2008 02 19 PNW Bolide

On February 19, 2008 at 13:30 UT, a large fireball entered the earth’s upper atmosphere. Visual reports of the bolide started streaming in at police stations and television stations. A regional airline pilot filed a report of a possible aircraft going down over western Washington.

At 13:30:59 UT the West Kelowna Sentinel all-sky camera caught was triggered by a extremely bright bolide. The video showed the bolide moving slowly downward towards my southeastern horizon. It disappeared behind the mountains across the Okanagan Lake. Despite being below my horizon behind the mountain range the sky pulsed with light as the bolide went through several terminal bursts as can be seen by the total amplitude light curve produced by the Sentinel camera:

 

A look at the total number of pixels above the triggering threshold shows most of the light was released during it’s terminal flares.

Total Pixels graph

The graphs as well as the movie was sent to Dr. Alan Hildebrand, Coordinator of the Canadian Fireball Reporting Centre, University of Calgary.

 

2002 11 19 Leonids Outbreak

Hiroshi Ogawa, head of the International Project for Radio Meteor Observation,  asked radio detection stations from around the world to observe the Leonids during the period of November 1 to November 25, 2002.

Note: Brower was located in Loveland, Colorado at the time of the study and not in West Kelowna.

The following graph shows three stations located in Slovenia, USA, and Japan. The three stations data help trace  the overall activity of the 2002 Leonids.  Notice how as the radian lowered in the sky in Slovenia the radiant was rising for Colorado. Similarly, as the radiant dipped to the west of Colorado it was climbing higher in the sky in Japan, thus giving a continuous view of the overall stream activity over time.

FS Radio results Leo 2002

One of the most rewarding part of the 2002 Leonid study was the recording of a predicted filament  of the comet’s ejecta by Yrjöllä and Brower.

In chapter 14 of Jennniskens book, Meteor Showers and their Parents (Jenniskens 2006:201-215) gives a detail discussion of the filament and why it is important. He states:

Jupiter’s past perturbations may have responsible for the sudden onset of the component in 1994…
I expected the dust component would remain visible post perihelion for at least slightly less than one orbit of Jupiter (<12 yr), thus until 2004 or 2005.

I saw this validated in 2002, when the Filament component was detected for the first time after the perihelion passage of the comet, underlying two very narrow Leonid storm profiles (Fig. 14.41) The observed shift in the peak time and constant width over the years 1994 to 2002 (Table 4) confirms that this component moves about the earth’s path much like individual dust trails in reflection to the ever changing gravitational field of the planets (shaded area in Fig 14.15). Again, more or less following the sun’s reflex motion. (Ibid:214-215)

(Place Fig 14-41 Yrjöllä and Brower here)

More to come…

Jenniskens, P. 2006. Meteor Showers and their Parents, Cambridge University Press, Cambridge, U.K.

Perseid Meteor Shower Thursday 11 Aug 2016

The college meteor camera is already seeing more bright meteors zipping overhead. The Perseid meteor shower started July 17, ends Aug 24 but peaks on Thursday night, August 11 and Friday morning Aug 12. If it’s cloudy Thursday, note that Wednesday night and Friday night will also be very active.

This year the Earth will cross the centre of the comet debris; so we should get the full show. We should also get three additional early peaks: Jupiter’s gravity has shifted some debris; and we’ll see debris from the 1862 and 1479 comet ejection trails to hit this year. Peak estimates (by Esko Lyytinen and Mikhail Maslov) are 150 to 160 meteors per hour, about three per minute.

There are four peaks in two waves; we’ll miss the first wave since it hits Thursday in daylight; and the last wave which hits in Friday’s morning light. But the whole night should be pretty constant at 100 meteors/hour. Best seeing times in the East Kootenays would be after midnight once the Moon sets (low in Scorpius) and the skies darken; continuing until dawn at 5am. We’ll miss the last wave at 7am. But these peak times are estimates, we can hope they arrive during darkness instead.

  (Mountain Daylight Savings Time-- minus 1 hr for Pacific) 1.  Thurs Aug 11 at 4:34pm [1862 comet trail] 2.  Aug 11 at 5:24pm [1479 comet trail] 3.  Aug 11 from 6 to 10pm [Jupiter shifts] 4.  Fri Aug 12 from 7 to 9am [Centre of comet orbit].  

