics
Science is successful because the physical laws we discover on Earth work everywhere and every when. We use laboratory experiments to expand our understanding of physical processes and then apply these results to the processes throughout the Universe. In some cases laboratory experiments can reproduce similar physics. For example, highly charged plasmas can be created in the laboratory to study the collisions between electrons and ions that occur in the hot solar corona. In other cases, such as in the extreme environments of black holes, we cannot reproduce the conditions. However, even in those cases, the pattern of observed spectral signatures allows us to identify the species and determine some of the physical conditions and processes. Spectral features observed in the solar corona are also observed from black hole sources.  

Useful Link

Thursday, 17 March 2011

Indonesian Space Force Command


Indonesian Space Force Command   

 Komando Untuk Keamanan Luar Angkasa 

Dari Angkatan Antariksa Indonesia

"Kami Menjelajahi Alam Raya untuk Menemukan Keagungan Sang Maha Kuasa"

 ~Gen. Arip Nurahman~

 

 

 

(Komando Pasukan Khusus Angkatan Antariksa Indonesia)

 

(Korps Pasukan Khas Angkatan Udara)

 

Jet-powered fighters

It has become common in the aviation community to classify jet fighters by "generations" for historical purposes. There are no official definitions of these generations; rather, they represent the notion that there are stages in the development of fighter design approaches, performance capabilities, and technological evolution.

The timeframes associated with each generation are inexact and are only indicative of the period during which their design philosophies and technology employment enjoyed a prevailing influence on fighter design and development. These timeframes also encompass the peak period of service entry for such aircraft.

Fifth generation jet fighters (2005 to the present)

The fifth generation was ushered in by the Lockheed Martin/Boeing F-22 Raptor in late 2005. Currently the cutting edge of fighter design, fifth-generation fighters are characterized by being designed from the start to operate in a network-centric combat environment, and to feature extremely low, all-aspect, multi-spectral signatures employing advanced materials and shaping techniques. They have multifunction AESA radars with high-bandwidth, low-probability of intercept (LPI) data transmission capabilities. The Infra-red search and track sensors incorporated for air-to-air combat as well as for air-to-ground weapons delivery in the 4.5th generation fighters are now fused in with other sensors for Situational Awareness IRST or SAIRST, which constantly tracks all targets of interest around the aircraft so the pilot need not guess when he glances. (Requires software upgrade on the F-22.)

These sensors, along with advanced avionics, glass cockpits, helmet-mounted sights (not available on F-22), and improved secure, jamming-resistant LPI datalinks are highly integrated to provide multi-platform, multi-sensor data fusion for vastly improved situational awareness while easing the pilot's workload.[9] Avionics suites rely on extensive use of very high-speed integrated circuit (VHSIC) technology, common modules, and high-speed data buses. Overall, the integration of all these elements is claimed to provide fifth-generation fighters with a "first-look, first-shot, first-kill capability".

The AESA radar offers unique capabilities for fighters (and it is also quickly becoming a sine qua non for Generation 4.5 aircraft designs, as well as being retrofitted onto some fourth-generation aircraft). In addition to its high resistance to ECM and LPI features, it enables the fighter to function as a sort of "mini-AWACS," providing high-gain electronic support measures (ESM) and electronic warfare (EW) jamming functions.

Other technologies common to this latest generation of fighters includes integrated electronic warfare system (INEWS) technology, integrated communications, navigation, and identification (CNI) avionics technology, centralized "vehicle health monitoring" systems for ease of maintenance, fiber optics data transmission, and stealth technology.
Maneuver performance remains important and is enhanced by thrust-vectoring, which also helps reduce takeoff and landing distances. Supercruise may or may not be featured; it permits flight at supersonic speeds without the use of the afterburner – a device that significantly increases IR signature when used in full military power.

A key attribute of fifth-generation fighters is very-low-observables stealth. Great care has been taken in designing its layout and internal structure to minimize RCS over a broad bandwidth of detection and tracking radar frequencies; furthermore, to maintain its VLO signature during combat operations, primary weapons are carried in internal weapon bays that are only briefly opened to permit weapon launch. Furthermore, stealth technology has advanced to the point where it can be employed without a tradeoff with aerodynamics performance, in contrast to previous stealth efforts. Some attention has also been paid to reducing IR signatures, especially on the F-22. Detailed information on these signature-reduction techniques is classified, but in general includes special shaping approaches, thermoset and thermoplastic materials, extensive structural use of advanced composites, conformal sensors, heat-resistant coatings, low-observable wire meshes to cover intake and cooling vents, heat ablating tiles on the exhaust troughs (seen on the Northrop YF-23), and coating internal and external metal areas with radar-absorbent materials and paint (RAM/RAP).



The expense of developing such sophisticated aircraft is as high as their capabilities. The U.S. Air Force had originally planned to acquire 650 F-22s, but it now appears that only 187 will be built. As a result, its unit flyaway cost (FAC) is reported to be around $140 million. To spread the development costs – and production base – more broadly, the Joint Strike Fighter (JSF) program enrolls eight other countries as cost- and risk-sharing partners. Altogether, the nine partner nations anticipate procuring over 3000 Lockheed Martin F-35 Lightning II fighters at an anticipated average FAC of $80–85 million.

The F-35, however, is designed to be a family of three aircraft, a conventional take-off and landing (CTOL) fighter, a short take-off and vertical landing (STOVL) fighter, and a Catapult Assisted Take Off But Arrested Recovery (CATOBAR) fighter, each of which has a different unit price and slightly varying specifications in terms of fuel capacity (and therefore range), size and payload.

Other countries have initiated fifth-generation fighter development projects, with Russia's Sukhoi PAK-FA anticipated to enter service circa 2012–2015. In October 2007, Russia and India signed an agreement for joint participation in a Fifth-Generation Fighter Aircraft Program (FGFA), which will give India responsibility for development of a two-seat model of the PAK-FA. India is also developing its own indigenous fifth generation aircraft named Medium Combat Aircraft. China is reported to be pursuing multiple fifth-generation projects under the westernJ-XX, while Japan is exploring their technical feasibility to produce fifth-generation fighters.
See also: List of fifth generation jet fighters



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Tentara Nasional Indonesia Angkatan Darat (Indonesian Army)
 


Tentara Nasional Indonesia Angkatan Laut (Indonesian Navy)

Tentara Nasional Indonesia Angkatan Udara (Indonesian Air Force)

Kepolisian Negara Republik Indonesia (Indonesian Police)



 
Sumber: Wikipedia

Monday, 14 March 2011

Kapal Luar Angkasa dalam Seni

The Mare Nostrum Spaceship is the central element of the Space art group El Club de los Astronautas.

The group has worked out a utopian plan for the spacecraft and they are going to adopt and actualize the plan over time as technologies will develop to turn the plan into reality.



Mare Nostrum represents a series of projects in the scientific, social and economic world that are building the foundation to its construction.