Friday, January 15, 2016

Comet Catalina and Whirlpool Galaxy

Comet Catalina and the Whirlpool Galaxy
as seen from Meadowcreek Park Observatory
(MPO)
Click image for larger version.
You can also go HERE for a high-resolution image from NASA.

Thursday, January 14, 2016

Jupiter and moons (Jan. 14, 2016)

Jupiter and it's 4 brightest moons
Canon Rebel t3, 300mm, f/4, ISO 100, 10 sec. (tracked)
Click image for larger version

Wednesday, January 13, 2016

6 Day Forward-Scatter (FM) Plot

12 day forward-scatter (FM) meteor plot show activity in the southern skies from my location...
(Daily average meteor rates are shown in green)
Click on image for larger version

Monday, January 11, 2016

Pleiades Star Cluster

A view of the Pleiades star cluster, in relation to the sky around it....
Click on image for larger version

My View From Here.....

The Whirlpool Galaxy is a "pinwheel-shaped" spiral galaxy near the end of the handle of the Big Dipper. This galaxy is located roughly 23 million light years from our own Milky Way Galaxy.
The Whirlpool Galaxy is the larger of two galaxies which are interacting with each other, being gravitationally connected.
During an imaging session on the night of Jan. 10 (2016), using a Canon Rebel DSLR camera, mounted on a portable tracking mount, I realized that this galaxy had shown up in some of my images.
Below, is the result of a 60-second photograph and some post-processing to bring out some detail.
I was using a 55mm lens on the camera, so this is a fairly wide-angle view of the sky.
Again....the distance to this galaxy is ~23,000,000 LIGHT YEARS.  1 light year is 6 TRILLION miles...

(click on image for a larger version)



Sunday, January 10, 2016

Forward-Scatter (FM) Radio Region

 Graph shows the 24-hour Forward-Scatter (FM)
meteor activity for Jan. 7-9 with hourly averages.
Click on image for larger version.
Map shows the location of the FM transmitter (Tx),
FM receiver (Rx) and the region of sky being monitored.
Click on image for larger version. 

Monday, January 4, 2016

Quadrantid Meteor Shower

The annual Quadrantid meteor shower has peaked and is now settling down. Peak meteor rates were predicted for the pre-dawn hours of January 4.
The forward-scatter observations from MPO show 3 distinct peaks...3 a.m., 2 p.m. and 6 p.m.
(Forward-scatter is simply FM radio signals reflected off of the ionized meteor trail).

(Click on image for larger version)

Sunday, December 20, 2015

FM RADIO METEORS

Meteors are very small bits of debris left from the tail of a comet when it passes through our Solar System. As Earth passes through these debris trails, the tiny meteoroids are swept up in the atmosphere and burn up. It is during this process that the "meteoroid" is known as a "meteor".

The meteor is traveling so fast through Earth's atmosphere, that it actually heats up (ionizes) the air around it which creates a (usually) very brief trail (or "train") behind the meteor.
These ionized trains reflect FM radio signals.

Radio signals travel in a straight line ("line-of-sight"), so if the receiver is far enough away to be over the horizon from the transmitter, nothing but static will be heard. The signal has simply continued off into space at that point.
HOWEVER....I have learned how to LISTEN to meteors!

I have an FM antenna mounted in my backyard, pointing south (toward an FM station 180 miles away) and tilted upwards at 34°. In other words, the antenna is pointed toward the sky in the direction of the radio station.

When a meteor enters Earth's atmosphere between my location and the transmitting station, the radio signal will be reflected off the meteor's trail and "bounced" back toward Earth....in my direction!! These bounced signals can last anywhere from a fraction of a second to a few minutes...depending on the characteristics of the meteor trail.

The annual Geminid meteor shower occurred earlier this month, peaking around the 14th. I was monitoring them, using the above technique, from December 7th - 19th.
Below, is a graph showing the total daily FM meteor reflections for that period. As you can see, the meteor shower peaked around the 15th, then quieted down....

(I get a kick out the look on people's faces when I tell them I enjoy LISTENING to meteors!)


Friday, November 27, 2015

Large Prominence (Nov. 27, 2015)

Solar prominences are large clouds of plasma (hot, energized gas) which lift off the surface of the Sun, and temporarily held in place by the Sun's strong magnetic fields.
Eventually, a prominence will either fall back to the surface or explode out into space.
This image shows the difference between "typical"- sized prominences and a "large" one.
For scale, a typical-size prominence is several time larger than Earth!

Sunday, November 1, 2015

Sunspot Region #2443 (Nov. 1, 2015)

Active Region #2443 (AR2443)
Colorized image.
 
Brief video clip of AR2443
(Monochrome)


Saturday, October 31, 2015

Sunshine On A Cloudy Day

Even on a cloudy, rainy day I can "see" what's happening on the Sun......
 
This graph is from my Very Low Frequency (VLF) receiver, which monitors VLF transmitting stations around the world.
VLF is used by the Navy to communicate with submarines out at sea. The VLF signals not only penetrate water, but also bounce off Earth's ionosphere in order to travel around the world.
The ionosphere is affected by solar flares that erupt on the Sun and these flares create what is called Sudden Ionospheric Disturbances (SID).
The SID, in turn, affects the VLF signal and my receiver can detect these changes.
Attached, is a small portion of the plot from Oct. 30, showing a C-class solar flare. (The time on the plot is UTC, or Greenwich Mean Time).
The red numbers above the spike in the plot indicate the start/peak/end time, intensity and sunspot region where the flare occurred....


Wednesday, October 21, 2015

Mars, Jupiter and Moons

Mars and Jupiter
(pre-dawn, Oct. 16, 2015)
Three of Jupiter's 4 brightest moons can be seen.