It takes the Earth a week to pass through all the ice and dust from comet Swift-Tuttle. The shower will gradually taper off and end by Aug 24. The meteors are travelling at a speed of 59 km/s when they enter the Earth’s atmosphere. Their trails will all point to Perseus (if it’s a Perseid). The closer they are, the smaller their trail: and the further away, the longer the trail. Look for their colours—at high speed they ionize the air to a green; then that fades to yellow, orange, red as it slows down. If they disrupt and flare, you may see green/bluish wide streaks that glow afterward for a second or two (mainly it’s water ice, but there may be metals present like copper or cobalt).

Allsky Cam Meteor Images Aug 11-12
Allsky Cam Meteor Images Aug 11-12

Where to look? The composite photo above shows the entire sky, and all the meteors that fell on 11 and 12 Aug 2015 over Cranbrook; taken by our college meteor camera. Perseus is the constellation to the North East (middle left side of the photo). Normally there are fewer meteors seen straight overhead, since there is less volume of atmosphere overhead. There are slightly more meteors seen high to the West around Hercules and above the handle of the big dipper; since the meteor trails are longer there, and the meteors skim lower in a greater volume of atmosphere. That’s where I aim my cameras. (Or where it’s darkest, away from the Moon or city streetlight glow).

Allsky Captures Stacked for 13 Aug 2015
Allsky Captures Stacked for 13 Aug 2015

Some of the meteors seen will be from the k-Cygnids running from August 6–19. These peak on August 18 at 3 meteors per hour. They show a number of slow falling fireballs moving at 25km/second.

Small Fireball from Cygnus
Small k-Cygnid Fireball Crossing Cygnus

This photo shows a k-Cygnid meteor crossing through Cygnus the Swan as seen during the last Perseid shower of 2015 (it’s tail is short and it points from Cygnus). Photo taken with a Nikon D100, Tamron 28mm f/2.5 lens, 30 second exposure. I outlined Cygnus in yellow against the Milky Way. The bright star Deneb is the tail at top, and Albireo is the beak at bottom. Photo credit: Rick Nowell.

Starmap of Northeast Sky with Perseus for 13Aug
Starmap of Northeast Sky with Perseus for 13Aug

While you’re out stargazing, here is a starmap showing the Perseus region of the sky, looking Northeast late after midnight in August. The Milky Way band (grey in the map) runs through Perseus; who is the Greek hero coming to rescue Andromeda (daughter of Cassiopeia) who is chained to the rocks. Look below the W of Cassiopeia (the Queen of Ethiopia). You should also see the great square of Pegasus, the winged horse to the right. If you have good eyes (or binoculars), you can spot the fuzzy cloud of the Andromeda Galaxy (M31 in the Map) just above Andromeda’s stick-figure knee. (Andromeda’s head is one corner of the square of Pegasus.) The big dipper, little dipper and Polaris are easy to locate to the left. (Starmap generated by Skyglobe software).

Note: to zoom in a picture or map and see the lines, right-click and open in new tab.

Preparation for calibrating a Sentinel Camera

Steps to take prior to calibrating a Sentinel Camera

Flesh out – PLACEHOLDER ONLY!

Put the procedure here.

  1. Make long exposure after each capture… TIF format
  2. Use GIMP, Paint, PhotoShop or other image processing program and push the brightness and contrast
  3. After photo brings out the hidden starts run a planetarium program. Looking south, elv 90, fov 180.
  4. Match the stars noting pixel x/y on photo and az/el on the planetarium.
  5. run python program calpos.py This produces a personalized correction file that will be used for triangulation. (See Ken’s pdf on the process)

Northern Lights Flare of 7 May 2016

The strongest solar storm so far of 2016 hit us Saturday night at 10:48pm and again between 2 to 3am (according to our college meteor camera). The clear starry East Kootenay sky lit up with glowing curtains and spikes that reached a third of the way up from the Northern horizon.

Our meteor cam has some nifty video on it. And I zipped out of town and took some photos. I missed the best at 11pm, but got some shots at 11:45. But I packed up at 1:50 am, too soon. According to the meteor cam, if I had waited until 2:10 I would have got the big proton arc spiral. Later it died down to a green glow to the North that lasted all night. It was as bright outside as though the Moon was up.

Yet just before 2am, the whole North half of the sky was pulsating; with dim patches travelling from North to South, at about 2 cycles per second, like sheet lightning (I was getting a sore neck watching this over Ft. Steele, 15 km out of Cranbrook). Some kind of oscillation involving the trapped charge bouncing back and forth in the ionosphere, at right angles to the Earth’s magnetic field, creating waves of its own local magnetic field. Anyhow, at 2:10 the build-up must have discharged in a nice arc.

