Composition No. 2 will be transmitted as a part of the October 2022 experiment campaign.  Composition No. 2 is half an hour long involving multiple frequencies and will be transmitted four times.  A condensed daily schedule of times and frequencies is posted at the top of this page. If you scroll down further there is detailed information on each movement.

 

ALL MODES ARE AM

October 23, 06:00 UTC
XI.     06:00:00 - 06:01:00 (4.85 MHz)
XII.   06:01:30 - 06:05:00  (4.8 MHz ; 5.4 MHz)
XIII.  06:05:30 - 06:12:00  (9.5 MHz ; 3.3 MHz)
XIV.   06:12:00 - 06:13:00  (4.85 MHz)
XV.     06:13:30 - 06:17:00  (4.8 MHz ; 5.4 MHz)
XVI.   06:17:30 - 06:18:30  (4.85MHz)
XVII.  06:19:00 - 06:22:30 (4.8 MHz ; 5.4 MHz)
XVIII. 06:23:00 - 06:24:00 (4.85 MHz)
XIX.   06:24:30 - 06:28:00 (4.8 MHz ; 5.4MHz)
XX.     06:28:30 - 06:29:30  (4.85MHz)

October 24, 06:00 UTC
XI.     06:00:00 - 06:01:00 (3.2 MHz)
XII.   06:01:30 - 06:05:00  (2.8 MHz ; 3.5 MHz)
XIII.  06:05:30 - 06:12:00  (9.5 MHz ; 3.3 MHz)
XIV.   06:12:00 - 06:13:00  (3.2 MHz)
XV.     06:13:30 - 06:17:00  (2.8 MHz ; 3.5 MHz)
XVI.   06:17:30 - 06:18:30  (3.2 MHz)
XVII.  06:19:00 - 06:22:30 (2.8 MHz ; 3.5 MHz)
XVIII. 06:23:00 - 06:24:00 (3.2 MHz)
XIX.   06:24:30 - 06:28:00 (2.8 MHz ; 3.5 MHz)
XX.     06:28:30 - 06:29:30  (3.2 MHz)

October 25, 16:30 UTC
XI.     16:30:00 - 16:31:00 (3.35 MHz)

XII.   16:31:30 - 16:35:00  (3.35 MHz ; 2.8 MHz)
XIII.  16:35:30 - 16:41:30 (2.8 MHz ; 5.9 MHz)
XIV.   16:42:00 - 16:43:00  (3.35MHz)
XV.     16:43:30 - 16:47:00  (3.35 MHz ; 2.8 MHz)
XVI.   16:47:30 - 16:48:30 (3.35 MHz)
XVII.  16:49:00 - 16:52:30 (3.35 MHz ; 2.8 MHz)
XVIII. 16:53:00- 16:54:00(3.35 MHz)
XIX.   16:54:30 - 16:58:00 (3.35 MHz ; 2.8 MHz)
XX.     16:58:30 - 16:59:30(3.35 MHz)

October 26, 16:30 UTC
XI.     16:30:00 - 16:31:00 (9.45 MHz)

XII.   16:31:30 - 16:35:00  (9.06 MHz ; 9.56 MHz)
XIII.  16:35:30 - 16:41:30 (2.8 MHz ; 5.9 MHz)
XIV.   16:42:00 - 16:43:00  (9.45 MHz)
XV.     16:43:30 - 16:47:00  (9.06 MHz ; 9.56 MHz)
XVI.   16:47:30 - 16:48:30 (9.45 MHz)
XVII.  16:49:00 - 16:52:30 (9.06 MHz ; 9.56 MHz)
XVIII. 16:53:00- 16:54:00(9.45 MHz)
XIX.   16:54:30 - 16:58:00 (9.06 MHz ; 9.56 MHz)
XX.     16:58:30 - 16:59:30(9.45 MHz)

XI. Ricochet

Air Glow Experiment
Beam directed straight up, at Magnetic Zenith, to generate artificial aurora.
Shortwave listeners around the world could expect to receive the side lobes.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful air glow creation - this however means that it might not propagate as far.

Frequencies for October 26 will be directed downward 45 degrees off zenith aimed at my home town in New Brunswick at an azimuth of 72 degrees.

UTC
4.85 MHz
UTC
3.2 MHz
UTC
3.35 MHz
UTC
9.45 MHz
45 degrees off zenith; directed at azimuth 72 degrees - Atlantic Canada

XII. Where do I start?

Luxembourg Experiment
Two 6x12 arrays - approx 600 kHz apart
If Luxembourg effect is present, both signals should be received on each individual frequency -- mixed in the ionosphere.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful Luxembourg mixing - this however means that it might not propagate as far.

UTC
East
4.8 MHz
West
5.4 MHz
UTC
East
2.8 MHz
West
3.35 MHz
UTC
East
2.8 MHz
West
3.35 MHz
UTC
East
9.06 MHz
45 degrees off zenith; directed at azimuth 108 degrees - middle America
West
9.56 MHz
45 degrees off zenith; directed at azimuth 108 degrees - middle America

XIII. Mixing Moving Pictures (NBTV)

NBTV (Narrow Band Television) Experiment
Two 6x12 arrays
One aimed toward the light side of the planet, the other aimed toward the dark side

In order to view the video one must decode the signal with NBTV viewing software.
Three versions of the software can be downloaded here: http://users.tpg.com.au/users/gmillard/nbtv/nbtv.htm

NOTE: decoding the NBTV can be tricky and requires adjusting the levels, brightness, contrast, and sync pulse.  There is a good possibility that the sync pulse may become lost or distorted in transmission, which will result in a "rolling" image as a best case scenario.
There is a good chance that reception of the video may be very distorted and abstract - I am still interested in receiving screen capture videos of attempts at decoding the video, no matter how distorted or abstract.

