Swansea Astronomical Society Blog

Sunday, December 26, 2010

 

Narrowband filters and false colour images

When red, green and blue filters are used to capture monochrome images which are then assigned to the appropriate colour channel in an RGB colour image, the additive properties of the three primary colours are being used:


We can see that when red light and green light are combined, yellow light results and that when red, green and blue light are combined, white light results, etc.

Sometimes a luminance channel is included with no colour information to provide detail. This would be an LRGB image.
This is an LRGB image of M1, the Crab nebula:

Narrowband filters are used to show the presence of particular elements in structures such as nebulae. The three filters used here are:
Sll with a wavelength of 672.4 nm in the red;
H-alpha with a wavelength of 656.3 nm also in the red;
Olll with a wavelength of 500.7 nm in the blue-green part of the spectrum.
Images of M1 were captured through each of these narrowband filters which have a bandpass of about 7 nm.
The images taken through the different filters can be assigned to the red, green and blue channels of a colour image to produce a false colour image. They can be combined in various ways but one such combination is called the Hubble Palette where Sll is assigned to the red channel, H-alpha is assigned to the Green channel and Olll is assigned to the blue channel. Some of the colourful images produced by the Hubble Space telescope have used this palette.

M1 with the Hubble Palette

Note how this narrowband false colour image highlights the filamentous structure and composition of the nebula. The green is H-alpha, red is Sll and blue is Olll. Looking at the original diagram of the combination of the primary colours will enable you to deduce the composition of parts of the nebula based on its colour. For example, yellow regions contain H-alpha and Sll etc.
Below is presented an animation which cycles through the various ways of combining the data from the Sll, H-alpha and Olll filters into a false colour image. For example, if an image is labelled SHO, this represents the Hubble palette etc:
False colour images of M1, the Crab nebula:


Nikki Mackin

 

Christmas Planets

This image of Jupiter was captured on the evening of December 24th with a DBK camera, an 11" SCT and a 1.5x Barlow:

Saturn was captured at 5-30am on Christmas day with exactly the same setup:

Keith Davies

Saturday, December 25, 2010

 

Andrew Sprott's astronomical software in 2010

During 2010 SAS member Andrew Sprott has produced software that has been published in the SPA magazine 'Popular Astronomy'. Andrew has worked with Steve Wainwright on the programs with Steve working on specifications, algorithms and testing, but Andrew has done the hard, skilled work of coding it up into useable programs.
Popular Astronomy, April-June issue 2010
Add Image
This article is about a program called Dark-Frame-Scaler, essential for frame-accumulating videography of deep-sky objects.

Popular Astronomy, September-December issue 2010

This article is about a program called 'CAP' (Colour Alignment Processor) that can be used to construct RGB colour images from monochrome images taken through red, green and blue filters. It can also be used to correct for atmospheric chromatic dispersion that produces red and blue edges to colour planetary images.
A new version of this program called AUTOCAP has now been completed. This version is completely automatic. Look out for this in 2011.
Whenever you see on this site a H-alpha solar image showing both details of the solar disk and prominences, it is highly likely that Andrew Sprott's 'Solar Layers' program will have been used to combine images exposed differently for the disk and prominences. Similarly images of the Orion nebula showing both details of the trapezium and the large clouds of luminosity in the rest of the nebula, may well have been processed in Andrew's 'FIC', (Flexible Image Combine) software.
Andrew is now working on ideas for a new computer environment in which software can be developed.

Thursday, December 23, 2010

 

Afocal imaging and the Moon December 22

It is possible to get quite good images of the Moon by using afocal techniques (photographing through the eyepiece). The choice of eyepiece can be important as is the level of zoom used with the camera to avoid vignetting. These things can be improved with experience. There are a number of afocal mounting devices (often called digiscoping mounts) that allow a digital camera to be attached to an eyepiece to facilitate the afocal process. Here is a simple device attaching a digital compact camera to a 25mm eyepiece that has been placed on a 5" Maksutov:
Remember to click on an image to get a larger view:


The image can be framed in the camera preview screen and focused. Then the 10s timer is used so that vibrations dampen down after the shutter is pressed and before the exposure is made. This is the view from above and to the side:


Here are some results obtained this way:

Can you see the cat on the Moon?





Focus, of course, is everything and patience is needed to get it right.
Happy Christmas one and all.
Steve Wainwright

Sunday, December 19, 2010

 

Daytime Moon and Jupiter

On Saturday 18th, using a newly discovered method of daytime aligning a Synscam AZ GOTO mount, the Moon and then Jupiter were located in a daytime sky. The Moon, of course, was visible, but Jupiter could not be seen with the naked eye in the blue sky.
A DMK camera was placed at the prime focus of a 5", f/5 Newtonian and two ends of the Moon were imaged.

Copernicus area


Tycho area


Daytime Jupiter through a 3x Barlow

Look carefully and you will see some of Jupiter's moons.


A candid shot ... hmmm !




Nikki Mackin

Saturday, December 18, 2010

 

Daytime Moon and night-time Jupiter

An 80mm Apo refractor was placed on a Merlin Mount and aligned on the Moon in the daytime sky as it rose through the trees:

A compact camera was placed afocally to the 25mm eyepiece as the Moon was about to clear the trees and this image was captured.
Click on an image to get a larger view:

A red filter was placed on the nosepiece of a 1.3Mp monochrome Opticstar PL-130M CMOS camera. This camera was able to capture the whole lunar disk in the chip. The resulting AVIs were processed in Registax.


