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Saturday, September 12, 2009

SolderSmoke Podcast #115


http://www.soldersmoke.com
Camping in Sabina
Michelangelo's late start
Anniversaries: Internet, SolderSmoke, Hack-A-Day
From Kitty Hawk to the Moon
Carrington flares and childhood aurora
Calculating speed of light (using cheese)
Mythbusters
Hubble Space Telescope, Sliding Spring Observatory
Europa
Transistor Museum
Understanding Mixer products
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Friday, September 11, 2009

Mixing it up

OK, enough of the pretty pictures from outer space, now it's time to go back to mixer math.

In the podcast, on this blog, and in the SolderSmoke book I have chronicled my efforts to understand how mixer circuits REALLY work. For some of us, the trig is just not enough. We want intuitive understanding. Ya' gotta draw us a picture. Mike KC7IT, and Dennis W6DWF, both alerted me to a good one. It is from a new book "RF Front-End: World Class Designs", Edited by Jane Sullivan Love. The chapter on mixers is available online here:
http://i.cmpnet.com/rfdesignline/2009/08/C0429pt1.pdf

I really like figure 9.6 (above). You can really SEE how the switching action that is driven by the LO kind of "chops up" the RF signal and produces the complex waveform that is the IF. The neat thing about the IF waveform in this drawing is that you can clearly see both the sum freq (the smaller squiggles) AND the difference freq (the overall movement inside which the smaller squiggles are present). Go ahead, count them up! Sums and differences!
This is a special kind of mixer: a polarity-reversing switching mixer. When the LO is negative, it inverts whatever is at the RF port. From this you can see why mixers are described mathematically as "multipliers." This mixer is multiplying the instantaneous value of the RF input by +1 (when the LO is positive) and then by -1 (when the LO is negative).
I think it is quite a bit harder to "see" the genesis of the sum and difference freqs when you are working with non-switching mixers, but this diagram is, I think, really useful in gaining an intuitive understanding of what goes on in the mixing process.

Wednesday, September 9, 2009

Hubble Space Telescope: New and Improved!

I know, I know, it is not exactly ham radio, but look at it this way: electromagnetic waves from far, far away! REAL DX. And some very cool gear to receive the signals. And some recent repair and modification work... So you see, this is really not so far afield after all.

I've been a big fan of the Hubble Space Telescope for a long time. When I was closer to the equator (in Santo Domingo) sitings of the HST were quite common. I'm glad to see that the recent repairs and mods worked out so well. Here is a really nice video on the new and improved Hubble: Hubble Space Telescope Video

Saving the world, finding comets....

Well I guess the hours are not great, but how about the job satisfaction! Rob McNaught works at the Sliding Spring Observatory about 400 km from Sydney, Australia. The observatory searches for comets and asteroids that could do to us what they may have done to the dinosaurs (see below). A significant fringe benefit of this job is that Rob gets to discover new comets. He recently set world record by finding his 50th. Congrats Rob!

The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. The identification of the iridium anomaly at the Cretaceous-Tertiary boundary (Alvarez et al., 1980) and associated Chicxulub impact crater (Hildebrand et al., 1991) and perhaps recently the Australian Bedout crater (Becker et al., 2004) associated with the Permian- Triassic "great dying" (although the presence of shock metamorphism has not yet been adequately demonstrated), strongly suggests that impacts by minor planets play an important role in the evolution of life. These are a natural result of the accretionary process that formed the Earth and planets. Indeed, the 1994 impact of D/Shoemaker-Levy 9 on Jupiter provided tangible evidence of this. Although the collision frequency is much lower than in the past, the question is not whether there will be other impacts, but when.

Tuesday, September 8, 2009

Early Crystal Set in Altoids-like Box


Even way back then, British homebrewers had an affinity for Altoids-like boxes!
David, M0VTG, sent me the above pictures, and this description:

I enclose some pictures of a kit produced in the early to mid 1900s of crystals and a holder for use in a crystal radio; unfortunately the cats whisker is missing! The box is marked:

Front: NEUTRON Back: Neutron Ltd
Trade Mark Sicilian House
Wireless Crystal Southhampton Row
1/6 Phone Museum 2017
Catswisker and
Directions Enclosed

The 1/6 refers to the price (one shilling and six pence) pre-decimalization and converts to seven and a half pence today (although the half pence has been dropped thorough inflation). I should add that the box measures about an inch and a half in length.

Saturday, September 5, 2009

Carrington Flares, Aurora, Where were you on August 4, 1972?

Greg, KC2DWF, sent me a really interesting story about the work of the English solar astronomer Richard Carrington. He discovered a kind of solar flare (named for him) that comes along every few centuries and could knock us all off the air.

As I was reading the article, I started to think about a childhood event that I think I mentioned in one of the podcasts. I have vivid memories of a summer night in which the skies were filled with really bright colorful lights. The article about Carrington notes that there was a major solar flare (but not of Carrington levels) on August 4, 1972 that caused auroral displays far into the southern part of the USA. The year is a bit later than I thought (I was 13 at that time) but the time of year is correct. And that flare was big enough to have caused really vivid aurora over New York.
The NASA site "Brushfires in the Sky" provides this very helpful list for people, like me, trying to figure out what we saw, and when:

The Aurora Watchers Handbook lists the following "Great Geomagnetic Storms" of the 20th century when auroras were seen much farther south than usual. If you have a childhood memory of aurora borealis, it may have come from one of these storms.

  • October 31 - November 1, 1903
  • September 25, 1909
  • May 13-16, 1921
  • April 16, 1938
  • February 11, 1958
  • July 8, 1958
  • August 4, 1972
  • December 19, 1980
  • March 13-14, 1989
Looks to me like my event was August 4, 1972. Anyone else have memories of this storm?

Here is the article that Greg sent:
http://science.nasa.gov/headlines/y2008/06may_carringtonflare.htm

The Transistor Museum

Wes, W7ZOI, relayed to us this great site found by from Jeff Damm, WA7MLH. This is a real treasure trove of transistor history:
http://semiconductormuseum.com/Museum_Index.htm
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