UTC
East
9.5 MHz
Daytime in Asia; directed at 290 Azimuth - grating lobe will be quite large and possibly be recieved in other parts of the world as well.
West
3.3 MHz
Nighttime in North America; directed at 110 Azimuth
UTC
East
9.5 MHz
Daytime in Asia; directed at 290 Azimuth - grating lobe will be quite large and possibly be recieved in other parts of the world as well.
West
3.3 MHz
Nighttime in North America; directed at 110 Azimuth
UTC
East
2.8 MHz
Darkness in Asia; directed at 290 Azimuth
West
5.9 MHz
Daytime in North America; directed at 110 Azimuth
UTC
East
2.8 MHz
Darkness in Asia; directed at 290 Azimuth
West
5.9 MHz
Daytime in North America; directed at 110 Azimuth

XIV. Polar Mesospheric Summer Ekho

Air Glow Experiment
Beam directed straight up, at Magnetic Zenith, to generate artificial aurora.
Shortwave listeners around the world could expect to receive the side lobes.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful air glow creation - this however means that it might not propagate as far.

UTC
4.8 MHz
UTC
3.20 MHz
UTC
3.35 MHz
UTC
9.45 MHz
45 degrees off zenith; directed at azimuth 180 degrees - Antarctica

XV. Artificial Periodic Imhogeneity Experiments

Luxembourg Experiment
Two 6x12 arrays - approx 600 kHz apart
If Luxembourg effect is present, both signals should be received on each individual frequency -- mixed in the ionosphere.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful Luxembourg mixing - this however means that it might not propagate as far.

UTC
West
4.8 MHz
East
5.4 MHz
UTC
West
2.8 MHz
East
3.35 MHz
UTC
West
2.8 MHz
East
3.35 MHz
UTC
West
9.06 MHz
45 degrees of zenith; directed at azimuth 216 degrees - Antarctica
East
9.56 MHz
45 degrees of zenith; directed at azimuth 216 degrees - Antarctica

XVI. Measure and Perturb

Air Glow Experiment
Beam directed straight up, at Magnetic Zenith, to generate artificial aurora.
Shortwave listeners around the world could expect to receive the side lobes.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful air glow creation - this however means that it might not propagate as far.

UTC
4.85 MHz
UTC
3.2 MHz
UTC
3.35 MHz
UTC
9.45 MHz
45 degrees off zenith; directed at azimuth 252 - Australia

XVII. Confession

Luxembourg Experiment
Two 6x12 arrays - approx 600 kHz apart
If Luxembourg effect is present, both signals should be received on each individual frequency -- mixed in the ionosphere.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful Luxembourg mixing - this however means that it might not propagate as far.

UTC
West
4.8 MHz
East
5.4 MHz
UTC
West
2.8 MHz
East
3.35 MHz
UTC
West
2.8 MHz
East
3.35 MHz
UTC
West
9.06 MHz
45 degrees off zenith; directed at azimuth 288 - Malaysia
East
9.56 MHz
45 degrees off zenith; directed at azimuth 288 - Malaysia

XVIII. Our Own Bodies

Air Glow Experiment
Beam directed straight up, at Magnetic Zenith, to generate artificial aurora.
Shortwave listeners around the world could expect to receive the side lobes.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful air glow creation - this however means that it might not propagate as far.

UTC
4.85 MHz
UTC
3.2 MHz
UTC
3.35 MHz
UTC
9.45 MHz
45 degrees off zenith; directed at azimuth 324 - India

XIX. Snowy Owl

Luxembourg Experiment
Two 6x12 arrays - approx 600 kHz apart
If Luxembourg effect is present, both signals should be received on each individual frequency -- mixed in the ionosphere.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful Luxembourg mixing - this however means that it might not propagate as far.

UTC
West
4.8 MHz
East
5.4 MHz
UTC
West
2.8 MHz
East
3.35 MHz
UTC
West
2.8 MHz
East
3.35 MHz
UTC
West
9.06 MHz
45 degrees off zenith; directed at azimuth 360 - Ukraine
East
9.56 MHz
45 degrees off zenith; directed at azimuth 360 - Ukraine

XX. Where Does Your Apparatus End?

Air Glow Experiment
Beam directed straight up, at Magnetic Zenith, to generate artificial aurora.
Shortwave listeners around the world could expect to receive the side lobes.

Frequencies for October 24 were lowered to accomodate ionospheric conditions in order to increase likely-hood of ionospheric modificiation and successful air glow creation - this however means that it might not propagate as far.

UTC
4.85 MHz
UTC
3.2 MHz
UTC
3.35 MHz
UTC
9.45 MHz
45 degrees off zenith; directed at azimuth 36 - Greenland