LakitFtS_6s_537_50pc.JPG

Shot from Ft. Steele hill, facing Northeast over Lakit Mountain. The W of the constellation Cassiopeia (Queen of Ethiopia) just above. Rippling, but just greens, no reds or blues. Photos taken with a Nikon and a 28mm f/2.5 lens, with 6 to 15 second exposures.

Perseus_6s_545_50pc.JPG

Looking at the Western edge of the glowing cloud, groups of spikes. Perseus in background. Pale traces of a narrow vertical streamer west of that.

Fisher_6s_448_50pc.JPG

Even Fisher Peak to the East was backlit by rippling bands.

EagerHill_Steeples_30s_1600_554.JPG

Pine trees and the Steeples silhouetted from Eager Hill outside of Cranbrook.

7 May 2016: The National Oceanic and Atmospheric Administration (NOAA) Space Weather Prediction Center has issued a 48 hour magnetic storm watch indicating a Coronal Mass Ejection (CME) or a high speed solar wind stream emanating from the Sun may be heading towards Earth. These fast moving charged particles can cause a Northern Lights display.

The current Geomagnetic Activity level (Kp number) is 5.33 — STORM LEVEL, peaking over the Northern BC and Alberta border.

NorthernLightsFernieMay2016_Sasha3619.JPG

Fernie had it even better, since they saw blues as well. Facing North from Fernie BC, Cassiopeia above. Sent by Sasha Prystae of Kimberley.

Electrons cause most of the glow. The dim red glow at the top of the curtain occurs above 200 km, when fast moving electrons hit low-pressure oxygen atoms in the atmosphere. The middle green is from glowing oxygen molecules between 100 and 200 km. Below 100 km, nitrogen atoms will glow a dim purplish colour and blue. Below that, the air pressure is too high and no effect is seen.

https://www.instagram.com/vanexusphotography/ NorthernLights_Vancouver_ProtonArc_Vanexusphotography_7May2016.JPG

This is a brief spiraling proton arc pillar hitting the Pacific Ocean North of Vancouver in Porteau Cove Provincial Park taken by Karina and Amir around 11pm Saturday, and another at 2am. Wow. See https://www.instagram.com/vanexusphotography/ for a video of that.

Those vertical spiraling curtains are likely ionized oxygen atoms corkscrewing down around the Earth’s magnetic field lines.

This was the strongest flare of 2016 so far. Reportedly, as the Earth moved in its orbit, it crossed a wrinkle in the Sun’s magnetic field, where it reversed polarity briefly. This briefly buffeted the Earth’s protective magnetic field, which let in a gust of protons and electrons.

Fireball Hits Near Canal Flats 20 Dec 2014

On the Hunt for rare rock after meteorite falls in December

University of Calgary geoscience professor asking for the public’s help.

A month after a spectacular fireball December 20, 2014, over the Rocky Mountains, University of Calgary researcher Alan Hildebrand is on a quest for rare meteorites.

In the early morning hours of December 20 a small piece of an asteroid entered Earth’s atmosphere high above Canal Flats, British Columbia, headed northeastwards towards Calgary, Alberta. Although western B.C. and eastern Alberta were overcast, the fireball was seen and imaged over the region between the clouds in both provinces. One spectacular still image was luckily taken by Brett Abernethy who was out with a friend imaging the night sky over Mt. Rundle near Banff when the fireball blazed an 80 km-long trail across the sky (See attached figure 1). Brett says, “We were looking north when everything lit up and we turned to see the fireball. It broke into at least three pieces and turned bright orange before fading away. After the initial shock I remembered that I was exposing a shot during the fireball and was overjoyed to discover that the shot was not overexposed.” Brett alerted the Calgary Herald to the event, who published his image which stimulated on-line discussion from other eyewitnesses.

In his search for more information about the fireball Hildebrand contacted Rick Nowell at the College of the Rockies in Cranbrook, B.C., who recorded it with his Sandia all-sky video camera through patchy clouds, and was able to correctly mark the fireball’s start time to precisely 00:25:00. With this accurate time, another all-sky still image was obtained from the University of Calgary’s Rothney Astrophysical Observatory (RAO). With these additional images in hand, he and his team were able to triangulate its location in the sky.

“It was very interesting to see how precisely a fireball path could be located just from two pictures taken more than 100 km away. We probably know where it was, start to finish within 100 metres,” says Lincoln Hanton, a recent University of Calgary graduate working with Hildebrand. The video recorded in Cranbrook and the fireball’s trajectory also show that it was a relatively slow entry velocity which favours the fall of meteorites.

