SEE AND HEAR MORSE CODE
ASTRA Malaysia
Sunday, May 16, 2010
Thursday, May 13, 2010
Radio Amateur Examination Results (RAE 2010-1)
To check results online visit http://rae.skmm.gov.my/rae_2010_1.asp
Wednesday, May 12, 2010
Tuesday, May 11, 2010
Image Of The Day
This image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter covers a small portion of the northwest quadrant of Hellas Planitia on Mars. With a diameter of about 1,400 miles and a depth reaching the lowest elevations on Mars, Hellas is one of the largest impact craters in the solar system.The area has a number of unusual features, which are thought to be quite old because of the high crater density. The crater inside Hellas has been filled with material, which may be related to volcanic activity on the basin's northwestern rim. It also might be related to the presence water and water ice. However, there is evidence elsewhere that the ground here is rich with ice. HiRISE will be used to investigate this in more detail when the basin is free from atmospheric dust.
NEEMO 14 Mission
Analog missions, like this one, allow NASA to evaluate the interactions of multiple concept mission systems in remote field locations with similarities to conditions astronauts might face during a space mission. › Learn Monday, May 10, 2010
Wednesday, May 5, 2010
Image Of The Day
This image from the European Space Agency's Herschel Space Observatory shows the cloud associated with the Rosette Nebula, a stellar nursery about 5,000 light-years from Earth in the Monoceros, or Unicorn, constellation. Herschel collects the infrared light given out by dust. The bright smudges are dusty cocoons containing massive embryonic stars, which will grow up to 10 times the mass of our sun. The small spots near the center of the image are lower mass stellar embryos. The Rosette Nebula itself, and its massive cluster of stars, is located to the right of the picture. This image is a three-color composite showing infrared wavelengths of 70 microns (blue), 160 microns (green), and 250 microns (red). It was made with observations from Herschel's Photoconductor Array Camera and Spectrometer and the Spectral and Photometric Imaging Receiver instruments.Herschel is an ESA cornerstone mission, with science instruments provided by consortia of European institutes and with participation by NASA. A media day celebrating the release of the first results from ESA’s Herschel infrared space telescope will take place on May 6, 2010, at Space Expo, at the European Space Research and Technology Centre (ESTEC), Noordwijk, The Netherlands. Doors open at 11:30 CEST. The media day is organized in connection with the Herschel First Results Symposium taking place this week at ESTEC and the theme is Revealing the Hidden Side of Star Formation. For more information on the day's activities, see the press release.For more information on this image, visit ESA's Herschel Program site.
MyEQSLCard
eQSL Card (Recieved)
igq107 QSL Card
THE POSTCARD CROSSING PROJECT
ABOUT AMATEUR RADIO
AMATEUR RADIO OPERATOR'S CERTIFICATE
INTERFERENCE
Regulation 15(2) of the regulation denotes that a person who contravenes this regulation commits an offence and shall, on conviction, be liable to a fine not exceeding three hundred thousand ringgit (RM 300,000.00) or to imprisonment for a term of not exceeding three years or to both.
To eliminate the potential of interferences, the following procedures must be followed strictly:-
a) Ensure that suffient equipment, tools and test gear is available and can used to monitor and verify that your transmission does not cause any interference to other radio services.
b) You must responsible if your amateur radio is found to be the caused of interference. Immediate remedy action must be taken to rectify the problems in case of interference.
c) Ensure that the transmission do not exceed the level of over deviation.
d) Ensure that the radiated energy is always within the narrowest posible frequency bands for any class of emission in use.
e) The radiation of harmonics and spurious emissions should be suppressed to minimize interference.














