BBC Sky at Night Magazine

STEP BY STEP

How to record the data you need to determine a shower’s ZHR photograph­ically

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Step 1

Use a fast mid- to wide-angle lens (eg 14-40mm). A 12V hairdryer or heater band can help keep it moisture free. Set to manual focus and use lowest f-number. Set the camera to manual, and ISO to half to two-thirds of maximum.

Step 2

Tracking or fixed mounts are fine. Focus at infinity. Selecting JPG over RAW reduces frame transfer times albeit with reduced quality. Choose exposures of 30-60 seconds. Up to 30 seconds, set camera to continuous shooting and lock the button down on a remote shutter release.

Step 3

For longer exposures, use a programmab­le release with the camera in bulb mode. Record the limiting magnitude (dimmest star visible) and radiant altitude every 15 minutes. Estimate the radiant altitude using a planetariu­m program or app.

Step 4

Download images and check for trails. Add a prefix of ‘meteor_’ onto every image in which you find one. Count how many belong to the shower. For the relative ZHR calculatio­n, you’ll also need to estimate the fraction of the sky covered by the camera.

Step 5

To calculate relative ZHR unique to your setup, chop the session into hours. Determine the shower trail count (N), fraction of sky covered (F; for example, for one-quarter sky coverage, F would equal 4), radiant height (Rh) and the average limiting magnitude (lm).

Step 6

Calculate your camera’s relative ZHR (which isn’t equivalent to a true ZHR) for the time spent observing (T obs). The population index (r) is unique for each shower and can be obtained from sources such as the Internatio­nal Meteor Organisati­on (www.imo.net).

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