TOTAL
SOLAR ECLIPSE - 29 MARCH 2006
SIDE, TURKEY (31d
22'
38.7"E, 36d 45' 15"N)
Glenn Schneider
Steward Observatory, University of Arizona
All images and
movies on and linked from this page © Glenn Schneider and/or Joel
Moskowitz 2006
Chromosphere & Prominences (at contact
II)
The ephemeral and transitory
appearance of the solar chromosphere (thin, red, horizontal layer
between the photosphere and the corona), surrounded by
prominences, is captured in this time-lapse image sequence along
the Sun's western limb at, and shortly after, second contact --
unwrapped into a rectilinear projection. Time progresses from the
bottom up: (
105501.68,
105509.63,
105517.57, and
105525.52 U.T;
<-- click on times to see unprojected frames).
Click HERE
(or on the image) to see the above image sequence at twice the image
scale.
Inner Corona & Prominences
The Moon's west-to-east motion across the face of the
Sun reveals prominence on the Sun's eastern limb soon after
second contact (
left at 10:55:17.6 U.T
[<--
click to see at 2x]),
and on the Sun's western limb (
right
at 10:58:28.3 U.T. [<--
click
to see at 2x]) in these inner/mid coronal
images. Both images are composites made from the individual high
resolution (1.2 m EFL) images described below (left: images 7-19, right
images
19-30).
Click HERE (or
on the image) to see an
overlay of
the two composites, showing the solar prominences seen on both limbs.
The Diamonds & Baggets of the Contact
III Diamond Ring
...and
then, following the re-emergence of the chromosphere, the
photosphere erupted into a tight series of Baley's beads - the glinting
sparkle before the diamond ring heralding the end of a glorious
totality. Compare the above four images (
click HERE, or on the
image to see at twice the image scale), to the four, below, taken
at exactly the same instants (left to right: 105844.15
, 105846.15
, 105848.15
and 105850.15)
with a synchronously exposed wide-field camera showing the evolution of
the diamond ring against the corona enshrouded moon.
Click HERE, or on the the above image
to see at twice the image scale.
Outer Corona : Streamers & Coronal Holes
The structure of the TSE2006 corona appears roughly bi-laterally
symmetric on large spatial scales. The complexity of the outer corona,
and smaller angular-scale azimuthal anisotropies, are none-the-less
apparent in deeply exposed imagery (here, to a distance of
> 4.5 solar
radii). Composite imagery from the 400 mm EFL "wide field" camera.
Mid-Corona & Polar Brushes
An intermediate image scale details the structure of the mid-corona,
and lower surface brightness polar brushes.
Click the
above image to see at 2x finer detail.
How were the above images made?
Inner Corona/Prominences & Outer Corona
TSE 2006 was imaged with two
synchronously exposed 35mm film cameras.
The image scales, f/ ratios, film sensitivities, and exposure durations
were selected to capture the wide dynamic range and differing spatial
scales of eclipse phenomena.
CAMERA
|
1
|
2
|
Focal Length
|
1200 mm
|
400 mm
|
f/ratio
|
12
|
6.3
|
Film Speed
|
25
|
200
|
Function
|
High
Resolution
|
"Wide"
Field
|
Phenomena
|
Chromosphere/Inner Corona
|
Mid/Outer Corona
|
The two camera systems differed
in sensitivity (for equal exposure durations) by a factor of 29. (Near)
log-normal exposure ramps (15 to 1000 ms exposure durations) were
identically executed in both cameras
from CII to mid-eclipse (and, symmetrically from mid eclipse to CIII),
providing an imaging dynamic range for the imaging sequences of ~ 2000
(11 "f" stops) in addition to the intrinsic latitude of the films used
for individual exposures.
|
Camera system sensitivities "overlapped" with exposures in Camera
2 at/near contacts and Camera 1 at/near mid-eclipse (green line).
Left image
pairs shows Camera 1 exp # 22 (left) and Camera 2 exposure #33 (right),
(reproduced at the same image scale for comparison).
|
Mid-Corona
A third, asynchronous, but autonomously operated 500 mm EFL
digital camera was used to capture the mid-corona.
The three camera and imaging systems, and the images obtained
with them, are discussed below.
"High
Resolution" Chromospheric/Inner Coronal Imagery with "the Lug-a-scope"
1200 mm EFL ("Narrow" FOV) f/12 Achromatic Refractor
5-3/4" 1/8-wave coelestat (solar tracking mirror)
Kodachrome (ISO) 25 P, (UMBRAPHILE
camera controller)
Click image to view at 2x
View
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Size, 6fps] QuickTime viewer
Click on any image to view a
larger version