After dark an SPC900 NC with a x2 Barlow lens assembly on the end of the nosepiece was used with an 11" SCT to obtain this animation of Jupiter.
The south equatorial belt seems to be re-appearing.
Steve Wainwright

Friday, December 17, 2010

 

Intrepid Maksutov and a high-resolution Moon

On the night of the 16th the first snowfall came, followed by a patch of clear Sky. I mounted the Skymax 127 Maksutov on a Synscan AZ GOTO mount:

I placed a 1.3MP monochrome Opticstar PL-130M camera at the prime focus and captured 3x 30s frame AVIs on the Clavius region and the same on the Plato region of the Moon. The AVIs were processed in Registax to produce high-resolution images. Click on an image to have a larger view:
Clavius-Tycho region


Plato region
Steve Wainwright

Tuesday, December 14, 2010

 

M42 with an Atik camera and a focally reduced 80mm refractor

This image is composed from 10x 30s exposures and 15x 90s exposures:
Visible are M42/3 and NGC1977


Keith Davies
 

Geminids observations

Last night, (13th) SAS member Chris Playle went to a dark observing site at Mewslade where he observed 20 Geminids and 2 fireballs over a two hour period.

Rachael Sweeting and Jo Rosney-Lee observed for about 45 min from Llanelli starting at 10-30 (13th). They observed 6 Geminids and one of them was a fireball

Colin Miles observed the Geminids (14th) between 11-10pm and 11-30pm from Llanon. During this time, he saw 7 Geminids.

Colin Elphic and Don Morgan spent several hours at Fairwood and observed a large number of Geminids over their observing session

I saw 2 Geminids during a 5 minute sortie into the garden at 11-00pm (14th)

Steve Wainwright
 

Sunspots and Prominences

I used a DMK camera fitted with the lens assembly from a x2 Barlow and H-alpha & Ca K-line PST solar scopes.
AR1131 is almost over the limb and AR1133 is getting close:

Ca K-line image:

H-alpha image:

This image shows swirling magnetic activity and an arching filament, dark against the disk.

Filaments and prominences are the same structures, appearing dark when viewed against the disk of the Sun and light when viewed against the dark sky.

The next image is an animation showing a filament becoming a prominence as it crosses the limb of the Sun. 1.5s are shown with no brightness or contrast changes and it can be seen that the filament and the prominence have the same brightness. The next 1.5s shows the same image with the prominences enhanced by combining an image exposed to optimally reveal the prominence:

The human eye has the dynamic range to be able to see the prominences brighter against the sky.
Steve Wainwright

Sunday, December 12, 2010

 

The Sun and Moon today

I used a H-alpha PST and a Ca K_line PST with a DMK camera fitted with the lens assembly of a x2 Barlow and an 80mm Apochromatic refractor fitted with a 1000 Oaks glass solar filter.
Sometimes, when you are imaging, the unexpected happens:

Click on images to get a larger view.
AR1131 and AR1133 in H-alpha light

A hedgerow Prominence in H-alpha light


AR1131 and AR1133 in Ca K-line ligh


AR1131 and 1133 in white light with an 80mm apochromatic refractor and a glass 1000 Oaks Solar filter:

Tonight the Moon was a target for two cameras with the 80mm refractor:
DMK Image:

1.3 Mp Trust webcam image with the camera in monochrome mode:


Steve Wainwright

 

The Christmas Lecture of the Swansea Astronomical Society

Prof Mike Edmunds gave his first rate one man dramatisation of 'Sir Isaac Remembers' in the Waterfront Museum today at 2-30pm:


The audience was enthralled and gave enthusiastic applause when the lecture/play was over:
Members of the Swansea Astronomical Society, the Historical Society and members of the public attended the event.

Friday, December 10, 2010

 

M82 with an Atik 314E colour camera and a 6", f/5 refractor

23 x 1 min exposures and 4 x 1 min 40s exposures were captured and stacked in Deep-Sky Stacker. The resulting 16bit Tiff image was post processed in Photoshop to produce this image of M82, the cigar galaxy:


A larger view

The Orion Nebula with the same camera in 2x2 binned monopchrome mode. With an 80mm refractor and an 0.5 focal reducer.
Keith Davies

Thursday, December 9, 2010

 

H-alpha narrowband image of the Horsehead and Flame nebulae

This narrowband image of the flame and horse head region was taken using a Atik 314L CCD camera with an ultra narrowband Hydrogen Alpha filter. The scope was a 80mm achromatic refractor and was guided using Guidemaster software with Shoestring Astronomy Guide USB Guideport Adapter. The image has been built up from 7 x 15 minute subs, dark-frame and bias-frame corrected and post processed in Photoshop CS5.

This image constitutes a "Work in Progress" as more colours channels will be added when possible.



Nikki Mackin
 

Deep Sky and the Sun

Deep Sky Astronomers have two lights to plague their efforts.
I wonder which is the worse:

'A lesser light to rule the night'

A modified SDC-435 video camera fitted with a very short nosepiece, a light pollution filter and a 0.5 focal reducer was used to obtain the following images with an, f/4.8, 10" Newtonian:

The Horsehead nebula

The Flame nebula

The Running Man nebula

A Trust 1.3 Mp webcam was put at the prime focus of a H-alpha PST to obtain this full disk image of the Sun.

A DMK21AS camera fitted with the lens assembly of a x2 Barlow was used with a H-alpha PST to obtain this image of AR1131 and AR1133:

The same camera setup was placed on a Ca K-line PST to obtain this image of AR1131 and AR1133

Steve Wainwright

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