Nor'West News: November 11, 2021
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4<br />
Thursday <strong>November</strong> <strong>11</strong> <strong>2021</strong><br />
Capturing Sol in all its glory<br />
THE<br />
• From page 1<br />
“It amazes me that we are<br />
living in a time when we can<br />
do something that’s been out<br />
of reach of most amateurs<br />
photographers up until now.<br />
“With the help of an ordinary<br />
refractive telescope and some<br />
affordable specialist equipment<br />
we can now see the sun up<br />
close, it’s quite an experience to<br />
look at it with your own eyes,”<br />
he said.<br />
Shankar said it’s all achieved<br />
by using specialist filters and<br />
some free online software.<br />
“We start off with a white light<br />
filter which lets all the colours<br />
of the visible spectrum through,<br />
but reduces them down to a tiny<br />
percentage, less than one per<br />
cent of what we see.<br />
“This filter shows us the<br />
photosphere of the sun, the layer<br />
of the sun with all the sun spots<br />
happening on it.”<br />
Next he uses is a hydrogen<br />
alpha optical filter designed<br />
to transmit only a narrow<br />
bandwidth of light.<br />
“This filter only lets in a<br />
wavelength of light that is<br />
less than one nanometre<br />
in size; a human hair is<br />
600,000 nanometres in<br />
thickness.<br />
“It gives me amazing views<br />
of a different layer of the sun’s<br />
atmosphere, now I can now see<br />
the chromosphere,” he said.<br />
SOLAR FLARE: A big prominence exploding on the north<br />
east limb of the sun, estimated as high as five or six<br />
earths. Below – a small eruption is bigger than three<br />
earths.<br />
PHOTOS: SAI SHANKAR<br />
This layer has the temperature<br />
ranging from 6000 deg C to<br />
about 20,000 deg C.<br />
“You can still see sun spots<br />
but you can now see<br />
prominences exploding on the<br />
edge of the sun plus a lot of<br />
surface detail.<br />
“It looks amazing and it’s<br />
dynamic, over an hour it can<br />
change immensely,” Shankar<br />
said.<br />
Using a monochromatic<br />
video camera that captures at<br />
100 frames per second, he then<br />
records 30 seconds of imagery at<br />
a time.<br />
“The atmosphere of the sun<br />
is quite turbulent so it’s called<br />
‘lucky photography,’ as over that<br />
30 seconds there will be brief<br />
moments of clarity in the surface<br />
turbulence.<br />
“On screen, your watching<br />
blurry images then suddenly it<br />
jumps into clear sharp focus,“ he<br />
said.<br />
Free photographic stacking<br />
software quickly sorts the<br />
best one-to-five per cent of all<br />
the images captured to produce<br />
a clear, sharp result as a mosaic.<br />
“It finds the best frames and<br />
matches them together into a<br />
black and white image which I<br />
can then colourise to show the<br />
sun.”<br />
From there Shankar said he<br />
will manipulate with them in<br />
Photoshop and produce the<br />
images he is becoming well<br />
known for.<br />
Shanker said he plans to<br />
display his unique imagery<br />
online in the coming weeks.<br />
FACTS:<br />
•The sun is Yellow Dwarf<br />
star composed primarily of<br />
hydrogen and helium.<br />
•It is over 4.6 billion years old<br />
and compared to the largest<br />
known stars, red giants, isn’t<br />
very big, but compared to<br />
the most common type of<br />
star in the universe, the red<br />
dwarf, the sun is quite a bit<br />
larger than most.<br />
•The sun alone contains 99.8<br />
per cent of the total mass in<br />
our solar system.<br />
•It’s almost <strong>11</strong>0 times the<br />
diameter of earth.<br />
•About one million earth’s<br />
could fit inside the sun while<br />
the surface area of the sun is<br />
<strong>11</strong>,990 times that of earth.<br />
•The sun is spinning in<br />
the opposite direction to<br />
earth and is travelling at<br />
220km per second, light<br />
takes eight minutes to reach<br />
earth.<br />
•The atmosphere of the<br />
sun is composed of three<br />
layers – the photosphere,<br />
the chromosphere, and the<br />
corona – and its surface<br />
temperature is 5500 deg C<br />
•The nuclear explosions on<br />
the surface generate solar<br />
winds, which are ejections<br />
of extremely hot, charged<br />
particles of plasma and can<br />
travel through the solar<br />
system at up to 450km per<br />
second.<br />
•Our orbital speed<br />
around the sun is about<br />
(107,000km/h.<br />
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