Hildebrand says the fireball shows extraordinary properties. “In the photo taken by Brett, the fireball becomes visible at approximately 100 km altitude, starts fragmenting at approximately 60 km, and has its last and biggest explosion at 43 km. Those altitudes are much higher than normal. That means the rock was likely a weak type of asteroid.”

Rare carbonaceous chondrite rock

Hildebrand says the apparent weakness displayed indicates that this rock was unusual, probably a carbonaceous chondrite, which is a specific type of stony meteorite that originates from the Outer Asteroid Belt. At that distance from the Sun water and carbon-bearing compounds condensed and mixed into asteroidal bodies. Carbonaceous chondrites represent only approximately three per cent of meteorites that fall on Earth.

“Eyewitness accounts indicate that meteorites fell after surviving the trip through the atmosphere; the estimated rock mass entering the atmosphere was about 100 kg, but the largest pieces on the ground are probably only 2 kg,” says Hildebrand. “The meteorites fell in a forested area of the upper White River valley. It’s a tough area to search.” (See Figure 2)

Map of Impact Area
Satellite Map of Impact Area

Hildebrand says with the possibility of such a rare find his team will do some searching in the spring and encourage any others who can travel safely in this relatively remote area to search as well. How you can help

Hildebrand and his team are eager to talk with anyone who saw the fireball from Canal Flats, Fairmont Hot Springs, or Elkford, B.C. He encourages property owners in that region to check security camera systems for any shadows cast by the fireball. Anyone who had a wildlife camera in the region is also asked to check that date and time for moving shadows. Contact the University of Calgary at 403-220-8969 or via email at ltjhanto@ucalgary.ca.

  Contact information: Brett Abernethy   403-620-6929 Lincoln Hanton     403-220-8969 Alan Hildebrand   403-220-2291 Rick Nowell       250-489-2751 ext 3585  

Figure 1: Brett Abernethy’s image of the Dec 20 fireball looking south over Mt. Rundle from near Johnson Lake. The fireball crossed the constellation of Orion and then began fragmenting where the trail brightens and broadens. Note the slight reddening at the fireball’s end as the surviving rock fragments slowed and cooled before falling to the ground. Image is a 40 second exposure taken with a Canon 5D Mark III with a wide angle Zeiss 21 mm lens which slightly compresses the vertical aspect of the image. (All rights reserved)

Figure 2: Satellite image of eastern British Columbia showing location of the fireball trajectory projected onto the ground and estimated meteorite fall area as a yellow ellipse. The end of the fireball was about 40 km east of Fairmont Hot Springs. An eyewitness in Canal Flats would have seen the fireball travel almost straight downwards in the sky. (Figure constructed on Google Earth base)

2010-09-05 ABMO W Kelowna

All times UT

20100905 061055 NE quad going SE -2 mag

20100905 080720 SW quad going S -3 mag

20100905 080746 NE&NW quad going NW -1.7 mag long trail

20100905 093915 NE quad going N -2.6 mag

20100905 094200 SW quad going SW -2.2 mag

20100905 120316 NE quad going NNE mag unknown (Sentinel III) All others UFOC2

The RA and Dec and Az/El for all the events but last are available.

Camera systems introduction

Temp Place holder

Camera systems currently in use by network members include the Sentinel camera a Sony, the Watec 902H, and the PC164CEX-2.

Sentinel camera:

The Sentinel III camera is a Sony HiCam HB-710E. The CCD (Charge Coupled Device) is a 1.27 cm (0.5 inch) interlined chip with 410K pixels. Effective Pixels 768 (Horizontal) X 494 (Vertical). It has a super-low illumination environment of 0.0005 Lux(F1.2 /20 IRE at AGC Max). It is powered by +12VDC and consumes 150 mA at maximum load.

The lens is Rainbow L163VDC4P fisheye lens with a 180 degree field.

For a pictorial tour of the Sony HiCam HB-710E camera, it’s housing and frame grabber click here.

The Sentinel – video frame grabber comes in an external box. It contains a micro-controller, a RCM3200, from Rabbit Semiconductor. There are three connections on the box, 1) +3.3V DC input, 2) a BNC male connector for the 1Vp-p video input from the Sony camera via 75 ohm coax, and 3) an Ethernet jack. The frame grabber communicates with a PC via the ethernet cable either directly with a crossover cable or through a LAN hub via a conventional ethernet cable.

The Sentinel III system is being replaced by the Sentinel IV system which uses the same camera but uses an internal Hauppaugue model 188 video  card.

Watec 902H

PC164CEX-2

acrylic domes from EZ Tops in New Brunswick.

fisheye lens, sources