Cloud Studies

Clouds are important indicators of weather since they make visible the conditions of the atmosphere, and they featured as an object of study throughout nineteenth- and twentieth-century meteorology. In 1802, Luke Howard (1772-1864), a chemist and amateur meteorologist, proposed a nomenclature of clouds to the Askesian Society.

In his system, Howard outlined three principle categories of cloud - cumulus, stratus and cirrus - from which all formations were based. Intermediary cloud types could be expressed as combinations of the basic three formations: cirrostratus and stratocumulus are two such examples.

Howard was not the first individual to attempt a cloud nomenclature. In 1801, Jean-Baptiste Lamarck (1744-1829) proposed a system of cloud nomenclature, but it never gained traction amongst meteorologists.

Wondered what it’s like to work in a museum?

If you’re aged 14 – 18 and interested in finding out more about a museum career, the Whipple Museum hosts two placements a year. The placements last one week but can also be combined with a week placement in the Whipple Library, giving you the opportunity to experience different types of special collections.

We host up to two placements per year within these periods:

29^th April – 10^th May

17^th – 28^th June

8^th – 19^th July

To apply, please download our Expression of Interest form and return it to hps-whipple-museum@lists.cam.ac.uk or send by post to the Learning Coordinator, Whipple Museum of the History of Science, Free School Lane, Cambridge, CB2 3RH. 

Priority will be given to state schools and schools within target areas. The deadline for the April-May dates is the 12th January. For the remaining dates, the deadline for applications is the end of February half term. 

Interested in experiences in different museums? The University of Cambridge Museums also offer work experience taster days and placements across the year. Find out more about how to apply here: https://www.museums.cam.ac.uk/Opportunities

Volunteers play a significant role at the Whipple, helping out with events, audience research and taught sessions. You don’t need to have any previous experience in order to get involved with volunteering at the Whipple, although enthusiasm about the History of Science and museums and heritage is encouraged. We have an excellent team of volunteers, and hugely appreciate the time they give up to help us fulfil our aims.

Training will be provided for each role, and volunteers will be encouraged to take on new tasks when opportunities arise.

We regularly recruit Events and Outreach Volunteers as well as Audience Research Volunteers. All applications are taken via the University of Cambridge Museum's Volunteer Makers platform, here: https://ucm.volunteermakers.org. 

November 2019 marked the 75th anniversary of Robert Whipple's donation of scientific instruments and rare books to the University of Cambridge

In 1944, Robert S. Whipple (1871-1953) presented his collection of more than 1,000 scientific instruments and a similar number of related rare books to the University, hoping to promote history of science as a subject of study and research. In November of that year, an exhibition was held in the East Room of the Old Schools to mark the official presentation of R. S. Whipple's gift.

We are celebrating this with our 75th Anniversary Exhibition in our Special Exhibition Gallery, which explores the founding of the Whipple Museum and Library through objects, books and archive material.

The nephoscope

The nephoscope was invented in the nineteenth-century to measure the altitude, direction and velocity of clouds. Seventeenth- and eighteenth-century methods of determining cloud height required triangulation from the ends of two baselines. Other techniques involved using a map to trace the passage of cloud-shadows over the countryside, or a camera obscura to measure a cloud's angular height and bearing from 0º north, (known in astronomy as 'azimuth').

Early nineteenth-century mirror nephoscopes used a shallow tank of inky water to reflect the sky and employed the same triangulating technique as the camera obscura, in which the angle of reflection was used to calculate the height of a cloud. Unfortunately, the image produced using the reflecting pool was rather restricted and wind easily disrupted its surface.

In 1846, the French meteorologist G. Aimé incorporated a horizontal mirror into nephoscope design, which significantly improved the instrument. Fineman's nephoscope, first manufactured in 1886, employed darkened glass and was fitted with a compass needle (Image 1). A vertical pointer rotated around the glass edge to be aligned with a cloud observed in the glass reflection. Engraved on the surface of the glass, concentric circles functioned as a measurement guide.

This example of a Fineman's Mirror Nephoscope was produced by the French firm Pellin, which Philibért Pellin (1847-1923) acquired from Jules Duboscq (1817-1886) after several years of collaboration and partnership. Maintaining Duboscq's excellent reputation, Pellin and his son Félix produced optical and meteorological instruments of the highest calibre.

Cloud cameras

Photography also developed into another technology used for studying clouds and became an essential tool for training young meteorologists during the twentieth century.

By 1924, Robert Hill (1899-1991) had developed a fish-eye lens that produced a horizon-to-horizon image of the sky (Image 2 & above). The resulting photograph is distorted according to orthographic and equidistant projection so that the fish-eye image appears to bulge out at the viewer; however, it is possible to produce a 'normal' viewing vantage using the negative of Hill's fish-eye image.

If the camera apparatus is set up like a magic lantern, in which light travels through the negative and fish-eye lens to be projected onto a flat surface, a portion of the image appears in 'normal' perspective. In this way, photographs of many different views of the same cloud conditions can be printed from a single fish-eye negative.

Cloud Chambers

In addition to studying clouds in the field, late nineteenth-century scientists created artificial clouds for research in the laboratory. In 1895, C. T. R. Wilson (1869-1959) constructed a cloud chamber that produced a supersaturated water-vapour environment from which he studied the physical and optical properties of clouds (Image 3).

Early experiments with the cloud chamber enabled Wilson to determine the process of droplet formation. In his experiments, water vapour condensed around ions, which were produced from exposing the chamber to high-energy particles, such as x-rays.

In 1911, Wilson successfully photographed condensation from ionized radiation. High-energy particles, interacting with the water vapours, ionize and leave a visible and distinctive cloud trail. For instance, an electron produces thin and straight lines.

Wilson's cloud chamber experiments and the subsequent ray-track photography significantly contributed to physicists' understanding of particle behaviour and enabled scientists to establish different categories of particle 'type'. While physicists adopted the cloud chamber for their own research pursuits, Wilson remained dedicated to investigations of meteorological optics until his death.