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 "Movie": [Full Size, 1fps] [Half Size, 6fps]   QuickTime viewer

Click on any image to view a larger version

01  105447.73  0.015

02  105449.73  0.015

03  105451.73  0.015

04  105453.73  0.022

05  105501.68  0.045

06  105509.63  0.073
07  105517.57  0.105
08  105525.52  0.144

09  105533.46  0.189

10  105541.41  0.241
11  105549.35  0.303 12  105557.30  0.375

13  105605.24  0.457

14  105605.24  0.457

15  105621.14  0.656

16  105621.14  0.656

17  105637.03  0.886

18*  105644.97  0.994

19   105644.97  0.994

20  105700.86  0.886

21  105700.86 0.770

22  105716.75  0.656

23  105724.70  0.551

24  105732.64  0.457

25  105740.59  0.375

26  105748.54  0.303

27  105756.48  0.241

28  105804.43  0.189

29  105812.37  0.144

30  105820.32  0.105

31  105828.26  0.073

32  105836.21  0.045

33  105844.15  0.022

34  105846.15  0.015

35  105848.15  0.015
36  105850.15  0.015
Image annotations: Frame Number (01-36), Universal Time (HHMMSS.ff), Exposure Time (seconds)
*Image not obtained (tracking mirror shadowed by ill-placed eclipse-viewer walking by!)



Mid/Outer Coronal Imagery
400 mm EFL
("Wide" FOV) f/6.3 Camera Lens (All Refractive Optics) - Unguided
Fuji Superia (ISO) 200, (UMBRAPHILE camera controller)
(Exposure sequence synchronous with (above) High-Resolution Images)



View "Movie": [Full Size, 1fps] [Half Size, 6fps]

Click on any image to view a larger version

01  105447.73  0.015
02  105449.73  0.015
03  105451.73  0.015
04  105453.73  0.022
05  105501.68  0.045
06  105509.63  0.073
07  105517.57  0.105
08  105525.52  0.144
09  105533.46  0.189
10  105541.41  0.241
11  105549.35  0.303 12  105557.30  0.375
13  105605.24  0.457
14  105605.24  0.457
15  105621.14  0.656
16  105621.14  0.656
17  105637.03  0.886
18  105644.97  0.994
19   105644.97  0.994
20  105700.86  0.886
21  105700.86 0.770
22  105716.75  0.656
23  105724.70  0.551
24  105732.64  0.457
25  105740.59  0.375
26  105748.54  0.303
27  105756.48  0.241
28  105804.43  0.189
29  105812.37  0.189
30  105820.32  0.189
31  105828.26  0.073
32  105836.21  0.045
33  105844.15  0.022
34  105846.15  0.015
35  105848.15  0.015
36  105850.15  0.015
Image annotations: Frame Number (01-36), Universal Time (HHMMSS.ff), Exposure Time (seconds)
*Image #01 not obtained (film leader fogged).



Intermediate Field-of-View Digital (Nikon DX2) Camera
Takahashi Sky 90 Refractor, Equatorial Tracking Mount
Image Acquisition by Joel Moskowitz using UMBRAPHILE camera controller

View "Movie": [30 Mbytes]

"Quick Look" Umbraphillic Imagery by Joel Moskowitz & Glenn Schneider (More to come!)

DX2 - 3 Frame flux-scaled median combination with weighted radial median subtraction and gradient edge enhancement

Click Image Below for CII Sequence



Click Image Below for CIII Sequence




The Side-Gang (with a few in abstencia..)

(courtesy of Rowland Burley)



See eclipse imagery by David Harvey (Steward Observatory, University of Arizona) who was located ~ 100 km west of the "Side Gang".