Solar
& Planetary LtE Now in September 2021
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necessarily cited in the PDF’s CMO LtE
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¤¤••••• Subject: Jupiter
images, September 22nd 2021
Received:
Hi all,
There
is a series of Jupiter images taken in infrared. There is a large sector of low
altitude in the EZ (CH4/Y) and note a curious patch in the south polar hood in
methane band.
Christophe PELLIER
(Nantes, FRANCE)
Planetary astronomy and imaging
¤¤••••• Subject: Jupiter
images September 16th 2021
Received:
Hi all,
Some images taken under fairly good seeing. With
an "image spectrum" of all filters used that shows how the relative
albedo of each belt and zone change in function of the wavelength.
Regards
Christophe PELLIER (
Planetary astronomy and imaging
¤¤••••• Subject: Jupiter
Image 25th Sept 2021
Received:
Finally a bit of reasonable seeing for me. I
missed the spell on the 15th as I was away.
This taken with the ASI224MC colour camera.
Best Regards
Ian SHARP (Ham,
nr.Selsey, the
¤¤••••• Subject: Jupiter
(September 16th)
Received:
Hi all,
Here is
an image from September 16th. Oval BA on view.
http://www.damianpeach.com/jup21/2021-09-16-2207_9-RGBdp.jpg
Best
wishes,
Damian PEACH
(Selsey, WS, the
¤¤••••• Subject: Jupiter
2021-09-21 (UT)
Received:
Jupiter
images on
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Jupiter
& satellites
Received:
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Saturn
(September 16th)
Received:
Hi all,
Here is
an image from September 16th. Some moments of sharpness with
the planet 20º high.
http://www.damianpeach.com/sat21/2021-09-16-2052_2-RGBdp.jpg
Best
wishes,
Damian PEACH
(Selsey, WS, the
¤¤••••• Subject: Jupiter
2021-09-20(UT)
Received:
Jupiter
images on 20 Setember 2021.
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Jupiter (September
15th)
Received:
Hi all,
Here is
an image from Sep 15th. Poor seeing. The GRS is nicely
seen.
http://www.damianpeach.com/jup21/2021-09-15-2159_3-RGBdp.jpg
Best
wishes,
Damian PEACH
(Selsey, WS, the
¤¤••••• Subject: Jupiter
images September 5th 2021
Received:
Hi all
Some
images from the 5th that I forgot to send. Good seeing.
RGB,
Is, z', CH4, Y. The EZ bright patch is on the preceding limb.
Regards
Christophe PELLIER (
Planetary astronomy and imaging
¤¤••••• Subject: Jupiter
2021-09-16(UT) UV CH4
IR(1000nm)
Received:
Jupiter
images on
UV, CH4(890nm), IR(1000nm).
45cm
(Newtonian) Neptune-C
II.
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Jupiter
2021-09-16(UT)
Received:
Jupiter
images on
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Jupiter
2021-09-15(UT)
Received:
Jupiter
images on
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Jupiter
2021-09-13(UT)
Received:
Jupiter image on
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Jupiter with
Oval BA and impact site (Sep 13-14th)
Received:
Hi all,
Here is
an image from last night from Rico and myself. A spell of
fairly good seeing.
This
was taken 1hr following the impact flash event at
We did
not capture the flash itself unfortunately. No visible marking across the
cloud tops is seen.
Much
like all the previous impact flash events no visible scar was left.
http://www.damianpeach.com/jup21/2021-09-13-2340_4-RGBeedp.jpg
Best
wishes,
Damian PEACH
(Selsey, WS, the
¤¤••••• Subject: Jupiter with
GRS and Europa (Sep 13th)
Received:
Hi all,
Here is an image from last night obtained by Rico and myself
using the 50cm telescope on
A brief spell of reasonable seeing. The
GRS is central surrounded by a grayish collar. Europa in
transit at left.
http://www.damianpeach.com/jup21/2021-09-13-0056_0-RGBeedp.jpg
Best wishes,
Damian PEACH
(Selsey, WS, the
¤¤••••• Subject: Planets in
the 20th century
Received:
By the use of a 32cmNewtonian with a
Teleris 2 CCD Camera.
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Spectroscopy
of Jupiter on 2021/08/31: albedo, colors and reflectances
Received:
Hi all,
Here
are some results obtained with the Aply600 spectroscope on Jupiter.
To
summarize:
1)
I have
been able to obtain a full albedo spectrum by summing 9 individual spectra taken
over the different domains of the planet (slit width = 23µm and 5"). No
solar star was observed (too faint, it failed) and so the albedo has been found
first by the spectrophotometry method (apparent magnitudes taken from a flux
spectrum), then by calculating normalized magnitudes, and then the photometric
albedos. Vmag was -2,88 that night (ephemerides:
-2,86). More explanations are on the graph.
The comparison with the reference from Erich Karkoschka show a correct profile
but a noticeably slope difference. This would more likely come from an error
while correcting the instrument's response ; but
despite looking for it I have not been able to find one.
I have also some data taken with photometric filters ;
this could help me to evaluate if and how the slope is really wrong!
2)
I'm
adding a simple color spectrum of the planet, just like we see it through eyes
and camera.
3)
Finally,
I have tried to compare the relative individual reflectances of the different
domains observed. The third graph correctly finds the
Best
regards,
Christophe
Christophe PELLIER (
Planetary astronomy and imaging
¤¤••••• Subject: Jupiter 2021-09-10 (UT)
Received:
Jupiter
images on
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Solar image
2021-09-10 (UT)
Received: 10 September 2021 at 13:46 JST
Solar image on
Best
regards,
Tomio AKUTSU (
¤¤••••• Subject: Jupiter
images, 30th August 2021 - test of the Chroma Technology CH4 filter
Received:
Hi all,
This was
mainly a test under poor seeing of the Chroma Technology CH4 filter, which
looks to be as perfect of their UV (so-called "Bessel U") filter.
A comparison with my good old Idas CH4 filter shows an equal
luminosity of the image... but with a noticeable higher contrast. This is due
to the "square" transmission of the Chroma filter, while the IDAS presents lower transmission before, and after, the CH4
absorption band. On such a narrow band, the design of the transmission of a
given filter is critical and will lead to noticeable differences on the
performances.
Christophe
Christophe PELLIER (
Planetary astronomy and imaging
¤¤••••• Subject: Jupiter 2021-09-07
(UT)
Received:
Jupiter
images on
Best
regards,
Tomio AKUTSU (