wavelength photography - colourful landscape photography, Australian wilderness photography, architectural photography, stock photography, total solar eclipse posters, travel photos, images of nature and more

multiple exposure sequence - technical details


2002 Total Solar Eclipse Sequence, Lake Everard, South Australia.


The following is a detailed summary of the equipment and exposures used to create this multiple exposure sequence of the 2002 Total Solar Eclipse.

Event
  • Total solar eclipse, 4th December 2002.
Location
  • Near Lake Everard, South Australia
    (31o 25.95' South, 135o 21.24' East)
Equipment
  • Pentax 645 medium format camera
  • 150 mm Pentax A f/3.5 lens (φ = 58mm, field of view = 17o x 23o)
  • Manfrotto tripod with weight bags (filled with sand)
  • Cable release
  • Hand held spot meter
  • Darkroom timer
Film
  • Fuji Velvia ISO 50 transparency (120 roll film)
Filters
  • Hoya ND 400 (+8 stops)
  • Hoya ND 8 (+3 stops)
  • Hoya ND 4 (+2 stops)
        Total = +13 stops (equivalent to 4.0 ND, filter factor = 104, but visually unsafe)

Exposures

The table below shows the times and corresponding exposures:

Event

Time (ACST)

Shutter Speed

Aperture

Notes

1st contact

18:41:29

-

-

18:55:55

-

-

Sun placed in top corner of frame

1st photo

19:05:55

1/250

f/22-32

19:10:55

1/250

f/22-32

19:15:55

1/250

f/22-32

19:20:55

1/250

f/22-32

19:25:55

1/250

f/22

19:30:55

1/250

f/16-22

1/2 stop increase

19:35:55

1/250

f/16

1 stop increase

Totality

19:40:55

1/4

f/3.5-5.6

No filter

19:45:55

1/250

f/11-16

1 stop increase

19:50:55

1/250

f/11-16

1/2 stop increase

19:55:55

1/250

f/11

20:00:55

1/250

f/8

20:05:55

1/250

f/5.6

20:10:55

1/125

f/5.6

Last photo

20:15:55

1/30

f/5.6-8

Sunset

20:21:00

-

-

Sky exposure

20:24:00

1/500

f/11

No filter



Notes
  • At 18:55:55 the Sun was placed in the top right corner of the viewfinder to allow it to track into frame before the first exposure. This was practised beforehand.
  • The 1/2 stop and 1 stop increases in exposure around totality were made to compensate for solar limb darkening.
  • A spot meter reading taken on the horizon during totality suggested an exposure of roughly 1/2 sec at f/5.6, however the actual exposure used (1/4 sec at f/3.5-5.6) was chosen in advance, making it about 1 1/2 stops under what the meter reading suggested.
  • The sky exposure, made after sunset, was taken at 4 stops under the meter reading and probably did not contribute much to the overall image. Most of the colour in the sky was therefore formed during the totality shot.


  All images and text © Logan / Lloyd Shield 2000-2012